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  <front>
    <journal-meta><journal-id journal-id-type="publisher">GMD</journal-id><journal-title-group>
    <journal-title>Geoscientific Model Development</journal-title>
    <abbrev-journal-title abbrev-type="publisher">GMD</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Geosci. Model Dev.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1991-9603</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/gmd-19-2349-2026</article-id><title-group><article-title>A Bayesian statistical method to estimate the climatology of extreme temperature under multiple scenarios: the ANKIALE package</article-title><alt-title>The ANKIALE package</alt-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Robin</surname><given-names>Yoann</given-names></name>
          <email>yoann.robin@lsce.ipsl.fr</email>
        <ext-link>https://orcid.org/0000-0003-3437-4126</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Vrac</surname><given-names>Mathieu</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-6176-0439</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Ribes</surname><given-names>Aurélien</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-5102-7885</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff3">
          <name><surname>Barbaux</surname><given-names>Occitane</given-names></name>
          
        <ext-link>https://orcid.org/0009-0004-2930-0581</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Naveau</surname><given-names>Philippe</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-7231-6210</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Laboratoire des Sciences du Climat et de l'Environnement (LSCE), CEA, CNRS, UVSQ, Université Paris-Saclay, Gif-sur-Yvette, France</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>CNRM, Université de Toulouse, Météo France, CNRS, Toulouse, France</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Autorité de sûreté nucléaire et de radioprotection (ASNR), PSE-ENV/SCAN/BEHRIG, 92260, Fontenay-aux-Roses, France</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Yoann Robin (yoann.robin@lsce.ipsl.fr)</corresp></author-notes><pub-date><day>24</day><month>March</month><year>2026</year></pub-date>
      
      <volume>19</volume>
      <issue>6</issue>
      <fpage>2349</fpage><lpage>2372</lpage>
      <history>
        <date date-type="received"><day>10</day><month>March</month><year>2025</year></date>
           <date date-type="rev-request"><day>8</day><month>May</month><year>2025</year></date>
           <date date-type="rev-recd"><day>16</day><month>February</month><year>2026</year></date>
           <date date-type="accepted"><day>11</day><month>March</month><year>2026</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2026 Yoann Robin et al.</copyright-statement>
        <copyright-year>2026</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://gmd.copernicus.org/articles/19/2349/2026/gmd-19-2349-2026.html">This article is available from https://gmd.copernicus.org/articles/19/2349/2026/gmd-19-2349-2026.html</self-uri><self-uri xlink:href="https://gmd.copernicus.org/articles/19/2349/2026/gmd-19-2349-2026.pdf">The full text article is available as a PDF file from https://gmd.copernicus.org/articles/19/2349/2026/gmd-19-2349-2026.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d2e131">We describe an improved method and the associated package for estimating the statistics of temperature extremes in a Bayesian framework. Building on previous work, this method uses a range of climate model simulations to provide a prior of the real-world changes, and then considers observations to derive a posterior estimate of past and future changes. The new version described in this study makes it possible to process several scenarios simultaneously, while keeping one single counterfactual world (i.e., the world without human influence). We offer a free licensed, easy-to-use command-line tool called ANKIALE (ANalysis of Klimate with bayesian Inference: AppLication to extreme Events), which can be used to reproduce the analyses presented here, as well as to process user-defined events. ANKIALE is based on a python code, but is designed to be used from the command line interface. ANKIALE is natively parallel, enabling it to be used on a personal computer as well as on a supercomputer. To derive the posterior, ANKIALE uses state of art MCMC-methods to sample the posterior distribution. The potential of this method and tool is illustrated via an application to maximum temperature over Europe between 1850 and 2100 (the posterior is derived from ERA5, covering the period from 1940 to 2024), at a 0.25° resolution, for a range of four emission scenarios, including a particular focus on the city of Paris (France).</p>
  </abstract>
    
<funding-group>
<award-group id="gs1">
<funding-source>Agence Nationale de la Recherche</funding-source>
<award-id>ANR-22-EXTR-0005 (TRACCS-PC4-EXTENDING project)</award-id>
</award-group>
<award-group id="gs2">
<funding-source>Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung</funding-source>
<award-id>200021_200337/1</award-id>
</award-group>
<award-group id="gs3">
<funding-source>H2020 European Research Council</funding-source>
<award-id>101003469</award-id>
</award-group>
</funding-group>
</article-meta>
  </front>
<body>
      

      
<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d2e145">Heatwaves are extreme phenomena whose frequency and intensity have increased with global warming <xref ref-type="bibr" rid="bib1.bibx85 bib1.bibx40" id="paren.1"><named-content content-type="pre">see, e.g.</named-content></xref>. Humans <xref ref-type="bibr" rid="bib1.bibx13 bib1.bibx38 bib1.bibx50" id="paren.2"><named-content content-type="pre">see, e.g.</named-content></xref>, plants <xref ref-type="bibr" rid="bib1.bibx35 bib1.bibx8" id="paren.3"><named-content content-type="pre">see, e.g.</named-content></xref>, ecosystems <xref ref-type="bibr" rid="bib1.bibx4" id="paren.4"><named-content content-type="pre">see, e.g.</named-content></xref> and infrastructure <xref ref-type="bibr" rid="bib1.bibx108" id="paren.5"><named-content content-type="pre">see, e.g.</named-content></xref>, can suffer significant damage beyond certain thresholds, so it has become necessary to be able to predict and anticipate these events. Over recent decades, these findings have led to the development of the so-called <italic>extreme event attribution studies</italic>, which consist in establishing the weight of human influence in the occurrence or intensity of an extreme event <xref ref-type="bibr" rid="bib1.bibx63" id="paren.6"/>. A number of methods and protocols have been developed <xref ref-type="bibr" rid="bib1.bibx72 bib1.bibx64 bib1.bibx77" id="paren.7"><named-content content-type="pre">see, e.g.</named-content></xref> which have enabled the analysis and attribution of a number of extreme events. The World Weather Attribution <xref ref-type="bibr" rid="bib1.bibx100" id="paren.8"/> group has specialized in producing attribution studies within a short time (typically within a week) following the occurrence of an event. Notable examples include the heatwave in Siberia in 2020 <xref ref-type="bibr" rid="bib1.bibx14" id="paren.9"/>, the heatwave in the USA and Canada in 2021 <xref ref-type="bibr" rid="bib1.bibx65" id="paren.10"/>, and the wet heatwave in India in  2023 <xref ref-type="bibr" rid="bib1.bibx103" id="paren.11"/>. Other types of event can also be analyzed, such as extreme rainfall <xref ref-type="bibr" rid="bib1.bibx102 bib1.bibx104 bib1.bibx16" id="paren.12"/>, drought <xref ref-type="bibr" rid="bib1.bibx15" id="paren.13"/>, or wildfire <xref ref-type="bibr" rid="bib1.bibx3" id="paren.14"/>, and others.</p>
      <p id="d2e207">The attribution methods listed above typically infer the climatology (i.e. the <italic>statistical distribution</italic>) of the extremes of interest by assuming that the maxima of a variable (such as annual temperature) follow a Generalized Extreme Value distribution <xref ref-type="bibr" rid="bib1.bibx17" id="paren.15"><named-content content-type="pre">see, e.g.</named-content></xref>. This distribution is characterized by three parameters, which vary with external forcings (such as global or regional mean temperature). This statistical model is inferred either independently from observations, from climate models <xref ref-type="bibr" rid="bib1.bibx64" id="paren.16"/>, or from both.</p>
      <p id="d2e222">Several recent studies have proposed to implement the latter option, i.e., combining models and observations, within a Bayesian framework. In this context, a synthesis of climate models is used as <italic>a prior</italic> of the reality, and then observations are used to derive <italic>the posterior</italic> distribution of past and future changes. For example, <xref ref-type="bibr" rid="bib1.bibx33" id="text.17"/> proposes a Bayesian approach to predicting regional climate change. Several methods for synthesizing climate models have also been proposed by <xref ref-type="bibr" rid="bib1.bibx81" id="text.18"/>, <xref ref-type="bibr" rid="bib1.bibx43" id="text.19"/>, and <xref ref-type="bibr" rid="bib1.bibx11" id="text.20"/>. <xref ref-type="bibr" rid="bib1.bibx12" id="text.21"/> also provides a summary of different observational constraint methods. More recently, <xref ref-type="bibr" rid="bib1.bibx86" id="text.22"/> studied an observational constraint approach on an Energy Balance Model trained on multiple CMIP6 models to derive estimates of historical aerosol forcing. <xref ref-type="bibr" rid="bib1.bibx105" id="text.23"/> studied the effect of short observations on the statistics of extreme events considering a Bayesian approach. Finally, <xref ref-type="bibr" rid="bib1.bibx2" id="text.24"/> also works on the changes in the distribution of the annual maximum daily maximum temperature (TXx) over Europe with CO<sub>2</sub> as covariate.</p>
      <p id="d2e265">We describe several improvements to the <xref ref-type="bibr" rid="bib1.bibx77" id="text.25"/> and <xref ref-type="bibr" rid="bib1.bibx74" id="text.26"/> method, where the Bayesian approach enables the estimation of the statistics of extremes at the end of the century according to a climate scenario and conditioned on observed data over the historical period. Firstly, the statistical method has to be re-run separately for each emission scenario considered, with no guarantee for consistency across scenarios, especially for the confidence intervals. In particular, the inferred counter-factual world (i.e., the world without human influence), is different according to the scenario, leading to communication issues for key attribution diagnoses such as the probability ratio. Our improved implementation enables us to infer all scenarios simultaneously, which ensures that only one counterfactual world is calculated. Second, we revise the sampling procedure – based on a Metropolis Hasting Monte-Carlo <xref ref-type="bibr" rid="bib1.bibx53 bib1.bibx34" id="paren.27"><named-content content-type="pre">MCMC</named-content></xref> method –, to make it consistent with recent progress in the Bayesian community. This revised implementation runs much faster than the previous one, and offers many guarantees in terms of properties and convergence of the MCMC chain.</p>
      <p id="d2e280">The improved method comes with a deeply revised python package and command-line tool. The original method of <xref ref-type="bibr" rid="bib1.bibx77" id="text.28"/> used a python code <xref ref-type="bibr" rid="bib1.bibx78" id="paren.29"><named-content content-type="pre">Non-Stationary Statistics for Extreme Attribution, NSSEA</named-content></xref>, developed for the attribution of a univariate extreme event. This code was not parallelized and required advanced knowledge of python in order to be used. Running this package over a high-resolution grid could require as long as around 20 years of CPU time. We therefore propose a new massively parallel code, developed in Python but with a command-line interface, which can process the entire domain in 10 000 h, with approximately 2.5 h per grid point (in CPU time, so about a week with 60 cores), and which is designed to be more accessible. Note that calculation times may vary if, for example, the data does not fit entirely into memory and must be split up and temporarily stored on disk (which is provided for by our new tool).</p>
      <p id="d2e291">An illustration of the potential of our revised method and packages, we analyse extreme temperature over Europe, extended to the Mediterranean basin, giving us a box from 22° W to 45.5° E, and from 26.5 to 72.5° N, as shown in Fig. <xref ref-type="fig" rid="F1"/>a. This domain contains 54 countries, 11 of which are only partially included. The exact ratio and list are given in Table S1 in the Supplement. Our attribution study focuses on the analysis of observed events as represented in ERA5, but the statistical methods and models used can describe their future evolution.  Here, we focus on estimating the climatology of the strongest temperature events already observed for each grid point in Europe (see Fig. <xref ref-type="fig" rid="F1"/>b).</p>

      <fig id="F1" specific-use="star"><label>Figure 1</label><caption><p id="d2e300">The European domain of this study, stretching from 22° W to 45.5° E, and from 26.5 to 72.5° N, here delimited by the black box. <bold>(a)</bold> The ISO-3166-1 codes of the countries in the domain have been added (see Table S1). The colored areas follow the <xref ref-type="bibr" rid="bib1.bibx90" id="text.30"/> M49 norm. <bold>(b)</bold> Maximum temperature observed (ERA5) between 1940 and 2024.</p></caption>
        <graphic xlink:href="https://gmd.copernicus.org/articles/19/2349/2026/gmd-19-2349-2026-f01.png"/>

      </fig>

      <p id="d2e318">The paper is organized as follows. In Sect. <xref ref-type="sec" rid="Ch1.S2"/>, we present the data used: observations, climate models, and the variables we derive from them. In Sect. <xref ref-type="sec" rid="Ch1.S3"/>, the methodology is presented, using extreme temperatures at the Paris location (France) as an example. We also analyse the improvements of the new method compared to the case where the scenarios are estimated independently of each other. Section <xref ref-type="sec" rid="Ch1.S4"/> describes the new code, how it is used and what is implemented. Section <xref ref-type="sec" rid="Ch1.S5"/> then looks at current and future maxima over Europe, using a method derived from attribution. Finally, conclusions and perspectives are provided in Sect. <xref ref-type="sec" rid="Ch1.S6"/>.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Data used</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Observations</title>
      <p id="d2e346">We use the “European Reanalysis of the Atmosphere, version 5” data <xref ref-type="bibr" rid="bib1.bibx36" id="paren.31"><named-content content-type="pre">ERA5</named-content></xref> to characterize the historical observation-based extremes, and in the following, ERA5 will be referred to as “observations”. This atmospheric reanalysis combines data from weather forecasting model with observations using assimilation to produce a large number of atmospheric variables. The ERA5 reanalysis provides variables by pressure level at hourly time steps, with surface values <italic>calculated by interpolating between the lowest model level and the Earth's surface, taking account of the atmospheric conditions</italic> (<uri>https://cds.climate.copernicus.eu/datasets/reanalysis-era5-land-timeseries</uri>, last access: 19 March 2026). Note that ERA5 is a dataset that may be biased compared to actual observations, particularly for extreme events. Figure S1 in the Supplement shows the difference compared to E-OBS <xref ref-type="bibr" rid="bib1.bibx19" id="paren.32"/> – which is constructed by spatially interpolating surface observations – on average (Fig. S1a) and at maximum (Fig. S1b). The mean bias varies from 1 to 2 K, but locally can grow up to more than 10 K, particularly over North Africa. Despite such well-known limitations, ERA5 has decisive advantages in our context: global coverage (E-OBS is only available for Europe) for the entire time period, with some spatial consistency.</p>
      <p id="d2e363">From this dataset, we retain temperatures over our European zone, aggregated on a daily time step, taking daily maxima between 00:00 and 23:00 (UTC), from 1940 to 2024, at the spatial resolution 0.25°. We only retain the land grid points (<inline-formula><mml:math id="M2" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">52</mml:mn></mml:mrow></mml:math></inline-formula> % of <inline-formula><mml:math id="M3" display="inline"><mml:mrow><mml:mn mathvariant="normal">185</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">271</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M4" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 50 135 grid points), see Fig. <xref ref-type="fig" rid="F1"/>a (the Fig. <xref ref-type="fig" rid="F1"/>b is used in the Sect. <xref ref-type="sec" rid="Ch1.S5"/>).</p>
      <p id="d2e402">Let us now take a look at how the variable representing a heatwave is constructed for each ERA5 grid point. Starting with daily maximum temperatures (TX), to account for a heatwave extending over several days, we work with the <italic>annual maximum of the 3 d moving average</italic>, noted TX3x. In general, mortality increases sharply with the duration of heatwaves <xref ref-type="bibr" rid="bib1.bibx22" id="paren.33"/>, and a duration of three days allows us to capture this effect. To illustrate our methodology we zoom over the location of Paris (France). The bias of this time series compared to E-OBS has been represented on the Fig. S1c–d.</p>
      <p id="d2e411">In the statistical method used, changes in extremes are assumed to scale with global or regional average temperature – which is used as a covariate. Changes in these spatially averaged temperatures are assumed to capture the response to external forcings. The temperature over Europe will be taken from HadCRUT5 <xref ref-type="bibr" rid="bib1.bibx55 bib1.bibx61" id="paren.34"/>, available from 1850 to the present day. We have chosen to use GISTEMP <xref ref-type="bibr" rid="bib1.bibx46" id="paren.35"/> for the global temperature.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Climate models used in this study</title>
      <p id="d2e428">Global Climate Models (GCMs) from the Climate Model Intercomparison Project phase 6 <xref ref-type="bibr" rid="bib1.bibx28" id="paren.36"><named-content content-type="pre">CMIP6</named-content></xref> simulate climate evolution on a global scale, with a spatial resolution of the order of 100 to 200 km. The simulations feed into numerous scientific projects to understand physical mechanisms, evaluate models, lead multidisciplinary impact studies and serve as a reference for IPCC reports <xref ref-type="bibr" rid="bib1.bibx39 bib1.bibx40 bib1.bibx41" id="paren.37"><named-content content-type="pre">see, e.g., AR6 reports</named-content></xref>.</p>
      <p id="d2e441">These simulations consist of a historical part, covering the period from 1850 to 2014, and several future emission scenarios ranging from 2015 to 2100. These scenarios are called <italic>Shared Socio-economic Pathways</italic> <xref ref-type="bibr" rid="bib1.bibx59 bib1.bibx93 bib1.bibx60" id="paren.38"><named-content content-type="pre">SSP</named-content></xref>, and describe climate evolution under assumptions of socio-economic evolution of human societies. Four scenarios will be used in this study, describing four levels of warming: the SSP1-2.6 (<inline-formula><mml:math id="M5" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1.8</mml:mn></mml:mrow></mml:math></inline-formula> K by the end of the century with respect to 1850/1900 period), the SSP2-4.5 (<inline-formula><mml:math id="M6" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2.8</mml:mn></mml:mrow></mml:math></inline-formula> K), the SSP3-7.0 (<inline-formula><mml:math id="M7" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">4.1</mml:mn></mml:mrow></mml:math></inline-formula> K) and the SSP5-8.5 (<inline-formula><mml:math id="M8" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> K) see, e.g. <xref ref-type="bibr" rid="bib1.bibx73" id="text.39"/>.</p>

<table-wrap id="T1" specific-use="star"><label>Table 1</label><caption><p id="d2e499">List of CMIP6 models used. The value is the number of members for each scenarios.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="8">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right"/>
     <oasis:colspec colnum="6" colname="col6" align="right"/>
     <oasis:colspec colnum="7" colname="col7" align="right"/>
     <oasis:colspec colnum="8" colname="col8" align="justify" colwidth="5.5cm"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">GID</oasis:entry>
         <oasis:entry colname="col2">GCM</oasis:entry>
         <oasis:entry colname="col3">Hist.</oasis:entry>
         <oasis:entry rowsep="1" namest="col4" nameend="col7" align="center">SSP </oasis:entry>
         <oasis:entry colname="col8" align="left">References</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4">1-2.6</oasis:entry>
         <oasis:entry colname="col5">2-4.5</oasis:entry>
         <oasis:entry colname="col6">3-7.0</oasis:entry>
         <oasis:entry colname="col7">5-8.5</oasis:entry>
         <oasis:entry colname="col8" align="left"/>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">AS-RCEC</oasis:entry>
         <oasis:entry colname="col2">TaiESM1</oasis:entry>
         <oasis:entry colname="col3">1</oasis:entry>
         <oasis:entry colname="col4">1</oasis:entry>
         <oasis:entry colname="col5">1</oasis:entry>
         <oasis:entry colname="col6">1</oasis:entry>
         <oasis:entry colname="col7">1</oasis:entry>
         <oasis:entry colname="col8" align="left">
                      <xref ref-type="bibr" rid="bib1.bibx45" id="text.40"/>
                    </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">AWI</oasis:entry>
         <oasis:entry colname="col2">AWI-CM-1-1-MR</oasis:entry>
         <oasis:entry colname="col3">5</oasis:entry>
         <oasis:entry colname="col4">1</oasis:entry>
         <oasis:entry colname="col5">1</oasis:entry>
         <oasis:entry colname="col6">5</oasis:entry>
         <oasis:entry colname="col7">1</oasis:entry>
         <oasis:entry colname="col8" align="left">
                      <xref ref-type="bibr" rid="bib1.bibx84" id="text.41"/>
                    </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">BCC</oasis:entry>
         <oasis:entry colname="col2">BCC-CSM2-MR</oasis:entry>
         <oasis:entry colname="col3">3</oasis:entry>
         <oasis:entry colname="col4">1</oasis:entry>
         <oasis:entry colname="col5">1</oasis:entry>
         <oasis:entry colname="col6">1</oasis:entry>
         <oasis:entry colname="col7">1</oasis:entry>
         <oasis:entry colname="col8" align="left">
                      <xref ref-type="bibr" rid="bib1.bibx99" id="text.42"/>
                    </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CAMS</oasis:entry>
         <oasis:entry colname="col2">CAMS-CSM1-0</oasis:entry>
         <oasis:entry colname="col3">1</oasis:entry>
         <oasis:entry colname="col4">1</oasis:entry>
         <oasis:entry colname="col5">1</oasis:entry>
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       <oasis:row>
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         <oasis:entry colname="col2">FGOALS-g3</oasis:entry>
         <oasis:entry colname="col3">5</oasis:entry>
         <oasis:entry colname="col4">4</oasis:entry>
         <oasis:entry colname="col5">4</oasis:entry>
         <oasis:entry colname="col6">5</oasis:entry>
         <oasis:entry colname="col7">4</oasis:entry>
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                      <xref ref-type="bibr" rid="bib1.bibx67" id="text.44"/>
                    </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CCCma</oasis:entry>
         <oasis:entry colname="col2">CanESM5</oasis:entry>
         <oasis:entry colname="col3">50</oasis:entry>
         <oasis:entry colname="col4">50</oasis:entry>
         <oasis:entry colname="col5">50</oasis:entry>
         <oasis:entry colname="col6">50</oasis:entry>
         <oasis:entry colname="col7">50</oasis:entry>
         <oasis:entry colname="col8" align="left"><xref ref-type="bibr" rid="bib1.bibx88" id="text.45"/>, <xref ref-type="bibr" rid="bib1.bibx95" id="text.46"/></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CMCC</oasis:entry>
         <oasis:entry colname="col2">CMCC-ESM2</oasis:entry>
         <oasis:entry colname="col3">1</oasis:entry>
         <oasis:entry colname="col4">1</oasis:entry>
         <oasis:entry colname="col5">1</oasis:entry>
         <oasis:entry colname="col6">1</oasis:entry>
         <oasis:entry colname="col7">1</oasis:entry>
         <oasis:entry colname="col8" align="left">
                      <xref ref-type="bibr" rid="bib1.bibx47" id="text.47"/>
                    </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CNRM-CERFACS</oasis:entry>
         <oasis:entry colname="col2">CNRM-CM6-1</oasis:entry>
         <oasis:entry colname="col3">30</oasis:entry>
         <oasis:entry colname="col4">1</oasis:entry>
         <oasis:entry colname="col5">1</oasis:entry>
         <oasis:entry colname="col6">3</oasis:entry>
         <oasis:entry colname="col7">1</oasis:entry>
         <oasis:entry colname="col8" align="left">
                      <xref ref-type="bibr" rid="bib1.bibx96" id="text.48"/>
                    </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CNRM-CERFACS</oasis:entry>
         <oasis:entry colname="col2">CNRM-ESM2-1</oasis:entry>
         <oasis:entry colname="col3">10</oasis:entry>
         <oasis:entry colname="col4">1</oasis:entry>
         <oasis:entry colname="col5">1</oasis:entry>
         <oasis:entry colname="col6">3</oasis:entry>
         <oasis:entry colname="col7">1</oasis:entry>
         <oasis:entry colname="col8" align="left">
                      <xref ref-type="bibr" rid="bib1.bibx82" id="text.49"/>
                    </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CSIRO</oasis:entry>
         <oasis:entry colname="col2">ACCESS-ESM1-5</oasis:entry>
         <oasis:entry colname="col3">40</oasis:entry>
         <oasis:entry colname="col4">10</oasis:entry>
         <oasis:entry colname="col5">18</oasis:entry>
         <oasis:entry colname="col6">10</oasis:entry>
         <oasis:entry colname="col7">40</oasis:entry>
         <oasis:entry colname="col8" align="left">
                      <xref ref-type="bibr" rid="bib1.bibx107" id="text.50"/>
                    </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CSIRO-ARCCSS</oasis:entry>
         <oasis:entry colname="col2">ACCESS-CM2</oasis:entry>
         <oasis:entry colname="col3">10</oasis:entry>
         <oasis:entry colname="col4">3</oasis:entry>
         <oasis:entry colname="col5">3</oasis:entry>
         <oasis:entry colname="col6">3</oasis:entry>
         <oasis:entry colname="col7">5</oasis:entry>
         <oasis:entry colname="col8" align="left">
                      <xref ref-type="bibr" rid="bib1.bibx23" id="text.51"/>
                    </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">EC-Earth-Consortium</oasis:entry>
         <oasis:entry colname="col2">EC-Earth3</oasis:entry>
         <oasis:entry colname="col3">71</oasis:entry>
         <oasis:entry colname="col4">2</oasis:entry>
         <oasis:entry colname="col5">29</oasis:entry>
         <oasis:entry colname="col6">52</oasis:entry>
         <oasis:entry colname="col7">58</oasis:entry>
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                      <xref ref-type="bibr" rid="bib1.bibx25" id="text.52"/>
                    </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">EC-Earth-Consortium</oasis:entry>
         <oasis:entry colname="col2">EC-Earth3-Veg</oasis:entry>
         <oasis:entry colname="col3">9</oasis:entry>
         <oasis:entry colname="col4">5</oasis:entry>
         <oasis:entry colname="col5">6</oasis:entry>
         <oasis:entry colname="col6">4</oasis:entry>
         <oasis:entry colname="col7">8</oasis:entry>
         <oasis:entry colname="col8" align="left">
                      <xref ref-type="bibr" rid="bib1.bibx26" id="text.53"/>
                    </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">EC-Earth-Consortium</oasis:entry>
         <oasis:entry colname="col2">EC-Earth3-Veg-LR</oasis:entry>
         <oasis:entry colname="col3">3</oasis:entry>
         <oasis:entry colname="col4">3</oasis:entry>
         <oasis:entry colname="col5">3</oasis:entry>
         <oasis:entry colname="col6">3</oasis:entry>
         <oasis:entry colname="col7">3</oasis:entry>
         <oasis:entry colname="col8" align="left">
                      <xref ref-type="bibr" rid="bib1.bibx27" id="text.54"/>
                    </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">INM</oasis:entry>
         <oasis:entry colname="col2">INM-CM4-8</oasis:entry>
         <oasis:entry colname="col3">1</oasis:entry>
         <oasis:entry colname="col4">1</oasis:entry>
         <oasis:entry colname="col5">1</oasis:entry>
         <oasis:entry colname="col6">1</oasis:entry>
         <oasis:entry colname="col7">1</oasis:entry>
         <oasis:entry colname="col8" align="left">
                      <xref ref-type="bibr" rid="bib1.bibx98" id="text.55"/>
                    </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">INM</oasis:entry>
         <oasis:entry colname="col2">INM-CM5-0</oasis:entry>
         <oasis:entry colname="col3">10</oasis:entry>
         <oasis:entry colname="col4">1</oasis:entry>
         <oasis:entry colname="col5">1</oasis:entry>
         <oasis:entry colname="col6">5</oasis:entry>
         <oasis:entry colname="col7">1</oasis:entry>
         <oasis:entry colname="col8" align="left">
                      <xref ref-type="bibr" rid="bib1.bibx97" id="text.56"/>
                    </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">IPSL</oasis:entry>
         <oasis:entry colname="col2">IPSL-CM6A-LR</oasis:entry>
         <oasis:entry colname="col3">33</oasis:entry>
         <oasis:entry colname="col4">6</oasis:entry>
         <oasis:entry colname="col5">11</oasis:entry>
         <oasis:entry colname="col6">11</oasis:entry>
         <oasis:entry colname="col7">7</oasis:entry>
         <oasis:entry colname="col8" align="left">
                      <xref ref-type="bibr" rid="bib1.bibx7" id="text.57"/>
                    </oasis:entry>
       </oasis:row>
       <oasis:row>
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         <oasis:entry colname="col2">MIROC-ES2L</oasis:entry>
         <oasis:entry colname="col3">31</oasis:entry>
         <oasis:entry colname="col4">3</oasis:entry>
         <oasis:entry colname="col5">30</oasis:entry>
         <oasis:entry colname="col6">1</oasis:entry>
         <oasis:entry colname="col7">1</oasis:entry>
         <oasis:entry colname="col8" align="left">
                      <xref ref-type="bibr" rid="bib1.bibx32" id="text.58"/>
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       <oasis:row>
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         <oasis:entry colname="col2">MIROC6</oasis:entry>
         <oasis:entry colname="col3">50</oasis:entry>
         <oasis:entry colname="col4">50</oasis:entry>
         <oasis:entry colname="col5">50</oasis:entry>
         <oasis:entry colname="col6">3</oasis:entry>
         <oasis:entry colname="col7">50</oasis:entry>
         <oasis:entry colname="col8" align="left">
                      <xref ref-type="bibr" rid="bib1.bibx89" id="text.59"/>
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       </oasis:row>
       <oasis:row>
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         <oasis:entry colname="col2">UKESM1-0-LL</oasis:entry>
         <oasis:entry colname="col3">16</oasis:entry>
         <oasis:entry colname="col4">16</oasis:entry>
         <oasis:entry colname="col5">16</oasis:entry>
         <oasis:entry colname="col6">16</oasis:entry>
         <oasis:entry colname="col7">5</oasis:entry>
         <oasis:entry colname="col8" align="left">
                      <xref ref-type="bibr" rid="bib1.bibx31" id="text.60"/>
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       <oasis:row>
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         <oasis:entry colname="col2">MPI-ESM1-2-LR</oasis:entry>
         <oasis:entry colname="col3">31</oasis:entry>
         <oasis:entry colname="col4">10</oasis:entry>
         <oasis:entry colname="col5">10</oasis:entry>
         <oasis:entry colname="col6">10</oasis:entry>
         <oasis:entry colname="col7">30</oasis:entry>
         <oasis:entry colname="col8" align="left"><xref ref-type="bibr" rid="bib1.bibx52" id="text.61"/>, <xref ref-type="bibr" rid="bib1.bibx48" id="text.62"/>, <xref ref-type="bibr" rid="bib1.bibx51" id="text.63"/></oasis:entry>
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         <oasis:entry colname="col2">MRI-ESM2-0</oasis:entry>
         <oasis:entry colname="col3">12</oasis:entry>
         <oasis:entry colname="col4">1</oasis:entry>
         <oasis:entry colname="col5">9</oasis:entry>
         <oasis:entry colname="col6">5</oasis:entry>
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         <oasis:entry colname="col4">1</oasis:entry>
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         <oasis:entry colname="col6">3</oasis:entry>
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         <oasis:entry colname="col3">3</oasis:entry>
         <oasis:entry colname="col4">1</oasis:entry>
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         <oasis:entry colname="col3">3</oasis:entry>
         <oasis:entry colname="col4">1</oasis:entry>
         <oasis:entry colname="col5">1</oasis:entry>
         <oasis:entry colname="col6">1</oasis:entry>
         <oasis:entry colname="col7">1</oasis:entry>
         <oasis:entry colname="col8" align="left">
                      <xref ref-type="bibr" rid="bib1.bibx44" id="text.68"/>
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      <p id="d2e1358">For each model (see Table <xref ref-type="table" rid="T1"/>) we take the same variables as for the observations: TX3x on each European grid point, mean annual temperature over Europe, and over the world. These variables cover the period from 1850 to 2100, thus including the historical part as well as the future projections of the four SSPs scenarios described above.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Methodology</title>
      <p id="d2e1373">The aim of this section is to calculate the statistical parameters (of the law of extremes and covariates, but this could be more general) describing these variables, based on global and regional average temperatures and local extremes (for several simulations from climate models and observations). The method we will present here uses a Bayesian approach, where we first seek to construct a prior distribution of reality (using climate models), which we then constrain using observations, defining the posterior distribution. A key point of this approach is that the prior describes a much longer period than the one observed – typically 1850–2100 for climate models versus 1940–2024 for observations – which allows the construction of a posterior over a period where observations are absent.</p>
      <p id="d2e1376">The Sect. <xref ref-type="sec" rid="Ch1.S3.SS1"/> will present the statistical model. The inference method is described in Sect. <xref ref-type="sec" rid="Ch1.S3.SS2"/> and illustrated with a concrete example in Sect. <xref ref-type="sec" rid="Ch1.S3.SS3"/>. The Sect. <xref ref-type="sec" rid="Ch1.S3.SS4"/> will discuss the benefits of using or not using several climate scenarios simultaneously.</p>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Definition of the statistical model</title>
      <p id="d2e1395">The aim of <monospace>ANKIALE</monospace> is to enable the inference of a statistical model describing a climate variable (such as the annual maximum temperature) from either a climate model or observations (or similar product, such as reanalyses). The inference strategy, developed by <xref ref-type="bibr" rid="bib1.bibx72" id="text.69"/> in the case of a normal distribution, then by <xref ref-type="bibr" rid="bib1.bibx77" id="text.70"/> in the case of extremes, is based on a <italic>frequency analysis</italic> for climate models and a <italic>Bayesian analysis</italic> for observations. This difference in treatment stems from the idea, already exploited by <xref ref-type="bibr" rid="bib1.bibx71" id="text.71"/>, that a set of climate models can be used to construct an approximation of reality, called a <italic>prior</italic>, and that observations can be used to <italic>constrain</italic> this prior to what has been observed, allowing the construction of what is called the <italic>posterior</italic>. This posterior therefore incorporates information from climate models, constrained in such a way as to be made compatible with observations.</p>
      <p id="d2e1426">Formally, we have a climate variable <inline-formula><mml:math id="M9" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> that follows a parametric probability distribution, whose parameters can be summarised in a vector <inline-formula><mml:math id="M10" display="inline"><mml:mi mathvariant="bold-italic">θ</mml:mi></mml:math></inline-formula>. This vector <inline-formula><mml:math id="M11" display="inline"><mml:mi mathvariant="bold-italic">θ</mml:mi></mml:math></inline-formula> can incorporate parameters that control a large number of elements, such as those parameterising the intensity of external forcings that apply at a time <inline-formula><mml:math id="M12" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>, as well as the parameters of the underlying distribution. In this paper, we take as an example the annual maximum temperatures (over 3 d), which are assumed to follow a GEV (Generalised Extreme Value) distribution (see Appendix <xref ref-type="sec" rid="App1.Ch1.S1"/>), which is a standard choice in the literature for this variable <xref ref-type="bibr" rid="bib1.bibx66 bib1.bibx103 bib1.bibx3 bib1.bibx91" id="paren.72"><named-content content-type="pre">see, e.g.,</named-content></xref>. It should be noted that our method can be adapted to other types of statistical models (such as Gaussian models). This distribution has three parameters: <inline-formula><mml:math id="M13" display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula> (location parameter, similar to the mean), <inline-formula><mml:math id="M14" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> (scale parameter, similar to the standard deviation) and <inline-formula><mml:math id="M15" display="inline"><mml:mi mathvariant="italic">ξ</mml:mi></mml:math></inline-formula> (shape parameter, controlling whether or not the extremes are bounded). The first two of these parameters are assumed to evolve over time scaling with a covariable <inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, which is representative of a mean climate change.</p>
      <p id="d2e1501">A statistical model typically used in attribution, as for example by <xref ref-type="bibr" rid="bib1.bibx64" id="text.73"/> or <xref ref-type="bibr" rid="bib1.bibx62" id="text.74"/> (assuming <inline-formula><mml:math id="M17" display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is known), is given by:

            <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M18" display="block"><mml:mrow><mml:mfenced close="" open="{"><mml:mtable class="array" columnalign="left left"><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>∼</mml:mo><mml:mi mathvariant="normal">GEV</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">ξ</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:msub><mml:mi>X</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mi>log⁡</mml:mi><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>≡</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi mathvariant="italic">ξ</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>≡</mml:mo><mml:msub><mml:mi mathvariant="italic">ξ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced></mml:mrow></mml:math></disp-formula>

          The idea is that climate change modifies the location parameter <inline-formula><mml:math id="M19" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> over time (which is similar to the increase of the mean), but that the variability and shape of the extremes remain unchanged. The indicator describing climate change <inline-formula><mml:math id="M20" display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is generally given by a smoothing of the global temperature (e.g. a 15-year moving average). Then, the vector <inline-formula><mml:math id="M21" display="inline"><mml:mi mathvariant="bold-italic">θ</mml:mi></mml:math></inline-formula> of the parameters of our statistical model can be written:

            <disp-formula id="Ch1.E2" content-type="numbered"><label>2</label><mml:math id="M22" display="block"><mml:mrow><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo>:=</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">ξ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>)</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

          <inline-formula><mml:math id="M23" display="inline"><mml:mi mathvariant="bold-italic">θ</mml:mi></mml:math></inline-formula> can be estimated directly from observations or from climate simulations using maximum likelihood. Confidence intervals on <inline-formula><mml:math id="M24" display="inline"><mml:mi mathvariant="bold-italic">θ</mml:mi></mml:math></inline-formula> are constructed using bootstrap. In this model, uncertainty on the climate change indicator <inline-formula><mml:math id="M25" display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is not taken into account.</p>
      <p id="d2e1729">One further difficulty for practical application to climate data, is that the covariate <inline-formula><mml:math id="M26" display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> representing the response to climate change, is not fully well-known in general, and brings it's own uncertainty. This also applies to the breakdown between the response to natural forcings <inline-formula><mml:math id="M27" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">N</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> and the response to anthropogenic forcings <inline-formula><mml:math id="M28" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>. One possibility to include this additional uncertainty in our statistical model is to include <inline-formula><mml:math id="M29" display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> on the model parameters, thus extending the vector <inline-formula><mml:math id="M30" display="inline"><mml:mi mathvariant="bold-italic">θ</mml:mi></mml:math></inline-formula>. This type of statistical model has been studied by <xref ref-type="bibr" rid="bib1.bibx72" id="text.75"/> for the normal distribution and <xref ref-type="bibr" rid="bib1.bibx77" id="text.76"/> for the GEV distribution, including a dependence on <inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> for the scale parameter <inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. It is written as follows:

            <disp-formula id="Ch1.E3" content-type="numbered"><label>3</label><mml:math id="M33" display="block"><mml:mrow><mml:mfenced open="{" close=""><mml:mtable class="array" columnalign="left left"><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>∼</mml:mo><mml:mi mathvariant="normal">GEV</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">ξ</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:msub><mml:mi>X</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mi>log⁡</mml:mi><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:msub><mml:mi>X</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi mathvariant="italic">ξ</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>≡</mml:mo><mml:msub><mml:mi mathvariant="italic">ξ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:msup><mml:mi>X</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msup><mml:mo>+</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">N</mml:mi></mml:msubsup><mml:mo>+</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msubsup></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced></mml:mrow></mml:math></disp-formula>

          For this statistical model, <inline-formula><mml:math id="M34" display="inline"><mml:mi mathvariant="bold-italic">θ</mml:mi></mml:math></inline-formula> therefore takes the following form:

            <disp-formula id="Ch1.E4" content-type="numbered"><label>4</label><mml:math id="M35" display="block"><mml:mrow><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo>:=</mml:mo><mml:mo>(</mml:mo><mml:msup><mml:mi>X</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msup><mml:mo>,</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">N</mml:mi></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msubsup><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">ξ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>)</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

          This statistical model has several limitations: <list list-type="bullet"><list-item>
      <p id="d2e2051">It does not incorporate the work of <xref ref-type="bibr" rid="bib1.bibx68" id="text.77"/>, who worked on how to simultaneously account for global and regional covariates (which is important, for example, when the regional response differs significantly from the global response, due to aerosols).</p></list-item><list-item>
      <p id="d2e2058">Only one scenario for the future period can be used at a time, which may lead to different estimates for the historical period;</p></list-item><list-item>
      <p id="d2e2062">The parameters <inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:msup><mml:mi>X</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> (a constant) and <inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">N</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>, which model the response to natural forcings, should not depend on the scenario.</p></list-item></list> In <monospace>ANKIALE</monospace>, we propose using a statistical model that meets the following constraints: <list list-type="bullet"><list-item>
      <p id="d2e2095">The covariate can be global (denoted <inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">G</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>) and / or regional (denoted <inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">R</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>);</p></list-item><list-item>
      <p id="d2e2125">Allow for the simultaneous consideration of multiple future SSP scenarios;</p></list-item><list-item>
      <p id="d2e2129">The response to natural forcings do not depend on the SSP (or historical) scenario.</p></list-item></list></p>
      <p id="d2e2133">Starting from several climate variables <inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:msubsup><mml:mi>T</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">SSP</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M41" display="inline"><mml:mrow><mml:mi mathvariant="normal">SSP</mml:mi><mml:mo>∈</mml:mo><mml:mo mathvariant="italic">{</mml:mo><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">…</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">SSP</mml:mi></mml:msub></mml:mrow></mml:msub><mml:mo mathvariant="italic">}</mml:mo></mml:mrow></mml:math></inline-formula> (the term SSP here referring to one of the possible future scenarios, but the time series include also the historical period), this model can be written as:

            <disp-formula id="Ch1.E5" content-type="numbered"><label>5</label><mml:math id="M42" display="block"><mml:mrow><mml:mfenced open="{" close=""><mml:mtable class="array" columnalign="left left"><mml:mtr><mml:mtd><mml:mrow><mml:msubsup><mml:mi>T</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:msubsup></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>∼</mml:mo><mml:mi mathvariant="normal">GEV</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">μ</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi mathvariant="italic">ξ</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:msubsup></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">μ</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:msubsup></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi>R</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:msubsup><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mi>log⁡</mml:mi><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:msubsup></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi>R</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:msubsup><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">ξ</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:msubsup></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>≡</mml:mo><mml:msub><mml:mi mathvariant="italic">ξ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi>R</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:msubsup></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:msup><mml:mi>X</mml:mi><mml:mrow><mml:mi>R</mml:mi><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:msup><mml:mo>+</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi>R</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">N</mml:mi></mml:mrow></mml:msubsup><mml:mo>+</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi>R</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">A</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi>G</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:msubsup></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:msup><mml:mi>X</mml:mi><mml:mrow><mml:mi>G</mml:mi><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:msup><mml:mo>+</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi>G</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">N</mml:mi></mml:mrow></mml:msubsup><mml:mo>+</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi>G</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">A</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mi mathvariant="normal">⋮</mml:mi></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">⋮</mml:mi></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msubsup><mml:mi>T</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">SSP</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:msubsup></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>∼</mml:mo><mml:mi mathvariant="normal">GEV</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">μ</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">SSP</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">SSP</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi mathvariant="italic">ξ</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">SSP</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:msubsup></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">μ</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">SSP</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:msubsup></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi>R</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">SSP</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:msubsup><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mi>log⁡</mml:mi><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">SSP</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:msubsup></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi>R</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">SSP</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:msubsup><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">ξ</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">SSP</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:msubsup></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>≡</mml:mo><mml:msub><mml:mi mathvariant="italic">ξ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi>R</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">SSP</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:msubsup></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:msup><mml:mi>X</mml:mi><mml:mrow><mml:mi>R</mml:mi><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:msup><mml:mo>+</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi>R</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">N</mml:mi></mml:mrow></mml:msubsup><mml:mo>+</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi>R</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">SSP</mml:mi></mml:msub></mml:mrow></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">A</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi>G</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">SSP</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:msubsup></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:msup><mml:mi>X</mml:mi><mml:mrow><mml:mi>G</mml:mi><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:msup><mml:mo>+</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi>G</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">N</mml:mi></mml:mrow></mml:msubsup><mml:mo>+</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi>G</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">SSP</mml:mi></mml:msub></mml:mrow></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">A</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced></mml:mrow></mml:math></disp-formula>

          This model appears to be an extension of the one defined by Eq. (<xref ref-type="disp-formula" rid="Ch1.E1"/>) for each of the SSP scenarios, while incorporating the response to external forcings on <inline-formula><mml:math id="M43" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in addition to <inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. The two variables <inline-formula><mml:math id="M45" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">R</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">SSP</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M46" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">G</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">SSP</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> correspond respectively to the <italic>Regional</italic> and <italic>Global</italic> forcings of historical and each SSP scenario. They are both decomposed as the sum of a constant (<inline-formula><mml:math id="M47" display="inline"><mml:mrow><mml:msup><mml:mi>X</mml:mi><mml:mrow><mml:mi mathvariant="normal">R</mml:mi><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M48" display="inline"><mml:mrow><mml:msup><mml:mi>X</mml:mi><mml:mrow><mml:mi mathvariant="normal">G</mml:mi><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, respectively), a response to <italic>Natural</italic> forcings (<inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">R</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">N</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">G</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">N</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>, respectively) and a response to <italic>Anthropogenic</italic> forcings (<inline-formula><mml:math id="M51" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">R</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">SSP</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">A</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">G</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">SSP</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">A</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>, respectively), see Sect. S1.1 in the Supplement for the exact mathematical description and how the decomposition is performed. The vector <inline-formula><mml:math id="M53" display="inline"><mml:mi mathvariant="bold-italic">θ</mml:mi></mml:math></inline-formula>, equivalent to Eq. (<xref ref-type="disp-formula" rid="Ch1.E2"/>), and obtained after including all these terms, is given by:

            <disp-formula id="Ch1.E6" content-type="numbered"><label>6</label><mml:math id="M54" display="block"><mml:mtable rowspacing="0.2ex" class="split" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mo>:=</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo mathsize="1.1em">(</mml:mo><mml:msup><mml:mi>X</mml:mi><mml:mrow><mml:mi>R</mml:mi><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:msup><mml:mo>,</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">R</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">N</mml:mi></mml:mrow></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">R</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">A</mml:mi></mml:mrow></mml:msubsup><mml:mo>,</mml:mo><mml:mi mathvariant="normal">…</mml:mi><mml:mo>,</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">R</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">SSP</mml:mi></mml:msub></mml:mrow></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">A</mml:mi></mml:mrow></mml:msubsup><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:msup><mml:mi>X</mml:mi><mml:mrow><mml:mi mathvariant="normal">G</mml:mi><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:msup><mml:mo>,</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">G</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">N</mml:mi></mml:mrow></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">G</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">A</mml:mi></mml:mrow></mml:msubsup><mml:mo>,</mml:mo><mml:mi mathvariant="normal">…</mml:mi><mml:mo>,</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">G</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">SSP</mml:mi></mml:msub></mml:mrow></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">A</mml:mi></mml:mrow></mml:msubsup><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">ξ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo mathsize="1.1em">)</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>

          In this statistical model, only anthropogenic terms depend on the historical and SSP scenario. Compared to the model defined in Eq. (<xref ref-type="disp-formula" rid="Ch1.E1"/>), the scale parameter <inline-formula><mml:math id="M55" display="inline"><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">SSP</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> depends on <inline-formula><mml:math id="M56" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">R</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">SSP</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> and is therefore no longer constant over time. Note that the parameters <inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">μ</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">SSP</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M58" display="inline"><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">SSP</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> depend directly only on the regional forcings <inline-formula><mml:math id="M59" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">R</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">SSP</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>. They depend indirectly on the global forcings <inline-formula><mml:math id="M60" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">G</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">SSP</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> through the knowledge of the dependence between the parameters in the vector <inline-formula><mml:math id="M61" display="inline"><mml:mi mathvariant="bold-italic">θ</mml:mi></mml:math></inline-formula> (a vector that integrates all the information in the statistical model). This makes it possible to link global warming to local events. We also assume that the coefficients of the GEV distribution <inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M63" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M64" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M65" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M66" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ξ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> are independent of external forcings. This model is flexible and allows the underlying distribution to be easily modified. For example, it is possible to replace the GEV law with a Gaussian law (this statistical model is also proposed in <monospace>ANKIALE</monospace>). Other statistical models (with possibly others probability distributions), not necessarily implemented immediately, are proposed in Sect. S2.</p>
      <p id="d2e3447">In the following, in order to facilitate notation, we will break down <inline-formula><mml:math id="M67" display="inline"><mml:mi mathvariant="bold-italic">θ</mml:mi></mml:math></inline-formula> as follows:

            <disp-formula id="Ch1.Ex1"><mml:math id="M68" display="block"><mml:mrow><mml:mfenced open="{" close=""><mml:mtable class="array" columnalign="left left"><mml:mtr><mml:mtd><mml:mi mathvariant="bold-italic">θ</mml:mi></mml:mtd><mml:mtd><mml:mrow><mml:mo>:=</mml:mo><mml:mo>(</mml:mo><mml:msup><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mi mathvariant="normal">R</mml:mi></mml:msup><mml:mo>,</mml:mo><mml:msup><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mi mathvariant="normal">G</mml:mi></mml:msup><mml:mo>,</mml:mo><mml:msup><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mi mathvariant="normal">GEV</mml:mi></mml:msup><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msup><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mi mathvariant="normal">R</mml:mi></mml:msup></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>:=</mml:mo><mml:mfenced close=")" open="("><mml:mrow><mml:msup><mml:mi>X</mml:mi><mml:mrow><mml:mi mathvariant="normal">R</mml:mi><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:msup><mml:mo>,</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">R</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">N</mml:mi></mml:mrow></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">R</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">A</mml:mi></mml:mrow></mml:msubsup><mml:mo>,</mml:mo><mml:mi mathvariant="normal">…</mml:mi><mml:mo>,</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">R</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">SSP</mml:mi></mml:msub></mml:mrow></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">A</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msup><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mi mathvariant="normal">G</mml:mi></mml:msup></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>:=</mml:mo><mml:mfenced open="(" close=")"><mml:mrow><mml:msup><mml:mi>X</mml:mi><mml:mrow><mml:mi mathvariant="normal">G</mml:mi><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:msup><mml:mo>,</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">G</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">N</mml:mi></mml:mrow></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">G</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">A</mml:mi></mml:mrow></mml:msubsup><mml:mo>,</mml:mo><mml:mi mathvariant="normal">…</mml:mi><mml:mo>,</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">G</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">SSP</mml:mi><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">SSP</mml:mi></mml:msub></mml:mrow></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">A</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msup><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mi mathvariant="normal">GEV</mml:mi></mml:msup></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>:=</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">ξ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>)</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced></mml:mrow></mml:math></disp-formula></p>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Estimation strategy</title>
      <p id="d2e3738">As mentioned at the beginning of the previous section, estimation in <monospace>ANKIALE</monospace> is carried out in three steps, which are summarised in Fig. <xref ref-type="fig" rid="F2"/>. This strategy can be summarised as follows: <list list-type="order"><list-item>
      <p id="d2e3748">Inference in climate models. For each climate model <inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mi mathvariant="normal">…</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi>M</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, let <inline-formula><mml:math id="M70" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> be the value of <inline-formula><mml:math id="M71" display="inline"><mml:mi mathvariant="bold-italic">θ</mml:mi></mml:math></inline-formula> for model <inline-formula><mml:math id="M72" display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula>. We derive an estimate <inline-formula><mml:math id="M73" display="inline"><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> of <inline-formula><mml:math id="M74" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, as well as the covariance matrix describing the estimation error, denoted <inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">Σ</mml:mi><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="italic">θ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>, using a standard frequentist approach. Details are given in Appendix <xref ref-type="sec" rid="App1.Ch1.S2.SS1"/>.</p></list-item><list-item>
      <p id="d2e3846">Construction of the multi-model synthesis. At this stage, we switch to a Bayesian approach. The vector <inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is now considered a random variable for each climate model <inline-formula><mml:math id="M77" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mi mathvariant="normal">…</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi>M</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, for which we seek to estimate the probability distribution <inline-formula><mml:math id="M78" display="inline"><mml:mrow><mml:mi mathvariant="double-struck">P</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mi>m</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. Since we have an estimate <inline-formula><mml:math id="M79" display="inline"><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and a covariance matrix <inline-formula><mml:math id="M80" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">Σ</mml:mi><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="italic">θ</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>, the multivariate normal distribution is the natural choice:<disp-formula id="Ch1.Ex2"><mml:math id="M81" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mi>m</mml:mi></mml:msub><mml:mo>∼</mml:mo><mml:mi mathvariant="double-struck">P</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mi>m</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>:=</mml:mo><mml:mi mathvariant="script">N</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mover accent="true"><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mi>m</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="bold">Σ</mml:mi><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="italic">θ</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:msub><mml:mo>)</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>The multi-model synthesis, denoted <inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub></mml:mrow></mml:math></inline-formula>, follows also a multivariate normale distribution:<disp-formula id="Ch1.E7" content-type="numbered"><label>7</label><mml:math id="M83" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub><mml:mo>∼</mml:mo><mml:mi mathvariant="double-struck">P</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub><mml:mo>)</mml:mo><mml:mo>:=</mml:mo><mml:mi mathvariant="script">N</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mover accent="true"><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mo>∗</mml:mo></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="bold">Σ</mml:mi><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="italic">θ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mo>∗</mml:mo></mml:msub></mml:mrow></mml:msub><mml:mo>)</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>The mean <inline-formula><mml:math id="M84" display="inline"><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mo>∗</mml:mo></mml:msub></mml:mrow></mml:math></inline-formula> is just given by the multi-model mean, but the covariance matrix <inline-formula><mml:math id="M85" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">Σ</mml:mi><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="italic">θ</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mo>∗</mml:mo></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is more complex, and takes into account of intra and inter model uncertainy. Details are given in the Appendix <xref ref-type="sec" rid="App1.Ch1.S2.SS2"/>. It is this random variable that will serve as our <italic>prior</italic> in the following.</p></list-item><list-item>
      <p id="d2e4097">Derivation of the posterior with observations. Knowing the observations <inline-formula><mml:math id="M86" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">R</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M87" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">G</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M88" display="inline"><mml:mrow><mml:msubsup><mml:mi>T</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> (regional, global and extreme average temperatures, defined in Sect. <xref ref-type="sec" rid="Ch1.S2.SS1"/>) and the prior <inline-formula><mml:math id="M89" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub></mml:mrow></mml:math></inline-formula>, the aim here is to estimate the distribution <inline-formula><mml:math id="M90" display="inline"><mml:mrow><mml:mi mathvariant="double-struck">P</mml:mi><mml:mo>[</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mo>|</mml:mo><mml:mspace width="0.33em" linebreak="nobreak"/><mml:mo>(</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">R</mml:mi></mml:mrow></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">G</mml:mi></mml:mrow></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi>T</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msubsup><mml:mo>)</mml:mo><mml:mo>]</mml:mo></mml:mrow></mml:math></inline-formula>, i.e. the distribution of <inline-formula><mml:math id="M91" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub></mml:mrow></mml:math></inline-formula> <italic>knowing</italic> what has been observed. This conditional distribution thus incorporates information from climate models (through the prior) while being compatible with observations (via the conditioning). The derivation of the posterior from the prior is detailed in Appendix <xref ref-type="sec" rid="App1.Ch1.S2.SS3"/>.</p></list-item></list></p>
      <p id="d2e4240">We will now illustrate these different steps using temperatures in Paris.</p>

      <fig id="F2" specific-use="star"><label>Figure 2</label><caption><p id="d2e4245">Illustration of the procedure for estimating the parameter vector <inline-formula><mml:math id="M92" display="inline"><mml:mi mathvariant="bold-italic">θ</mml:mi></mml:math></inline-formula>, defined by Eqs. (<xref ref-type="disp-formula" rid="Ch1.E5"/>) and (<xref ref-type="disp-formula" rid="Ch1.E6"/>).</p></caption>
          <graphic xlink:href="https://gmd.copernicus.org/articles/19/2349/2026/gmd-19-2349-2026-f02.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Illustration with the TX3x at Paris</title>
      <p id="d2e4273">In this section, we illustrate our procedure using the annual maximum daily temperatures over 3 d (<inline-formula><mml:math id="M93" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>:=</mml:mo><mml:mtext>TX3x</mml:mtext></mml:mrow></mml:math></inline-formula>, with a slight abuse of notation in the omission of time in TX3x). According to the block-maxima theorem <xref ref-type="bibr" rid="bib1.bibx17" id="paren.78"><named-content content-type="pre">see, e.g.,</named-content></xref>, we assume that the random variable TX3x follows a GEV distribution.</p>
<sec id="Ch1.S3.SS3.SSS1">
  <label>3.3.1</label><title>Step 1: Estimations for the climate models</title>
      <p id="d2e4303">The first step is to estimate <inline-formula><mml:math id="M94" display="inline"><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M95" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">Σ</mml:mi><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="italic">θ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> for the different climate models <inline-formula><mml:math id="M96" display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula>. We can see the result for the climate model <monospace>IPSL-CM6A-LR</monospace> <xref ref-type="bibr" rid="bib1.bibx7" id="paren.79"/>, over the historical period followed by the SSP5-8.5 scenario, in Fig. <xref ref-type="fig" rid="F3"/>.</p>

      <fig id="F3" specific-use="star"><label>Figure 3</label><caption><p id="d2e4356">Illustration of the methodology described in Sect. <xref ref-type="sec" rid="Ch1.S3"/>. <bold>(a)</bold> Mean forcing (red line) for the Europe covariate of the IPSL model (grey dots), for the SSP5-8.5 scenario. The 95 % confidence interval is given by the solid red area. <bold>(b)</bold> Multi-model synthesis (light red) and posterior (dark red) after constraint by observations (in grey) for the Europe covariate, for the SSP5-8.5 scenario. <bold>(c)</bold> TX3x series in Paris from the IPSL model (grey dots) for the SSP5-8.5 scenario. The red line passing through the model data is the median, with its 95 % confidence interval (filled area). The red line above the data is the upper bound, also with its 95 % confidence interval. <bold>(d)</bold> Same as <bold>(c)</bold>, for the prior (multi-model synthesis, in light red) and the posterior (constrained by observations, in dark red). The grey dots are observations from ERA5. <bold>(e)</bold> Parameters <inline-formula><mml:math id="M97" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> as a function of <inline-formula><mml:math id="M98" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> for climate models (in grey), the multi-model synthesis (in blue), the posterior after constraint (in green), and the direct estimate from observations (orange). The ellipses represent the 95 % confidence interval for the pair of parameters. The parameters are those estimated in Paris. <bold>(f)</bold> Same as <bold>(e)</bold>, for <inline-formula><mml:math id="M99" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> as a function of <inline-formula><mml:math id="M100" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. <bold>(g)</bold> Same as <bold>(e)</bold>, for <inline-formula><mml:math id="M101" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> as a function de <inline-formula><mml:math id="M102" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. <bold>(h)</bold> Same as <bold>(e)</bold>, for <inline-formula><mml:math id="M103" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ξ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> as a function de <inline-formula><mml:math id="M104" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. </p></caption>
            <graphic xlink:href="https://gmd.copernicus.org/articles/19/2349/2026/gmd-19-2349-2026-f03.png"/>

          </fig>

      <p id="d2e4494">In Fig. <xref ref-type="fig" rid="F3"/>a, showing the regional covariate over Europe, the values of the 33 members of the IPSL model are shown in grey, and the estimate of <inline-formula><mml:math id="M105" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">R</mml:mi><mml:mo>,</mml:mo><mml:mi>m</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> in red, with the 95 % confidence interval. The covariate appears to pass through the centre of the data set (as expected), with dips caused by volcanic activity. In Fig. <xref ref-type="fig" rid="F3"/>c, showing the variable TX3x, the values of the 33 members of the IPSL model are shown in grey. The red line passing through the data is the median, with its 95 % interval. The red line above the data set is the upper bound (see Appendix <xref ref-type="sec" rid="App1.Ch1.S1"/>), with its 95 % interval.</p>
      <p id="d2e4522">We have also represented the estimates of <inline-formula><mml:math id="M106" display="inline"><mml:mrow><mml:msubsup><mml:mover accent="true"><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mi>m</mml:mi><mml:mi mathvariant="normal">GEV</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> as pairs between <inline-formula><mml:math id="M107" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and the other parameters <inline-formula><mml:math id="M108" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M109" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M110" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M111" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ξ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, in Fig. <xref ref-type="fig" rid="F3"/>e–h. These estimates are represented with the ellipse defined by the covariance matrix <inline-formula><mml:math id="M112" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">Σ</mml:mi><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="italic">θ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> at the 95 % level, in grey. We can see that the parameter <inline-formula><mml:math id="M113" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, which drives the average trend of extremes, ranges from a value of almost zero in some models to a factor of 4. The equivalent parameter for scale, <inline-formula><mml:math id="M114" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, is centred at 0. The shape parameter <inline-formula><mml:math id="M115" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ξ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is strictly negative regardless of the model, which is typical for temperatures. Note that the model with the lower <inline-formula><mml:math id="M116" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, which differs from the other climate models, is the <monospace>NorESM2-LM</monospace> model <xref ref-type="bibr" rid="bib1.bibx5" id="paren.80"><named-content content-type="pre">Norwegian</named-content></xref>.</p>
</sec>
<sec id="Ch1.S3.SS3.SSS2">
  <label>3.3.2</label><title>Step 2: construction of the prior with the multi-model synthesis</title>
      <p id="d2e4678">The next step is the multi-model synthesis, which is shown in Fig. <xref ref-type="fig" rid="F3"/>b, d (for the covariable) and Fig. <xref ref-type="fig" rid="F3"/>e–h (for the GEV parameters).</p>
      <p id="d2e4685">In Fig. <xref ref-type="fig" rid="F3"/>b, the regional covariate over Europe is shown in light red. Compared to Fig. <xref ref-type="fig" rid="F3"/>a, the 95 % confidence interval is much wider, encompassing all climate models. Since we are working with anomalies relative to the 1961–1990 period, the uncertainty is much lower in this period.</p>
      <p id="d2e4692">Figure <xref ref-type="fig" rid="F3"/>d shows in light red the median and upper bound of the GEV distribution (see Appendix <xref ref-type="sec" rid="App1.Ch1.S1"/> for the definitions of the quantile function and the upper bound), with their 95 % confidence intervals. We can see that the intervals are particularly wide compared to those of the IPSL model in Fig. <xref ref-type="fig" rid="F3"/>c, as they encompass the uncertainty from all climate models. ERA5 observations have been added (grey dots), as well as the average of observations over the period 1961/1990 (black dotted line). The median of the synthesis seems strongly biased compared to the observations, as the confidence interval does not contain the 1961/1990 mean (the median and the mean are quite close for the GEV distribution).</p>
      <p id="d2e4701">In Fig. <xref ref-type="fig" rid="F3"/>e–h, the multi-model synthesis is shown in blue. We can see that it encompasses all the parameters from each of the climate models, thus taking into account their uncertainties.</p>
</sec>
<sec id="Ch1.S3.SS3.SSS3">
  <label>3.3.3</label><title>Step 3: derivation of the posterior with observations</title>
      <p id="d2e4714">The final step is a constraint by the observations, which is shown in Fig. <xref ref-type="fig" rid="F3"/>b, d (for the covariable) and Fig. <xref ref-type="fig" rid="F3"/>e–h (for the GEV parameters).</p>
      <p id="d2e4721">Figure <xref ref-type="fig" rid="F3"/>b displays the observations in grey and the posterior in dark red for the European covariate. The posterior fits the observations well (modulo natural variability). The 95 % confidence interval appears considerably reduced (from 2° at the beginning of the century to 4° at the end of the century). The posterior is shown in dark red in Fig. <xref ref-type="fig" rid="F3"/>d. The confidence interval (both for the median and the upper bound) has been considerably reduced compared to the prior (in light red). The median also appears unbiased, with a confidence interval close to the 1961/1990 average for the historical part.</p>
      <p id="d2e4728">In Fig. <xref ref-type="fig" rid="F3"/>e–h, the posterior is shown in green. For comparison, we have also added a direct estimate from ERA5 by maximum likelihood in orange: the statistical model of Eq. (<xref ref-type="disp-formula" rid="Ch1.E1"/>) is inferred (with the addition of <inline-formula><mml:math id="M117" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> which depends on <inline-formula><mml:math id="M118" display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), and for the covariate <inline-formula><mml:math id="M119" display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> we use the posterior of <inline-formula><mml:math id="M120" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mi>R</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>. Compared to the prior (in blue), the posterior shows a significant reduction in uncertainty. It should also be noted that the posterior is not centred on the prior, but may appear shifted. With the exception of <inline-formula><mml:math id="M121" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, the direct estimate of ERA5 appears to be compatible with the prior, albeit with extremely high uncertainty: the parameter <inline-formula><mml:math id="M122" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ξ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> may even be positive in this case, allowing for extreme TX3x events with potentially colossal values. Two specific cases stand out: <list list-type="order"><list-item>
      <p id="d2e4806"><inline-formula><mml:math id="M123" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> shows significant uncertainty in ERA5 (although centred at 0), which is strongly constrained to 0 by Bayesian inference methods.</p></list-item><list-item>
      <p id="d2e4820"><inline-formula><mml:math id="M124" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> also shows significant uncertainty in ERA5, but also significant <italic>bias</italic>: the values can exceed <inline-formula><mml:math id="M125" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula> °C (in the 95 % confidence interval), whereas they do not exceed <inline-formula><mml:math id="M126" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> °C in the posterior (which implies a slope that is twice as small). The explanation lies in the fact that <inline-formula><mml:math id="M127" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in ERA5 is estimated from a very small number of values (the climate change signal is almost imperceptible before the 1990s, as we can see in Fig. <xref ref-type="fig" rid="F3"/>b). As our approach uses information from models, this parameter is estimated from future scenarios and becomes much less uncertain.</p></list-item></list></p>
</sec>
</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><title>Contribution of the multi-scenario approach in an attribution context</title>
<sec id="Ch1.S3.SS4.SSS1">
  <label>3.4.1</label><title>Analysis through the attribution of the 2019 French heatwave</title>
      <p id="d2e4885">A new feature of the statistical model developed in Eqs. (<xref ref-type="disp-formula" rid="Ch1.E5"/>) and (<xref ref-type="disp-formula" rid="Ch1.E6"/>) is the simultaneous consideration of several scenarios while requiring that the natural part of external forcings be common to the different scenarios. In order to measure the contribution of this approach, we attributed the 2019 heatwave in Paris, which has a <italic>Factual Intensity</italic> of <inline-formula><mml:math id="M128" display="inline"><mml:mrow><mml:msubsup><mml:mi>I</mml:mi><mml:mn mathvariant="normal">2019</mml:mn><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup><mml:mo>:=</mml:mo><mml:mn mathvariant="normal">38.7</mml:mn></mml:mrow></mml:math></inline-formula> °C in ERA5. Our statistical model is inferred in five cases: <list list-type="bullet"><list-item>
      <p id="d2e4914">A case where four SSP scenarios are used simultaneously, i.e. <inline-formula><mml:math id="M129" display="inline"><mml:mrow><mml:mtext>SSP</mml:mtext><mml:mo>∈</mml:mo><mml:mo mathvariant="italic">{</mml:mo><mml:mtext>SSP1-2.6</mml:mtext><mml:mo>,</mml:mo><mml:mtext>SSP2-4.5</mml:mtext><mml:mo>,</mml:mo><mml:mtext>SSP3-7.0</mml:mtext><mml:mo>,</mml:mo><mml:mtext>SSP5-8.5</mml:mtext><mml:mo mathvariant="italic">}</mml:mo></mml:mrow></mml:math></inline-formula>,</p></list-item><list-item>
      <p id="d2e4946">A case where SSP is only the SSP1-2.6 scenario,</p></list-item><list-item>
      <p id="d2e4950">A case where SSP is only the SSP2-4.5 scenario,</p></list-item><list-item>
      <p id="d2e4954">A case where SSP is only the SSP3-7.0 scenario,</p></list-item><list-item>
      <p id="d2e4958">A case where SSP is only the SSP5-8.5 scenario,</p></list-item></list> For each of these cases and each scenarios, we calculated the regional covariates <italic>Factual</italic> <inline-formula><mml:math id="M130" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> (with human influence) and <italic>Counterfactual</italic> <inline-formula><mml:math id="M131" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> (natural forcings only) as follows:

              <disp-formula id="Ch1.Ex3"><mml:math id="M132" display="block"><mml:mrow><mml:mfenced open="{" close=""><mml:mtable class="aligned" rowspacing="0.2ex" columnspacing="1em" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mo>=</mml:mo><mml:msup><mml:mi>X</mml:mi><mml:mrow><mml:mi mathvariant="normal">R</mml:mi><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:msup><mml:mo>+</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">R</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">N</mml:mi></mml:mrow></mml:msubsup><mml:mo>+</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">R</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">A</mml:mi></mml:mrow></mml:msubsup><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msubsup></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mo>=</mml:mo><mml:msup><mml:mi>X</mml:mi><mml:mrow><mml:mi mathvariant="normal">R</mml:mi><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:msup><mml:mo>+</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">R</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">N</mml:mi></mml:mrow></mml:msubsup><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced></mml:mrow></mml:math></disp-formula>

            By inserting these two terms into the parameters of locations, scales and shapes of the GEV distribution, survival functions and quantile functions can be calculated in factual and counterfactual worlds. This makes it possible to calculate the probability of exceeding the threshold <inline-formula><mml:math id="M133" display="inline"><mml:mrow><mml:msubsup><mml:mi>I</mml:mi><mml:mn mathvariant="normal">2019</mml:mn><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> each year <inline-formula><mml:math id="M134" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>, in factual and counterfactual worlds. Using the equations recalled in Appendix <xref ref-type="sec" rid="App1.Ch1.S1"/>, for a GEV distribution, the probability in the factual world <inline-formula><mml:math id="M135" display="inline"><mml:mrow><mml:msubsup><mml:mi>p</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> (resp. counterfactual <inline-formula><mml:math id="M136" display="inline"><mml:mrow><mml:msubsup><mml:mi>p</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>) that the TX3x exceeds <inline-formula><mml:math id="M137" display="inline"><mml:mrow><mml:msubsup><mml:mi>I</mml:mi><mml:mn mathvariant="normal">2019</mml:mn><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> in year <inline-formula><mml:math id="M138" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>, and the intensity <inline-formula><mml:math id="M139" display="inline"><mml:mrow><mml:msubsup><mml:mi>I</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> (or <inline-formula><mml:math id="M140" display="inline"><mml:mrow><mml:msubsup><mml:mi>I</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>) of an event with the same probability (as 2019) are given by: 

              <disp-formula id="Ch1.E8" content-type="numbered"><label>8</label><mml:math id="M141" display="block"><mml:mtable class="split" rowspacing="0.2ex" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mfenced close="" open="{"><mml:mtable class="array" columnalign="left left"><mml:mtr><mml:mtd><mml:mrow><mml:msubsup><mml:mi>p</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>:=</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">GEV</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:msubsup><mml:mi>I</mml:mi><mml:mn mathvariant="normal">2019</mml:mn><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup><mml:mo>;</mml:mo><mml:msubsup><mml:mi mathvariant="italic">μ</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi mathvariant="italic">ξ</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msubsup><mml:mi>I</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>:=</mml:mo><mml:msub><mml:mi mathvariant="script">Q</mml:mi><mml:mi mathvariant="normal">GEV</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:msubsup><mml:mi>p</mml:mi><mml:mn mathvariant="normal">2019</mml:mn><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup><mml:mo>;</mml:mo><mml:msubsup><mml:mi mathvariant="italic">μ</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi mathvariant="italic">ξ</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">μ</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mi>log⁡</mml:mi><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">ξ</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>≡</mml:mo><mml:msub><mml:mi mathvariant="italic">ξ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mfenced close="" open="{"><mml:mtable class="array" columnalign="left left"><mml:mtr><mml:mtd><mml:mrow><mml:msubsup><mml:mi>p</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msubsup></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>:=</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">GEV</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:msubsup><mml:mi>I</mml:mi><mml:mn mathvariant="normal">2019</mml:mn><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup><mml:mo>;</mml:mo><mml:msubsup><mml:mi mathvariant="italic">μ</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi mathvariant="italic">ξ</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msubsup><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msubsup><mml:mi>I</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msubsup></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>:=</mml:mo><mml:msub><mml:mi mathvariant="script">Q</mml:mi><mml:mi mathvariant="normal">GEV</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:msubsup><mml:mi>p</mml:mi><mml:mn mathvariant="normal">2019</mml:mn><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup><mml:mo>;</mml:mo><mml:msubsup><mml:mi mathvariant="italic">μ</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi mathvariant="italic">ξ</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msubsup><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">μ</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msubsup></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msubsup></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mi>log⁡</mml:mi><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msubsup></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msubsup></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">ξ</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msubsup></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>≡</mml:mo><mml:msub><mml:mi mathvariant="italic">ξ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>

            These formulas can be used to construct the classic indicators of change in intensity (<inline-formula><mml:math id="M142" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>I</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>:=</mml:mo><mml:msubsup><mml:mi>I</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup><mml:mo>-</mml:mo><mml:msubsup><mml:mi>I</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>) and probability ratio (<inline-formula><mml:math id="M143" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">PR</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>:=</mml:mo><mml:msubsup><mml:mi>p</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup><mml:mo>/</mml:mo><mml:msubsup><mml:mi>p</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>). Note that the definition of <inline-formula><mml:math id="M144" display="inline"><mml:mrow><mml:msubsup><mml:mi>I</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> naturally implies that <inline-formula><mml:math id="M145" display="inline"><mml:mrow><mml:msubsup><mml:mi>I</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2019</mml:mn></mml:mrow><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup><mml:mo>=</mml:mo><mml:msubsup><mml:mi>I</mml:mi><mml:mn mathvariant="normal">2019</mml:mn><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> (the left term is the value of a function, while the term on the right is the value of the intensity of the event, defined from the data).</p>
      <p id="d2e5744">We will use these six indicators <inline-formula><mml:math id="M146" display="inline"><mml:mrow><mml:msubsup><mml:mi>p</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M147" display="inline"><mml:mrow><mml:msubsup><mml:mi>p</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M148" display="inline"><mml:mrow><mml:msubsup><mml:mi>I</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M149" display="inline"><mml:mrow><mml:msubsup><mml:mi>I</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M150" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M151" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>, calculated in cases where scenarios are inferred together or separately, in order to analyse the contribution of our approach. To do this, we performed 5000 samples of each of these indicators according to the law defined by the posterior, and we constructed quantile-quantile diagrams between the different scenarios for the years 1850, 1884, 1950, 1992, 2050 and 2100. The last two years are only available for counterfactual variables, as the factual variables show divergences from the scenarios. The years 1884 and 1992 correspond to two minima in natural forcings (see Fig. S2). If the scenarios are analysed separately, the counterfactual worlds associated with each scenario may be different, and the quantile-quantile plots will show deviations. Our approach is expected to greatly reduce these differences. The quantile-quantile plots are shown in Fig. <xref ref-type="fig" rid="F4"/>. For each panel and each colour (blue for simultaneous scenarios, red for independent scenarios), we have six QQ plots (all possible pairs for four scenarios).</p>

      <fig id="F4" specific-use="star"><label>Figure 4</label><caption><p id="d2e5830">Quantile-quantile plot between 5000 draws of the indicators <inline-formula><mml:math id="M152" display="inline"><mml:mrow><mml:msubsup><mml:mi>p</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M153" display="inline"><mml:mrow><mml:msubsup><mml:mi>p</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M154" display="inline"><mml:mrow><mml:msubsup><mml:mi>I</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M155" display="inline"><mml:mrow><mml:msubsup><mml:mi>I</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M156" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M157" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>, for the years 1850, 1884, 1950, 1992, 2050, and 2100. The <inline-formula><mml:math id="M158" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula>-axis is the same as the <inline-formula><mml:math id="M159" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula>-axis (hence the presence of the diagonal), which is given in the first column. These indicators are constructed based on the attribution of the 2019 heatwave for the variable TX3x for all the scenarios. In red, the quantile-quantile plot is constructed when the attribution is performed considering the SSP scenarios independently. In blue, the quantile-quantile plot is constructed when the attribution is performed considering the SSP scenarios simultaneously. The years 1884 and 1992 correspond to minima in natural forcings (see Fig. S2). </p></caption>
            <graphic xlink:href="https://gmd.copernicus.org/articles/19/2349/2026/gmd-19-2349-2026-f04.png"/>

          </fig>

      <p id="d2e5933">Let us begin with the probabilities <inline-formula><mml:math id="M160" display="inline"><mml:mrow><mml:msubsup><mml:mi>p</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M161" display="inline"><mml:mrow><mml:msubsup><mml:mi>p</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>, lines a and b. In the counterfactual world in the case of joint scenarios (blue values), the quantile-quantile diagrams are almost perfectly aligned on the diagonal, showing that the data distributions of the four scenarios are indeed the same. In the case where the scenarios are handled separately (in red) in the counterfactual world, the values are much more dispersed, showing a significant deviation between the different counterfactuals. In the factual world, the results are similar in 1850 and 1884, but the dispersion around the diagonal of the dependent case is greater in 1950 and 1992, due to the influence of the scenarios. The scenarios are not supposed to intervene at these points in time (in CMIP6, the SSPs begin in 2015), but inference on the complete series makes the smoothed values of the historical part partially dependent on the values of the part where the scenarios intervene.</p>
      <p id="d2e5962">Let us continue with the intensities in the factual and counterfactual worlds, lines c and d. The results are the same as for probabilities, with the dispersion appearing greater for probabilities due to the log scale.</p>
      <p id="d2e5965">Let us conclude with the two factual and counterfactual regional covariates, lines e and f. The results are similar to the intensities and the probabilities.</p>
</sec>
<sec id="Ch1.S3.SS4.SSS2">
  <label>3.4.2</label><title>Influence of the intensity of the event</title>
      <p id="d2e5976">During an attribution exercise, the analysed event may have a probability of zero (particularly in the counterfactual world), even within the entire confidence interval. This phenomenon may lead to the appearance of ceiling or floor values through the propagation of this 0. In order to quantify the significance of this phenomenon and how the multi-scenario behaves, we propose to perform two attributions, where <inline-formula><mml:math id="M162" display="inline"><mml:mrow><mml:msubsup><mml:mi>I</mml:mi><mml:mn mathvariant="normal">2019</mml:mn><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> is defined as the median of the GEV distribution in 2019, and the 99.9 % quantile (value that may pose a problem). We have reproduced Fig. <xref ref-type="fig" rid="F4"/> for these two events in Figs. S3 and S4.</p>
      <p id="d2e5994">Figure S4, which is in a similar context to the attribution of a very strong event, is equivalent to Fig. <xref ref-type="fig" rid="F4"/>, showing the same behavior. However, Fig. S3, constructed from a probable event (50 %), shows a smaller difference between factual and counterfactual probabilities. The latter are now also distributed around the diagonal, showing equivalence between the multi-scenario and single-scenario approaches. We therefore conclude that the multi-scenario approach does indeed allow for a more consistent estimation of counterfactual probabilities between scenarios for the most extreme events, but that the contribution is weaker for more common events.</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>ANKIALE: ANalysis of Klimate with bayesian Inference: AppLication to extreme Events</title>
      <p id="d2e6010">The original method, proposed by <xref ref-type="bibr" rid="bib1.bibx77" id="text.81"/>, was accompanied by a package written in python <xref ref-type="bibr" rid="bib1.bibx92" id="paren.82"/> or R <xref ref-type="bibr" rid="bib1.bibx70" id="paren.83"/>: <italic>Non-Stationary Statistics for Extreme Attribution</italic> <xref ref-type="bibr" rid="bib1.bibx78" id="paren.84"><named-content content-type="pre">NSSEA</named-content></xref> to reproduce their results. Although this package can be used for attribution studies, the construction of its non-parallel code is not suitable for the simultaneous analysis of several thousand grid points, as is the case for a domain the size of Europe. Furthermore, its use requires in-depth knowledge of either the Python language or the R language.</p>
      <p id="d2e6030">We are therefore proposing a new package, which although written in Python, is presented as a command line tool that can be called in a bash script with the command “ank”. The architecture of the package is described in Sect. <xref ref-type="sec" rid="Ch1.S4.SS1"/>. The various steps in Sect. <xref ref-type="sec" rid="Ch1.S3.SS2"/> are broken down into sub-commands allowing them to be estimated, and are described in Sect. <xref ref-type="sec" rid="Ch1.S4.SS2"/>. Examples are provided within the package, allowing reproduction of the results presented in this paper.</p>
<sec id="Ch1.S4.SS1">
  <label>4.1</label><title>Architecture</title>
      <p id="d2e6046">The ANKIALE package contains two main classes: <monospace>ANKParams</monospace> which contains the computer parameters (temporary directories, number of CPUs, amount of memory, etc.) and <monospace>Climatology</monospace> which describes the <inline-formula><mml:math id="M163" display="inline"><mml:mi mathvariant="bold-italic">θ</mml:mi></mml:math></inline-formula> law. These two classes are instantiated when ANKIALE is launched. The first by the parameters of the user and the configuration of the system, the second either by a file passed by the user, or it is waiting to be built. The sub-module <monospace>ANKIALE.stats</monospace> then contains the classes and functions necessary for the estimations of <inline-formula><mml:math id="M164" display="inline"><mml:mi mathvariant="bold-italic">θ</mml:mi></mml:math></inline-formula>: <list list-type="bullet"><list-item>
      <p id="d2e6075">Class <monospace>ANKIALE.stats.MultiGAM</monospace>: inference of the covariates,</p></list-item><list-item>
      <p id="d2e6082">Function <monospace>ANKIALE.stats.nslaw_fit</monospace>: maximum likelihood estimation, this function is generic and accepts the different laws grouped in the sub-module <monospace>ANKIALE.stats.models</monospace>. Note that minimisation calls the external package SDFC <xref ref-type="bibr" rid="bib1.bibx75" id="paren.85"><named-content content-type="pre">Statistical Distribution Fit with Covariates</named-content></xref>.</p></list-item><list-item>
      <p id="d2e6097">Function <monospace>ANKIALE.stats.synthesis</monospace>: to build the multi-model synthesis.</p></list-item><list-item>
      <p id="d2e6104">Function <monospace>ANKIALE.stats.gaussian_</monospace><monospace>conditionning</monospace>: application of the Gaussian conditioning theorem.</p></list-item><list-item>
      <p id="d2e6114">As explained in Sect. <xref ref-type="sec" rid="Ch1.S3.SS2"/>, the bayesian constraint uses the STAN <xref ref-type="bibr" rid="bib1.bibx87" id="paren.86"/> tool, which is used by default. It is possible to revert to the original algorithm with the <monospace>-</monospace><monospace>-no-STAN</monospace> option.</p></list-item></list></p>
      <p id="d2e6127">Furthermore, the display functions are grouped in the sub-module <monospace>ANKIALE.plot</monospace>, the commands in the sub-module <monospace>ANKIALE.cmd</monospace> and the data in the sub-module <monospace>ANKIALE.data</monospace>.</p>
      <p id="d2e6139">Parallelization and memory are controlled by several parameters: <list list-type="bullet"><list-item>
      <p id="d2e6144"><monospace>-</monospace><monospace>-n-workers</monospace>: numbers of CPUs,</p></list-item><list-item>
      <p id="d2e6152"><monospace>-</monospace><monospace>-memory-per-worker</monospace>: memory for each CPU, or,</p></list-item><list-item>
      <p id="d2e6160"><monospace>-</monospace><monospace>-total-memory</monospace>: for the total available memory.</p></list-item></list></p>
      <p id="d2e6167">Parallelization occurs on several levels: <list list-type="bullet"><list-item>
      <p id="d2e6172">The samples to construct covariance matrices or confidence intervals, which are independent;</p></list-item><list-item>
      <p id="d2e6176">The grid, which can be unstructured, potentially allowing the analysis of several completely different events;</p></list-item><list-item>
      <p id="d2e6180">The scenarios, in cases where there is independence (such as when constructing confidence intervals).</p></list-item></list></p>
</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><title>Package commands</title>
      <p id="d2e6191"><def-list>
            <def-item><term><monospace>ank</monospace> <monospace>-</monospace><monospace>-help</monospace></term><def>

      <p id="d2e6205">Displays the documentation.</p>
            </def></def-item>
            <def-item><term><monospace>ank fit</monospace></term><def>

      <p id="d2e6215">Starts the estimation of <inline-formula><mml:math id="M165" display="inline"><mml:mi mathvariant="bold-italic">θ</mml:mi></mml:math></inline-formula> in the climate models simulations. The models data should be netcdf files of dimension <monospace>(time,period,run)</monospace>, where <monospace>time</monospace> is the time axis, <monospace>period</monospace> the scenarios (historical and SSPs) and <monospace>run</monospace> the different members available. Additional dimensions can be added, representing spatial coordinates (e.g. latitude and longitude). The <inline-formula><mml:math id="M166" display="inline"><mml:mi mathvariant="bold-italic">θ</mml:mi></mml:math></inline-formula> parameters are saved as a netcdf file containing the mean and covariance matrix for each estimated spatial dimensions.</p>
            </def></def-item>
            <def-item><term><monospace>ank synthesize</monospace></term><def>

      <p id="d2e6252">Performs the multi-model synthesis calculation. All the netcdf files produced by the previous command must be supplied. An important point at this stage is that each model is on its own grid, and they are interpolated onto the observation grid by nearest neighbor.</p>
            </def></def-item>
            <def-item><term><monospace>ank constrain</monospace></term><def>

      <p id="d2e6262">Starts the observation-based constraint estimation, from the output file of the previous command.</p>
            </def></def-item>
            <def-item><term><monospace>ank attribute</monospace></term><def>

      <p id="d2e6272">Starts an attribution by imposing either an event or a return time.</p>
            </def></def-item>
            <def-item><term><monospace>ank draw</monospace></term><def>

      <p id="d2e6283">Draws <inline-formula><mml:math id="M167" display="inline"><mml:mi mathvariant="bold-italic">θ</mml:mi></mml:math></inline-formula> parameters, and constructs the parameters of the statistical model given by Eq. (<xref ref-type="disp-formula" rid="Ch1.E5"/>).</p>
            </def></def-item>
            <def-item><term><monospace>ank show</monospace></term><def>

      <p id="d2e6302">Construct figures to analyze the different stages of the method.</p>
            </def></def-item>
            <def-item><term><monospace>ank example</monospace></term><def>

      <p id="d2e6312">Places in a directory ready-to-use examples including data and scripts. Currently the following examples are supported: <list list-type="bullet"><list-item>
      <p id="d2e6317">GSMT: global warming estimation, allowing to reproduce the Fig. S5. The values of global warming is in agreement with the work of <xref ref-type="bibr" rid="bib1.bibx73" id="text.87"/>.</p></list-item><list-item>
      <p id="d2e6324">Paris: estimation and attribution of TX3x at Paris, allowing to reproduce the example used in the Sect. <xref ref-type="sec" rid="Ch1.S3"/>,</p></list-item><list-item>
      <p id="d2e6330">Ile-de-France: this example reproduces the results of Sect. <xref ref-type="sec" rid="Ch1.S5"/>, except that the grid has been reduced to cover only the Ile-de-France region (France) in order to reduce the size of the data and the computing time.</p></list-item></list></p>
            </def></def-item>
            <def-item><term><monospace>Optional arguments</monospace></term><def>

      <p id="d2e6342">The optional arguments <monospace>-</monospace><monospace>-n-workers</monospace> and <monospace>-</monospace><monospace>-total-memory</monospace> allow to user to control the number of CPUs to be used, as well as the memory available. The parallelization and memory management tools are based on the package <monospace>dask</monospace> <xref ref-type="bibr" rid="bib1.bibx20" id="paren.88"><named-content content-type="pre">automatic parallelization</named-content></xref> as well as <monospace>zarr</monospace> <xref ref-type="bibr" rid="bib1.bibx54" id="paren.89"><named-content content-type="pre">temporary files on disk to minimise memory usage</named-content></xref>.</p>
            </def></def-item>
          </def-list></p>
</sec>
<sec id="Ch1.S4.SS3">
  <label>4.3</label><title>Our example with <monospace>ANKIALE</monospace></title>
      <p id="d2e6386">With <monospace>ANKIALE</monospace>, the entire procedure described in Sect. <xref ref-type="sec" rid="Ch1.S3.SS3"/> can be performed in just a few lines of commands. For inference in climate models, this estimation can be done with two successive commands, one to estimate the parameters of the covariates <inline-formula><mml:math id="M168" display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:msubsup><mml:mover accent="true"><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mi>m</mml:mi><mml:mi mathvariant="normal">R</mml:mi></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mover accent="true"><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mi>m</mml:mi><mml:mi mathvariant="normal">G</mml:mi></mml:msubsup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, and the other to estimate <inline-formula><mml:math id="M169" display="inline"><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (thus including the GEV part). Noting <monospace>&lt;file&gt;</monospace> as the input files and <monospace>&lt;climX&gt;</monospace>, <monospace>&lt;climY&gt;</monospace> as the files saving the estimates of <inline-formula><mml:math id="M170" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, this gives: <preformat><![CDATA[ank fit X --input G,<file> R,<file>
--save-clim <climX>

ank fit Y --input <file>
--load-clim <climX>  --save-clim <climY>]]></preformat> For the multi-model synthesis, noting <monospace>&lt;climY1&gt;</monospace>, <monospace>&lt;climYNM&gt;</monospace> the files of the inferred <inline-formula><mml:math id="M171" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> for each of the climate models, the command is: <preformat><![CDATA[ank synthesize --input <climY0>
<climY1> ... <climYm> --save-clim <climS>]]></preformat> Constraints based on observations are applied using the two commands: <preformat><![CDATA[ank constrain X --input <obs>
--load-clim <climS> --save-clim <climCX>

ank constrain Y --input <obs>
--load-clim <climCX> --save-clim <climCY>]]></preformat></p>
</sec>
</sec>
<sec id="Ch1.S5">
  <label>5</label><title>Highest temperatures in Europe</title>
      <p id="d2e6496">In order to study how the observed maxima behave (see Fig. <xref ref-type="fig" rid="F1"/>b) and could behave in the future, we propose to carry out their attribution. Classically, attributions, such as those carried out by the WWA <xref ref-type="bibr" rid="bib1.bibx14 bib1.bibx65 bib1.bibx103" id="paren.90"><named-content content-type="pre">see, e.g.</named-content></xref>, consider as a statistical variable the average of a climate variable (temperature, heat index, precipitation, etc.) over a domain (geographical area, country), and study an observed event and its impacts. For us, on the one hand, each ERA5 grid point in our domain will be a variable to be analyzed, and, on the other hand, we are not analyzing a specific event. No spatial dependency is considered, so the occurrence of an event at one location does not imply anything about another location. For example, we cannot use these values to calculate the probability of an event occurring across the entire region.</p>
      <p id="d2e6506">We have plotted the maps of the parameters <inline-formula><mml:math id="M172" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M173" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M174" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M175" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M176" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ξ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in Fig. <xref ref-type="fig" rid="F5"/>. The ERA5 bias for TX3x over the period 1961–1990 has also been added. None of these parameters show any particular spatial artifacts, leading us to believe that the inference was consistent between grid points. The parameter <inline-formula><mml:math id="M177" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, which drives the trend of extremes, is positive (increase of the intensity of the extremes over time) and show values between <inline-formula><mml:math id="M178" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">0.2</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M179" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2.7</mml:mn></mml:mrow></mml:math></inline-formula>, with a mean value equal to <inline-formula><mml:math id="M180" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.1</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.3</mml:mn></mml:mrow></mml:math></inline-formula>. Its value close to 1 shows an increase of the intensity parallel to regional warming. The parameter <inline-formula><mml:math id="M181" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is very close to 0 (<inline-formula><mml:math id="M182" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.008</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.03</mml:mn></mml:mrow></mml:math></inline-formula> over the map), showing that variability remains constant until the end of the century. Finally, note that <inline-formula><mml:math id="M183" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ξ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is systematically negative (which is consistent with the bounded nature of temperatures).</p>

      <fig id="F5" specific-use="star"><label>Figure 5</label><caption><p id="d2e6647">Map of the different parameters of the GEV model after observational constraints. <bold>(a)</bold> Constant of the location parameter <inline-formula><mml:math id="M184" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. <bold>(b)</bold> Trend of the location parameter <inline-formula><mml:math id="M185" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. <bold>(c)</bold> Constant of the scale parameter <inline-formula><mml:math id="M186" display="inline"><mml:mrow><mml:mi>exp⁡</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. <bold>(d)</bold> Trend of the scale parameter <inline-formula><mml:math id="M187" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. <bold>(e)</bold> Constant of the shape parameter <inline-formula><mml:math id="M188" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ξ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. <bold>(f)</bold> Bias of TX3x from ERA5 (mean over 1961/1990). </p></caption>
        <graphic xlink:href="https://gmd.copernicus.org/articles/19/2349/2026/gmd-19-2349-2026-f05.png"/>

      </fig>

      <p id="d2e6737">We start by looking at the current state of return times and intensity change, defined as <inline-formula><mml:math id="M189" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>I</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>:=</mml:mo><mml:msubsup><mml:mi>I</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">F</mml:mi></mml:msubsup><mml:mo>-</mml:mo><mml:msubsup><mml:mi>I</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> (from Eq. <xref ref-type="disp-formula" rid="Ch1.E8"/>), see Sect. <xref ref-type="sec" rid="Ch1.S5.SS1"/>. We then continue with the near future in 2040, see Sect. <xref ref-type="sec" rid="Ch1.S5.SS2"/>. We finish with the end of the 21st century, see Sect. <xref ref-type="sec" rid="Ch1.S5.SS3"/>.</p>
<sec id="Ch1.S5.SS1">
  <label>5.1</label><title>Current situation: 2024</title>
      <p id="d2e6786">Figure <xref ref-type="fig" rid="F6"/> shows the estimated return times of the maximum observed in between 2024 and 1940 in the counterfactual and factual world (Fig. <xref ref-type="fig" rid="F6"/>a–b), as well as the change in intensity (Fig. <xref ref-type="fig" rid="F6"/>c). The 95 % confidence intervals are given in Figs. S6 and S7. It should be noted that in 2024 we are in the projection period (2015 to 2100), and therefore we potentially have several choices. At this point, we consider the influence of the choice of scenario to be too weak (compared to the internal variability), and we have therefore represented the average of the four scenarios.</p>

      <fig id="F6" specific-use="star"><label>Figure 6</label><caption><p id="d2e6797"><bold>(a)</bold> Return time of the maximum observed between 1940 and 2024 in TX3x over Europe, in 2024, without human influence. <bold>(b)</bold> Same as <bold>(a)</bold>, but for the factual world. <bold>(c)</bold> Change in intensity in 2024. Lower and upper confidence intervals (95 %) are given in Figs. S6 and S7.</p></caption>
          <graphic xlink:href="https://gmd.copernicus.org/articles/19/2349/2026/gmd-19-2349-2026-f06.png"/>

        </fig>

      <p id="d2e6817">We can see that the counterfactual world shows return times (Fig. <xref ref-type="fig" rid="F6"/>a) greater than 1000 years over almost the whole of Europe, showing that the maxima currently recorded are almost impossible without anthropogenic climate change. The 95 % confidence interval shows values down to 30 years over North Africa, Central Europe and Northern Europe, but almost the entire domain shows return periods of the order of at least 500 years.</p>
      <p id="d2e6823">In the factual world, North Africa shows return periods of 2 to 5 years (Fig. <xref ref-type="fig" rid="F6"/>b), whereas in the counter-factual world they were in excess of 1000 years, showing that near-impossible events are currently becoming the new standard in this part of Europe. The same phenomenon can be seen over Western and Southern Asia, with equivalent values. The 95 % confidence intervals show the same phenomenon.</p>
      <p id="d2e6828">The temperature increase from the counter-factual to the factual world (Fig. <xref ref-type="fig" rid="F6"/>c) is fairly uniform across the domain, with values around <inline-formula><mml:math id="M190" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K. The change is nevertheless marked in Northern Europe, with values of around <inline-formula><mml:math id="M191" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1.5</mml:mn></mml:mrow></mml:math></inline-formula> K. The signal remains clearly positive, with the low value of the confidence interval around <inline-formula><mml:math id="M192" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1.5</mml:mn></mml:mrow></mml:math></inline-formula> K, and falling to <inline-formula><mml:math id="M193" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">0.6</mml:mn></mml:mrow></mml:math></inline-formula> K in Northern Europe. The high end of the confidence interval is closer to <inline-formula><mml:math id="M194" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> K, with peaks at <inline-formula><mml:math id="M195" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">3.7</mml:mn></mml:mrow></mml:math></inline-formula> K.</p>
      <p id="d2e6894">In line with all the studies on the attribution of extreme temperatures, it is clear that anthropogenic climate change implies a sharp increase in extreme temperatures. The sign of this change is unambiguous, as the low value of the confidence interval does not include a zero or negative change.</p>
      <p id="d2e6897">Let us finish with spatial variability, which appears to show breaks. Indeed, we can see that in Algeria, the return periods in Fig. <xref ref-type="fig" rid="F6"/>b can vary very rapidly from a value greater than 1000 years to less than 30 years. To understand this phenomenon, we have shown three series extracted from ERA5 in Fig. S8: one in Paris and two in Algeria showing very different return periods. On these series (the black dots), we superimposed return periods of 2, 5, 10, 30, 50, 100, and 1000 years. In order to verify the quality of the fit for our three series, we have also displayed a histogram of the <inline-formula><mml:math id="M196" display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula>-values of the Kolomogorov-Smirnov (KS) tests between 1000 draws of the GEV and ERA5 parameters. We can see that in at least 89 % of cases, the KS test gives a <inline-formula><mml:math id="M197" display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula>-value greater than 5 %, showing that we cannot reject the hypothesis that the data are indeed derived from the inferred distribution. This therefore validates our fit. The difference between the series with a return period of <inline-formula><mml:math id="M198" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">1000</mml:mn></mml:mrow></mml:math></inline-formula> years and the series with a return period of <inline-formula><mml:math id="M199" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> years is the existence of an extreme event which does not change the adjustment but alters the value of the maximum observed. The spatial variability can therefore be explained by the existence or absence of an intense heatwave.</p>
</sec>
<sec id="Ch1.S5.SS2">
  <label>5.2</label><title>Mid-term: 2040</title>
      <p id="d2e6944">First and third rows of the Fig. <xref ref-type="fig" rid="F7"/> show the return times in 2040 in the counterfactual and factual world (Fig. <xref ref-type="fig" rid="F7"/>a–e), as well as the change in intensity (Fig. <xref ref-type="fig" rid="F7"/>k–n). The 95 % confidence intervals are given in Figs. S9a–e, k–n and S10a–e, k–n. Table S2 gives a summary of the statistics by scenario and country. The 95 % confidence interval is given in Tables S3 and S4.</p>

      <fig id="F7" specific-use="star"><label>Figure 7</label><caption><p id="d2e6955">Projection of return time (1st and 2nd row) and change in intensity (3rd and 4th row) in 2040 (1st and 3rd row) and 2100 (2nd and 4th row) of the attribution of the maximum event observed in TX3x between 1940 and 2024. In columns: in the counter-factual world and for the four scenarios SSP1-2.6, SSP2-4.5, SSP3-7.0 and SSP5-8.5. Lower and upper confidence intervals (95 %) are given in Figs. S9 and S10.</p></caption>
          <graphic xlink:href="https://gmd.copernicus.org/articles/19/2349/2026/gmd-19-2349-2026-f07.png"/>

        </fig>

      <p id="d2e6964">For return times, the counterfactual world (Fig. <xref ref-type="fig" rid="F7"/>a) is the same as that in 2024 (Fig. <xref ref-type="fig" rid="F6"/>a), and shows return times of over 1000 years. The SSP2-4.5, SSP3-7.0 and SSP5-8.5 scenarios (Fig. <xref ref-type="fig" rid="F7"/>c–e) are extremely close to each other, with values between 10 and 30 years over most of Europe, falling to 1 to 2 years over North Africa. Overall, the events are more likely than at present, reflecting the rise in temperatures over 16 years. However, these 3 scenarios have not yet been differentiated, unlike SSP1-2.6, which shows slightly longer return periods. Northern France, Belgium, Great Britain and Russia also show slightly longer return periods, between 50 and 500 years.  The 95 % confidence interval (Figs. S9a–e and S10a–e) shows a similar message: the three scenarios SSP2-4.5, SSP3-7.0 and SSP5-8.5 are extremely close, and SSP1-2.6 has slightly longer return times.</p>
      <p id="d2e6974">The change in intensity in 2040, visible in Fig. <xref ref-type="fig" rid="F7"/>k–n, shows, similarly to the return times, very close values – around <inline-formula><mml:math id="M200" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M201" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> K – for the three scenarios SSP2-4.5, SSP3-7.0 and SSP5-8.5, and a scenario SSP1-2.6 with lower intensity changes of around 0.5 K. Northern Europe shows lower values, below <inline-formula><mml:math id="M202" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> K, while Eastern and Southern Europe reach almost <inline-formula><mml:math id="M203" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula> K. The 95 % confidence intervals (Figs. S9k–n and S10k–n) show a similar spatial dispersion of values, with 1 K lower values for the lower bound, and 1 K higher values for the upper bound. Some countries even show changes of more than <inline-formula><mml:math id="M204" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> K.</p>
</sec>
<sec id="Ch1.S5.SS3">
  <label>5.3</label><title>Long-term: 2100</title>
      <p id="d2e7039">Figure <xref ref-type="fig" rid="F7"/>f shows the return times in 2100 of the maximums observed in the counterfactual world, as the values are the same as for Fig. <xref ref-type="fig" rid="F7"/>a, the conclusions of Sect. <xref ref-type="sec" rid="Ch1.S5.SS2"/> apply.</p>
      <p id="d2e7048">Let us continue with the scenarios, represented on the Fig. <xref ref-type="fig" rid="F7"/>g–j. Return times decrease with simulated climate change intensity. For SSP1-2.6, only 12 countries (on 55) show return times beyond 50 years, with 28 countries already having a return time of 10 years or less. From SSP2-4.5 onwards, the current maximums are almost commonplace, with only one country showing a return period in excess of 50 years. From SSP3-7.0 onwards, current maximums are the “normal” situation, with return times between 1 to 10 years and 1 to 2 years.  The 95 % confidence interval is shown in Figs. S9g–d and S10g–d, and shows that return periods can fall below 10 years over the whole of Europe.</p>
      <p id="d2e7053">The scenarios for intensity change are represented on the Fig. <xref ref-type="fig" rid="F7"/>o–r. For scenario SSP1-2.6, the change ranges from <inline-formula><mml:math id="M205" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1.7</mml:mn></mml:mrow></mml:math></inline-formula> K for Northern Europe to <inline-formula><mml:math id="M206" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">4.1</mml:mn></mml:mrow></mml:math></inline-formula> K for Southern Europe, with the change relative to 2024 being almost the same everywhere, around <inline-formula><mml:math id="M207" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> K. For the SSP2-4.5 scenario, the change ranges from <inline-formula><mml:math id="M208" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2.7</mml:mn></mml:mrow></mml:math></inline-formula> K for Northern Europe to <inline-formula><mml:math id="M209" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">6.5</mml:mn></mml:mrow></mml:math></inline-formula> K for Southern Europe. The different regions of Europe show different changes compared to today, ranging from <inline-formula><mml:math id="M210" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1.5</mml:mn></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M211" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">3.8</mml:mn></mml:mrow></mml:math></inline-formula> K. The SSP3-7.0 and SSP5-8.5 scenarios show increasing intensity increases, from <inline-formula><mml:math id="M212" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M213" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">9</mml:mn></mml:mrow></mml:math></inline-formula> K. The 95 % confidence interval (Figs. S9o–r and S10o–r) even shows changes in intensity of up to <inline-formula><mml:math id="M214" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">18</mml:mn></mml:mrow></mml:math></inline-formula> K.</p>
</sec>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <label>6</label><title>Conclusions and perspectives</title>
<sec id="Ch1.S6.SS1">
  <label>6.1</label><title>Conclusions</title>
      <p id="d2e7175">In this paper, we have presented an extension of the <xref ref-type="bibr" rid="bib1.bibx77" id="text.91"/> method for estimating probabilities of extremes following a GEV law. Our new method allows us, on the one hand, to treat several scenarios simultaneously, and on the other, to force a counter-factual world that is common to all scenarios. We first applied this method to temperature extremes over Paris (France), and demonstrated not only its validity, but also that it drastically reduces differences in the counter-factual probabilities, reinforcing the inter-scenario consistency of our estimates. We have also verified that our estimates of current and future global climate change are consistent with current literature.</p>
      <p id="d2e7181">We also offer an open-source software that can be used to reproduce our results and easily applied to other fields.  This tool is natively parallelized, with particular attention paid to the memory used. It can be deployed just as easily on a personal computer, a computing cluster or a supercomputer.  This software is also extensible, and other probability distributions – such as the Normal or Generalized Pareto Distribution – may be integrated in the future.</p>
      <p id="d2e7184">We have applied this new approach and tool to the attribution of observed maxima over Europe, enabling us to analyze these statistics up to the end of the 21st century for four climate scenarios.  In the future, the observed maxima will become the new norm for scenarios greater than the SSP2-4.5 and SSP3-7.0, and will be 2 to 3 K warmer even for a low-emission scenario like the SSP1-2.6. An increase in extreme temperatures of more than 10 K is conceivable within the 95 % confidence interval. We have focused on Europe here, but an extension to the rest of the world and to temperature-like variables such as the heat-index would enable a global map of future heat hazards to be drawn up.</p>
      <p id="d2e7188">Compared to other studies <xref ref-type="bibr" rid="bib1.bibx94 bib1.bibx10" id="paren.92"><named-content content-type="pre">such as</named-content></xref>, the estimated return times and intensity changes can be different. This is due to different choices in the statistical model (regional covariate, smoothing method, counterfactual construction), as well as in the estimation method. As shown with the example of Paris, the use of direct observations gives a much stronger (and much more uncertain) trend, while the use of climate simulations as a prior allows for a stronger constraint on the signal. From this perspective, our approach appears much more robust. We should also note the strong influence of the choice of observation data (or similar), given the significant biases on extremes between E-OBS and ERA5. Even though datasets like ERA5 are available on a global scale, the calculation of return times (especially for impact studies) should probably be done from datasets closer to observations (such as E-OBS or stations). Several additional studies are needed to validate or refine the choices made, particularly with regard to the statistical model and the smoothing method.</p>
</sec>
<sec id="Ch1.S6.SS2">
  <label>6.2</label><title>Perspectives</title>
      <p id="d2e7204">Even improvements to the GEV model are possible. For example, the GEV model tends to overestimate return times <xref ref-type="bibr" rid="bib1.bibx21 bib1.bibx105 bib1.bibx42" id="paren.93"><named-content content-type="pre">see, e.g.</named-content></xref>. Recent work by <xref ref-type="bibr" rid="bib1.bibx58" id="text.94"/> proposed a new GEV model where the upper bound on temperatures is imposed by physics <xref ref-type="bibr" rid="bib1.bibx106 bib1.bibx57" id="paren.95"/>. This approach would fit in naturally with the tools developed here. A similar method could be applied to precipitation by mixing an estimation of the upper bound <xref ref-type="bibr" rid="bib1.bibx49" id="paren.96"/> with a statistical model as the extended Generalized Pareto Distribution <xref ref-type="bibr" rid="bib1.bibx56" id="paren.97"/>. Another interesting possibility would be to use external forcings directly as covariates rather than their responses (global and regional temperatures).</p>
      <p id="d2e7224">Further work is also needed to extend our model to other variables such as wind and precipitation. The tools and statistical model developed here were developed in the context of attribution, particularly in relation to heat waves. Several studies use other types of covariates <xref ref-type="bibr" rid="bib1.bibx86 bib1.bibx2" id="paren.98"><named-content content-type="pre">such as CO<sub>2</sub> or <inline-formula><mml:math id="M216" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, see, e.g., </named-content></xref> or statistical models. Extending this to other variables would require work similar to that of <xref ref-type="bibr" rid="bib1.bibx77" id="text.99"/>, where the validity of the statistical model was verified in each climate model, as well as its quality after applying observational constraints.</p>
      <p id="d2e7255">It should also be noted that, on the one hand, we have remained in a univariate context, while the estimation of concurrent events increasing impacts appears increasingly necessary; and on the other hand, spatial structures are ignored. We also used only GCMs, which do not capture local specificities. The use of regional models (when those from CMIP6 become available) will allow us to refine the results obtained here <xref ref-type="bibr" rid="bib1.bibx10" id="paren.100"><named-content content-type="pre">work in this direction has already been carried out by </named-content></xref>, and ANKIALE will make this easy to do.</p>
      <p id="d2e7263">Finally, the analyses produced here provide local information on the worst possible future events, and show the need for rapid adaptation to extremes warming faster than global warming.</p>
</sec>
</sec>

      
      </body>
    <back><app-group>

<app id="App1.Ch1.S1">
  <label>Appendix A</label><title>Generalized Extreme Value distribution</title>
      <p id="d2e7278">The maxima of a variable can be modelled using the GEV distribution <xref ref-type="bibr" rid="bib1.bibx17" id="paren.101"><named-content content-type="pre">Generalised Extreme Value, see the book by</named-content></xref>. This distribution has three parameters:</p>
      <p id="d2e7286"><list list-type="bullet">
          <list-item>

      <p id="d2e7291">The location parameter <inline-formula><mml:math id="M217" display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula>, similar to the mean;</p>
          </list-item>
          <list-item>

      <p id="d2e7304">The scale parameter <inline-formula><mml:math id="M218" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>, similar to the standard deviation;</p>
          </list-item>
          <list-item>

      <p id="d2e7317">The shape parameter <inline-formula><mml:math id="M219" display="inline"><mml:mi mathvariant="italic">ξ</mml:mi></mml:math></inline-formula> which controls the type of extreme. If <inline-formula><mml:math id="M220" display="inline"><mml:mrow><mml:mi mathvariant="italic">ξ</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>, the extremes are bounded, if <inline-formula><mml:math id="M221" display="inline"><mml:mrow><mml:mi mathvariant="italic">ξ</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> the distribution is said to be <italic>heavy-tailed</italic>.</p>
          </list-item>
        </list></p>
      <p id="d2e7356">Noting <inline-formula><mml:math id="M222" display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mo>+</mml:mo></mml:msub><mml:mo>:=</mml:mo><mml:mo>max⁡</mml:mo><mml:mo>(</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo><mml:mi>x</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, the cumulative distribution function <inline-formula><mml:math id="M223" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">GEV</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (and the survival function <inline-formula><mml:math id="M224" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">GEV</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) of a random variable <inline-formula><mml:math id="M225" display="inline"><mml:mrow><mml:mi>T</mml:mi><mml:mo>∼</mml:mo><mml:mi mathvariant="normal">GEV</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">σ</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">ξ</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is given by an analytical equation (when <inline-formula><mml:math id="M226" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>+</mml:mo><mml:mi mathvariant="italic">ξ</mml:mi><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mrow><mml:mi>x</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="italic">μ</mml:mi></mml:mrow><mml:mi mathvariant="italic">σ</mml:mi></mml:mfrac></mml:mstyle><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>:

          <disp-formula id="App1.Ch1.S1.Ex1"><mml:math id="M227" display="block"><mml:mtable class="split" rowspacing="0.2ex" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">GEV</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>;</mml:mo><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">σ</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">ξ</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>:=</mml:mo><mml:mi mathvariant="double-struck">P</mml:mi><mml:mo>(</mml:mo><mml:mi>T</mml:mi><mml:mo>&lt;</mml:mo><mml:mi>x</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mi>exp⁡</mml:mi><mml:mfenced close="]" open="["><mml:mrow><mml:mo>-</mml:mo><mml:msubsup><mml:mfenced open="(" close=")"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>+</mml:mo><mml:mi mathvariant="italic">ξ</mml:mi><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi>x</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="italic">μ</mml:mi></mml:mrow><mml:mi mathvariant="italic">σ</mml:mi></mml:mfrac></mml:mstyle></mml:mrow></mml:mfenced><mml:mo>+</mml:mo><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mi mathvariant="italic">ξ</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:mfenced><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula></p>
      <p id="d2e7558">The quantile function <inline-formula><mml:math id="M228" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="script">Q</mml:mi><mml:mi mathvariant="normal">GEV</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (inverse of the distribution function) is also given by:

          <disp-formula id="App1.Ch1.S1.Ex2"><mml:math id="M229" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="script">Q</mml:mi><mml:mi mathvariant="normal">GEV</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>;</mml:mo><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">σ</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">ξ</mml:mi><mml:mo>)</mml:mo><mml:mo>:=</mml:mo><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="italic">ξ</mml:mi></mml:mfrac></mml:mstyle><mml:mfenced close="]" open="["><mml:mrow><mml:mo>(</mml:mo><mml:mo>-</mml:mo><mml:mi>log⁡</mml:mi><mml:mi>p</mml:mi><mml:msup><mml:mo>)</mml:mo><mml:mrow><mml:mo>-</mml:mo><mml:mi mathvariant="italic">ξ</mml:mi></mml:mrow></mml:msup><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:mfenced><mml:mo>=</mml:mo><mml:msubsup><mml:mi>F</mml:mi><mml:mi mathvariant="normal">GEV</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>)</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula></p>
      <p id="d2e7656">Note that if <inline-formula><mml:math id="M230" display="inline"><mml:mrow><mml:mi mathvariant="italic">ξ</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>, the distribution is not bounded and is said <italic>heavy tail</italic>. If <inline-formula><mml:math id="M231" display="inline"><mml:mrow><mml:mi mathvariant="italic">ξ</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>, the extremes are bounded, with the upper bound <inline-formula><mml:math id="M232" display="inline"><mml:mi>B</mml:mi></mml:math></inline-formula> given by:

          <disp-formula id="App1.Ch1.S1.Ex3"><mml:math id="M233" display="block"><mml:mrow><mml:mi>B</mml:mi><mml:mo>:=</mml:mo><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="italic">ξ</mml:mi></mml:mfrac></mml:mstyle><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula></p>
      <p id="d2e7714">In general, to use the GEV distribution, we use the block-maxima theorem, which states that if we divide a data set into blocks and take the maximum of each block, then asymptotically this random variable follows a GEV distribution. Here, annual maximums are used, and this works well overall with temperature.</p>
</app>

<app id="App1.Ch1.S2">
  <label>Appendix B</label><title>Some details about the inference of <inline-formula><mml:math id="M234" display="inline"><mml:mi mathvariant="italic">θ</mml:mi></mml:math></inline-formula></title>
<sec id="App1.Ch1.S2.SS1">
  <label>B1</label><title>Fit in the climate models</title>
      <p id="d2e7739">Our approach therefore begins by inferring the <inline-formula><mml:math id="M235" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> of the statistical model in Eq. (<xref ref-type="disp-formula" rid="Ch1.E5"/>) using data from <inline-formula><mml:math id="M236" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi>M</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> climate models.</p>
      <p id="d2e7766">For each climate model <inline-formula><mml:math id="M237" display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula>, we have three time series (with possible repetitions of the time steps for each member) for each SSP scenario: <list list-type="bullet"><list-item>
      <p id="d2e7778"><inline-formula><mml:math id="M238" display="inline"><mml:mrow><mml:msubsup><mml:mover accent="true"><mml:mi>X</mml:mi><mml:mo stretchy="false" mathvariant="normal">̃</mml:mo></mml:mover><mml:mrow><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>m</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">R</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">SSP</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>, regional average temperature series, here for Europe;</p></list-item><list-item>
      <p id="d2e7807"><inline-formula><mml:math id="M239" display="inline"><mml:mrow><mml:msubsup><mml:mover accent="true"><mml:mi>X</mml:mi><mml:mo stretchy="false" mathvariant="normal">̃</mml:mo></mml:mover><mml:mrow><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>m</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">G</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">SSP</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>, global average temperature series,</p></list-item><list-item>
      <p id="d2e7836"><inline-formula><mml:math id="M240" display="inline"><mml:mrow><mml:msubsup><mml:mover accent="true"><mml:mi>T</mml:mi><mml:mo stretchy="false" mathvariant="normal">̃</mml:mo></mml:mover><mml:mrow><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>m</mml:mi></mml:mrow><mml:mi mathvariant="normal">SSP</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>, series of annual maximum temperatures over 3 d.</p></list-item></list></p>
      <p id="d2e7859">The inference begins by estimating the parameters of the covariates. Starting from the series <inline-formula><mml:math id="M241" display="inline"><mml:mrow><mml:msubsup><mml:mover accent="true"><mml:mi>X</mml:mi><mml:mo stretchy="false" mathvariant="normal">̃</mml:mo></mml:mover><mml:mrow><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>m</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">R</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">SSP</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M242" display="inline"><mml:mrow><mml:msubsup><mml:mover accent="true"><mml:mi>X</mml:mi><mml:mo mathvariant="normal" stretchy="false">̃</mml:mo></mml:mover><mml:mrow><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>m</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">G</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">SSP</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>, the pair <inline-formula><mml:math id="M243" display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:msubsup><mml:mover accent="true"><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mi>m</mml:mi><mml:mi mathvariant="normal">R</mml:mi></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mover accent="true"><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mi>m</mml:mi><mml:mi mathvariant="normal">G</mml:mi></mml:msubsup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is estimated using the approaches described in Sect. S1.1, as well as the covariance matrix <inline-formula><mml:math id="M244" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">Σ</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:msubsup><mml:mi mathvariant="italic">θ</mml:mi><mml:mi>m</mml:mi><mml:mi mathvariant="normal">R</mml:mi></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi mathvariant="italic">θ</mml:mi><mml:mi>m</mml:mi><mml:mi mathvariant="normal">G</mml:mi></mml:msubsup><mml:mo>)</mml:mo></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> describing the uncertainty in this estimation.</p>
      <p id="d2e7976">Next, we estimate <inline-formula><mml:math id="M245" display="inline"><mml:mrow><mml:msubsup><mml:mover accent="true"><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mi>m</mml:mi><mml:mi mathvariant="normal">GEV</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> from the series <inline-formula><mml:math id="M246" display="inline"><mml:mrow><mml:msubsup><mml:mover accent="true"><mml:mi>T</mml:mi><mml:mo stretchy="false" mathvariant="normal">̃</mml:mo></mml:mover><mml:mrow><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>m</mml:mi></mml:mrow><mml:mi mathvariant="normal">SSP</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> of each model. To do this, we use the vector <inline-formula><mml:math id="M247" display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:msubsup><mml:mover accent="true"><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mi>m</mml:mi><mml:mi mathvariant="normal">R</mml:mi></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mover accent="true"><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mi>m</mml:mi><mml:mi mathvariant="normal">G</mml:mi></mml:msubsup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> to generate the forcings <inline-formula><mml:math id="M248" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>m</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">R</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">SSP</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>. The vector <inline-formula><mml:math id="M249" display="inline"><mml:mrow><mml:msubsup><mml:mover accent="true"><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mi>m</mml:mi><mml:mi mathvariant="normal">GEV</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> can thus be calculated by maximum likelihood, which allows us to estimate <inline-formula><mml:math id="M250" display="inline"><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mi>m</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>(</mml:mo><mml:msubsup><mml:mover accent="true"><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mi>m</mml:mi><mml:mi mathvariant="normal">R</mml:mi></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mover accent="true"><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mi>m</mml:mi><mml:mi mathvariant="normal">G</mml:mi></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mover accent="true"><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mi>m</mml:mi><mml:mi mathvariant="normal">GEV</mml:mi></mml:msubsup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. The covariance matrix <inline-formula><mml:math id="M251" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">Σ</mml:mi><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="italic">θ</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="bold">Σ</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:msubsup><mml:mi mathvariant="italic">θ</mml:mi><mml:mi>m</mml:mi><mml:mi mathvariant="normal">R</mml:mi></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi mathvariant="italic">θ</mml:mi><mml:mi>m</mml:mi><mml:mi mathvariant="normal">G</mml:mi></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi mathvariant="italic">θ</mml:mi><mml:mi>m</mml:mi><mml:mi mathvariant="normal">GEV</mml:mi></mml:msubsup><mml:mo>)</mml:mo></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> of <inline-formula><mml:math id="M252" display="inline"><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is estimated using a bootstrap on the series <inline-formula><mml:math id="M253" display="inline"><mml:mrow><mml:msubsup><mml:mover accent="true"><mml:mi>T</mml:mi><mml:mo stretchy="false" mathvariant="normal">̃</mml:mo></mml:mover><mml:mrow><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>m</mml:mi></mml:mrow><mml:mi mathvariant="normal">SSP</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> and the forcings <inline-formula><mml:math id="M254" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>m</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">R</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">SSP</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>, forcings constructed from several samples according to the normal distribution <inline-formula><mml:math id="M255" display="inline"><mml:mrow><mml:mi mathvariant="script">N</mml:mi><mml:mo>(</mml:mo><mml:mo>(</mml:mo><mml:msubsup><mml:mover accent="true"><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mi>m</mml:mi><mml:mi mathvariant="normal">R</mml:mi></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mover accent="true"><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mi>m</mml:mi><mml:mi mathvariant="normal">G</mml:mi></mml:msubsup><mml:mo>)</mml:mo><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="bold">Σ</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:msubsup><mml:mi mathvariant="italic">θ</mml:mi><mml:mi>m</mml:mi><mml:mi mathvariant="normal">R</mml:mi></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi mathvariant="italic">θ</mml:mi><mml:mi>m</mml:mi><mml:mi mathvariant="normal">G</mml:mi></mml:msubsup><mml:mo>)</mml:mo></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>.</p>
      <p id="d2e8318">Note that this approach is purely frequentist, in the sense that we estimate the value of <inline-formula><mml:math id="M256" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and its covariance matrix, as opposed to the Bayesian view, where we want to determine the distribution of <inline-formula><mml:math id="M257" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>.</p>
</sec>
<sec id="App1.Ch1.S2.SS2">
  <label>B2</label><title>Construction of the prior</title>
      <p id="d2e8351">The prior is then constructed as a synthesis of climate models. This is where we switch to a Bayesian view: <inline-formula><mml:math id="M258" display="inline"><mml:mi mathvariant="bold-italic">θ</mml:mi></mml:math></inline-formula> is no longer seen as a value to be estimated but as a <italic>random</italic> vector. For each climate model, we then define the random variable <inline-formula><mml:math id="M259" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, which follows the following multivariate normal distribution:

            <disp-formula id="App1.Ch1.S2.Ex1"><mml:math id="M260" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mi>m</mml:mi></mml:msub><mml:mo>∼</mml:mo><mml:mi mathvariant="script">N</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mi>m</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="bold">Σ</mml:mi><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="italic">θ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></disp-formula></p>
      <p id="d2e8413">Following the work of <xref ref-type="bibr" rid="bib1.bibx71" id="text.102"/>, we assume that <italic>reality is statistically indistinguishable from a set of climate models</italic> <xref ref-type="bibr" rid="bib1.bibx1 bib1.bibx80" id="paren.103"><named-content content-type="pre">see also</named-content></xref>. This allows us to construct a multi-model synthesis <inline-formula><mml:math id="M261" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub><mml:mo>∼</mml:mo><mml:mi mathvariant="script">N</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mo>∗</mml:mo></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="bold">Σ</mml:mi><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="italic">θ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mo>∗</mml:mo></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> which also follows a normal distribution with parameters:

            <disp-formula id="App1.Ch1.S2.Ex2"><mml:math id="M262" display="block"><mml:mrow><mml:mfenced open="{" close=""><mml:mtable class="array" columnalign="left left"><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mo>∗</mml:mo></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mstyle displaystyle="false"><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mn mathvariant="normal">1</mml:mn><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi>M</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:mstyle><mml:munder><mml:mo movablelimits="false">∑</mml:mo><mml:mi>m</mml:mi></mml:munder><mml:msub><mml:mover accent="true"><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mi>m</mml:mi></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi mathvariant="bold">Σ</mml:mi><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="italic">θ</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mo>∗</mml:mo></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mfenced close=")" open="("><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>+</mml:mo><mml:mstyle displaystyle="false"><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mn mathvariant="normal">1</mml:mn><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi>M</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:mstyle></mml:mrow></mml:mfenced><mml:msub><mml:mover accent="true"><mml:mi mathvariant="bold">Σ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mi>u</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:msubsup><mml:mi>N</mml:mi><mml:mi>M</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:munder><mml:mo movablelimits="false">∑</mml:mo><mml:mi>m</mml:mi></mml:munder><mml:msub><mml:mi mathvariant="bold">Σ</mml:mi><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="italic">θ</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:msub><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced></mml:mrow></mml:math></disp-formula></p>
      <p id="d2e8590">In this last equation, the matrix <inline-formula><mml:math id="M263" display="inline"><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="bold">Σ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mi>u</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> describes the internal variability of the models. The mathematics describing this approach can be found in Sect. S1.2.</p>
</sec>
<sec id="App1.Ch1.S2.SS3">
  <label>B3</label><title>Derivation of the posterior</title>
      <p id="d2e8615">For the construction of the posterior, we have the observations <inline-formula><mml:math id="M264" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">R</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M265" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">G</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M266" display="inline"><mml:mrow><mml:msubsup><mml:mi>T</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> (regional average temperature, global average temperature and temperature extremes). Let us start again from the calculation in <xref ref-type="bibr" rid="bib1.bibx77" id="text.104"><named-content content-type="post">Sect. 3.5</named-content></xref>, which allows us to separate the conditioning by <inline-formula><mml:math id="M267" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">R</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M268" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">G</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> from that by <inline-formula><mml:math id="M269" display="inline"><mml:mrow><mml:msubsup><mml:mi>T</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>. We then have:

            <disp-formula id="App1.Ch1.S2.E9" content-type="numbered"><label>B1</label><mml:math id="M270" display="block"><mml:mtable rowspacing="0.2ex" class="split" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mi mathvariant="double-struck">P</mml:mi><mml:mfenced close="]" open="["><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub><mml:mo>|</mml:mo><mml:mo>(</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">R</mml:mi></mml:mrow></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">G</mml:mi></mml:mrow></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi>T</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msubsup><mml:mo>)</mml:mo></mml:mrow></mml:mfenced><mml:mo>=</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mspace width="1em" linebreak="nobreak"/><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="double-struck">P</mml:mi><mml:mfenced open="[" close="]"><mml:mrow><mml:msubsup><mml:mi>T</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msubsup><mml:mo>|</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub><mml:mo>|</mml:mo><mml:mo>(</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">R</mml:mi></mml:mrow></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">G</mml:mi></mml:mrow></mml:msubsup><mml:mo>)</mml:mo><mml:mo>)</mml:mo></mml:mrow></mml:mfenced><mml:mi mathvariant="double-struck">P</mml:mi><mml:mfenced close="]" open="["><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub><mml:mo>|</mml:mo><mml:mo>(</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">R</mml:mi></mml:mrow></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">G</mml:mi></mml:mrow></mml:msubsup><mml:mo>)</mml:mo></mml:mrow></mml:mfenced></mml:mrow><mml:mrow><mml:mi mathvariant="double-struck">P</mml:mi><mml:mo>(</mml:mo><mml:msubsup><mml:mi>T</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msubsup><mml:mo>)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula></p>
      <p id="d2e8900">The important point is that, starting from the prior <inline-formula><mml:math id="M271" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub></mml:mrow></mml:math></inline-formula>, we can construct the posterior <inline-formula><mml:math id="M272" display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub><mml:mo>|</mml:mo><mml:mo>(</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">R</mml:mi></mml:mrow></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">G</mml:mi></mml:mrow></mml:msubsup><mml:mo>)</mml:mo><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, thus defining a new random variable. This latter variable can itself be considered as a prior to be constrained by <inline-formula><mml:math id="M273" display="inline"><mml:mrow><mml:msubsup><mml:mi>T</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>, which allows us to derive the complete posterior. This constraint is therefore applied in two steps.</p>
<sec id="App1.Ch1.S2.SS3.SSS1">
  <label>B3.1</label><title>Covariables constraint</title>
      <p id="d2e8981">The estimate of <inline-formula><mml:math id="M274" display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub><mml:mo>|</mml:mo><mml:mo>(</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">R</mml:mi></mml:mrow></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">G</mml:mi></mml:mrow></mml:msubsup><mml:mo>)</mml:mo><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is in fact analytical, and the Gaussian conditioning theorem <xref ref-type="bibr" rid="bib1.bibx24" id="paren.105"/> applies. Let <inline-formula><mml:math id="M275" display="inline"><mml:mrow><mml:msup><mml:mi>X</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula> be a global vector of observations that concatenates <inline-formula><mml:math id="M276" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">R</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M277" display="inline"><mml:mrow><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">G</mml:mi></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> over time, and <inline-formula><mml:math id="M278" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">ε</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msup><mml:mo>∼</mml:mo><mml:mi mathvariant="script">N</mml:mi><mml:mo>(</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo><mml:msup><mml:mi mathvariant="bold">Σ</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> be white noise of the same dimension as <inline-formula><mml:math id="M279" display="inline"><mml:mrow><mml:msup><mml:mi>X</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula>. If we find a matrix <inline-formula><mml:math id="M280" display="inline"><mml:mi mathvariant="bold">A</mml:mi></mml:math></inline-formula> such that <inline-formula><mml:math id="M281" display="inline"><mml:mrow><mml:msup><mml:mi>X</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msup><mml:mo>=</mml:mo><mml:mi mathvariant="bold">A</mml:mi><mml:mo>⋅</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub><mml:mo>+</mml:mo><mml:msup><mml:mi mathvariant="italic">ε</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula>, and since <inline-formula><mml:math id="M282" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub></mml:mrow></mml:math></inline-formula> follows a normal distribution, then <inline-formula><mml:math id="M283" display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub><mml:mo>|</mml:mo><mml:msup><mml:mi>X</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msup><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub><mml:mo>|</mml:mo><mml:mo>(</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">R</mml:mi></mml:mrow></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">G</mml:mi></mml:mrow></mml:msubsup><mml:mo>)</mml:mo><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> also follows a normal distribution, i.e. <inline-formula><mml:math id="M284" display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub><mml:mo>|</mml:mo><mml:msup><mml:mi>X</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msup><mml:mo>)</mml:mo><mml:mo>∼</mml:mo><mml:mi mathvariant="script">N</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub><mml:mo>|</mml:mo><mml:msup><mml:mi>X</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="bold">Σ</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub><mml:mo>|</mml:mo><mml:msup><mml:mi>X</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, with value:

              <disp-formula id="App1.Ch1.S2.Ex3"><mml:math id="M285" display="block"><mml:mrow><mml:mfenced close="" open="{"><mml:mtable class="array" columnalign="left left"><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub><mml:mo>|</mml:mo><mml:msup><mml:mi>X</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub><mml:mo>+</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="bold">Σ</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub></mml:mrow></mml:msub><mml:msup><mml:mi mathvariant="bold">A</mml:mi><mml:mi>T</mml:mi></mml:msup><mml:mo>)</mml:mo><mml:mo>⋅</mml:mo><mml:mo>(</mml:mo><mml:mi mathvariant="bold">A</mml:mi><mml:msub><mml:mi mathvariant="bold">Σ</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub></mml:mrow></mml:msub><mml:msup><mml:mi mathvariant="bold">A</mml:mi><mml:mi>T</mml:mi></mml:msup><mml:mo>+</mml:mo><mml:msup><mml:mi mathvariant="bold">Σ</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msup><mml:msup><mml:mo>)</mml:mo><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>⋅</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>(</mml:mo><mml:msup><mml:mi>X</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msup><mml:mo>-</mml:mo><mml:mi mathvariant="bold">A</mml:mi><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi mathvariant="bold">Σ</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub><mml:mo>|</mml:mo><mml:msup><mml:mi>X</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="bold">Σ</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="bold">Σ</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub></mml:mrow></mml:msub><mml:msup><mml:mi mathvariant="bold">A</mml:mi><mml:mi>T</mml:mi></mml:msup><mml:mo>)</mml:mo><mml:mo>⋅</mml:mo><mml:mo>(</mml:mo><mml:mi mathvariant="bold">A</mml:mi><mml:msub><mml:mi mathvariant="bold">Σ</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub></mml:mrow></mml:msub><mml:msup><mml:mi mathvariant="bold">A</mml:mi><mml:mi>T</mml:mi></mml:msup><mml:mo>+</mml:mo><mml:msup><mml:mi mathvariant="bold">Σ</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msup><mml:msup><mml:mo>)</mml:mo><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>⋅</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>(</mml:mo><mml:mi mathvariant="bold">A</mml:mi><mml:msub><mml:mi mathvariant="bold">Σ</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub></mml:mrow></mml:msub><mml:mo>)</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced></mml:mrow></mml:math></disp-formula></p>
      <p id="d2e9546">The difficulties here are constructing the matrix <inline-formula><mml:math id="M286" display="inline"><mml:mi mathvariant="bold">A</mml:mi></mml:math></inline-formula>, which models how our parameters are transformed into the observation signal, and estimating <inline-formula><mml:math id="M287" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="bold">Σ</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula>, which models the internal variability of the observations.</p>
      <p id="d2e9567">For matrix <inline-formula><mml:math id="M288" display="inline"><mml:mi mathvariant="bold">A</mml:mi></mml:math></inline-formula>, two approaches are proposed in Sect. S1.3.1. One is based on the idea that, over the observed period, the scenarios are sufficiently similar that their mean can be projected onto the observations. The second requires choosing a scenario. In this article, we will use the first approach.</p>
      <p id="d2e9577">For the covariance matrix <inline-formula><mml:math id="M289" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="bold">Σ</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula>, two approaches are also proposed in Sect. S1.3.2. The first is simply to consider it as white noise, estimates of observations from which a trend has been removed. The second approach was developed by <xref ref-type="bibr" rid="bib1.bibx73" id="text.106"/> and <xref ref-type="bibr" rid="bib1.bibx68" id="text.107"/>, and assumes that <inline-formula><mml:math id="M290" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">ε</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula> takes the form of a sum of two first-order autoregressive processes. One is <italic>fast</italic> to model inter-annual variability, while the second is <italic>slow</italic> to model decadal variability. In this article, we will use the first approach.</p>
</sec>
<sec id="App1.Ch1.S2.SS3.SSS2">
  <label>B3.2</label><title>Variable constraint</title>
      <p id="d2e9623">With our knowledge of the distribution  <inline-formula><mml:math id="M291" display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub><mml:mo>|</mml:mo><mml:mo>(</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">R</mml:mi></mml:mrow></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">G</mml:mi></mml:mrow></mml:msubsup><mml:mo>)</mml:mo><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, we now want to obtain samples of the distribution <inline-formula><mml:math id="M292" display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:mo>[</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub><mml:mo>|</mml:mo><mml:mo>(</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">R</mml:mi></mml:mrow></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">G</mml:mi></mml:mrow></mml:msubsup><mml:mo>)</mml:mo><mml:mo>]</mml:mo><mml:mo>|</mml:mo><mml:msubsup><mml:mi>T</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msubsup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. The whole problem is that <inline-formula><mml:math id="M293" display="inline"><mml:mrow><mml:msubsup><mml:mi>T</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> follows a GEV distribution, and there is no explicit expression for the posterior. Let us start again from the Eq. (<xref ref-type="disp-formula" rid="App1.Ch1.S2.E9"/>).</p>
      <p id="d2e9749"><list list-type="bullet">
              <list-item>

      <p id="d2e9754">The term <inline-formula><mml:math id="M294" display="inline"><mml:mrow><mml:mi mathvariant="double-struck">P</mml:mi><mml:mo>[</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub><mml:mo>|</mml:mo><mml:mo>(</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">R</mml:mi></mml:mrow></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">G</mml:mi></mml:mrow></mml:msubsup><mml:mo>)</mml:mo><mml:mo>]</mml:mo></mml:mrow></mml:math></inline-formula> is known, it is our prior.</p>
              </list-item>
              <list-item>

      <p id="d2e9809">The term <inline-formula><mml:math id="M295" display="inline"><mml:mrow><mml:mi mathvariant="double-struck">P</mml:mi><mml:mo>[</mml:mo><mml:msubsup><mml:mi>T</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msubsup><mml:mo>|</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mo>∗</mml:mo></mml:msub><mml:mo>|</mml:mo><mml:mo>(</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">R</mml:mi></mml:mrow></mml:msubsup><mml:mo>,</mml:mo><mml:msubsup><mml:mi>X</mml:mi><mml:mi>t</mml:mi><mml:mrow><mml:mi mathvariant="normal">o</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">G</mml:mi></mml:mrow></mml:msubsup><mml:mo>)</mml:mo><mml:mo>)</mml:mo><mml:mo>]</mml:mo></mml:mrow></mml:math></inline-formula> is directly calculable: the draws generate the parameters of the GEV law, which can thus be evaluated.</p>
              </list-item>
              <list-item>

      <p id="d2e9878">When the denominator is analytically intractable, numerical methods are necessary to sample from the posterior distribution.</p>
              </list-item>
            </list></p>
      <p id="d2e9883">A common approach to perform this sampling is the Metropolis-Hasting algorithm <xref ref-type="bibr" rid="bib1.bibx53" id="paren.108"/>, <xref ref-type="bibr" rid="bib1.bibx34" id="paren.109"/>. This is the sampling algorithm originally used by <xref ref-type="bibr" rid="bib1.bibx77" id="text.110"/>. This Markov chain Monte Carlo algorithm relies on a random walk proposal: a new proposal is created by starting from an initial value <inline-formula><mml:math id="M296" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and adding a random noise to generate a <inline-formula><mml:math id="M297" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. The new value is either accepted or rejected with a probability defined using the likelihood ratio of the proposal and the previous value. A key element of this procedure is the transition function between <inline-formula><mml:math id="M298" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M299" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> that is used to sample successive possible values of the posterior.</p>
      <p id="d2e9945">In the <xref ref-type="bibr" rid="bib1.bibx77" id="text.111"/> original implementation, the transition function was of the form <inline-formula><mml:math id="M300" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">θ</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="italic">ε</mml:mi></mml:mrow></mml:math></inline-formula> where <inline-formula><mml:math id="M301" display="inline"><mml:mi mathvariant="italic">ε</mml:mi></mml:math></inline-formula> follows a normal distribution with the same scale for all parameters. This can become an issue when the scale of the target parameters is very different from one another. The transition also determines the rate of convergence and mixing, so this implementation can be computationally sub-optimal. Various diagnostics showed the algorithm suffered from slow-mixing chains <xref ref-type="bibr" rid="bib1.bibx29" id="paren.112"/>, high autocorrelation <xref ref-type="bibr" rid="bib1.bibx9" id="paren.113"/>, and low effective sample size <xref ref-type="bibr" rid="bib1.bibx30" id="paren.114"/>.</p>
      <p id="d2e9996">To deal with these issues, we leverage the <italic>No-U-Turn Sampler</italic> algorithm NUTS, <xref ref-type="bibr" rid="bib1.bibx37" id="paren.115"/>, as implemented in STAN <xref ref-type="bibr" rid="bib1.bibx87" id="paren.116"/>. This algorithm is based on the Hamiltonian Monte Carlo algorithm <xref ref-type="bibr" rid="bib1.bibx69" id="paren.117"/>, a variant of the Metropolis-Hasting algorithm where the proposal is not generated using a random walk. Instead, the proposal is created through a series of gradient-informed steps <xref ref-type="bibr" rid="bib1.bibx6" id="paren.118"/>. This allows for better parameter space exploration, especially in the multidimensional case. The NUTS variant relies on a specific criteria to select adaptively various hyper-parameters such as the steps length and stopping conditions. This adaptation makes the algorithm more robust against correlation in the posterior. The NUTS algorithm is particularly effective when the posterior dimensions are correlated or of different scales. It is very efficient to explore the parameter space and draw samples from the posterior.</p>
</sec>
</sec>
</app>
  </app-group><notes notes-type="codedataavailability"><title>Code and data availability</title>

      <p id="d2e10020">GISTEMP data are available at <uri>https://data.giss.nasa.gov/gistemp</uri> (last access: 19 March 2026; <xref ref-type="bibr" rid="bib1.bibx46" id="altparen.119"/>). HadCRUT5 data were obtained from <uri>https://www.metoffice.gov.uk/hadobs/hadcrut5</uri> (last access: 19 March 2026; <xref ref-type="bibr" rid="bib1.bibx55 bib1.bibx61" id="altparen.120"/>) on 2025 and are © British Crown Copyright, Met Office 2020, provided under an Open Government License, <uri>https://www.nationalarchives.gov.uk/doc/open-government-licence/version/3/</uri> (last acess: 19 March 2026). ERA5 data are available in the Climate Data Store at <ext-link xlink:href="https://doi.org/10.24381/cds.adbb2d47" ext-link-type="DOI">10.24381/cds.adbb2d47</ext-link> <xref ref-type="bibr" rid="bib1.bibx18 bib1.bibx36" id="paren.121"/>. The CMIP6 model simulations can be downloaded through the Earth System Grid Federation portals. Instructions to access the data are available at <uri>https://pcmdi.llnl.gov/</uri> (last access: 19 March 2026).</p>

      <p id="d2e10048">The current version of ANKIALE is available from the project website: <uri>https://github.com/yrobink/ANKIALE</uri> (last access: 19 March 2026) under the GNU-GPL3 licence. The exact version of the model used to produce the results used in this paper is archived on Zenodo under <ext-link xlink:href="https://doi.org/10.5281/zenodo.15038388" ext-link-type="DOI">10.5281/zenodo.15038388</ext-link> <xref ref-type="bibr" rid="bib1.bibx76" id="paren.122"/>, as are input data and scripts to run the model and produce the plots for all the simulations presented in this paper.</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d2e10060">The supplement related to this article is available online at <inline-supplementary-material xlink:href="https://doi.org/10.5194/gmd-19-2349-2026-supplement" xlink:title="pdf">https://doi.org/10.5194/gmd-19-2349-2026-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d2e10069">YR had the initial idea of the study, which has been completed and enriched by all co-authors. YR developed the multi-scenarios methods, and OB developed the MCMC, both helped by MV, AR, and PN for the statistical modelling and inferential schemes. YR developed the ANKIALE package and applied it to Europe for the different experiments and wrote the codes for the analyses and to plot the figures. All authors contributed to the methodology and the analyses. YR wrote the first draft of the article with inputs from all the co-authors.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d2e10075">The contact author has declared that none of the authors has any competing interests.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d2e10082">Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. The authors bear the ultimate responsibility for providing appropriate place names. Views expressed in the text are those of the authors and do not necessarily reflect the views of the publisher.</p>
  </notes><ack><title>Acknowledgements</title><p id="d2e10088">We acknowledge the World Climate Research Programme, which, through its Working Group on Coupled Modelling, coordinated and promoted CMIP6. We thank the climate modeling groups for producing and making available their model output, the Earth System Grid Federation (ESGF) for archiving the data and providing access, and the multiple funding agencies who support CMIP6 and ESGF.</p><p id="d2e10090"><xref ref-type="bibr" rid="bib1.bibx36" id="text.123"><named-content content-type="pre">ERA5,</named-content></xref> was downloaded from the Copernicus Climate Change Service (2025). The results contain modified Copernicus Climate Change Service information 2020. Neither the European Commission nor ECMWF is responsible for any use that may be made of the Copernicus information or data it contains.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d2e10099">This work has benefited from state aid managed by the National Research Agency under France 2030 bearing the references ANR-22-EXTR-0005 (TRACCS-PC4-EXTENDING project), and has been supported by the European Union's Horizon 2020 research and innovation programme under grant agreement No. 101003469 (“XAIDA”).</p>

      <p id="d2e10102">MV has also been supported by the “COMBINE” project funded by the Swiss National Science Foundation (grant no. 200021_200337/1).</p>

      <p id="d2e10105">Part of PN's research work was supported by the French national programs: 80 PRIME CNRS-INSU, Agence Nationale de la Recherche (ANR) under reference   ANR EXSTA,  the PEPR TRACCS programme under grant number ANR-22-EXTR-0005, and  the Mines Paris/INRAE chair Geolearning.</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d2e10111">This paper was edited by Dan Lu and reviewed by Richard Chandler and three anonymous referees.</p>
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