J/MNRAS/484/3042ivo://CDS.VizieR/J/MNRAS/484/3042doi:10.26093/cds/vizier.74843042CDSSanchez S.F.Barrera-Ballesteros J.K.Lopez-Coba C.Brough S.,Bryant J.J.Bland-Hawthorn J.Croom S.M.van de Sande J.Cortese L.,Goodwin M.Lawrence J.S.Lopez-Sanchez A.R.Sweet S.M.Owers M.S.,Richards S.N.Walcher C.J.(the Sami Team)2024-08-19T20:16:36Z2022-09-30T12:43:34ZCDS support team

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

cds-question@unistra.frspectroscopychemical-abundancesgalaxiesinterstellar-mediumvisible-astronomyWe present a detailed exploration of the stellar mass versus gas-phase metallicity relation (MZR) using integral field spectroscopy data obtained from ~1000 galaxies observed by the SAMI galaxy survey. These spatially resolved spectroscopic data allow us to determine the metallicity within the same physical scale (R_eff_) for different calibrators. The shape of the MZ relations is very similar between the different calibrators, while there are large offsets in the absolute values of the abundances. We confirm our previous results derived using the spatially resolved data provided by the CALIFA and MaNGA surveys: (1) we do not find any significant secondary relation of the MZR with either the star formation rate (SFR) or the specific SFR (SFR/M_*_) for any of the calibrators used in this study, based on the analysis of the individual residuals; (2) if there is a dependence with the SFR, it is weaker than the reported one (r_c_~-0.3), it is confined to the low-mass regime (M_*_<10^9^M_{sun}_) or high-SFR regimes, and it does not produce any significant improvement in the description of the average population of galaxies. The apparent disagreement with published results based on single-fibre spectroscopic data could be due to (i) the interpretation of the secondary relation itself; (ii) the lower number of objects sampled at the low-mass regime by the current study; or (iii) the presence of extreme star-forming galaxies that drive the secondary relation in previous results.2019MNRAS.484.3042Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/484/3042CatalogResearchIsServedByTAP VizieR generic servicerelated-tohttp://sami-survey.org : SAMI Galaxy Survey Home Pagehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/484/3042https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/484/3042http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/484/3042https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/484/3042https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/484/3042http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/484/3042GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/MNRAS/484/3042/tablee1Stellar Masses, star-formation rates, and characteristics abundances for the all the considered calibratorse_OHm08? Error on OHm08stat.errordoublenullablee_logMassError on logMasslog(solMass)stat.error;phys.massdoublelogSFRStar formation ratelog(solMass.yr**-1)phys.SFRdoublee_logSFRError on logSFRlog(solMass.yr**-1)stat.error;phys.SFRdoubleOHo3n2-m13? Oxygen abundance based on the O3N2 calibrator from Marino et al. (2013A&A...559A.114M, Cat. J/A+A/559/A114) (1)phys.abunddoublenullablee_OHo3n2-m13? Error on OHo3n2-m13stat.errordoublenullableSimbadNameSimbad column added by the CDSmeta.idcharnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameGalaxy name (SAMINNNNNNNNN)meta.id;meta.maincharlogMassStellar masslog(solMass)phys.massdoubleOHn2-m13? Oxygen abundance based on the N2 calibrator from Marino et al. (2013A&A...559A.114M, Cat. J/A+A/559/A114) (1)phys.abunddoublenullablee_OHn2-m13? Error on OHn2-m13stat.errordoublenullableOHons? Oxygen abundance based on the ONS calibrator from Pilyugin, Vilchez & Thuan (2010ApJ...720.1738P) (1)phys.abunddoublenullablee_OHons? Error on OHonsstat.errordoublenullableOHr23? Oxygen abundance based on the R23 calibrator from Kobulnicky & Kewley (2004ApJ...617..240K, Cat. J/ApJ/617/240) (1)phys.abunddoublenullablee_OHr23? Error on OHr23stat.errordoublenullableOHo3n2-pp04? Oxygen abundance based on the O3N2 indicator by Pettini & Pagel (2004MNRAS.348L..59P) (3)phys.abunddoublenullablee_OHo3n2-pp04? Error on OHo3n2-pp04stat.errordoublenullableOHpyqz? Oxygen abundance provided by the pyqz code (Vogt et al. 2015MNRAS.450.2593V) as described by Dopita et al. (2013ApJS..208...10D Cat. J/ApJS/208/10) (4)phys.abunddoublenullablee_OHpyqz? Error on OHpyqzstat.errordoublenullableOHt2? t2 correction proposed by Pena-Guerrero, Peimbert & Peimbert (2012ApJ...756L..14P), for the average oxygen abundance estimated from the four calibrators included in the first family (2)arith.factordoublenullablee_OHt2? Error on OHt2stat.errordoublenullableOHm08? Oxygen abundance based on a combination or R23 and the previous one proposed by Maiolino et al. (2008A&A...488..463M) (3)phys.abunddoublenullableOHt04? Oxygen abundance based on the R23 calibrator described by Tremonti et al. (2004ApJ...613..898T) (4)phys.abunddoublenullablee_OHt04? Error on OHt04stat.errordoublenullableOHdop? Oxygen abundance described by Dopita et al. (2016Ap&SS.361...61D), based on the N2/S2 and N2 line ratios (4)phys.abunddoublenullablee_OHdop? Error on OHdopstat.errordoublenullableOHepm? Oxygen abundance based on a version of the O3N2 calibrator that corrects for relative abundance from nitrogen to oxygen from Perez-Montero & Contini (2009MNRAS.398..949P) (1)phys.abunddoublenullablee_OHepm? Error on OHepmstat.errordoublenullable