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<ri:Resource created="2022-06-28T14:25:40Z" 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>Head-tail radio galaxies from the VLA FIRST survey</title><shortName>J/ApJS/259/31</shortName><identifier>ivo://CDS.VizieR/J/ApJS/259/31</identifier><altIdentifier>doi:10.26093/cds/vizier.22590031</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sasmal T.K.</name></creator><creator><name>Bera S.</name></creator><creator><name>Pal S.</name></creator><creator><name>Mondal S.</name></creator><date role="Updated">2022-09-05T14:32:03Z</date><date role="Created">2022-06-28T14:25:40Z</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>radio-galaxies</subject><subject>redshifted</subject><subject>radio-continuum-emission</subject><subject>surveys</subject><description>The head-tail (HT) morphology of radio galaxies is seen for a class of radio sources where the primary lobes are being bent in the intercluster weather due to strong interactions between the radio jets and their respective intracluster medium. A systematic search has been carried out for new HT radio galaxies from the Very Large Array Faint Images of the Radio Sky at Twenty-Centimeters survey database at 1400MHz. Here, we present a catalog of 717 new HT sources, among which 287 are narrow-angle tail (NAT) sources whose opening angle between the two lobes is less than 90{deg}, and 430 are wide-angle tail (WAT) whose the opening angle between the two lobes is greater than 90{deg}. NAT radio sources are characterized by tails bent in a narrow "V"-like shape; the jet bending in the case of WAT radio galaxies are such that the WATs exhibit wide "C"-like morphologies. Optical counterparts are found for 359 HT sources. We report HT sources with luminosity ranges 10^38^&lt;=L_1.4GHz_&lt;=10^45^erg/s and redshifts up to 2.01. The various physical properties of these HT sources are mentioned here. Some statistical studies have been done for this large number of newly discovered HT sources.</description><source format="bibcode">2022ApJS..259...31S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/259/31</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/1">VIII/1 : The 3C and 3CR Catalogues (Edge+ 1959-1962)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/4">VIII/4 : Fourth Cambridge Survey (4C) (Pilkington+ 1965; Gower+ 1967)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/36">VIII/36 : The Second Bologna Survey (Colla+ 1970-1974)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/18">VIII/18 : 6C Survey of radio sources I. 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