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<ri:Resource created="2025-04-09T15:29:05Z" status="active" updated="2025-06-02T07:05:25Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>CEERS Key Paper. IV. JWST &amp; HST data</title><shortName>J/ApJ/946/L16</shortName><identifier>ivo://CDS.VizieR/J/ApJ/946/L16</identifier><altIdentifier>doi:10.26093/cds/vizier.19469016</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Perez-Gonzalez P.G.</name></creator><creator><name>Barro G.</name></creator><creator><name>Annunziatella M.</name></creator><creator><name>Costantin L.,Garcia-Argumanez A.</name></creator><creator><name>McGrath E.J.</name></creator><creator><name>Merida R.M.</name></creator><creator><name>Zavala J.A.</name></creator><creator><name>Haro P.A.,Bagley M.B.</name></creator><creator><name>Backhaus B.E.</name></creator><creator><name>Behroozi P.</name></creator><creator><name>Bell E.F.</name></creator><creator><name>Bisigello L.</name></creator><creator><name>Buat V.,Calabro A.</name></creator><creator><name>Casey C.M.</name></creator><creator><name>Cleri N.J.</name></creator><creator><name>Coogan R.T.</name></creator><creator><name>Cooper M.C.</name></creator><creator><name>Cooray A.R.,Dekel A.</name></creator><creator><name>Dickinson M.</name></creator><creator><name>Elbaz D.</name></creator><creator><name>Ferguson H.C.</name></creator><creator><name>Finkelstein S.L.,Fontana A.</name></creator><creator><name>Franco M.</name></creator><creator><name>Gardner J.P.</name></creator><creator><name>Giavalisco M.</name></creator><creator><name>Gomez-Guijarro C.,Grazian A.</name></creator><creator><name>Grogin N.A.</name></creator><creator><name>Guo Y.</name></creator><creator><name>Huertas-Company M.</name></creator><creator><name>Jogee S.,Kartaltepe J.S.</name></creator><creator><name>Kewley L.J.</name></creator><creator><name>Kirkpatrick A.</name></creator><creator><name>Kocevski D.D.,Koekemoer A.M.</name></creator><creator><name>Long A.S.</name></creator><creator><name>Lotz J.M.</name></creator><creator><name>Lucas R.A.</name></creator><creator><name>Papovich C.</name></creator><creator><name>Pirzkal N.,Ravindranath S.</name></creator><creator><name>Somerville R.S.</name></creator><creator><name>Tacchella S.</name></creator><creator><name>Trump J.R.</name></creator><creator><name>Wang W.,Wilkins S.M.</name></creator><creator><name>Wuyts S.</name></creator><creator><name>Yang G.</name></creator><creator><name>Aaron Yung L.Y.</name></creator><date role="Updated">2025-06-02T07:05:25Z</date><date role="Created">2025-04-09T15:29:05Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>galaxies</subject><subject>infrared-sources</subject><subject>infrared-photometry</subject><subject>redshifted</subject><subject>stellar-masses</subject><description>The new capabilities that JWST offers in the near- and mid-infrared (IR) are used to investigate in unprecedented detail the nature of optical/near-IR-faint, mid-IR-bright sources, with HST-dark galaxies among them. We gather JWST data from the CEERS survey in the Extended Groth Strip, jointly with HST data, and analyze spatially resolved optical-to-mid-IR spectral energy distributions to estimate photometric redshifts in two dimensions and stellar population properties on a pixel-by-pixel basis for red galaxies detected by NIRCam. We select 138 galaxies with F150W-F356W&gt;1.5mag and F356W&lt;27.5mag. The nature of these sources is threefold: (1) 71% are dusty star-forming galaxies (SFGs) at 2&lt;z&lt;6 with 9&lt;logM_*_/M_{sun}_&lt;11 and a variety of specific SFRs (&lt;1 to &gt;100 Gyr-1); (2) 18% are quiescent/dormant (i.e., subject to reignition/rejuvenation) galaxies (QGs) at 3&lt;z&lt;5, with logM_*_/M_{sun}_~10 and poststarburst mass-weighted ages (0.5-1.0Gyr); and (3) 11% are strong young starbursts with indications of high equivalent width emission lines (typically, [OIII]+H{beta}) at 6&lt;z&lt;7 (XELG-z6) and logM_*_/M_{sun}_~9.5. The sample is dominated by disk-like galaxies with remarkable compactness for XELG-z6 (effective radii smaller than 0.4kpc). Large attenuations in SFGs, 2&lt;A(V)&lt;5mag, are found within 1.5 times the effective radius, approximately 2kpc, while QGs present A(V) ~0.2mag. Our SED-fitting technique reproduces the expected dust emission luminosities of IR-bright and submillimeter galaxies. This study implies high levels of star formation activity between z~20 and z~10, where virtually 100% of our galaxies had already formed 10^8^M_{sun}_, 60% had assembled 10^9^M_{sun}_, and 10% up to 10^10^M_{sun}_ (in situ or ex situ).</description><source format="bibcode">2023ApJ...946L..16P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/946/L16</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/B/hst">B/hst : HST Archived Exposures Catalog (STScI, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/337">I/337 : Gaia DR1 (Gaia Collaboration, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/338/508">J/MNRAS/338/508 : Phot+spectroscopy of UCM galaxies (Perez-Gonzalez+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/622/772">J/ApJ/622/772 : Redshift survey of submillimeter galaxies (Chapman+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/675/234">J/ApJ/675/234 : Stellar mass functions for z&lt;4 gal. 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