Size - Stellar Mass Relation and Morphology of Quiescent Galaxies at $z\geq3$ in Public $JWST$ Fields
We present the results of a systematic study of the rest-frame optical morphology of quiescent galaxies at $z \geq 3$ using the Near-Infrared Camera (NIRCam) onboard $JWST$. Based on a sample selected by $UVJ$ color or $NUVUVJ$ color, we focus on 26 quiescent galaxies with $9.8
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| creator | Ito, Kei Valentino, Francesco Brammer, Gabriel Faisst, Andreas L Gillman, Steven Gomez-Guijarro, Carlos Gould, Katriona M. L Heintz, Kasper E Ilbert, Olivier Jespersen, Christian Kragh Kokorev, Vasily Kubo, Mariko Magdis, Georgios E McPartland, Conor Onodera, Masato Rizzo, Francesca Tanaka, Masayuki Toft, Sune Vijayan, Aswin P Weaver, John R Whitaker, Katherine E Wright, Lillian |
| description | We present the results of a systematic study of the rest-frame optical
morphology of quiescent galaxies at $z \geq 3$ using the Near-Infrared Camera
(NIRCam) onboard $JWST$. Based on a sample selected by $UVJ$ color or $NUVUVJ$
color, we focus on 26 quiescent galaxies with
$9.8 |
| doi_str_mv | 10.48550/arxiv.2307.06994 |
| format | Article |
| fullrecord | <record><control><sourceid>arxiv_GOX</sourceid><recordid>TN_cdi_arxiv_primary_2307_06994</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2307_06994</sourcerecordid><originalsourceid>FETCH-LOGICAL-a674-5fd500ca4e37a8653dedc3e6f4f5f9b86e9e0b33dec455a24a1e861facba8ab53</originalsourceid><addsrcrecordid>eNotzztPwzAUBWAvDKjwA5i4Q9YEp34kGVFFC6gVj0RiQYpu7OtiySQlSVHbX08pTEfnDEf6GLtKeSJzpfgN9jv_nUwFzxKui0KeMyr9gSCGcqQQsIcVDgO8UsDRdy1ga2HV9ZuPLnTrPXQOXraeBkPtCAsMuDsWwBGiw_uavkQEvoXnbRO8gejxrawimHsKdrhgZw7DQJf_OWHV_K6a3cfLp8XD7HYZo85krJxVnBuUJDLMtRKWrBGknXTKFU2uqSDeiONspFI4lZhSrlOHpsEcGyUm7Prv9uSsN73_xH5f_3rrk1f8AGiOUDU</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Size - Stellar Mass Relation and Morphology of Quiescent Galaxies at $z\geq3$ in Public $JWST$ Fields</title><source>arXiv.org</source><creator>Ito, Kei ; Valentino, Francesco ; Brammer, Gabriel ; Faisst, Andreas L ; Gillman, Steven ; Gomez-Guijarro, Carlos ; Gould, Katriona M. L ; Heintz, Kasper E ; Ilbert, Olivier ; Jespersen, Christian Kragh ; Kokorev, Vasily ; Kubo, Mariko ; Magdis, Georgios E ; McPartland, Conor ; Onodera, Masato ; Rizzo, Francesca ; Tanaka, Masayuki ; Toft, Sune ; Vijayan, Aswin P ; Weaver, John R ; Whitaker, Katherine E ; Wright, Lillian</creator><creatorcontrib>Ito, Kei ; Valentino, Francesco ; Brammer, Gabriel ; Faisst, Andreas L ; Gillman, Steven ; Gomez-Guijarro, Carlos ; Gould, Katriona M. L ; Heintz, Kasper E ; Ilbert, Olivier ; Jespersen, Christian Kragh ; Kokorev, Vasily ; Kubo, Mariko ; Magdis, Georgios E ; McPartland, Conor ; Onodera, Masato ; Rizzo, Francesca ; Tanaka, Masayuki ; Toft, Sune ; Vijayan, Aswin P ; Weaver, John R ; Whitaker, Katherine E ; Wright, Lillian</creatorcontrib><description><![CDATA[We present the results of a systematic study of the rest-frame optical
morphology of quiescent galaxies at $z \geq 3$ using the Near-Infrared Camera
(NIRCam) onboard $JWST$. Based on a sample selected by $UVJ$ color or $NUVUVJ$
color, we focus on 26 quiescent galaxies with
$9.8<\log{(M_\star/M_\odot)}<11.4$ at $2.8<z_{\rm phot}<4.6$ with publicly
available $JWST$ data. Their sizes are constrained by fitting the S\'ersic
profile to all available NIRCam images. We see a negative correlation between
the observed wavelength and the size in our sample and derive their size at the
rest-frame $0.5\, {\rm \mu m}$ taking into account this trend. Our quiescent
galaxies show a significant correlation between the rest-frame $0.5\, {\rm \mu
m}$ size and the stellar mass at $z\geq3$. The analytical fit for them at
$\log{(M_\star/M_\odot)}>10.3$ implies that our size - stellar mass relations
are below those at lower redshifts, with the amplitude of $\sim0.6\, {\rm kpc}$
at $M_\star = 5\times 10^{10}\, M_\odot$. This value agrees with the
extrapolation from the size evolution of quiescent galaxies at $z<3$ in the
literature, implying that the size of quiescent galaxies increases
monotonically from $z\sim3-5$. Our sample is mainly composed of galaxies with
bulge-like structures according to their median S\'ersic index and axis ratio
of $n\sim3-4$ and $q\sim0.6-0.8$, respectively. On the other hand, there is a
trend of increasing fraction of galaxies with low S\'ersic index, suggesting
$3<z<5$ might be the epoch of onset of morphological transformation with a
fraction of very notable disky quenched galaxies.]]></description><identifier>DOI: 10.48550/arxiv.2307.06994</identifier><language>eng</language><subject>Physics - Astrophysics of Galaxies</subject><creationdate>2023-07</creationdate><rights>http://creativecommons.org/licenses/by/4.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,885</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/2307.06994$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.2307.06994$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Ito, Kei</creatorcontrib><creatorcontrib>Valentino, Francesco</creatorcontrib><creatorcontrib>Brammer, Gabriel</creatorcontrib><creatorcontrib>Faisst, Andreas L</creatorcontrib><creatorcontrib>Gillman, Steven</creatorcontrib><creatorcontrib>Gomez-Guijarro, Carlos</creatorcontrib><creatorcontrib>Gould, Katriona M. L</creatorcontrib><creatorcontrib>Heintz, Kasper E</creatorcontrib><creatorcontrib>Ilbert, Olivier</creatorcontrib><creatorcontrib>Jespersen, Christian Kragh</creatorcontrib><creatorcontrib>Kokorev, Vasily</creatorcontrib><creatorcontrib>Kubo, Mariko</creatorcontrib><creatorcontrib>Magdis, Georgios E</creatorcontrib><creatorcontrib>McPartland, Conor</creatorcontrib><creatorcontrib>Onodera, Masato</creatorcontrib><creatorcontrib>Rizzo, Francesca</creatorcontrib><creatorcontrib>Tanaka, Masayuki</creatorcontrib><creatorcontrib>Toft, Sune</creatorcontrib><creatorcontrib>Vijayan, Aswin P</creatorcontrib><creatorcontrib>Weaver, John R</creatorcontrib><creatorcontrib>Whitaker, Katherine E</creatorcontrib><creatorcontrib>Wright, Lillian</creatorcontrib><title>Size - Stellar Mass Relation and Morphology of Quiescent Galaxies at $z\geq3$ in Public $JWST$ Fields</title><description><![CDATA[We present the results of a systematic study of the rest-frame optical
morphology of quiescent galaxies at $z \geq 3$ using the Near-Infrared Camera
(NIRCam) onboard $JWST$. Based on a sample selected by $UVJ$ color or $NUVUVJ$
color, we focus on 26 quiescent galaxies with
$9.8<\log{(M_\star/M_\odot)}<11.4$ at $2.8<z_{\rm phot}<4.6$ with publicly
available $JWST$ data. Their sizes are constrained by fitting the S\'ersic
profile to all available NIRCam images. We see a negative correlation between
the observed wavelength and the size in our sample and derive their size at the
rest-frame $0.5\, {\rm \mu m}$ taking into account this trend. Our quiescent
galaxies show a significant correlation between the rest-frame $0.5\, {\rm \mu
m}$ size and the stellar mass at $z\geq3$. The analytical fit for them at
$\log{(M_\star/M_\odot)}>10.3$ implies that our size - stellar mass relations
are below those at lower redshifts, with the amplitude of $\sim0.6\, {\rm kpc}$
at $M_\star = 5\times 10^{10}\, M_\odot$. This value agrees with the
extrapolation from the size evolution of quiescent galaxies at $z<3$ in the
literature, implying that the size of quiescent galaxies increases
monotonically from $z\sim3-5$. Our sample is mainly composed of galaxies with
bulge-like structures according to their median S\'ersic index and axis ratio
of $n\sim3-4$ and $q\sim0.6-0.8$, respectively. On the other hand, there is a
trend of increasing fraction of galaxies with low S\'ersic index, suggesting
$3<z<5$ might be the epoch of onset of morphological transformation with a
fraction of very notable disky quenched galaxies.]]></description><subject>Physics - Astrophysics of Galaxies</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNotzztPwzAUBWAvDKjwA5i4Q9YEp34kGVFFC6gVj0RiQYpu7OtiySQlSVHbX08pTEfnDEf6GLtKeSJzpfgN9jv_nUwFzxKui0KeMyr9gSCGcqQQsIcVDgO8UsDRdy1ga2HV9ZuPLnTrPXQOXraeBkPtCAsMuDsWwBGiw_uavkQEvoXnbRO8gejxrawimHsKdrhgZw7DQJf_OWHV_K6a3cfLp8XD7HYZo85krJxVnBuUJDLMtRKWrBGknXTKFU2uqSDeiONspFI4lZhSrlOHpsEcGyUm7Prv9uSsN73_xH5f_3rrk1f8AGiOUDU</recordid><startdate>20230713</startdate><enddate>20230713</enddate><creator>Ito, Kei</creator><creator>Valentino, Francesco</creator><creator>Brammer, Gabriel</creator><creator>Faisst, Andreas L</creator><creator>Gillman, Steven</creator><creator>Gomez-Guijarro, Carlos</creator><creator>Gould, Katriona M. L</creator><creator>Heintz, Kasper E</creator><creator>Ilbert, Olivier</creator><creator>Jespersen, Christian Kragh</creator><creator>Kokorev, Vasily</creator><creator>Kubo, Mariko</creator><creator>Magdis, Georgios E</creator><creator>McPartland, Conor</creator><creator>Onodera, Masato</creator><creator>Rizzo, Francesca</creator><creator>Tanaka, Masayuki</creator><creator>Toft, Sune</creator><creator>Vijayan, Aswin P</creator><creator>Weaver, John R</creator><creator>Whitaker, Katherine E</creator><creator>Wright, Lillian</creator><scope>GOX</scope></search><sort><creationdate>20230713</creationdate><title>Size - Stellar Mass Relation and Morphology of Quiescent Galaxies at $z\geq3$ in Public $JWST$ Fields</title><author>Ito, Kei ; Valentino, Francesco ; Brammer, Gabriel ; Faisst, Andreas L ; Gillman, Steven ; Gomez-Guijarro, Carlos ; Gould, Katriona M. L ; Heintz, Kasper E ; Ilbert, Olivier ; Jespersen, Christian Kragh ; Kokorev, Vasily ; Kubo, Mariko ; Magdis, Georgios E ; McPartland, Conor ; Onodera, Masato ; Rizzo, Francesca ; Tanaka, Masayuki ; Toft, Sune ; Vijayan, Aswin P ; Weaver, John R ; Whitaker, Katherine E ; Wright, Lillian</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a674-5fd500ca4e37a8653dedc3e6f4f5f9b86e9e0b33dec455a24a1e861facba8ab53</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>Physics - Astrophysics of Galaxies</topic><toplevel>online_resources</toplevel><creatorcontrib>Ito, Kei</creatorcontrib><creatorcontrib>Valentino, Francesco</creatorcontrib><creatorcontrib>Brammer, Gabriel</creatorcontrib><creatorcontrib>Faisst, Andreas L</creatorcontrib><creatorcontrib>Gillman, Steven</creatorcontrib><creatorcontrib>Gomez-Guijarro, Carlos</creatorcontrib><creatorcontrib>Gould, Katriona M. L</creatorcontrib><creatorcontrib>Heintz, Kasper E</creatorcontrib><creatorcontrib>Ilbert, Olivier</creatorcontrib><creatorcontrib>Jespersen, Christian Kragh</creatorcontrib><creatorcontrib>Kokorev, Vasily</creatorcontrib><creatorcontrib>Kubo, Mariko</creatorcontrib><creatorcontrib>Magdis, Georgios E</creatorcontrib><creatorcontrib>McPartland, Conor</creatorcontrib><creatorcontrib>Onodera, Masato</creatorcontrib><creatorcontrib>Rizzo, Francesca</creatorcontrib><creatorcontrib>Tanaka, Masayuki</creatorcontrib><creatorcontrib>Toft, Sune</creatorcontrib><creatorcontrib>Vijayan, Aswin P</creatorcontrib><creatorcontrib>Weaver, John R</creatorcontrib><creatorcontrib>Whitaker, Katherine E</creatorcontrib><creatorcontrib>Wright, Lillian</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Ito, Kei</au><au>Valentino, Francesco</au><au>Brammer, Gabriel</au><au>Faisst, Andreas L</au><au>Gillman, Steven</au><au>Gomez-Guijarro, Carlos</au><au>Gould, Katriona M. L</au><au>Heintz, Kasper E</au><au>Ilbert, Olivier</au><au>Jespersen, Christian Kragh</au><au>Kokorev, Vasily</au><au>Kubo, Mariko</au><au>Magdis, Georgios E</au><au>McPartland, Conor</au><au>Onodera, Masato</au><au>Rizzo, Francesca</au><au>Tanaka, Masayuki</au><au>Toft, Sune</au><au>Vijayan, Aswin P</au><au>Weaver, John R</au><au>Whitaker, Katherine E</au><au>Wright, Lillian</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Size - Stellar Mass Relation and Morphology of Quiescent Galaxies at $z\geq3$ in Public $JWST$ Fields</atitle><date>2023-07-13</date><risdate>2023</risdate><abstract><![CDATA[We present the results of a systematic study of the rest-frame optical
morphology of quiescent galaxies at $z \geq 3$ using the Near-Infrared Camera
(NIRCam) onboard $JWST$. Based on a sample selected by $UVJ$ color or $NUVUVJ$
color, we focus on 26 quiescent galaxies with
$9.8<\log{(M_\star/M_\odot)}<11.4$ at $2.8<z_{\rm phot}<4.6$ with publicly
available $JWST$ data. Their sizes are constrained by fitting the S\'ersic
profile to all available NIRCam images. We see a negative correlation between
the observed wavelength and the size in our sample and derive their size at the
rest-frame $0.5\, {\rm \mu m}$ taking into account this trend. Our quiescent
galaxies show a significant correlation between the rest-frame $0.5\, {\rm \mu
m}$ size and the stellar mass at $z\geq3$. The analytical fit for them at
$\log{(M_\star/M_\odot)}>10.3$ implies that our size - stellar mass relations
are below those at lower redshifts, with the amplitude of $\sim0.6\, {\rm kpc}$
at $M_\star = 5\times 10^{10}\, M_\odot$. This value agrees with the
extrapolation from the size evolution of quiescent galaxies at $z<3$ in the
literature, implying that the size of quiescent galaxies increases
monotonically from $z\sim3-5$. Our sample is mainly composed of galaxies with
bulge-like structures according to their median S\'ersic index and axis ratio
of $n\sim3-4$ and $q\sim0.6-0.8$, respectively. On the other hand, there is a
trend of increasing fraction of galaxies with low S\'ersic index, suggesting
$3<z<5$ might be the epoch of onset of morphological transformation with a
fraction of very notable disky quenched galaxies.]]></abstract><doi>10.48550/arxiv.2307.06994</doi><oa>free_for_read</oa></addata></record> |
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| subjects | Physics - Astrophysics of Galaxies |
| title | Size - Stellar Mass Relation and Morphology of Quiescent Galaxies at $z\geq3$ in Public $JWST$ Fields |
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