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<ri:Resource created="2009-09-03T09:46:17Z" 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>2LC Compact Radio Sources in the galactic center</title><shortName>J/ApJS/174/481</shortName><identifier>ivo://CDS.VizieR/J/ApJS/174/481</identifier><altIdentifier>doi:10.26093/cds/vizier.21740481</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lazio T.J.W.</name></creator><creator><name>Cordes J.M.</name></creator><date role="Updated">2017-12-15T10:54:42Z</date><date role="Created">2009-09-03T09:46:17Z</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>astronomical-object-identification</subject><subject>pulsars</subject><subject>radio-sources</subject><description>We have used the VLA at 1.4GHz to survey the inner 2{deg} of the Galactic center for radio pulsar candidates. Because of the large pulse broadening suffered by Galactic center radio pulsars, our strategy has been to identify compact radio sources, without regard to whether they are pulsed radio sources. We describe our survey and present the catalog of 170 sources. Comparison with other radio surveys of the area shows that just over half of these sources have not been detected previously; this same comparison reveals 29 sources that are not in higher frequency surveys, suggesting that the sources are either variable or steep spectrum, and a comparable number of sources in other surveys that should have been detected in this survey but were not. Comparison with infrared surveys shows that 59 (35%) sources have infrared counterparts and are likely to be HII regions.</description><source format="bibcode">2008ApJS..174..481L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/174/481</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/VIII/42">VIII/42 : Texas Survey of radio sources at 365MHz (Douglas+ 1996)</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/J/ApJS/74/181">J/ApJS/74/181 : Small-diameter radiosources catalogue (Zoonematkermani+, 1990)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/91/347">J/ApJS/91/347 : A 5-GHz VLA Survey of the Galactic Plane (Becker+ 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/136/571">J/A+AS/136/571 : Pulsars identified from the NRAO VLA Sky Survey (Han+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/128/1646">J/AJ/128/1646 : The Galactic Center region at 330MHz (Nord+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/171/376">J/ApJS/171/376 : MOJAVE. 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