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<ri:Resource created="2020-10-13T10:29:30Z" 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>Sources detected at 325 and 610 MHz in Cygnus</title><shortName>J/A+A/642/A136</shortName><identifier>ivo://CDS.VizieR/J/A+A/642/A136</identifier><altIdentifier>doi:10.26093/cds/vizier.36420136</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Benaglia P.</name></creator><creator><name>Ishwara-Chandra C.H.</name></creator><creator><name>Intema H.</name></creator><creator><name>Colazo M.E.</name></creator><creator><name>Gaikwad M.</name></creator><date role="Updated">2021-04-27T11:58:14Z</date><date role="Created">2020-10-13T10:29:30Z</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-continuum-emission</subject><subject>radio-sources</subject><description>Observations at the radio continuum band below the gigahertz band are key when the nature and properties of non-thermal sources are investigated because their radio radiation is strongest at these frequencies. The low radio frequency range is therefore the best to spot possible counterparts to very high-energy (VHE) sources: relativistic particles of the same population are likely to be involved in radio and high-energy radiation processes. Some of these counterparts to VHE sources can be stellar sources. The Cygnus region in the northern sky is one of the richest in this type of sources that are potential counterparts to VHEsources. We surveyed the central ~15 sq deg of the Cygnus constellation at the 325 and 610MHz bands with angular resolutions and sensitivities of 10" and 6", and 0.5 and 0.2mJy/beam, respectively. The data were collected during 172 hours in 2013-2017, using the Giant Metrewave Radio Telescope (GMRT) with 32MHz bandwidth, and were calibrated using the SPAM routines. The source extraction was carried out with the PyBDSF tool,followed by verification through visual inspection of every putative catalog candidate source in order to determine its reliability. In this first paper we present the catalog of sources, consisting of 1048 sources at 325MHz and 2796 sources at 610MHz. By cross-matching the sources from both frequencies with the objects of the SIMBAD database, we found possible counterparts for 143 of them. Most of the sources from the 325MHz catalog (993) were detected at the 610MHz band, and their spectral index alpha was computed adopting S(nu){prop.to}nu^alpha^. The maximum of the spectral index distribution is at alpha=-1, which is characteristic of non-thermal emitters and might indicate an extragalactic population.</description><source format="bibcode">2020A&amp;A...642A.136B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/642/A136</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/AJ/107/1433">J/AJ/107/1433 : Cygnus OB2 polarimetry (Kobulnicky+, 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/643/238">J/ApJ/643/238 : Chandra/2MASS sources in Cygnus OB2 (Butt+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/464/211">J/A+A/464/211 : Cyg OB2 Chandra and near-IR obs. (Albacete Colombo+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/472/557">J/A+A/472/557 : Cygnus OB2 region 610MHz sources (Marti+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/184/84">J/ApJS/184/84 : X-ray sources in Cyg OB2 region (Wright+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/713/871">J/ApJ/713/871 : X-ray sources in star-forming region Cyg-OB2 (Wright+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/202/19">J/ApJS/202/19 : riz photometry in Cyg OB2 (Guarcello+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/460/2593">J/MNRAS/460/2593 : Cygnus OB2 DANCe: Proper motion study (Wright+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/603/A106">J/A+A/603/A106 : Rotational periods in Cygnus OB2 (Roquette+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/612/A50">J/A+A/612/A50 : New massive members of Cygnus OB2 (Berlanas+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/484/1838">J/MNRAS/484/1838 : Spatial substructure of Cygnus OB2 (Berlanas+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/637/A64">J/A+A/637/A64 : Cygnus OB2 e-MERLIN 21cm survey (COBRaS) (Morford+, 2020)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/642/A136</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/642/A136</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/642/A136</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL 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