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<ri:Resource created="2021-04-07T10:35:46Z" 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>Lockman Hole Apertif map at 1.4GHz</title><shortName>J/A+A/648/A9</shortName><identifier>ivo://CDS.VizieR/J/A+A/648/A9</identifier><altIdentifier>doi:10.26093/cds/vizier.36480009</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Morganti R.</name></creator><creator><name>Oosterloo T.A.</name></creator><creator><name>Brienza M.</name></creator><creator><name>Jurlin N.</name></creator><creator><name>Prandoni I.</name></creator><creator><name>Orru E.,Shabala S.S.</name></creator><creator><name>Adams E.A.K.</name></creator><creator><name>Adebahr B.</name></creator><creator><name>Best P.N.</name></creator><creator><name>Coolen A.H.W.M.,Damstra S.</name></creator><creator><name>de Blok W.J.G.</name></creator><creator><name>de Gasperin F.</name></creator><creator><name>Denes H.</name></creator><creator><name>Hardcastle M.,Hess K.M.</name></creator><creator><name>Hut B.</name></creator><creator><name>Kondapally R.</name></creator><creator><name>Kutkin A.M.</name></creator><creator><name>Loose G.M.</name></creator><creator><name>Lucero D.M.,Maan Y.</name></creator><creator><name>Maccagni F.M.</name></creator><creator><name>Mingo B.</name></creator><creator><name>Moss V.A.</name></creator><creator><name>Mostert R.I.J.</name></creator><creator><name>Norden M.J.,Oostrum L.C.</name></creator><creator><name>Roettgering H.J.A.</name></creator><creator><name>Ruiter M.</name></creator><creator><name>Shimwell T.W.</name></creator><creator><name>Schulz R.,Vermaas N.J.</name></creator><creator><name>Vohl D.</name></creator><creator><name>van der Hulst J.M.</name></creator><creator><name>van Diepen G.M.</name></creator><creator><name>van Leeuwen J.,Ziemke J.</name></creator><date role="Updated">2021-09-16T09:12:59Z</date><date role="Created">2021-04-07T10:35:46Z</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-sources</subject><description>Supermassive black holes at the centres of galaxies can cycle through periods of activity and quiescence. Characterising the duty cycle of active galactic nuclei (AGN) is crucial for understanding the impact of the energy they release on the host galaxy. For radio AGN, this can be done by identifying dying (remnant) and restarted radio galaxies from their radio spectral properties. Using the combination of the images at 1400MHz produced by Apertif, the new phased-array feed receiver installed on the Westerbork Synthesis Radio Telescope, and images at 150MHz provided by LOFAR, we have derived resolved spectral index images (at a resolution of 15 arcsec) for all the sources within an approximately 6 deg^2^ area of the Lockman Hole region. In this way, we were able to select 15 extended radio sources with emission (partly or entirely) characterised by extremely steep spectral indices (steeper than 1.2). These objects represent cases of radio sources in the remnant or the restarted phases of their life cycle. Our findings confirm that these objects are not as rare as previously thought, suggesting a relatively fast cycle. They also show a variety of properties that can be relevant for modelling the evolution of radio galaxies. For example, the restarted activity can occur while the remnant structure from a previous phase of activity is still visible. This provides constraints on the duration of the 'off' (dying) phase. In extended remnants with ultra-steep spectra at low frequencies, the activity likely stopped a few hundred megayears ago, and they correspond to the older tail of the age distribution of radio galaxies, in agreement with the results of simulations of radio source evolution. We find remnant radio sources with a variety of structures (from double-lobed to amorphous), possibly suggesting different types of progenitors. The present work sets the stage for exploiting the powerful tool of low-frequency spectral index studies of extended sources by taking advantage of the large areas common to the LOFAR and the Apertif surveys.</description><source format="bibcode">2021A&amp;A...648A...9M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/648/A9</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/A+A/329/482">J/A+A/329/482 : ROSAT Deep Survey in the Lockman Hole (Hasinger+, 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/53/445">J/PASJ/53/445 : ASCA Deep survey in Lockman Hole Field (Ishisaki+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/393/425">J/A+A/393/425 : Spectral analysis of Lockman Hole (Mainieri+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/398/901">J/A+A/398/901 : VLA survey at 6 cm in the Lockman Hole (Ciliegi+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/125/2521">J/AJ/125/2521 : 2MASS6x survey of the Lockman Hole (Beichman+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/413/843">J/A+A/413/843 : Far IR survey in the Lockman Hole (Kawara+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/427/23">J/A+A/427/23 : 14.3um survey in the Lockman Hole (Fadda+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/427/773">J/A+A/427/773 : ISOCAM 14.3{mu}m Deep Survey in Lockman Hole</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/479/283">J/A+A/479/283 : XMM observations of the Lockman Hole (Brunner+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/387/1037">J/MNRAS/387/1037 : 610-MHz survey of Lockman Hole with GMRT (Garn+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/397/281">J/MNRAS/397/281 : Radio imaging in Lockman Hole (Ibar+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/185/433">J/ApJS/185/433 : SWIRE/Chandra survey in Lockman Hole Field (Wilkes+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/198/1">J/ApJS/198/1 : Photometry catalogs for the Lockman Hole (Fotopoulou+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/BASI/38.103">J/other/BASI/38.103 : 6Lockman Hole 10-MHz survey with GMRT. II. (Garn+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/551/A97">J/A+A/551/A97 : Lockman Hole/XMM VLBI observations (Middelberg+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/462/2934">J/MNRAS/462/2934 : Lockman Hole North 3GHz catalogue (Vernstrom+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/463/2997">J/MNRAS/463/2997 : Lockman Hole low-frequency radio sources (Mahony+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/429/2080">J/MNRAS/429/2080 : Lockman Hole 10C sources radio spectral indices</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/856/67">J/ApJ/856/67 : Lockman Hole VLA 3GHz radio source catalog (Cotton+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/495/4084">J/MNRAS/495/4084 : Lockman Hole region 325MHz source catalog (Mazumder+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/622/A1">J/A+A/622/A1 : LOFAR Two-metre Sky Survey DR1 source catalog</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/648/A2">J/A+A/648/A2 : LOFAR Two-metre Sky Survey Deep Fields DR1 (Sabater+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/648/A3">J/A+A/648/A3 : LOFAR Two-metre Sky Survey Deep Fields DR1 (Kondapally+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/648/A4">J/A+A/648/A4 : LoTSS Deep Fields DR1 photometric redshifts (Duncan+, 2021)</relatedResource><relatedResource>https://lofar-surveys.org/releases.html : LOFAR Home Page</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/648/A9</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/648/A9</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/648/A9</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/648/A9</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/648/A9</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/648/A9</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/A+A/648/A9/list (Information of fits map)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/648/A9/list?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/648/A9/list?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/648/A9/list?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>163.49928</ra><dec>57.8455</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/6112</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/648/A9?format=ascii</footprint><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/648/A9/list</name><description>Information of fits map</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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