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<ri:Resource created="2015-12-24T13:47:20Z" 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>NuSTAR surveys: COSMOS catalog</title><shortName>J/ApJ/808/185</shortName><identifier>ivo://CDS.VizieR/J/ApJ/808/185</identifier><altIdentifier>doi:10.26093/cds/vizier.18080185</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Civano F.</name></creator><creator><name>Hickox R.C.</name></creator><creator><name>Puccetti S.</name></creator><creator><name>Comastri A.</name></creator><creator><name>Mullaney J.R.,Zappacosta L.</name></creator><creator><name>Lamassa S.M.</name></creator><creator><name>Aird J.</name></creator><creator><name>Alexander D.M.</name></creator><creator><name>Ballantyne D.R.,Bauer F.E.</name></creator><creator><name>Brandt W.N.</name></creator><creator><name>Boggs S.E.</name></creator><creator><name>Christensen F.E.</name></creator><creator><name>Craig W.W.,Del-Moro A.</name></creator><creator><name>Elvis M.</name></creator><creator><name>Forster K.</name></creator><creator><name>Gandhi P.</name></creator><creator><name>Grefenstette B.W.,Hailey C.J.</name></creator><creator><name>Harrison F.A.</name></creator><creator><name>Lansbury G.B.</name></creator><creator><name>Luo B.</name></creator><creator><name>Madsen K.</name></creator><creator><name>Saez C.,Stern D.</name></creator><creator><name>Treister E.</name></creator><creator><name>Urry M.C.</name></creator><creator><name>Wik D.R.</name></creator><creator><name>Zhang W.</name></creator><date role="Updated">2018-02-12T08:45:34Z</date><date role="Created">2015-12-24T13:47:20Z</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>x-ray-sources</subject><subject>redshifted</subject><subject>astronomical-object-identification</subject><subject>surveys</subject><description>To provide the census of the sources contributing to the X-ray background peak above 10keV, Nuclear Spectroscopic Telescope Array (NuSTAR) is performing extragalactic surveys using a three-tier "wedding cake" approach. We present the NuSTAR survey of the COSMOS field, the medium sensitivity, and medium area tier, covering 1.7deg^2^ and overlapping with both Chandra and XMM-Newton data. This survey consists of 121 observations for a total exposure of ~3Ms. To fully exploit these data, we developed a new detection strategy, carefully tested through extensive simulations. The survey sensitivity at 20% completeness is 5.9, 2.9, and 6.4x10^-14^erg/cm^2^/s in the 3-24, 3-8, and 8-24keV bands, respectively. By combining detections in 3 bands, we have a sample of 91 NuSTAR sources with 10^42^-10^45.5^erg/cm^2^/s luminosities and redshift z=0.04-2.5. Thirty-two sources are detected in the 8-24keV band with fluxes ~100 times fainter than sources detected by Swift-BAT. Of the 91 detections, all but 4 are associated with a Chandra and/or XMM-Newton point-like counterpart. One source is associated with an extended lower energy X-ray source. We present the X-ray (hardness ratio and luminosity) and optical-to-X-ray properties. The observed fraction of candidate Compton-thick active galactic nuclei measured from the hardness ratio is between 13%-20%. We discuss the spectral properties of NuSTAR J100259+0220.6 (ID 330) at z=0.044, with the highest hardness ratio in the entire sample. The measured column density exceeds 10^24^/cm2, implying the source is Compton-thick. This source was not previously recognized as such without the &gt;10keV data.</description><source format="bibcode">2015ApJ...808..185C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/808/185</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/VIII/76">VIII/76 : Leiden/Argentine/Bonn (LAB) Survey of Galactic HI (Kalberla+ 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IX/15">IX/15 : Einstein EMSS Survey (Gioia+ 1990, Stocke+ 1991)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/808/184">J/ApJ/808/184 : NuSTAR surveys: ECDF-S catalog (Mullaney+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/436/3581">J/MNRAS/436/3581 : X-ray observations of Stripe 82 (LaMassa+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/207/19">J/ApJS/207/19 : Swift-BAT 2004-2010 hard X-ray survey (Baumgartner+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/763/111">J/ApJ/763/111 : X-ray spectral analysis of Swift/BAT AGNs (Vasudevan+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/202/6">J/ApJS/202/6 : XDEEP2 survey catalog (Goulding+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/201/30">J/ApJS/201/30 : The Chandra COSMOS survey. 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Error in F8-24 (6)</description><unit>mW.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>HR</name><description>Hardness ratio (7)(8)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b_HR</name><description>Lower bound on HR</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>B_HR</name><description>Upper bound on HR</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BR</name><description>[0/7] Band ratio (7)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b_BR</name><description>Lower bound on BR</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>B_BR</name><description>Upper bound on BR</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RAXdeg</name><description>? X-ray Right Ascension in decimal degrees (J2000) (9)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>nullable</flag></column><column><name>DEXdeg</name><description>? X-ray Declination in decimal degrees (J2000) (9)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag></column><column><name>F0.5-2</name><description>? Aperture corrected 0.5-2 keV band flux; erg/s/cm^2^ (10)</description><unit>mW.m**-2</unit><ucd>phot.flux;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>F2-10</name><description>? The 2-10 keV band flux (10)</description><unit>mW.m**-2</unit><ucd>phot.flux;em.X-ray.medium</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>zsp</name><description>[0.04/2.5]? Spectroscopic redshift (11)</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>n_zsp</name><description>? Classification type for zsp (12)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>zph</name><description>[0.05/2.5]? Photometric redshift (11)</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>n_zph</name><description>? Classification type for zph (13)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>XSep</name><description>[1/26]? NuSTAR position separation (6)(11)</description><unit>arcmin</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Dzsp</name><description>? Luminosity distance using zsp</description><unit>Mpc</unit><ucd>pos.distance;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Dzph</name><description>? Luminosity distance using zph</description><unit>Mpc</unit><ucd>pos.distance;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>logL3-24</name><description>? Log 3-24 keV band luminosity; erg/s</description><unit>log(1e-07W)</unit><ucd>phys.luminosity;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logL3-8</name><description>? Log 3-8 keV band luminosity; erg/s</description><unit>log(1e-07W)</unit><ucd>phys.luminosity;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logL8-24</name><description>? Log 8-24 keV band luminosity; erg/s</description><unit>log(1e-07W)</unit><ucd>phys.luminosity;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Flag</name><description>Multiple low energy counterpart flag (0:False; or 1:True)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table></schema></tableset></ri:Resource>