<?xml version="1.0" encoding="utf-8"?>
<TEI xmlns="http://www.tei-c.org/ns/1.0" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:hal="http://hal.archives-ouvertes.fr/" xmlns:gml="http://www.opengis.net/gml/3.3/" xmlns:gmlce="http://www.opengis.net/gml/3.3/ce" version="1.1" xsi:schemaLocation="http://www.tei-c.org/ns/1.0 http://api.archives-ouvertes.fr/documents/aofr-sword.xsd">
  <teiHeader>
    <fileDesc>
      <titleStmt>
        <title>HAL TEI export of insu-04054644</title>
      </titleStmt>
      <publicationStmt>
        <distributor>CCSD</distributor>
        <availability status="restricted">
          <licence target="https://creativecommons.org/publicdomain/zero/1.0/">CC0 1.0 - Universal</licence>
        </availability>
        <date when="2026-05-24T07:58:25+02:00"/>
      </publicationStmt>
      <sourceDesc>
        <p part="N">HAL API Platform</p>
      </sourceDesc>
    </fileDesc>
  </teiHeader>
  <text>
    <body>
      <listBibl>
        <biblFull>
          <titleStmt>
            <title xml:lang="en">Investigating Galaxy Evolution and Active Galactic Nucleus Feedback with the Sunyaev-Zel'dovich Effect</title>
            <author role="aut">
              <persName>
                <forename type="first">Alexander</forename>
                <surname>Spacek</surname>
              </persName>
              <idno type="halauthorid">1716728-0</idno>
            </author>
            <author role="aut">
              <persName>
                <forename type="first">Evan</forename>
                <surname>Scannapieco</surname>
              </persName>
              <idno type="halauthorid">644543-0</idno>
            </author>
            <author role="aut">
              <persName>
                <forename type="first">Seth H.</forename>
                <surname>Cohen</surname>
              </persName>
              <idno type="halauthorid">1115188-0</idno>
            </author>
            <author role="aut">
              <persName>
                <forename type="first">Bhavin</forename>
                <surname>Joshi</surname>
              </persName>
              <idno type="halauthorid">1294242-0</idno>
            </author>
            <author role="aut">
              <persName>
                <forename type="first">Philip</forename>
                <surname>Mauskopf</surname>
              </persName>
              <idno type="halauthorid">388380-0</idno>
            </author>
            <author role="aut">
              <persName>
                <forename type="first">Mark L. A.</forename>
                <surname>Richardson</surname>
              </persName>
              <idno type="halauthorid">2479996-0</idno>
            </author>
            <author role="aut">
              <persName>
                <forename type="first">Julien</forename>
                <surname>Devriendt</surname>
              </persName>
              <idno type="halauthorid">1192705-0</idno>
            </author>
            <author role="aut">
              <persName>
                <forename type="first">Yohan</forename>
                <surname>Dubois</surname>
              </persName>
              <email type="md5">1782362026c73fdfa5624f751bccb942</email>
              <email type="domain">iap.fr</email>
              <idno type="idhal" notation="string">yohan-dubois</idno>
              <idno type="idhal" notation="numeric">738810</idno>
              <idno type="halauthorid" notation="string">2528767-738810</idno>
              <idno type="ORCID">https://orcid.org/0000-0003-0225-6387</idno>
              <idno type="IDREF">https://www.idref.fr/130594628</idno>
              <idno type="ARXIV">https://arxiv.org/a/dubois_y_1</idno>
              <idno type="GOOGLE SCHOLAR">https://scholar.google.fr/citations?user=Vx0HM7cAAAAJ</idno>
              <affiliation ref="#struct-541701"/>
            </author>
            <author role="aut">
              <persName>
                <forename type="first">Sebastien</forename>
                <surname>Peirani</surname>
              </persName>
              <idno type="halauthorid">1192706-0</idno>
              <affiliation ref="#struct-541701"/>
            </author>
            <author role="aut">
              <persName>
                <forename type="first">Christophe</forename>
                <surname>Pichon</surname>
              </persName>
              <email type="md5">dbe2d587a0087530dfb9f6391bf2da66</email>
              <email type="domain">iap.fr</email>
              <idno type="idhal" notation="string">christophe-pichon</idno>
              <idno type="idhal" notation="numeric">738765</idno>
              <idno type="halauthorid" notation="string">9295-738765</idno>
              <idno type="ORCID">https://orcid.org/0000-0003-0695-6735</idno>
              <idno type="IDREF">https://www.idref.fr/091461618</idno>
              <idno type="GOOGLE SCHOLAR">4bdEIGEAAAAJ</idno>
              <affiliation ref="#struct-541701"/>
            </author>
            <editor role="depositor">
              <persName>
                <forename>Christophe</forename>
                <surname>Pichon</surname>
              </persName>
              <email type="md5">dbe2d587a0087530dfb9f6391bf2da66</email>
              <email type="domain">iap.fr</email>
            </editor>
          </titleStmt>
          <editionStmt>
            <edition n="v1" type="current">
              <date type="whenSubmitted">2023-03-31 20:36:07</date>
              <date type="whenModified">2025-02-23 21:17:21</date>
              <date type="whenReleased">2023-03-31 20:36:07</date>
              <date type="whenProduced">2018</date>
            </edition>
            <respStmt>
              <resp>contributor</resp>
              <name key="114283">
                <persName>
                  <forename>Christophe</forename>
                  <surname>Pichon</surname>
                </persName>
                <email type="md5">dbe2d587a0087530dfb9f6391bf2da66</email>
                <email type="domain">iap.fr</email>
              </name>
            </respStmt>
          </editionStmt>
          <publicationStmt>
            <distributor>CCSD</distributor>
            <idno type="halId">insu-04054644</idno>
            <idno type="halUri">https://insu.hal.science/insu-04054644</idno>
            <idno type="halBibtex">spacek:insu-04054644</idno>
            <idno type="halRefHtml">&lt;i&gt;American Astronomical Society&lt;/i&gt;, 2018, à renseigner, Unknown Region</idno>
            <idno type="halRef">American Astronomical Society, 2018, à renseigner, Unknown Region</idno>
            <availability status="restricted"/>
          </publicationStmt>
          <seriesStmt>
            <idno type="stamp" n="INSU">INSU - Institut National des Sciences de l'Univers</idno>
            <idno type="stamp" n="CNRS">CNRS - Centre national de la recherche scientifique</idno>
            <idno type="stamp" n="IAP" corresp="SORBONNE-UNIVERSITE">Institut d'Astrophysique de Paris</idno>
            <idno type="stamp" n="SORBONNE-UNIVERSITE">Sorbonne Université</idno>
            <idno type="stamp" n="SORBONNE-UNIV" corresp="SORBONNE-UNIVERSITE">Sorbonne Université 01/01/2018</idno>
            <idno type="stamp" n="SU-SCIENCES" corresp="SORBONNE-UNIVERSITE">Faculté des Sciences de Sorbonne Université</idno>
            <idno type="stamp" n="ALLIANCE-SU"> Alliance Sorbonne Université</idno>
            <idno type="stamp" n="SUPRA_ASTRO_PHYS">Astronomie, astrophysique et physique des plasmas</idno>
          </seriesStmt>
          <notesStmt>
            <note type="audience" n="2">International</note>
            <note type="popular" n="0">No</note>
            <note type="peer" n="1">Yes</note>
            <note type="proceedings" n="1">Yes</note>
          </notesStmt>
          <sourceDesc>
            <biblStruct>
              <analytic>
                <title xml:lang="en">Investigating Galaxy Evolution and Active Galactic Nucleus Feedback with the Sunyaev-Zel'dovich Effect</title>
                <author role="aut">
                  <persName>
                    <forename type="first">Alexander</forename>
                    <surname>Spacek</surname>
                  </persName>
                  <idno type="halauthorid">1716728-0</idno>
                </author>
                <author role="aut">
                  <persName>
                    <forename type="first">Evan</forename>
                    <surname>Scannapieco</surname>
                  </persName>
                  <idno type="halauthorid">644543-0</idno>
                </author>
                <author role="aut">
                  <persName>
                    <forename type="first">Seth H.</forename>
                    <surname>Cohen</surname>
                  </persName>
                  <idno type="halauthorid">1115188-0</idno>
                </author>
                <author role="aut">
                  <persName>
                    <forename type="first">Bhavin</forename>
                    <surname>Joshi</surname>
                  </persName>
                  <idno type="halauthorid">1294242-0</idno>
                </author>
                <author role="aut">
                  <persName>
                    <forename type="first">Philip</forename>
                    <surname>Mauskopf</surname>
                  </persName>
                  <idno type="halauthorid">388380-0</idno>
                </author>
                <author role="aut">
                  <persName>
                    <forename type="first">Mark L. A.</forename>
                    <surname>Richardson</surname>
                  </persName>
                  <idno type="halauthorid">2479996-0</idno>
                </author>
                <author role="aut">
                  <persName>
                    <forename type="first">Julien</forename>
                    <surname>Devriendt</surname>
                  </persName>
                  <idno type="halauthorid">1192705-0</idno>
                </author>
                <author role="aut">
                  <persName>
                    <forename type="first">Yohan</forename>
                    <surname>Dubois</surname>
                  </persName>
                  <email type="md5">1782362026c73fdfa5624f751bccb942</email>
                  <email type="domain">iap.fr</email>
                  <idno type="idhal" notation="string">yohan-dubois</idno>
                  <idno type="idhal" notation="numeric">738810</idno>
                  <idno type="halauthorid" notation="string">2528767-738810</idno>
                  <idno type="ORCID">https://orcid.org/0000-0003-0225-6387</idno>
                  <idno type="IDREF">https://www.idref.fr/130594628</idno>
                  <idno type="ARXIV">https://arxiv.org/a/dubois_y_1</idno>
                  <idno type="GOOGLE SCHOLAR">https://scholar.google.fr/citations?user=Vx0HM7cAAAAJ</idno>
                  <affiliation ref="#struct-541701"/>
                </author>
                <author role="aut">
                  <persName>
                    <forename type="first">Sebastien</forename>
                    <surname>Peirani</surname>
                  </persName>
                  <idno type="halauthorid">1192706-0</idno>
                  <affiliation ref="#struct-541701"/>
                </author>
                <author role="aut">
                  <persName>
                    <forename type="first">Christophe</forename>
                    <surname>Pichon</surname>
                  </persName>
                  <email type="md5">dbe2d587a0087530dfb9f6391bf2da66</email>
                  <email type="domain">iap.fr</email>
                  <idno type="idhal" notation="string">christophe-pichon</idno>
                  <idno type="idhal" notation="numeric">738765</idno>
                  <idno type="halauthorid" notation="string">9295-738765</idno>
                  <idno type="ORCID">https://orcid.org/0000-0003-0695-6735</idno>
                  <idno type="IDREF">https://www.idref.fr/091461618</idno>
                  <idno type="GOOGLE SCHOLAR">4bdEIGEAAAAJ</idno>
                  <affiliation ref="#struct-541701"/>
                </author>
              </analytic>
              <monogr>
                <meeting>
                  <title>American Astronomical Society</title>
                  <date type="start">2018</date>
                  <settlement>à renseigner</settlement>
                  <country key="ZZ">Unknown Region</country>
                </meeting>
                <imprint>
                  <biblScope unit="volume">232</biblScope>
                  <date type="datePub">2018</date>
                </imprint>
              </monogr>
              <idno type="bibcode">2018AAS...23220103S</idno>
            </biblStruct>
          </sourceDesc>
          <profileDesc>
            <langUsage>
              <language ident="en">English</language>
            </langUsage>
            <textClass>
              <classCode scheme="halDomain" n="sdu">Sciences of the Universe [physics]</classCode>
              <classCode scheme="halTypology" n="COMM">Conference papers</classCode>
              <classCode scheme="halOldTypology" n="COMM">Conference papers</classCode>
              <classCode scheme="halTreeTypology" n="COMM">Conference papers</classCode>
            </textClass>
            <abstract xml:lang="en">
              <p>Galaxy formation is a complex process with aspects that are still very uncertain. A mechanism that has been used in simulations to successfully resolve several of these outstanding issues is active galactic nucleus (AGN) feedback, where a large amount of energy is driven outwards through a galaxy and the surrounding region by a central supermassive black hole. A promising method for directly measuring this energy is by looking at small increases in the energy of the cosmic microwave background (CMB) photons as they pass through hot gas, known as the thermal Sunyaev-Zel'dovich (tSZ) effect. I will present work done to measure the tSZ effect around a large number of 0.5 &lt; z &lt; 1.5 elliptical galaxies using the South Pole Telescope (SPT), Atacama Cosmology Telescope (ACT), and Planck telescope, finding signals at 1-sigma to 3-sigma confindence levels depending on the dataset and redshift range. The results are mixed, including hints at non-gravitational energy possibly due to AGN feedback. Then I will present work done to analyze these results further by comparing them to matching simulated measurements, both including and not including AGN feedback, from the large-scale Horizon-AGN and Horizon-NoAGN cosmological simulations. In these comparisons, the SPT results, which tend to have lower-mass galaxies (&lt;5x10^11 M_Sun), favor the Horizon-AGN results at about a 1-sigma level, while the ACT results, which tend to have higher-mass galaxies (&gt;5x10^11 M_Sun), favor the Horizon-NoAGN results at more than a 6-sigma level. These results indicate that AGN feedback may be milder than often predicted, and they also highlight the promising nature of tSZ effect measurements and the need for further work using better data and more varied simulations.</p>
            </abstract>
          </profileDesc>
        </biblFull>
      </listBibl>
    </body>
    <back>
      <listOrg type="structures">
        <org type="laboratory" xml:id="struct-541701" status="VALID">
          <idno type="IdRef">028182030</idno>
          <idno type="ISNI">0000000105408249</idno>
          <idno type="RNSR">200112483U</idno>
          <idno type="ROR">022bnxw24</idno>
          <orgName>Institut d'Astrophysique de Paris</orgName>
          <orgName type="acronym">IAP</orgName>
          <date type="start">2018-01-01</date>
          <desc>
            <address>
              <addrLine>98bis, bd Arago - 75014 Paris France</addrLine>
              <country key="FR"/>
            </address>
            <ref type="url">http://www.iap.fr/</ref>
          </desc>
          <listRelation>
            <relation name="UMR7095" active="#struct-300045" type="direct"/>
            <relation active="#struct-413221" type="direct"/>
            <relation name="UMR7095" active="#struct-441569" type="direct"/>
          </listRelation>
        </org>
        <org type="institution" xml:id="struct-300045" status="VALID">
          <idno type="IdRef">029349265</idno>
          <idno type="ISNI">0000 0001 2154 1736</idno>
          <idno type="ROR">https://ror.org/04kdfz702</idno>
          <idno type="Wikidata">Q3152437</idno>
          <orgName>Institut national des sciences de l'Univers</orgName>
          <orgName type="acronym">INSU - CNRS</orgName>
          <date type="start">2007-04-19</date>
          <desc>
            <address>
              <addrLine>INSU-CNRS3 rue Michel-Ange, 75794 Paris Cedex 16</addrLine>
              <country key="FR"/>
            </address>
            <ref type="url">https://www.insu.cnrs.fr</ref>
          </desc>
        </org>
        <org type="regroupinstitution" xml:id="struct-413221" status="VALID">
          <idno type="IdRef">221333754</idno>
          <idno type="ROR">https://ror.org/02en5vm52</idno>
          <orgName>Sorbonne Université</orgName>
          <orgName type="acronym">SU</orgName>
          <date type="start">2018-01-01</date>
          <desc>
            <address>
              <addrLine>21 rue de l’École de médecine - 75006 Paris</addrLine>
              <country key="FR"/>
            </address>
            <ref type="url">http://www.sorbonne-universite.fr/</ref>
          </desc>
        </org>
        <org type="regroupinstitution" xml:id="struct-441569" status="VALID">
          <idno type="IdRef">02636817X</idno>
          <idno type="ISNI">0000000122597504</idno>
          <idno type="ROR">https://ror.org/02feahw73</idno>
          <orgName>Centre National de la Recherche Scientifique</orgName>
          <orgName type="acronym">CNRS</orgName>
          <date type="start">1939-10-19</date>
          <desc>
            <address>
              <country key="FR"/>
            </address>
            <ref type="url">https://www.cnrs.fr/</ref>
          </desc>
        </org>
      </listOrg>
    </back>
  </text>
</TEI>