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<ri:Resource created="2005-06-15T17:30:44Z" 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>Blazar counterparts for 3EG sources</title><shortName>J/ApJ/609/564</shortName><identifier>ivo://CDS.VizieR/J/ApJ/609/564</identifier><altIdentifier>doi:10.26093/cds/vizier.16090564</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sowards-Emmerd D.</name></creator><creator><name>Romani R.W.</name></creator><creator><name>Michelson P.F.</name></creator><creator><name>Ulvestad J.S.</name></creator><date role="Updated">2018-01-05T08:56:20Z</date><date role="Created">2005-06-15T17:30:44Z</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>bl-lacertae-objects</subject><subject>active-galactic-nuclei</subject><subject>redshifted</subject><subject>radio-sources</subject><subject>gamma-ray-astronomy</subject><description>Supplementing existing survey data with Very Large Array (VLA) observations, we have extended {gamma}-ray counterpart identifications down to decl.=-40{deg} using our "figure-of-merit" approach. We find blazar counterparts for 70% of EGRET sources above decl.=-40{deg} away from the Galaxy. Spectroscopic confirmation is in progress, and spectra for 24 sources are presented here. We find evidence that increased exposure in the bulge region allowed EGRET to detect relatively faint blazars; a clear excess of nonblazar objects in this region, however, argues for an additional (new) source class.</description><source format="bibcode">2004ApJ...609..564S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/609/564</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/J/ApJS/123/79">J/ApJS/123/79 : Third EGRET catalog (3EG) (Hartman+, 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Figure of Merit (4)</description><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>f_FoM</name><description>[)] Flag on FoM (2)</description><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>z</name><description>? Redshift (from optical observations)</description><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>PID</name><description>PID, remarks on Redshift (5)</description><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>RID</name><description>? Radio data origin (6)</description><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Mattox</name><description>[+-] Mattox et al. (2001, Cat. &lt;J/ApJS/135/155&gt;) selected blazars (7)</description><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>EGRET</name><description>[Aa] Third EGRET catalog (1999, Cat. &lt;J/ApJS/123/79&gt;) blazars (8)</description><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Class</name><description>Classification of the source (9)</description><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>f_Class</name><description>[)] Flag on Class (2)</description><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>3EGdat</name><description>Details from 3EG Catalog (J/ApJS/123/79) about this source</description><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Position from the 3EG catalog (J/ApJS/123/79) (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Position from the 3EG catalog (J/ApJS/123/79) (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/ApJ/609/564/table2</name><description>VLA A-Array 8.4GHz Observations</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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