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<ri:Resource created="2022-02-02T12:33:19Z" 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>X-ray weak quasars from SDSS &amp; Chandra</title><shortName>J/ApJ/900/141</shortName><identifier>ivo://CDS.VizieR/J/ApJ/900/141</identifier><altIdentifier>doi:10.26093/cds/vizier.19000141</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Pu X.</name></creator><creator><name>Luo B.</name></creator><creator><name>Brandt W.N.</name></creator><creator><name>Timlin J.D.</name></creator><creator><name>Liu H.</name></creator><creator><name>Ni Q.</name></creator><creator><name>Wu J.</name></creator><date role="Updated">2022-05-18T12:46:57Z</date><date role="Created">2022-02-02T12:33:19Z</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>quasars</subject><subject>x-ray-sources</subject><subject>redshifted</subject><subject>surveys</subject><subject>active-galactic-nuclei</subject><description>We investigate systematically the X-ray emission from type 1 quasars using a sample of 1825 Sloan Digital Sky Survey non-broad absorption line (non-BAL) quasars with Chandra archival observations. A significant correlation is found between the X-ray-to-optical power-law slope parameter ({alpha}_OX_) and the 2500{AA} monochromatic luminosity (L_2500{AA}_), and the X-ray weakness of a quasar is assessed via the deviation of its {alpha}_OX_ value from that expected from this relation. We demonstrate the existence of a population of non-BAL X-ray-weak quasars, and the fractions of quasars that are X-ray weak by factors of &gt;=6 and &gt;=10 are 5.8%+/-0.7% and 2.7%+/-0.5%, respectively. We classify X-ray-weak quasars (X-ray weak by factors of &gt;=6) into three categories based on their optical spectral features: weak emission-line quasars (WLQs; CIV rest-frame equivalent width &lt;16{AA}), red quasars ({Delta}(g-i)&gt;0.2), and unclassified X-ray-weak quasars. The X-ray-weak fraction of 35_-9_^+12^% within the WLQ population is significantly higher than that within non-WLQs, confirming previous findings that WLQs represent one population of X-ray-weak quasars. The X-ray-weak fraction of 13_-3_^+5^% within the red quasar population is also considerably higher than that within the normal quasar population. The unclassified X-ray-weak quasars do not have unusual optical spectral features, and their X-ray weakness may be mainly related to quasar X-ray variability.</description><source format="bibcode">2020ApJ...900..141P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/900/141</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/65">VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/294">II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/260">VII/260 : The SDSS-DR7 quasar catalog (Schneider+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/90">VIII/90 : The FIRST Survey Catalog, Version 12Feb16 (Becker+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/270">VII/270 : SDSS quasar catalog: tenth data release (Paris+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/147">V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/289">VII/289 : SDSS quasar catalog, sixteenth data release (DR16Q) (Lyke+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/92/53">J/ApJS/92/53 : Einstein database of quasars. 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Lower uncertainty on CtsBB</description><unit>ct</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_CtsBB</name><description>[2.7/41]? Upper uncertainty on CtsBB</description><unit>ct</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>CtsSB</name><description>[1.9/721] Soft-band (0.5-2keV) net counts in source region (2)</description><unit>ct</unit><ucd>phot.count;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_CtsSB</name><description>[1.3/29.1]? Lower uncertainty on CtsSB</description><unit>ct</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_CtsSB</name><description>[2.7/30.1]? Upper uncertainty on CtsSB</description><unit>ct</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>CtsHB</name><description>[1.9/212.8] Hard-band (2-7keV) net counts in source region (2)</description><unit>ct</unit><ucd>phot.count;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_CtsHB</name><description>[1.3/22.4]? Lower uncertainty on CtsHB</description><unit>ct</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_CtsHB</name><description>[2.7/23.6]? Upper uncertainty on CtsHB</description><unit>ct</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BRatio</name><description>[0.04/10.25]? Band ratio, hard-band to soft-band counts (3)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_BRatio</name><description>[0.02/9]? Lower uncertainty on BRatio</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_BRatio</name><description>[0.03/84]? Upper uncertainty on BRatio</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Gamma</name><description>[-1.4/4] 0.5-7keV effective power-law photon index (4)</description><ucd>meta.code;spect.index;em.X-ray.medium</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Gamma</name><description>[0.1/4.6]? Lower uncertainty on Gamma</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_Gamma</name><description>[0.1/2.3]? Upper uncertainty on Gamma</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SamC</name><description>[0/1] Member of sample C (5)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>iMag</name><description>[-29.7/-22.8] Absolute i-band magnitude</description><unit>mag</unit><ucd>phys.magAbs;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F2keV</name><description>[0.01/95] Rest-frame 2keV flux density, 10^-32^erg/cm^2^/s/Hz (6)</description><unit>1e-32mW.m**-2.Hz**-1</unit><ucd>phot.flux;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F0.5-7</name><description>[0.1/54] Observed-frame 0.5-7keV flux, 10^-14^erg/cm^2^/s (7)</description><unit>1e-14mW.m**-2</unit><ucd>phot.flux;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logLX</name><description>[43.2/46] Logarithm of the rest-frame 2-10 keV luminosity, erg/s (7)</description><unit>1e-07W</unit><ucd>phys.luminosity;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F2500</name><description>[0.02/12.4] Rest-frame 2500{AA} flux density, 10^-27^erg/cm^2^/s/Hz</description><unit>1e-27mW.m**-2.Hz**-1</unit><ucd>phot.flux.density</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>aOX</name><description>[-2.5/-0.9] Measured X-ray-to-optical power-law slope (6)</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DaOX</name><description>[-1/0.43] Difference between the measured and expected aOX (8)</description><ucd>stat.fit.residual</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>fweak</name><description>[0.1/415] X-ray weakness factor measured from DaOX</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>REW</name><description>[0.9/479.1] Rest-frame equivalent width, CIV1549{AA} emission line</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>D(g-i)</name><description>[-0.97/2.67] Relative g-i color index</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>R</name><description>[1.3/247.2] Radio-loudness parameter (9)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>XWeak</name><description>[0/1] X-ray weak flag (10)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>l_CtsHB</name><description>Limit flag on CtsHB (2)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>l_F2keV</name><description>Limit flag for f2keV</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>l_F0.5-7</name><description>Limit flag for F0.5-7</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>l_logLX</name><description>Limit flag for logLX</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>l_aOX</name><description>Limit flag for aOX</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>l_DaOX</name><description>Limit flag for DaOX</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>l_fweak</name><description>Limit flag for fweak</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>l_R</name><description>Limit flag on R</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Sloan</name><description>Display the online SDSS-DR14 data for the nearest object</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table></schema></tableset></ri:Resource>