J/ApJS/262/27ivo://CDS.VizieR/J/ApJS/262/27doi:10.26093/cds/vizier.22620027CDSBatalha R.M.Dupke R.A.Jimenez-Teja Y.2023-01-16T07:47:42Z2022-12-07T14:21:02ZCDS support team

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

cds-question@unistra.frgalaxy-clustersintergalactic-mediumchemical-abundancesx-ray-sourcesThe intracluster medium (ICM) is a reservoir of heavy elements synthesized by different supernovae (SNe) types over cosmic history. Different enrichment mechanisms contribute a different relative metal production, predominantly caused by different SNe type dominance. Using spatially resolved X-ray spectroscopy, one can probe the contribution of each metal-enrichment mechanism. However, a large variety of physically feasible supernova (SN) explosion models make the analysis of the ICM enrichment history more uncertain. This paper presents a nonparametric probability distribution function analysis to rank different theoretical SNe yields models by comparing their performance against observations. Specifically, we apply this new methodology to rank 7192 combinations of core-collapse SN and Type Ia SN models using eight abundance ratios from Suzaku observations of 18 galaxy systems (clusters and groups) to test their predictions. This novel technique can compare many SN models and maximize spectral information extraction, considering all the individual measurable abundance ratios and their uncertainties. We find that Type II SNe with nonzero initial metallicity progenitors in general performed better than pair-instability SN and hypernova models, and that 3D SNIa models (with a white dwarf progenitor central density of 2.9x10^9^g/cm^3^) performed best among all tested SN model pairs.2022ApJS..262...27Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/262/27CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/ApJ/608/405 : Explosive yields of massive star (Chieffi+, 2004)J/ApJS/182/12 : ICM entropy profiles (ACCEPT) (Cavagnolo+, 2009)J/ApJ/724/341 : Nucleosynthesis of massive metal-free stars (Heger+, 2010)http://heasarc.gsfc.nasa.gov/docs/suzaku : Suzaku home page on HEASARChttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/262/27https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/262/27http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/262/27https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/262/27https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/262/27http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/262/27GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJS/262/27/table1 (Observations of groups and clusters of galaxies)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/262/27/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/262/27/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/262/27/table1?GETtext/xml+votable180.050000true226.62341671.60250.0055555555555555566/1701 2251 2388 2432 7004 8173 8196 10182 22577 23306 24951 25769 27652 27719 29234 43626 43849 44554https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/262/27?format=asciiX-raydefaultJ/ApJS/262/27/table1Observations of groups and clusters of galaxiesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameCluster or group name (as in Table 2)meta.id;meta.maincharprimaryONameOther designationmeta.idcharRAJ2000Hour of right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Degree of declination (J2000)pos.eq.dec;meta.mainz[0.004/0.04] Redshift from NED to perform spectral fittings (see Section 2.2)src.redshiftdoublel_Rad[<~ ] Limit flag on Radmeta.code.errorRad[10/110] Cool-core radius (1)kpcphys.size.radiusintObsIDObservation identifiermeta.id;obs.param;obslongSimbadNameSimbad column added by the CDSmeta.idcharnullableNEDNED column added by the CDSmeta.ref.urlcharExp[10.8/155.9] Exposure timekstime.duration;obs.exposurefloatPIPrincipal Investigator on the proposalobs.observercharJ/ApJS/262/27/table2Error-weighted average of all XIS instruments for temperature and chemical abundance from inner, outer, and total (entire) Field of View spectra regions (see Section 2)NameName of the groups or clustermeta.id;meta.maincharprimarye_Fe[0.001/0.1] Uncertainty in Felog(Sun)stat.error;phys.abund.FefloatMg[0.1/1.53] Log abundance of Mglog(Sun)phys.abundfloate_Mg[0.01/0.4] Uncertainty in Mglog(Sun)stat.errorfloatNe[0.05/2.44] Log abundance of Nelog(Sun)phys.abundfloate_Ne[0.02/0.9] Uncertainty in Nelog(Sun)stat.errorfloatNi[0.05/3] Log abundance of Nilog(Sun)phys.abundfloate_Ni[0.03/0.9] Uncertainty in Nilog(Sun)stat.errorfloatO[0.009/1.6] Log abundance of Olog(Sun)phys.abundfloate_O[0.006/0.3] Uncertainty in Olog(Sun)stat.errorfloatS[0.24/3] Log abundance of Slog(Sun)phys.abundfloate_S[0.01/1] Uncertainty in Slog(Sun)stat.errorfloatSi[0.24/1.6] Log abundance of Silog(Sun)phys.abundfloate_Si[0.009/0.3] Uncertainty in Silog(Sun)stat.errorfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintLocGroup/cluster location (1)meta.codecharTemp[0.7/8.7] Log temperature of the group or clusterlog(kT)phys.temperature;pos.lgfloate_Temp[0.002/0.08] Uncertainty in Templog(kT)stat.errorfloatAr[0.2/2.6] Log abundance of Arlog(Sun)phys.abundfloate_Ar[0.03/1.0] Uncertainty in Arlog(Sun)stat.errorfloatCa[0.03/2.5] Log abundance of Calog(Sun)phys.abundfloate_Ca[0.02/0.9] Uncertainty in Calog(Sun)stat.errorfloatFe[0.03/0.9] Log abundance of Felog(Sun)phys.abundfloat