PittsburghV1, Canada, Analysis, bibRecord, 000541

THE DEPENDENCE OF QUENCHING UPON THE INNER STRUCTURE OF GALAXIES AT 0.5 ≤ z < 0.8 IN THE DEEP2/AEGIS SURVEY

Identifieur interne : 000541 ( Canada/Analysis ); précédent : 000540; suivant : 000542

THE DEPENDENCE OF QUENCHING UPON THE INNER STRUCTURE OF GALAXIES AT 0.5 ≤ z < 0.8 IN THE DEEP2/AEGIS SURVEY

Auteurs : Edmond Cheung [États-Unis] ; S. M. Faber [États-Unis] ; David C. Koo [États-Unis] ; Aaron A. Dutton [Canada] ; Luc Simard [Canada] ; Elizabeth J. Mcgrath [États-Unis] ; J.-S. Huang [États-Unis] ; Eric F. Bell [États-Unis] ; Avishai Dekel [Israël] ; Jerome J. Fang [États-Unis] ; Samir Salim [États-Unis] ; G. Barro [États-Unis] ; K. Bundy [Japon] ; A. L. Coil [États-Unis] ; Michael C. Cooper [États-Unis] ; C. J. Conselice [Royaume-Uni] ; M. Davis [États-Unis] ; A. Dominguez [États-Unis] ; Susan A. Kassin [États-Unis] ; Dale D. Kocevski [États-Unis] ; Anton M. Koekemoer [États-Unis] ; Lihwai Lin [Taïwan] ; Jennifer M. Lotz [États-Unis] ; J. A. Newman [États-Unis] ; Andrew C. Phillips [États-Unis] ; D. J. Izosario [Allemagne] ; Benjamin J. Weiner [États-Unis] ; C. N. A. Willmer [États-Unis]

Source :

The Astrophysical journal [ 0004-637X ] ; 2012.

RBID : Pascal:13-0041944

Descripteurs français

Pascal (Inist)
- Structure galaxies, Formation stellaire, Formation galaxies, Noyau galactique actif, Boucle réaction, Chauffage onde choc, Matière sombre, Galaxies bleues, Masse stellaire, Couleur, Corrélation, Déplacement vers le rouge, Fonction échelon, Galaxies N, Modèle, Taux formation, Instabilité, Catalogue astronomique, Bulbe galaxies, Evolution galaxies, Galaxies actives, Noyau galaxies.

English descriptors

KwdEn :
- Active galaxies, Active galaxy nuclei, Astronomical catalogues, Blue galaxies, Color, Correlations, Dark matter, Feedback, Formation rate, Galaxy bulge, Galaxy evolution, Galaxy formation, Galaxy nuclei, Galaxy structure, Instability, Models, N galaxies, Red shift, Shock heating, Star formation, Stellar mass, Step function.

Abstract

The shutdown of star formation in galaxies is generally termed "quenching." Quenching may occur through a variety of processes, e.g., active galactic nucleus (AGN) feedback, stellar feedback, or the shock heating of gas in the dark matter halo. However, which mechanism(s) is, in fact, responsible for quenching is still in question. This paper addresses quenching by searching for traces of possible quenching processes through their effects on galaxy structural parameters such as stellar mass (M_*), M_*/r_e, surface stellar mass density (∼M_*/r²_c), and Sérsic index (n). We analyze the rest-frame U - B color correlations versus these structural parameters using a sample of galaxies in the redshift range 0.5 ≤ z < 0.8 from the DEEP2/AEGIS survey. In addition to global radii, stellar masses, and Sérsic parameters, we also use "bulge" and "disk" photometric measurements from GIM2D fits to HST/ACS V and I images. We assess the tightness of the color relationships by measuring their "overlap regions," defined as the area in color-parameter space in which red and blue galaxies overlap; the parameter that minimizes these overlap regions is considered to be the most effective color discriminator.

Affiliations:

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Pascal:13-0041944

Le document en format XML

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<author><name sortKey="Izosario, D J" sort="Izosario, D J" uniqKey="Izosario D" first="D. J." last="Izosario">D. J. Izosario</name>
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<author><name sortKey="Weiner, Benjamin J" sort="Weiner, Benjamin J" uniqKey="Weiner B" first="Benjamin J." last="Weiner">Benjamin J. Weiner</name>
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<author><name sortKey="Willmer, C N A" sort="Willmer, C N A" uniqKey="Willmer C" first="C. N. A." last="Willmer">C. N. A. Willmer</name>
<affiliation wicri:level="1"><inist:fA14 i1="20"><s1>Steward Observatory, 933 N. Cherry Street. University of Arizona</s1>
<s2>Tucson, AZ 85721</s2>
<s3>USA</s3>
<sZ>27 aut.</sZ>
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<idno type="wicri:Area/Main/Curation">008507</idno>
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<sourceDesc><biblStruct><analytic><title xml:lang="en" level="a">THE DEPENDENCE OF QUENCHING UPON THE INNER STRUCTURE OF GALAXIES AT 0.5 ≤ z < 0.8 IN THE DEEP2/AEGIS SURVEY</title>
<author><name sortKey="Cheung, Edmond" sort="Cheung, Edmond" uniqKey="Cheung E" first="Edmond" last="Cheung">Edmond Cheung</name>
<affiliation wicri:level="1"><inist:fA14 i1="01"><s1>Department of Astronomy and Astrophysics, 1156 High Street, University of California</s1>
<s2>Santa Cruz, CA 95064</s2>
<s3>USA</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
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</inist:fA14>
<country>États-Unis</country>
<wicri:noRegion>Santa Cruz, CA 95064</wicri:noRegion>
</affiliation>
</author>
<author><name sortKey="Faber, S M" sort="Faber, S M" uniqKey="Faber S" first="S. M." last="Faber">S. M. Faber</name>
<affiliation wicri:level="1"><inist:fA14 i1="01"><s1>Department of Astronomy and Astrophysics, 1156 High Street, University of California</s1>
<s2>Santa Cruz, CA 95064</s2>
<s3>USA</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
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<country>États-Unis</country>
<wicri:noRegion>Santa Cruz, CA 95064</wicri:noRegion>
</affiliation>
<affiliation wicri:level="1"><inist:fA14 i1="02"><s1>UCO/Lick Observatory, University of California, 1156 High Street</s1>
<s2>Santa Cruz, CA 95064</s2>
<s3>USA</s3>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
</inist:fA14>
<country>États-Unis</country>
<wicri:noRegion>Santa Cruz, CA 95064</wicri:noRegion>
</affiliation>
</author>
<author><name sortKey="Koo, David C" sort="Koo, David C" uniqKey="Koo D" first="David C." last="Koo">David C. Koo</name>
<affiliation wicri:level="1"><inist:fA14 i1="01"><s1>Department of Astronomy and Astrophysics, 1156 High Street, University of California</s1>
<s2>Santa Cruz, CA 95064</s2>
<s3>USA</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
<sZ>6 aut.</sZ>
<sZ>10 aut.</sZ>
<sZ>12 aut.</sZ>
<sZ>20 aut.</sZ>
<sZ>25 aut.</sZ>
</inist:fA14>
<country>États-Unis</country>
<wicri:noRegion>Santa Cruz, CA 95064</wicri:noRegion>
</affiliation>
<affiliation wicri:level="1"><inist:fA14 i1="02"><s1>UCO/Lick Observatory, University of California, 1156 High Street</s1>
<s2>Santa Cruz, CA 95064</s2>
<s3>USA</s3>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
</inist:fA14>
<country>États-Unis</country>
<wicri:noRegion>Santa Cruz, CA 95064</wicri:noRegion>
</affiliation>
</author>
<author><name sortKey="Dutton, Aaron A" sort="Dutton, Aaron A" uniqKey="Dutton A" first="Aaron A." last="Dutton">Aaron A. Dutton</name>
<affiliation wicri:level="1"><inist:fA14 i1="03"><s1>Department of Physics and Astronomy, Elliot Building, 3800 Finnerty Road, University of Victoria</s1>
<s2>Victoria, BC V8P 5C2</s2>
<s3>CAN</s3>
<sZ>4 aut.</sZ>
</inist:fA14>
<country>Canada</country>
<wicri:noRegion>Victoria, BC V8P 5C2</wicri:noRegion>
</affiliation>
</author>
<author><name sortKey="Simard, Luc" sort="Simard, Luc" uniqKey="Simard L" first="Luc" last="Simard">Luc Simard</name>
<affiliation wicri:level="1"><inist:fA14 i1="04"><s1>Herzberg Institute of Astrophysics, National Research Council of Canada, 5071 West Saanich Road</s1>
<s2>Victoria, BC V9E 2E7</s2>
<s3>CAN</s3>
<sZ>5 aut.</sZ>
</inist:fA14>
<country>Canada</country>
<wicri:noRegion>Victoria, BC V9E 2E7</wicri:noRegion>
</affiliation>
</author>
<author><name sortKey="Mcgrath, Elizabeth J" sort="Mcgrath, Elizabeth J" uniqKey="Mcgrath E" first="Elizabeth J." last="Mcgrath">Elizabeth J. Mcgrath</name>
<affiliation wicri:level="1"><inist:fA14 i1="01"><s1>Department of Astronomy and Astrophysics, 1156 High Street, University of California</s1>
<s2>Santa Cruz, CA 95064</s2>
<s3>USA</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
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</affiliation>
</author>
<author><name sortKey="Huang, J S" sort="Huang, J S" uniqKey="Huang J" first="J.-S." last="Huang">J.-S. Huang</name>
<affiliation wicri:level="1"><inist:fA14 i1="05"><s1>Harvard-Smithsonian Center for Astrophysics, 60 Garden State</s1>
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<country>États-Unis</country>
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</affiliation>
</author>
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<affiliation wicri:level="1"><inist:fA14 i1="06"><s1>Department of Astronomy, University of Michigan, 500 Church St</s1>
<s2>Ann Arbor, MI 48109</s2>
<s3>USA</s3>
<sZ>8 aut.</sZ>
</inist:fA14>
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</affiliation>
</author>
<author><name sortKey="Dekel, Avishai" sort="Dekel, Avishai" uniqKey="Dekel A" first="Avishai" last="Dekel">Avishai Dekel</name>
<affiliation wicri:level="1"><inist:fA14 i1="07"><s1>Racah Institute of Physics. The Hebrew University</s1>
<s2>Jerusalem 91904</s2>
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</inist:fA14>
<country>Israël</country>
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</affiliation>
</author>
<author><name sortKey="Fang, Jerome J" sort="Fang, Jerome J" uniqKey="Fang J" first="Jerome J." last="Fang">Jerome J. Fang</name>
<affiliation wicri:level="1"><inist:fA14 i1="01"><s1>Department of Astronomy and Astrophysics, 1156 High Street, University of California</s1>
<s2>Santa Cruz, CA 95064</s2>
<s3>USA</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
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</affiliation>
</author>
<author><name sortKey="Barro, G" sort="Barro, G" uniqKey="Barro G" first="G." last="Barro">G. Barro</name>
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<s2>Santa Cruz, CA 95064</s2>
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<author><name sortKey="Bundy, K" sort="Bundy, K" uniqKey="Bundy K" first="K." last="Bundy">K. Bundy</name>
<affiliation wicri:level="4"><inist:fA14 i1="09"><s1>Kavli Institute for the Physics and Mathematics of the Universe, University of Tokyo</s1>
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<author><name sortKey="Cooper, Michael C" sort="Cooper, Michael C" uniqKey="Cooper M" first="Michael C." last="Cooper">Michael C. Cooper</name>
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<author><name sortKey="Conselice, C J" sort="Conselice, C J" uniqKey="Conselice C" first="C. J." last="Conselice">C. J. Conselice</name>
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<country>Royaume-Uni</country>
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</placeName>
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</affiliation>
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<author><name sortKey="Davis, M" sort="Davis, M" uniqKey="Davis M" first="M." last="Davis">M. Davis</name>
<affiliation wicri:level="1"><inist:fA14 i1="13"><s1>Department of Astronomy. University of California</s1>
<s2>Berkeley, CA 94720</s2>
<s3>USA</s3>
<sZ>17 aut.</sZ>
</inist:fA14>
<country>États-Unis</country>
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</affiliation>
</author>
<author><name sortKey="Dominguez, A" sort="Dominguez, A" uniqKey="Dominguez A" first="A." last="Dominguez">A. Dominguez</name>
<affiliation wicri:level="1"><inist:fA14 i1="14"><s1>Department of Physics and Astronomy, University of California</s1>
<s2>Riverside, CA 92521</s2>
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<sZ>18 aut.</sZ>
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<author><name sortKey="Kassin, Susan A" sort="Kassin, Susan A" uniqKey="Kassin S" first="Susan A." last="Kassin">Susan A. Kassin</name>
<affiliation wicri:level="1"><inist:fA14 i1="15"><s1>Astrophysics Science Division, Goddard Space Flight Center, Code 665</s1>
<s2>Greenbelt. MD 20771</s2>
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<author><name sortKey="Kocevski, Dale D" sort="Kocevski, Dale D" uniqKey="Kocevski D" first="Dale D." last="Kocevski">Dale D. Kocevski</name>
<affiliation wicri:level="1"><inist:fA14 i1="01"><s1>Department of Astronomy and Astrophysics, 1156 High Street, University of California</s1>
<s2>Santa Cruz, CA 95064</s2>
<s3>USA</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
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<author><name sortKey="Koekemoer, Anton M" sort="Koekemoer, Anton M" uniqKey="Koekemoer A" first="Anton M." last="Koekemoer">Anton M. Koekemoer</name>
<affiliation wicri:level="1"><inist:fA14 i1="16"><s1>Space Telescope Science Institute, 3700 San Martin Drive</s1>
<s2>Baltimore, MD 21218</s2>
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</author>
<author><name sortKey="Lin, Lihwai" sort="Lin, Lihwai" uniqKey="Lin L" first="Lihwai" last="Lin">Lihwai Lin</name>
<affiliation wicri:level="1"><inist:fA14 i1="17"><s1>Institute of Astronomy and Astrophysics, Academia Sinica</s1>
<s2>Taipei 106</s2>
<s3>TWN</s3>
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<country>Taïwan</country>
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<author><name sortKey="Lotz, Jennifer M" sort="Lotz, Jennifer M" uniqKey="Lotz J" first="Jennifer M." last="Lotz">Jennifer M. Lotz</name>
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</affiliation>
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<author><name sortKey="Newman, J A" sort="Newman, J A" uniqKey="Newman J" first="J. A." last="Newman">J. A. Newman</name>
<affiliation wicri:level="4"><inist:fA14 i1="18"><s1>Department of Physics and Astronomy. University of Pittsburgh, 3941 O'Hara Street</s1>
<s2>Pittsburgh, PA 15260</s2>
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</placeName>
</affiliation>
</author>
<author><name sortKey="Phillips, Andrew C" sort="Phillips, Andrew C" uniqKey="Phillips A" first="Andrew C." last="Phillips">Andrew C. Phillips</name>
<affiliation wicri:level="1"><inist:fA14 i1="01"><s1>Department of Astronomy and Astrophysics, 1156 High Street, University of California</s1>
<s2>Santa Cruz, CA 95064</s2>
<s3>USA</s3>
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</affiliation>
</author>
<author><name sortKey="Izosario, D J" sort="Izosario, D J" uniqKey="Izosario D" first="D. J." last="Izosario">D. J. Izosario</name>
<affiliation wicri:level="1"><inist:fA14 i1="19"><s1>Max Planck Institute for Extraterrestrial Physics. P.O. Box 1312, Giessenbachstrasse</s1>
<s2>85741 Garching</s2>
<s3>DEU</s3>
<sZ>26 aut.</sZ>
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<country>Allemagne</country>
<wicri:noRegion>85741 Garching</wicri:noRegion>
<wicri:noRegion>Giessenbachstrasse</wicri:noRegion>
<wicri:noRegion>85741 Garching</wicri:noRegion>
</affiliation>
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<author><name sortKey="Weiner, Benjamin J" sort="Weiner, Benjamin J" uniqKey="Weiner B" first="Benjamin J." last="Weiner">Benjamin J. Weiner</name>
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<sZ>27 aut.</sZ>
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<sZ>27 aut.</sZ>
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</analytic>
<series><title level="j" type="main">The Astrophysical journal</title>
<title level="j" type="abbreviated">Astrophys. j.</title>
<idno type="ISSN">0004-637X</idno>
<imprint><date when="2012">2012</date>
</imprint>
</series>
</biblStruct>
</sourceDesc>
<seriesStmt><title level="j" type="main">The Astrophysical journal</title>
<title level="j" type="abbreviated">Astrophys. j.</title>
<idno type="ISSN">0004-637X</idno>
</seriesStmt>
</fileDesc>
<profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Active galaxies</term>
<term>Active galaxy nuclei</term>
<term>Astronomical catalogues</term>
<term>Blue galaxies</term>
<term>Color</term>
<term>Correlations</term>
<term>Dark matter</term>
<term>Feedback</term>
<term>Formation rate</term>
<term>Galaxy bulge</term>
<term>Galaxy evolution</term>
<term>Galaxy formation</term>
<term>Galaxy nuclei</term>
<term>Galaxy structure</term>
<term>Instability</term>
<term>Models</term>
<term>N galaxies</term>
<term>Red shift</term>
<term>Shock heating</term>
<term>Star formation</term>
<term>Stellar mass</term>
<term>Step function</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr"><term>Structure galaxies</term>
<term>Formation stellaire</term>
<term>Formation galaxies</term>
<term>Noyau galactique actif</term>
<term>Boucle réaction</term>
<term>Chauffage onde choc</term>
<term>Matière sombre</term>
<term>Galaxies bleues</term>
<term>Masse stellaire</term>
<term>Couleur</term>
<term>Corrélation</term>
<term>Déplacement vers le rouge</term>
<term>Fonction échelon</term>
<term>Galaxies N</term>
<term>Modèle</term>
<term>Taux formation</term>
<term>Instabilité</term>
<term>Catalogue astronomique</term>
<term>Bulbe galaxies</term>
<term>Evolution galaxies</term>
<term>Galaxies actives</term>
<term>Noyau galaxies</term>
</keywords>
</textClass>
</profileDesc>
</teiHeader>
<front><div type="abstract" xml:lang="en">The shutdown of star formation in galaxies is generally termed "quenching." Quenching may occur through a variety of processes, e.g., active galactic nucleus (AGN) feedback, stellar feedback, or the shock heating of gas in the dark matter halo. However, which mechanism(s) is, in fact, responsible for quenching is still in question. This paper addresses quenching by searching for traces of possible quenching processes through their effects on galaxy structural parameters such as stellar mass (M<sub>*</sub>
), M<sub>*</sub>
/r<sub>e</sub>
, surface stellar mass density (∼M<sub>*</sub>
/r<sup>2</sup>
<sub>c</sub>
), and Sérsic index (n). We analyze the rest-frame U - B color correlations versus these structural parameters using a sample of galaxies in the redshift range 0.5 ≤ z < 0.8 from the DEEP2/AEGIS survey. In addition to global radii, stellar masses, and Sérsic parameters, we also use "bulge" and "disk" photometric measurements from GIM2D fits to HST/ACS V and I images. We assess the tightness of the color relationships by measuring their "overlap regions," defined as the area in color-parameter space in which red and blue galaxies overlap; the parameter that minimizes these overlap regions is considered to be the most effective color discriminator.</div>
</front>
</TEI>
<affiliations><list><country><li>Allemagne</li>
<li>Canada</li>
<li>Israël</li>
<li>Japon</li>
<li>Royaume-Uni</li>
<li>Taïwan</li>
<li>États-Unis</li>
</country>
<region><li>Angleterre</li>
<li>Nottinghamshire</li>
<li>Pennsylvanie</li>
<li>Région de Kantō</li>
</region>
<settlement><li>Nottingham</li>
<li>Pittsburgh</li>
<li>Tokyo</li>
</settlement>
<orgName><li>Université de Nottingham</li>
<li>Université de Pittsburgh</li>
<li>Université de Tokyo</li>
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<name sortKey="Kocevski, Dale D" sort="Kocevski, Dale D" uniqKey="Kocevski D" first="Dale D." last="Kocevski">Dale D. Kocevski</name>
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<name sortKey="Koo, David C" sort="Koo, David C" uniqKey="Koo D" first="David C." last="Koo">David C. Koo</name>
<name sortKey="Koo, David C" sort="Koo, David C" uniqKey="Koo D" first="David C." last="Koo">David C. Koo</name>
<name sortKey="Lotz, Jennifer M" sort="Lotz, Jennifer M" uniqKey="Lotz J" first="Jennifer M." last="Lotz">Jennifer M. Lotz</name>
<name sortKey="Mcgrath, Elizabeth J" sort="Mcgrath, Elizabeth J" uniqKey="Mcgrath E" first="Elizabeth J." last="Mcgrath">Elizabeth J. Mcgrath</name>
<name sortKey="Newman, J A" sort="Newman, J A" uniqKey="Newman J" first="J. A." last="Newman">J. A. Newman</name>
<name sortKey="Phillips, Andrew C" sort="Phillips, Andrew C" uniqKey="Phillips A" first="Andrew C." last="Phillips">Andrew C. Phillips</name>
<name sortKey="Salim, Samir" sort="Salim, Samir" uniqKey="Salim S" first="Samir" last="Salim">Samir Salim</name>
<name sortKey="Weiner, Benjamin J" sort="Weiner, Benjamin J" uniqKey="Weiner B" first="Benjamin J." last="Weiner">Benjamin J. Weiner</name>
<name sortKey="Willmer, C N A" sort="Willmer, C N A" uniqKey="Willmer C" first="C. N. A." last="Willmer">C. N. A. Willmer</name>
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<country name="Canada"><noRegion><name sortKey="Dutton, Aaron A" sort="Dutton, Aaron A" uniqKey="Dutton A" first="Aaron A." last="Dutton">Aaron A. Dutton</name>
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<name sortKey="Simard, Luc" sort="Simard, Luc" uniqKey="Simard L" first="Luc" last="Simard">Luc Simard</name>
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   |texte=   THE DEPENDENCE OF QUENCHING UPON THE INNER STRUCTURE OF GALAXIES AT 0.5 ≤ z < 0.8 IN THE DEEP2/AEGIS SURVEY
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THE DEPENDENCE OF QUENCHING UPON THE INNER STRUCTURE OF GALAXIES AT 0.5 ≤ z < 0.8 IN THE DEEP2/AEGIS SURVEY

THE DEPENDENCE OF QUENCHING UPON THE INNER STRUCTURE OF GALAXIES AT 0.5 ≤ z < 0.8 IN THE DEEP2/AEGIS SURVEY

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