<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2024-10-10T08:34:17Z" 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>RAdio Galaxy Environment Reference Survey</title><shortName>J/A+A/690/A196</shortName><identifier>ivo://CDS.VizieR/J/A+A/690/A196</identifier><altIdentifier>doi:10.26093/cds/vizier.36900196</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Zhou D.</name></creator><creator><name>Greve T.R.</name></creator><creator><name>Gullberg B.</name></creator><creator><name>Lee M.</name></creator><creator><name>Di Mascolo L.</name></creator><creator><name>Dicker S.R.,Romero C.E.</name></creator><creator><name>Chapman S.C.</name></creator><creator><name>Chen C.-C.</name></creator><creator><name>Cornish T.</name></creator><creator><name>Devlin M.J.</name></creator><creator><name>Ho L.C.,Kohno K.</name></creator><creator><name>Lagos C.D.P.</name></creator><creator><name>Mason B.S.</name></creator><creator><name>Mroczkowski T.</name></creator><creator><name>Wagg J.F.W.</name></creator><creator><name>Wang Q.D.,Wang R.</name></creator><creator><name>Brinch M.</name></creator><creator><name>Dannerbauer H.</name></creator><creator><name>Jiang X.-J.</name></creator><creator><name>Lauritsen L.R.B.,Vijayan A.P.</name></creator><creator><name>Vizgan D.</name></creator><creator><name>Wardlow J.L.</name></creator><creator><name>Sarazin C.L.</name></creator><creator><name>Sarmiento K.P.,Serjeant S.</name></creator><creator><name>Bhandarkar T.A.</name></creator><creator><name>Haridas S.K.</name></creator><creator><name>Moravec E.</name></creator><creator><name>Orlowski-Scherer J.,Sievers J.L.R.</name></creator><creator><name>Tanaka I.</name></creator><creator><name>Wang Y.-J.</name></creator><creator><name>Zeballos M.</name></creator><creator><name>Laza-Ramos A.</name></creator><creator><name>Liu Y.,Hassan M.S.R.</name></creator><creator><name>Jwel A.K.M.</name></creator><creator><name>Nazri A.</name></creator><creator><name>Lim M.K.</name></creator><creator><name>Ibrahim U.F.S.</name></creator><date role="Updated">2025-02-24T20:01:47Z</date><date role="Created">2024-10-10T08:34:17Z</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>galaxy-clusters</subject><subject>radio-galaxies</subject><subject>millimeter-astronomy</subject><subject>submillimeter-astronomy</subject><subject>redshifted</subject><description>High-redshift radio(-loud) galaxies (HzRGs) are massive galaxies with powerful radio-loud active galactic nuclei (AGNs) and serve as beacons for protocluster identification. However, the interplay between HzRGs and the large-scale environment remains unclear. To understand the connection between HzRGs and the surrounding obscured star formation, we investigated the overdensity and spatial distribution of submillimeter-bright galaxies (SMGs) in the field of 4C 23.56, a well-known HzRG at z=2.48. We used SCUBA-2 data ({sigma}~0.6mJy) to estimate the 850um source number counts and examine the radial and azimuthal overdensities of the 850um sources in the vicinity of the HzRG. The angular distribution of SMGs is inhomogeneous around the HzRG 4C 23.56, with fewer sources oriented along the radio jet. We also find a significant overdensity of bright SMGs (S_850um_&gt;=5mJy). Faint and bright SMGs exhibit different spatial distributions. The former are concentrated in the core region, while the latter prefer the outskirts of the HzRG field. High-resolution observations show that the seven brightest SMGs in our sample are intrinsically bright, suggesting that the overdensity of bright SMGs is less likely due to the source multiplicity.</description><source format="bibcode">2024A&amp;A...690A.196Z</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/690/A196</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></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/690/A196</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/690/A196</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/690/A196</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/690/A196</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/690/A196</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/690/A196</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/690/A196/tablea1 (Positions and fluxes of the 850um-selected SMGs (S/N&gt;=4{sigma}))</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/690/A196/tablea1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/690/A196/tablea1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/690/A196/tablea1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>21.12211</ra><dec>23.5147</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/2084</spatial><spectral>6.019532350082291e-23 5.675559809562688e-22</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/690/A196?format=ascii</footprint><waveband>Millimeter</waveband><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/690/A196/tablea1</name><description>Positions and fluxes of the 850um-selected SMGs (S/N&gt;=4{sigma})</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>ID</name><description>[1/50] Galaxy identification number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>F850</name><description>Observed SCUBA-2 flux density at 850um</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.200-400GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F850</name><description>Error on SCUBA-2 flux density at 850um (combined 1{sigma} uncertainty)</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>S/N</name><description>Signal-to-noise ratio at 850um</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>D</name><description>Deboosting factor</description><ucd>arith.factor</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F850D</name><description>Deboosted SCUBA-2 flux density at 850um</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.200-400GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F850D</name><description>Error on deboosted SCUBA-2 flux density at 850um (combined 1{sigma} uncertainty)</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/A+A/690/A196/tableb1</name><description>De-boosted photometry and redshift estimation from MMPz</description><column><name>e_F850</name><description>Error on SCUBA-2 flux density at 850um</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F1100</name><description>Error on AzTEC flux density at 1100um</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F3300</name><description>? MUSTANG-2 flux density at 3300um</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.50-100GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F3300</name><description>? Error on MUSTANG-2 flux density at 3300um</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>zph</name><description>Photometry redshift estimate</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_zph</name><description>Upper uncertainty in photometry redshift</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_zph</name><description>Lower uncertainty in photometry redshift</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>ID</name><description>[1/50] Galaxy identification number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>F250</name><description>SPIRE flux density at 250um</description><unit>deg</unit><ucd>phot.flux.density;em.mm.750-1500GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F250</name><description>Error on SPIRE flux density at 250um</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F350</name><description>SPIRE flux density at 350um</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.750-1500GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F350</name><description>Error on SPIRE flux density at 350um</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F500</name><description>SPIRE flux density at 500um</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.400-750GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F500</name><description>Error on SPIRE flux density at 500um</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F850</name><description>SCUBA-2 flux density at 850um</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.200-400GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F1100</name><description>AzTEC flux density at 1100um</description><unit>mJy</unit><ucd>phot.flux.density;em.mm.200-400GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>