J/A+A/684/A18ivo://CDS.VizieR/J/A+A/684/A18doi:10.26093/cds/vizier.36840018CDSAdam R.Ricci M.Eckert D.Ade P.Ajeddig H.Altieri B.Andre P.,Artis E.Aussel H.Beelen A.Benoist C.Benoit A.Berta S.Bing L.,Birkinshaw M.Bourrion O.Boutigny D.Bremer M.Calvo M.Cappi A.,Catalano A.De Petris M.Desert F.-X.Doyle S.Driessen E.F.C.,Faccioli L.Ferrari C.Gastaldello F.Giles P.Gomez A.Goupy J.,Hahn O.Hanser C.Horellou C.Keruzore F.Koulouridis E.Kramer C.,Ladjelate B.Lagache G.Leclercq S.Lestrade J.-F.Macias-Perez J.F.,Madden S.Maughan B.Maurogordato S.Maury A.Mauskopf P.,Monfardini A.Munoz-Echeverria M.Pacaud F.Perotto L.Pierre M.,Pisano G.Pompei E.Ponthieu N.Reveret V.Rigby A.Ritacco A.,Romero C.Roussel H.Ruppin F.Sereno M.Schuster K.Sievers A.,Tintore Vidal G.Tucker C.Zylka R.2024-11-07T20:02:31Z2024-03-28T14:23:13ZCDS support team

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

cds-question@unistra.frgalaxy-clustersradio-sourcesThe thermodynamical properties of the intracluster medium (ICM) are driven by scale-free gravitational collapse, but they also reflect the rich astrophysical processes at play in galaxy clusters. At low masses (~10^14^M_{sun}_) and high redshift (z>~1), these properties remain poorly constrained observationally, due to the difficulty in obtaining resolved and sensitive data. This paper aims at investigating the inner structure of the ICM as seen through the Sunyaev-Zel'dovich (SZ) effect in this regime of mass and redshift. Focus is set on the thermal pressure profile and the scaling relation between SZ flux and mass, namely the YSZ-M scaling relation. The three galaxy clusters XLSSC 072 (z=1.002), XLSSC 100 (z=0.915), and XLSSC 102 (z=0.969), with M500 ~2x10^14^M_{sun}_, were selected from the XXL X-ray survey and observed with the NIKA2 millimeter camera to image their SZ signal. XMM-Newton X-ray data were used in complement to the NIKA2 data to derive masses based on the YX-M relation and the hydrostatic equilibrium. Results. The SZ images of the three clusters, along with the X-ray and optical data, indicate dynamical activity related to merging events. The pressure profile is consistent with that expected for morphologically disturbed systems, with a relatively flat core and a shallow outer slope. Despite significant disturbances in the ICM, the three high-redshift low-mass clusters follow remarkably well the YSZ-M relation expected from standard evolution. These results indicate that the dominant physics that drives cluster evolution is already in place by z~1, at least for systems with masses above M500~10^14^M_{sun}_.2024A&A...684A..18Ahttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/684/A18CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toIX/49 : XXL Survey: First results (Pierre+, 2016)IX/52 : XXL Survey. DR2 (Chiappetti+, 2018)J/A+A/638/A46 : The XXL Survey. XLI. GMRT XXL-N 610MHz (Slaus+, 2020)J/A+A/638/A45 : Obscuration properties of red AGNs in XXL-N (Masoura+, 2020)J/A+A/663/A2 : XXL Survey. X-ray emission in opt. select. groupJ/A+A/684/A19 : The XXL Survey. LII. (Slaus+, 2024)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/684/A18https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/684/A18http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/684/A18https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/684/A18https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/684/A18http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/684/A18GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/684/A18/list (List of fits files)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/684/A18/list?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/684/A18/list?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/684/A18/list?GETtext/xml+votable180.050000true33.85-3.7260.005555555555555556Associated datahttps://cdsarc.cds.unistra.fr/assocdata/?obs_collection=J/A+A/684/A186/17697 17702 17712https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/684/A18?format=asciiRadiodefaultJ/A+A/684/A18/tf072Transfer function of the XLSSC072 150 GHz maprecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintkWavenumberarcmin**-1em.freqfloatTTransfer function (signal transmission)instr.det.psffloatJ/A+A/684/A18/tf100Transfer function of the XLSSC100 150 GHz maprecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintkWavenumberarcmin**-1em.freqfloatTTransfer function (signal transmission)instr.det.psffloatJ/A+A/684/A18/tf102Transfer function of the XLSSC102 150 GHz maprecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintkWavenumberarcmin**-1em.freqfloatTTransfer function (signal transmission)instr.det.psffloatJ/A+A/684/A18/listList of fits filesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRAJ2000Right Ascension of center (J2000)degpos.eq.ra;meta.mainDEJ2000Declination of center (J2000)degpos.eq.dec;meta.mainNxNumber of pixels along X-axismeta.numberintNyNumber of pixels along Y-axismeta.numberintNz? Number of slices for the datacubesmeta.numberintnullableFreqFrequency of the observationMHzem.freq;obsintObs.dateObservation datestime.epoch;obsnullablesizeSize of FITS fileKibytephys.size;meta.fitsintFileNameName of FITS file, in subdirectory fitsmeta.id;meta.fitscharTitleTitle of the FITS filemeta.title;meta.fitschar