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<ri:Resource created="2024-11-20T08:51:10Z" 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>New identifications of 4FGL sources with SPT-SZ</title><shortName>J/ApJ/939/117</shortName><identifier>ivo://CDS.VizieR/J/ApJ/939/117</identifier><altIdentifier>doi:10.26093/cds/vizier.19390117</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Zhang L.</name></creator><creator><name>Vieira J.D.</name></creator><creator><name>Ajello M.</name></creator><creator><name>Malkan M.A.</name></creator><creator><name>Archipley M.A.</name></creator><creator><name>Capota J.,Foster A.</name></creator><creator><name>Madejski G.</name></creator><date role="Updated">2025-02-18T20:14:18Z</date><date role="Created">2024-11-20T08:51:10Z</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>gamma-ray-astronomy</subject><subject>millimeter-astronomy</subject><subject>submillimeter-astronomy</subject><subject>radio-sources</subject><subject>surveys</subject><subject>infrared-astronomy</subject><subject>x-ray-sources</subject><subject>astronomical-object-identification</subject><description>The fourth Fermi Large Area Telescope catalog (4FGL) contains 5064 {gamma}-ray sources detected at high significance, but 26% of them still lack associations at other wavelengths. The SPT-SZ survey, conducted between 2008 and 2011 with the South Pole Telescope (SPT), covers 2500deg^2^ of the southern sky in three millimeter-wavelength (mm) bands and was used to construct a catalog of nearly 5000 emissive sources. In this study, we introduce a new cross-matching scheme to search for multiwavelength counterparts of extragalactic {gamma}-ray sources using a mm catalog. We apply a Poissonian probability to evaluate the rate of spurious false associations and compare the multiwavelength associations from the radio, mm, near-infrared, and X-ray with 4FGL {gamma}-ray sources. In the SPT-SZ survey field, 85% of 4FGL sources are associated with mm counterparts. These mm sources include 94% of previously associated 4FGL sources and 56% of previously unassociated 4FGL sources. The latter group contains 40 4FGL sources for which SPT has provided the first identified counterparts. Nearly all of the SPT-associated 4FGL sources can be described as flat-spectrum radio quasars or blazars. We find that the mm band is the most efficient wavelength for detecting {gamma}-ray blazars when considering both completeness and purity. We also demonstrate that the mm band correlates better to the {gamma}-ray band than the radio or X-ray bands. With the next generation of CMB experiments, this technique can be extended to greater sensitivities and more sky area to further complete the identifications of the remaining unknown {gamma}-ray blazars.</description><source format="bibcode">2022ApJ...939..117Z</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/939/117</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/IX/10">IX/10 : ROSAT All-Sky Bright Source Catalogue (1RXS) (Voges+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IX/29">IX/29 : ROSAT All-Sky Survey Faint Source Catalog (Voges+ 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/78">VIII/78 : Sydney University Molonglo Sky Survey (SUMSS) (Mauch+ 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/81">VIII/81 : Sydney University Molonglo Sky Survey (SUMSS V2.1) (Mauch+ 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/328">II/328 : AllWISE Data Release (Cutri+ 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/274">VII/274 : The Roma BZCAT - 5th edition (Massaro+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/380/199">J/MNRAS/380/199 : SCUBA Half-Degree Extragalactic Survey. III (Ivison+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/175/97">J/ApJS/175/97 : CGRaBS: survey of {gamma}-ray blazar cand. (Healey+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/719/763">J/ApJ/719/763 : Millimeter-wave sources in the SPT survey (Vieira+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/413/2314">J/MNRAS/413/2314 : Radio &amp; mid-IR counterpart of submm galaxies (Biggs+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/748/68">J/ApJ/748/68 : WISE IR colors of gamma-ray blazars (D'Abrusco+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/217/4">J/ApJS/217/4 : 2FGL sources observed between 5-9GHz (Schinzel+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/851/33">J/ApJ/851/33 : Multi-wavelength analysis of CGRaBS blazars (Paliya+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/838/139">J/ApJ/838/139 : Radio follow-up on 3FGL unassoc. sources (Schinzel+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/247/33">J/ApJS/247/33 : 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