J/ApJ/813/77ivo://CDS.VizieR/J/ApJ/813/77doi:10.26093/cds/vizier.18130077CDSYuan Z.S.Han J.L.Wen Z.L.2023-05-05T11:36:43Z2023-05-05T12:33:15ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frgalaxy-clustersradio-sourcesDiffuse radio emission in galaxy clusters is known to be related to cluster mass and cluster dynamical state. We collect the observed fluxes of radio halos, relics, and mini-halos for a sample of galaxy clusters from the literature, and calculate their radio powers. We then obtain the values of cluster mass or mass proxies from previous observations, and also obtain the various dynamical parameters of these galaxy clusters from optical and X-ray data. The radio powers of relics, halos, and mini-halos are correlated with the cluster masses or mass proxies, as found by previous authors, while the correlations concerning giant radio halos are in general the strongest. We found that the inclusion of dynamical parameters as the third dimension can significantly reduce the data scatter for the scaling relations, especially for radio halos. We therefore conclude that the substructures in X-ray images of galaxy clusters and the irregular distributions of optical brightness of member galaxies can be used to quantitatively characterize the shock waves and turbulence in the intracluster medium responsible for re-accelerating particles to generate the observed diffuse radio emission. The power of radio halos and relics is correlated with cluster mass proxies and dynamical parameters in the form of a fundamental plane.2015ApJ...813...77Yhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/813/77CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/MNRAS/281/799 : XBACs, the sample (Ebeling+, 1996)J/MNRAS/301/881 : The ROSAT brightest cluster sample - I. (Ebeling+, 1998)J/ApJ/519/533 : ROSAT observations of ACO clusters (David+, 1999)J/ApJS/129/435 : NORAS galaxy cluster survey. I. (Bohringer+, 2000)J/ApJ/580/774 : X-ray cluster of galaxies behind the Milky wayJ/A+A/423/449 : RASS-SDSS Galaxy Clusters Survey. I. (Popesso+, 2004)J/A+A/425/367 : REFLEX Galaxy Cluster Survey catalogue (Boehringer+, 2004)J/ApJ/662/224 : Second CIZA subsample (Kocevski+, 2007)J/A+A/534/A109 : MCXC Meta-Catalogue X-ray galaxy Clusters (Piffaretti+, 2011)J/ApJS/199/34 : Clusters of galaxies in SDSS-III (Wen+, 2012)J/A+A/551/A24 : GMRT Radio Halo Cluster Survey diffuse sourcesJ/MNRAS/436/275 : Relaxation parameter of 2092 rich galaxy clustersJ/ApJ/807/178 : Newly rich galaxy clusters identified in SDSS-DR12https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/813/77https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/813/77http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/813/77https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/813/77https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/813/77http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/813/77GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/813/77/table2 (Masses, Mass Proxies, and Dynamical Parameters for 75 Galaxy Clusters)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/813/77/table2?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/813/77/table2?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/813/77/table2?GETtext/xml+votable180.050000true13.997916726.32055560.0055555555555555566/87 97 206 1701 2813 2920 3703 5099 5483 6011 6039 6383 6827 7221 7242 7768 8033 8220 8969 9050 9052 9072 9588 9997 10379 10527 11080 11467 11591 11626 12121 12642 14225 15112 15351 16024 16486 17457 18779 19097 19848 19935 20481 20536 21061 21387 22607 22972 23451 23869 24735 25188 25675 26037 26166 26189 27428 27740 29234 30946 31537 32500 35043 38858 38973 40809 43837 44008 44802 44817 45044 45984 46424 48684 489662.1534725313611987e-25 9.276497240453405e-25https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/813/77?format=asciiRadiodefaultJ/ApJ/813/77/table2Masses, Mass Proxies, and Dynamical Parameters for 75 Galaxy ClustersSimbadNameSimbad column added by the CDSmeta.idcharnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameCluster namemeta.id;meta.maincharlogLX? Log of total X-ray luminosity used as mass proxy of cluster (in 10^44^ erg/s)log(1e+37W)phys.luminosity;em.X-rayfloatnullablee_logLX? Uncertainty in logLXlog(1e+37W)stat.errorfloatnullablen_logLX[*] Note on logLX (1)meta.notecharlogL500? Log of X-ray luminosity within R_500_ used as mass proxy of cluster (in 10^44^ erg/s)log(1e+37W)phys.luminosity;em.X-rayfloatnullablee_logL500? Uncertainty in logL500log(1e+37W)stat.errorfloatnullablelogMSZ? Log of cluster mass estimated from the Sunyaev-Zel'dovich (SZ) effectlog(1e+14solMass)phys.massfloatnullablee_logMSZ? Uncertainty in logMSZlog(1e+14solMass)stat.errorfloatnullablelogM500? Log of cluster mass within R_500_log(1e+14solMass)phys.massfloatnullablee_logM500? Uncertainty in logM500log(1e+14solMass)stat.errorfloatnullableRefReferences of mass proxies or mass (2)meta.ref;phys.masscharGamma? Optical dynamical parameterstat.fit.paramfloatnullablee_Gamma? Uncertainty in Gammastat.errorfloatnullablelogc? Log of X-ray dynamical parameterphot.mag.sb;arith.ratiofloatnullablee_logc? Uncertainty in logcstat.errorfloatnullablelogomega? Log of centroid shift (in 500 kpc)kpcpos.distance;arith.difffloatnullablee_logomega? Uncertainty in logomegakpcstat.errorfloatnullablelogP3/P0? Log of power ratio (in 500 kpc)kpcstat.fit.paramfloatnullablee_logP3/P0? Uncertainty in logP3/P0kpcstat.errorfloatnullableRef1References for dynamical parameters (2)(3)meta.ref;pos.framechar_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.main_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainJ/ApJ/813/77/table1Radio Flux and Power for Radio Halos, Relics, and Mini-halos from 75 Galaxy ClustersNameCluster namemeta.id;meta.maincharlogP610? Log of radio power at 610 MHz after the k-correctionlog(1e+24W.Hz**-1)arith.factor;phys.luminosity;em.radio.400-750MHzfloatnullablee_logP610? Uncertainty in logP610log(1e+24W.Hz**-1)stat.errorfloatnullablelogP325? Log of radio power at 325 MHz after the k-correctionlog(1e+24W.Hz**-1)arith.factor;phys.luminosity;em.radio.200-400MHzfloatnullablee_logP325? Uncertainty in logP325log(1e+24W.Hz**-1)stat.errorfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzRedshiftsrc.redshiftfloatTypeType of diffuse radio emission (1)src.morph.typecharSizeAngular sizearcminphys.angSizefloatS1.4GHz? Flux of halo/relic/mini-halo at 1.4 GHzmJyphot.flux.density;em.radio.750-1500MHzfloatnullablee_S1.4GHz? Uncertainty in S1.4GHzmJystat.errorfloatnullablen_S1.4GHz[abc] Note on S1.4GHz (2)meta.notecharS610MHz? Flux of halo/relic/mini-halo at 610 MHzmJyphot.flux.density;em.radio.400-750MHzfloatnullablee_S610MHz? Uncertainty in S610MHzmJystat.errorfloatnullablen_S610MHz[c] Note on S610MHz (2)meta.notecharS325MHz? Flux of halo/relic/mini-halo at 325 MHzmJyphot.flux.density;em.radio.200-400MHzfloatnullablee_S325MHz? Uncertainty in S325MHzmJystat.errorfloatnullablen_S325MHz[c] Note on S325MHz (2)meta.notecharRefReference(s) number(s) of these radio fluxes (see refs.dat file)meta.numbercharlogP1.4? Log of radio power at 1.4 GHz after the k-correctionlog(1e+24W.Hz**-1)arith.factor;phys.luminosity;em.radio.750-1500MHzfloatnullablee_logP1.4? Uncertainty in logP1.4log(1e+24W.Hz**-1)stat.errorfloatnullableJ/ApJ/813/77/refsReferencesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRef[0/57] Reference numbermeta.id;meta.mainintAutAuthor's name(s)meta.bib.authorcharBibcodeReference bibcodemeta.bib.bibcodecharComComment on referencemeta.notechar