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<ri:Resource created="2001-09-22T21:04:31Z" 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>QSOs in 2MASS second incremental data release</title><shortName>J/AJ/121/2843</shortName><identifier>ivo://CDS.VizieR/J/AJ/121/2843</identifier><altIdentifier>doi:10.26093/cds/vizier.51212843</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Barkhouse W.A.</name></creator><creator><name>Hall P.B.</name></creator><date role="Updated">2023-04-06T16:50:42Z</date><date role="Created">2001-09-22T21:04:31Z</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>radio-sources</subject><subject>infrared-photometry</subject><description>Using the 2MASS Second Incremental Data Release (Cat. &lt;B/2mass&gt;), we have searched for near-infrared counterparts to 13214 quasars from the Veron-Cetty &amp; Veron (Cat. &lt;VII/215&gt;) catalog. We have detected counterparts within 4" for 2277 of the approximately 6320 quasars within the area covered by the 2MASS Second Incremental Data Release. Only 1.6% of these are expected to be chance coincidences. Though this sample is heterogeneous, we find that known radio-loud quasars are more likely to have large near-infrared-to-optical luminosity ratios than radio-quiet quasars are, at a statistically significant level. This is consistent with dust-reddened quasars being more common in radio-selected samples than in optically selected samples, due to stronger selection effects against dust-reddened quasars in the latter. We also find a statistically significant dearth of optically luminous quasars with large near-infrared-to-optical luminosity ratios. This can be explained in a dust obscuration model but not in a model where synchrotron emission extends from the radio into the near-infrared and creates such large ratios. We also find that selection of quasar candidates from the B-J/J-K color-color diagram, modeled on the V-J/J-K selection method of Warren, Hewett, &amp; Foltz, is likely to be more sensitive to dust-obscured quasars than selection using only infrared-infrared colors.</description><source format="bibcode">2001AJ....121.2843B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/121/2843</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/VII/215">VII/215 : Quasars and Active Galactic Nuclei (9th Ed.) 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34691 34693 34696 34699 34715 34739 34746-34747 34758 34763 34770 34777 34781 34803 34808 35141-35142 35146 35153 35235 35241-35244 35246-35247 35294 35322 35327 35445 35557-35559 35565 35600 35602-35603 35607-35608 35611 35615 35632 35634-35636 35647 35651 35657 35666 35671 35679 35686 35702 35704 35706 35724-35726 35728-35729 35731 35734 35737 35741 35743 35756 35758 35764-35765 35787 35801 35806 35813 35816 35825 35833 35836 35867-35868 35893 35898 35901 35906-35907 35924 35927 35932 35945 35957 35960 35968-35969 35975 35981 35986-35987 35992-35994 35996-35998 36005 36011 36019-36020 36073-36075 36079 36086 36100-36101 36105 36111 36113 36123 36126 36130 36132 36139 36141-36142 36151 36160 36178-36179 36186 36188 36209 36211 36214 36230 36235 36241 36259-36261 36265 36268 36276 36281 36304 36313 36343 36346 36353 36355 36373 36383 36411 36414 36420 36423 36427 36443 36451 36457-36459 36467 36480 36495-36496 36505 36513 36516 36522 36528 36533 36550-36551 36554 36571 36648 36655 36658 36694 36717 36769 36771 36779 36788 36824 36828-36829 36834 36836 36840 36851-36853 36855 36857-36859 37385 37510 37547 38775 38871 38905 38911 38916 39664 40213 40219-40220 40255 40261 40263 40277 40289 40296 40307 40331 40340 40343-40344 40351 40360 40404 40407 40443 40446 40527 40533 40547 40658 40730 40762 40788 40809 40823 40825 40838 40931 42814 42901 42980 43501 43837 43870 43888 43894-43895 43900 43903 43925 43957 43964 43966-43967 44028 44075 44106 44258 44267 44269 44281-44282 44310 44330 44523 44553 44574 44584-44585 44587 44596 44629 44668 44670 44672-44673 44676 44679 44684 44690 44717 44724 44729 44764 44776 44779 44785 44788 44794 44805 44807 44832 44837 44933 44938 45032 45039 46299 46322 46326-46327 46331 46499 46501-46502 46547 46556 46559 46566 46570 46572 46581 46623 46658 46662 46666 46674-46675 46685 46692 46705 46708 46717 46836 46839 46850 46869 46881-46883 46921 46943 46948 46964-46965 46970 46972-46973 46975 47001-47002 47006-47007 47014 47016 47047 47054 47057 47067-47068 47080 47091 47095 47100 47481 47540 47542 47559 47567-47568 47570 47573 48149 48154 48158 48165-48167 48169-48170 48173-48175 48178 48181-48182 48185 48213 48228 48256-48257 48259-48262 48268 48280 48320 48337 48346 48362 48370 48389 48395 48406-48407 48420 48422 48437 48440 48455 48459 48464 48466-48467 48476 48478-48479 48488-48489 48508 48513 48529-48530 48542 48581 48595 48605 48692 48707 48714 48719 48737-48738 48797-48798 48846 48849 48858 49042 49048 49125 49127</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/121/2843?format=ascii</footprint><waveband>Infrared</waveband><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/121/2843/table1</name><description>VV00 Quasars Detected in 2MASS</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>f_2MASS</name><description>[*] Indicates an object having two 2MASS counterparts within 4''.</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>2MASS</name><description>The 2MASS identification</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="14*">char</dataType></column><column><name>VV00</name><description>Name entries of Veron-Cetty &amp; Veron 2000 (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension in degrees (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination in degrees (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>LNIR</name><description>Log of the NIR luminosity</description><unit>log(Jy)</unit><ucd>phys.luminosity;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Lopt</name><description>Log of the Optical luminosity</description><unit>log(Jy)</unit><ucd>phys.luminosity;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>bmag</name><description>The b_m_ band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rmag</name><description>The r_m_ band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Jmag</name><description>The J band magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Jmag</name><description>Uncertainty in Jmag</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Hmag</name><description>The H band magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Hmag</name><description>Uncertainty in Hmag</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Kmag</name><description>The K band magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Kmag</name><description>Uncertainty in Kmag</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BMag</name><description>Absolute B band magnitude (2)</description><unit>mag</unit><ucd>phys.magAbs;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dis</name><description>Distance to the associated optical source</description><unit>arcsec</unit><ucd>meta.id.assoc;pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Radio</name><description>? Flux density at 6 cm (3)</description><unit>Jy</unit><ucd>phot.flux.density;em.radio.3-6GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>z</name><description>Redshift (2)</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/AJ/121/2843/table2</name><description>VV00 Quasars With Only Upper Limits in 2MASS</description><column><name>z</name><description>Redshift</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>VV00</name><description>Name entry of Veron-Cetty &amp; Veron (2000) (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension in degrees (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination in degrees (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Lopt</name><description>Log of the optical luminosity</description><unit>log(Jy)</unit><ucd>phys.luminosity;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Radio</name><description>? Flux density measured at 6 cm (2)</description><unit>Jy</unit><ucd>phot.flux.density;em.radio.3-6GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>