J/MNRAS/405/857ivo://CDS.VizieR/J/MNRAS/405/857doi:10.26093/cds/vizier.74050857CDSGoddard Q.E.Bastian N.Kennicutt R.C.2024-07-11T20:16:58Z2011-07-30T18:13:13ZCDS support team

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

cds-question@unistra.frgalaxiesstellar-associationshst-photometryIn this paper we derive ages and masses for 276 clusters in the merger galaxy NGC 3256. This was achieved by taking accurate photometry in four wavebands from archival Hubble Space Telescope images. Photometric measurements are compared to synthetic stellar population (SSP) models to find the most probable age, mass and extinction. The cluster population of NGC 3256 reveals an increase in the star formation rate (SFR) over the last 100Myr and the initial cluster mass function (ICMF) is best described by a power-law relation with slope alpha=1.85+/-0.12.2010MNRAS.405..857Ghttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/405/857CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/405/857https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/405/857http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/405/857https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/405/857https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/405/857http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/405/857GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/405/857/table5 (Cluster photometry and parameters for the 276 good cluster fits)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/405/857/table5?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/405/857/table5?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/405/857/table5?GETtext/xml+votable180.050000true156.96504-43.907810.0055555555555555566/381392.3657755224268815e-19 6.059863979418323e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/405/857?format=asciiOpticaldefaultJ/MNRAS/405/857/table5Cluster photometry and parameters for the 276 good cluster fitsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/276] Sequential numbermeta.recordintoRAOffset in right ascension (1)spos.eq.ra;arith.difffloatoDEOffset in declination (1)arcsecpos.eq.dec;arith.difffloatUmagHST/HRC F330W (U) magnitudemagphot.mag;em.opt.Ufloate_Umagrms uncertainty in Umagmagstat.error;phot.mag;em.opt.UfloatBmagHST/ACS F435W (B) magnitudemagphot.mag;em.opt.Bfloate_Bmagrms uncertainty in Bmagmagstat.error;phot.mag;em.opt.BfloatVmagHST/ACS F555W (V) magnitudemagphot.mag;em.opt.Vfloate_Vmagrms uncertainty in Vmagmagstat.error;phot.mag;em.opt.VfloatImagHST/ACS F814W (I) magnitudemagphot.mag;em.opt.Ifloate_Imagrms uncertainty in Imagmagstat.error;phot.mag;em.opt.Ifloatb_E(B-V)Mimimun acceptable E(B-V) dust extinction from fitting methodmagphys.absorptionfloatE(B-V)Optimal E(B-V) dust extinction from fitting methodmagphot.color.excessfloatB_E(B-V)Maximum acceptable E(B-V) dust extinction from fitting methodmagphys.absorption;stat.maxfloatlogAgeOptimal age from fitting methodlog(yr)time.agefloatB_logAgeMaximum acceptable age from fitting methodlog(yr)time.age;stat.maxfloatb_MassMinimum acceptable mass from fitting methodlog(solMass)phys.mass;stat.minfloatMassOptimal mass from fitting methodlog(solMass)phys.massfloatB_MassMaximum acceptable mass from fitting methodlog(solMass)phys.mass;stat.maxfloat_RASimbad column added by the CDSdegpos.eq.ra;meta.main_DESimbad column added by the CDSdegpos.eq.dec;meta.main