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<ri:Resource created="2021-06-09T11:38:58Z" status="active" updated="2025-05-19T09:50:00Z" 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>SUPER GOODS. IV. 850um data of CDFS X-ray sources</title><shortName>J/ApJ/887/23</shortName><identifier>ivo://CDS.VizieR/J/ApJ/887/23</identifier><altIdentifier>doi:10.26093/cds/vizier.18870023</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Barger A.J.</name></creator><creator><name>Cowie L.L.</name></creator><creator><name>Bauer F.E.</name></creator><creator><name>Gonzalez-Lopez J.</name></creator><date role="Updated">2021-07-05T12:53:36Z</date><date role="Created">2021-06-09T11:38:58Z</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>active-galactic-nuclei</subject><subject>millimeter-astronomy</subject><subject>photometry</subject><subject>submillimeter-astronomy</subject><subject>x-ray-sources</subject><subject>redshifted</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>infrared-sources</subject><description>The Chandra Deep Field (CDF)-S is the deepest X-ray image available and will remain so for the near future. We provide a spectroscopic (64.5%; 64% with spectral classifications) and photometric redshift catalog for the full 7Ms sample, but much of our analysis focuses on the central (off-axis angles &lt;5.7') region, which contains a large, faint ALMA sample of 75 &gt;4.5{sigma} 850{mu}m sources. We measure the 850{mu}m fluxes at the X-ray positions using the ALMA images, where available, or an ultradeep SCUBA-2 map. We find that the full X-ray sample produces ~10% of the 850{mu}m extragalactic background light. We separate the submillimeter-detected X-ray sources into star-forming galaxies and active galactic nuclei (AGNs) using a star formation rate (SFR) versus X-ray luminosity calibration for high-SFR galaxies. We confirm this separation using the X-ray photon indices. We measure the X-ray fluxes at the accurate positions of the 75 ALMA sources and detect 70% at &gt;3{sigma} in either the 0.5-2 or 2-7keV bands. However, many of these may produce both their X-ray and submillimeter emission by star formation. Indeed, we find that only 20% of the ALMA sources have intermediate X-ray luminosities (rest-frame 8-28 keV luminosities of 10^42.5^-10^44^erg/s), and none has a high X-ray luminosity (&gt;10^44^erg/s). Conversely, after combining the CDF-S with the CDF-N, we find extreme star formation (SFR&gt;300M_{sun}_/yr) in some intermediate X-ray luminosity sources but not in any high X-ray luminosity sources. We argue that the quenching of star formation in the most luminous AGNs may be a consequence of the clearing of gas in these sources.</description><source format="bibcode">2019ApJ...887...23B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/887/23</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/chandra">B/chandra : The Chandra Archive Log (CXC, 1999-2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/250">III/250 : The VIMOS VLT deep survey (VVDS-DEEP) (Le Fevre+ 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/126/539">J/AJ/126/539 : The Chandra Deep Fields North and South (Alexander+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/155/271">J/ApJS/155/271 : CDF-South: Optical spectroscopy (Szokoly+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/437/883">J/A+A/437/883 : K20 survey: spectroscopic catalogue (Mignoli+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/478/83">J/A+A/478/83 : GOODS-South Field VLT/FORS2 redshifts. 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