J/ApJ/892/102ivo://CDS.VizieR/J/ApJ/892/102doi:10.26093/cds/vizier.18920102CDSLovisari L.Schellenberger G.Sereno M.Ettori S.Pratt G.W.,Forman W.R.Jones C.Andrade-Santos F.Randall S.Kraft R.2021-10-05T13:57:37Z2021-09-15T09:39:44ZCDS support team

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

cds-question@unistra.frgalaxy-clustersx-ray-sourcesredshiftedWe report the scaling relations derived by fitting the X-ray parameters determined from analyzing the XMM-Newton observations of 120 galaxy clusters in the Planck Early Sunyaev-Zel'dovich (SZ) sample spanning the redshift range of 0.059<z<0.546. We find that the slopes of all the investigated scaling relations significantly deviate from the self-similar predictions, if self-similar redshift evolution is assumed. When the redshift evolution is left free to vary, the derived slopes are more in agreement with the self-similar predictions. Relaxed clusters have on average ~30% higher X-ray luminosity than disturbed clusters at a given mass, a difference that, depending on the relative fraction of relaxed and disturbed clusters in the samples (e.g., SZ vs. X-ray selected), has a strong impact on the normalization obtained in different studies. Using the core-excised cluster luminosities reduces the scatter and brings into better agreement the L-M_tot_ and L-T relations determined for different samples. M_tot_-T, M_tot_-YX, and M_tot_-M_gas_ relations show little dependence on the dynamical state of the clusters, but the normalizations of these relations may depend on the mass range investigated. Although most of the clusters investigated in this work reside at relatively low redshift, the fits prefer values of {gamma}, the parameter accounting for the redshift evolution, different from the self-similar predictions. This suggests an evolution (<2{sigma} level, with the exception of the M_tot_-T relation) of the scaling relations. For the first time, we find significant evolution (>3{sigma}) of the M_tot_-T relation, pointing to an increase of the kinetic-to-thermal energy ratio with redshift. This is consistent with a scenario in which higher-redshift clusters are on average more disturbed than their lower-redshift counterparts.2020ApJ...892..102Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/892/102CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toB/xmm : XMM-Newton Obs. Log (XMM-Newton Science Operation Center, 2012)VIII/88 : Planck Early Release Compact Source Catalogue (Planck, 2011)VIII/91 : Planck Catalog of Compact Sources Release 1 (Planck, 2013)J/A+A/536/A8 : Planck early results. VIII. ESZ sample. (Planck+, 2011)J/A+A/535/A4 : X-ray galaxy clusters study (Reichert+, 2011)J/A+A/575/A30 : HIFLUGCS XMM/Chandra cross-calibration (Schellenberger+, 2015)J/MNRAS/450/3675 : CoMaLit. IV. Sigma Catalogue (Sereno+, 2015)J/MNRAS/457/4515 : X-ray_peak-BCG offset for PSZ1 clusters (Rossetti+, 2016)J/ApJ/843/76 : Cool-core clusters with Chandra obs. (Andrade-Santos+, 2017)J/MNRAS/468/1917 : Concentration parameter of galaxy clusters (Rossetti+, 2017)J/MNRAS/469/3738 : Complete sample of galaxy clusters (Schellenberger+, 2017)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/892/102https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/892/102http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/892/102https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/892/102https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/892/102http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/892/102GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/892/102/table3 (Cluster properties)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/892/102/table3?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/892/102/table3?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/892/102/table3?GETtext/xml+votable180.050000true316.0513-41.32520.0055555555555555566/97 207 4206 4965 5099 5701 6011 6383 6873 7242 7695 7768 9036 9168 9366 9476 9506 9593 9997 10527 10664 11080 11253 11591 11626 12072 12642 12732 13314 15192 15286 16024 16030 16486 16702 17457 18534 18566 18584 18683 18894 19009 19101 19451 19935 20507 20624 20731 20735 20874 21766 22972 23451 24579 24735 25188 25391 25451 26135 26189 26208 26302 27136 27595 28430 28448 30946 31537 31851 32379 32500 32602 32894 32960 33030 33235 33289 33586 33614 33692 33810 33894 33945 34087 34159 34174 34181 34186 34443 35147 35177 37095 37395 37404 38973 39067-39068 39443 39608 40564 41014 41081 45076 45235 45421 45506 45543 45562 45966 46237 46474 46687 46763 46855 46889 47139 47168 47225 47573 48966https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/892/102?format=asciiX-raydefaultJ/ApJ/892/102/table3Cluster propertiesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintPLCKESZPlanck identifier GLLL.ll+BB.bb (1)meta.id;meta.maincharf_PLCKESZ[*] * = not explained in the paperstat.fit.paramcharz[0.059/0.6] Cluster spectroscopic redshiftsrc.redshiftfloatM500[2.4/17.6] Total mass with R_500_1e+14solMassphys.massfloatE_M500[0.04/6] Upper uncertainty in M5001e+14solMassstat.error;stat.maxfloate_M500[0.03/5] Lower uncertainty in M5001e+14solMassstat.errorfloatMg500[2.87/32] Gas mass with R_500_1e+13solMassphys.massfloatE_Mg500[0.03/3] Upper uncertainty in Mg5001e+13solMassstat.error;stat.maxfloate_Mg500[0.03/6] Upper uncertainty in Mg5001e+13solMassstat.errorfloatkT[1.67/14.4] Core-included cluster temperaturekeVphys.temperature;em.X-rayfloatE_kT[0.03/1.4] Upper uncertainty in kTkeVstat.error;stat.maxfloate_kT[0.03/1.4] Lower uncertainty in kTkeVstat.error;phys.energyfloatkTexc[1.4/15.1] Core-excluded cluster temperaturekeVphys.temperature;em.X-rayfloatE_kTexc[0.04/1.6] Upper uncertainty in kTexckeVstat.error;stat.maxfloate_kTexc[0.04/1.6] Lower uncertainty in kTexckeVstat.errorfloatLX[1.28/27.1] Core-included cluster 0.1-2.4keV luminosity; erg/s1e-07Wphys.luminosity;em.X-rayfloatE_LX[0.04/1.7] Upper uncertainty in LX1e-07Wstat.error;stat.maxfloate_LX[0.04/1.7] Lower uncertainty in LX1e-07Wstat.errorfloatLXexc[0.86/18] Core-excluded cluster 0.1-2.4keV luminosity; erg/s1e-07Wphys.luminosity;em.X-rayfloatE_LXexc[0.01/1.3] Upper uncertainty in LXexc1e-07Wstat.error;stat.maxfloate_LXexc[0.01/1.3] Lower uncertainty in LXexc1e-07Wstat.errorfloatLbol[2.6/87] Core-included cluster bolometric (0.01-100keV) luminosity; erg/s1e-07Wphys.luminosityfloatE_Lbol[0.1/8] Upper uncertainty in Lbol1e-07Wstat.error;stat.maxfloate_Lbol[0.1/8] Lower uncertainty in Lbol1e-07Wstat.errorfloatLbolexc[1.87/61] Core-excluded cluster bolometric (0.01-100keV) luminosity; in erg/s units1e-07Wphys.luminosityfloatE_Lbolexc[0.01/4] Upper uncertainty in Lbolexc1e-07Wstat.error;stat.maxfloate_Lbolexc[0.01/4] Lower uncertainty in Lbolexc1e-07Wstat.errorfloatNT[1/33] Number of temperature profile binsmeta.numberintfT[0.3/1.3] Fraction of R_500_ covered by temperature profilestat.fit.paramfloatNsb[4/372] Number of surface brightness profile binsmeta.numberintfsb[0.5/1.7] Fraction of R_500_ covered by surface brightness profilestat.fit.paramfloatSimbadSimbad column added by the CDSmeta.ref.urlcharNEDNED column added by the CDSmeta.numberchar_RAPositions from Planck ESZ catalog (VIII/88) (right ascension part)degpos.eq.ra;meta.main_DEPositions from Planck ESZ catalog (VIII/88) (declination part)degpos.eq.dec;meta.main