J/ApJS/259/41ivo://CDS.VizieR/J/ApJS/259/41doi:10.26093/cds/vizier.22590041CDSGoldman S.R.Boyer M.L.Dalcanton J.McDonald I.Girardi L.,Williams B.F.Srinivasan S.Gordon K.2023-11-02T09:48:48Z2022-04-13T08:52:22ZCDS support team

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

cds-question@unistra.frgalaxiesvariable-starsphotometrylate-type-starsWe present a near-complete catalog of the metal-rich population of thermally pulsing asymptotic giant branch (AGB) stars in the northwest quadrant of M31. This metal-rich sample complements the equally complete metal-poor Magellanic Cloud AGB catalogs produced by the SAGE program. Our catalog includes Hubble Space Telescope (HST) wide-band photometry from the Panchromatic Hubble Andromeda Treasury survey, HST medium-band photometry used to chemically classify a subset of the sample, and Spitzer mid- and far-IR photometry that we have used to isolate dust-producing AGB stars. We have detected 346623 AGB stars; these include 4802 AGB candidates producing considerable dust, and 1356 AGB candidates that lie within clusters with measured ages, and in some cases metallicities. Using the Spitzer data and chemical classifications made with the medium-band data, we have identified both carbon- and oxygen-rich AGB candidates producing significant dust. We have applied color-mass-loss relations based on dusty-AGB stars from the LMC to estimate the dust injection by AGB stars in the PHAT footprint. Applying our color relations to a subset of the chemically classified stars producing the bulk of the dust, we find that ~97.8% of the dust is oxygen-rich. Using several scenarios for the dust lifetime, we have estimated the contribution of AGB stars to the global dust budget of M31 to be 0.9%-35.5%, which is in line with previous estimates in the Magellanic Clouds. Follow-up observations of the M31 AGB candidates with the JWST will allow us to further constrain stellar and chemical evolutionary models, and the feedback and dust production of metal-rich evolved stars.2022ApJS..259...41Ghttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/259/41CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/AJ/141/61 : Star clusters in M31. II. (Caldwell+, 2011)J/ApJS/215/9 : PHAT X. UV-IR photometry of M31 stars (Williams+, 2014)J/ApJ/802/127 : PHAT stellar cluster survey. II. AP catalog (Johnson+, 2015)J/ApJS/216/10 : DUSTiNGS. I. The Good Source Catalog (Boyer+, 2015)J/ApJS/228/5 : Spitzer photometry of ~1million stars in M31 + 15 gal.https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/259/41https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/259/41http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/259/41https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/259/41https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/259/41http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/259/41GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJS/259/41/table2 (Photometry of the M31 AGB sample; from erratum published in 2023ApJS..268...71G)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/259/41/table2?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/259/41/table2?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/259/41/table2?GETtext/xml+votable180.050000true10.65068721162541.23865277472760.0055555555555555566/2623 2666 2709 27522.0616683193919197e-20 7.886974166154988e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/259/41?format=asciidefaultJ/ApJS/259/41/table2Photometry of the M31 AGB sample; from erratum published in 2023ApJS..268...71Ge_F160W[0.001/0.4]? Uncertainty in F160W (5)magstat.errorfloatnullableS-F110W[-9.999/0.4]? HST/WFC3/IR F110W band sharpnessstat.fit.paramfloatnullableS-F160W[-9.999/3]? HST/WFC3/IR F160W band sharpnessstat.fit.paramfloatnullableS-F275W[-9.999/9.999]? HST/WFC3/UVIS F275W band sharpnessstat.fit.paramfloatnullableS-F336W[-9.999/9.999]? HST/WFC3/UVIS F336W band sharpnessstat.fit.paramfloatnullableS-F475W[-9.999/9.999]? HST/ACS/WFC F475W band sharpnessstat.fit.paramfloatnullableS-F814W[-9.999/9.999]? HST/ACS/WFC F814W band sharpnessstat.fit.paramfloatnullableR-F110w[-9.999/9.999]? HST/WFC3/IR F110W band roundnessstat.fit.paramfloatnullableR-F160W[-9.999/9.999]? HST/WFC3/IR F160W band roundnessstat.fit.paramfloatnullableR-F814W[-9.999/9.999]? HST/ACS/WFC F814W band roundnessstat.fit.paramfloatnullableC-F110W[0/9.999]? HST/WFC3/IR F110W band crowdednessmeta.codefloatnullableC-F160W[0/9.999]? HST/WFC3/IR F160W band crowdednessmeta.codefloatnullableC-F275W[0/9.999]? HST/WFC3/UVIS F275W band crowdednessmeta.codefloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintID[1/346623] This catalog's internal identifiermeta.id;meta.mainintRAJ2000Right Ascension (J2000)degpos.eq.ra;meta.mainindexedDEJ2000Declination (J2000)degpos.eq.dec;meta.mainindexedBrick[-99/23] PHAT brick identifier (1)meta.idintR[0/20] Deprojected radius from galaxy centerkpcphys.size.radiusfloat[M/H][-0.3/0.11] Estimated [M/H] based on R (Z-Rad) (2)phys.abund.ZfloatCl-ID[0/15121]? Cluster catalog identifier (Clst-ID) (3)meta.id;meta.tableintnullableR-F275W[-9.999/9.999]? HST/WFC3/UVIS F275W band roundnessstat.fit.paramfloatnullableR-F336W[-9.999/9.999]? HST/WFC3/UVIS F336W band roundnessstat.fit.paramfloatnullableR-F475W[-9.999/9.999]? HST/ACS/WFC F475W band roundnessstat.fit.paramfloatnullableCl-[Fe/H][-2.4/0.4]? Cluster [Fe/H] (Clst-Z) (3) (4)phys.abund.FefloatnullablelogCl-Age[0/10.3]? log cluster age (Clst-Age) (3)log(yr)time.agefloatnullablelogCl-Mass[0/7]? log cluster mass (Clst-M) (3)log(solMass)phys.massfloatnullableCl-Rad[0/6.4]? Cluster visible radius (Clst-R) (3)arcsecphys.angSize;srcfloatnullableCl-Dist[0/4.8]? Source distance to cluster center (Clst-D) (3)arcsecpos.angDistancefloatnullableF275W[15.6/41]? HST/WFC3/UVIS F275W band magnitude (5)magphot.mag;em.UV.200-300nmfloatnullablee_F275W[0.002/10]? Uncertainty in F275W (5)magstat.errorfloatnullableF336W[17.7/41]? HST/WFC3/UVIS F336W band magnitude (5)magphot.mag;em.opt.Ufloatnullablee_F336W[0.001/10]? Uncertainty in F336W (5)magstat.errorfloatnullableF475W[14.7/38]? HST/ACS/WFC F475W band magnitude (5)magphot.mag;em.opt.Bfloatnullablee_F475W[0.001/10]? Uncertainty in F475W (5)magstat.errorfloatnullableF814W[13.5/35.2]? HST/ACS/WFC F814W band magnitude (5)magphot.mag;em.opt.Ifloatnullablee_F814W[0.001/9]? Uncertainty in F814W (5)magstat.errorfloatnullableF110W[12/26.1]? HST/WFC3/IR F110W band magnitude (5)magphot.mag;em.IR.Jfloatnullablee_F110W[0.001/0.3]? Uncertainty in F110W (5)magstat.errorfloatnullableF127M[15/21]? HST/WFC3/IR F127M band magnitude (6)magphot.mag;em.IR.Jfloatnullablee_F127M[0.001/0.1]? Uncertainty in F127M (6)magstat.errorfloatnullableF139M[14.8/22]? HST/WFC3/IR F139M band magnitude (6)magphot.mag;em.IR.Jfloatnullablee_F139M[0.001/0.2]? Uncertainty in F139M (6)magstat.errorfloatnullableF153M[14.4/21]? HST/WFC3/IR F153M band magnitude (6)magphot.mag;em.IR.Hfloatnullablee_F153M[0.001/0.1]? Uncertainty in F153M (6)magstat.errorfloatnullableF160W[12.6/25.4]? HST/WFC3/IR F160W band magnitude (5)magphot.mag;em.IR.HfloatnullableC-F336W[0/9.999]? HST/WFC3/UVIS F336W band crowdednessmeta.codefloatnullableC-F475W[0/9.999]? HST/ACS/WFC F475W band crowdednessmeta.codefloatnullableC-F814W[0/9.999]? HST/ACS/WFC F814W band crowdednessmeta.codefloatnullableIRAC1[9.5/18]? Spitzer/IRAC 3.6um band magnitude (6)magphot.mag;em.IR.3-4umfloatnullablee_IRAC1[0.02/0.3]? Uncertainty in IRAC1 (6)magstat.errorfloatnullableIRAC2[9.3/18.3]? Spitzer/IRAC 4.5um band magnitude (6)magphot.mag;em.IR.4-8umfloatnullablee_IRAC2[0.01/0.3]? Uncertainty in IRAC2 (6)magstat.errorfloatnullableIRAC3[10.4/18.2]? Spitzer/IRAC 5.8um band magnitude (7)magphot.flux.density;em.IR.4-8umfloatnullablee_IRAC3[0.01/0.3]? Uncertainty in IRAC3 (7)magstat.errorfloatnullableIRAC4[8.7/17.4]? Spitzer/IRAC 8um band magnitude (7)magphot.flux.density;em.IR.8-15umfloatnullablee_IRAC4[0.01/0.3]? Uncertainty in IRAC4 (7)magstat.errorfloatnullableHST-AGB[0/1] Classified here as AGB candidate from HST criteriameta.codeintX-AGB[0/1] Classified here as AGB candidate from Spitzer criteriameta.codeintRHeB[0/1] Classified here as RHeB candidatemeta.codeintRSG[0/1] Classified here as Red supergiant candidate in Ren+ 2021ApJ...907...18Rmeta.codeintChem[cm] AGB photometric chemical type from HST small regions (8)meta.codecharSPLASH[cm] AGB photometric chemical type from SPLASH subset (8)meta.codecharGaia[0/1]? Gaia foreground candidatemeta.codeintnullable