J/MNRAS/441/2ivo://CDS.VizieR/J/MNRAS/441/2doi:10.26093/cds/vizier.74410002CDSDominguez Sanchez H.Bongiovanni A.Lara-Lopez M.A.Oteo I.Cepa J.,Perez Garcia A.M.Sanchez-Portal M.Ederoclite A.Lutz D.Cresci G.,Delvecchio I.Berta S.Magnelli B.Popesso P.Pozzi F.Riguccini L.2024-08-09T20:14:57Z2015-05-04T11:04:45ZCDS support team

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

cds-question@unistra.frgalaxiescatalogsinfrared-sourcesultraviolet-astronomyWe study a hundred of galaxies from the spectroscopic Sloan Digital Sky Survey (SDSS) with individual detections in the far-infrared Herschel Photodetector Array Camera and Spectrometer bands (100 or 160um) and in the GALEX far-ultraviolet band up to z~0.4 in the COSMOS and Lockman Hole fields. The galaxies are divided into four spectral and four morphological types. For the star-forming and unclassifiable galaxies, we calculate dust extinctions from the ultraviolet (UV) slope, the H{alpha}/H{beta} ratio and the L_IR_/L_UV_ ratio. There is a tight correlation between the dust extinction and both L_IR_ and metallicity. We calculate SFRtotal and compare it with other star formation rate (SFR) estimates (H{alpha}, UV, SDSS) finding very good agreement between them with smaller dispersions than typical SFR uncertainties. We study the effect of mass and metallicity, finding that it is only significant at high masses for SFRH{alpha}. For the AGN and composite galaxies, we find a tight correlation between SFR and L_IR_({sigma}~0.29), while the dispersion in the SFR-L_UV_ relation is larger ({sigma}~0.57). The galaxies follow the prescriptions of the Fundamental Plane in the M-Z-SFR space.2014MNRAS.441....2Dhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/441/2CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+A/532/A90 : PACS Evolutionary Probe (PEP-DR1) catalogs (Lutz+, 2011)J/A+A/525/A157 : SDSS automated morphology classificationhttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/441/2https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/441/2http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/441/2https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/441/2https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/441/2http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/441/2GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/441/2/tabled (Properties of SDSS-DR7/POP galaxies)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/441/2/tabled?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/441/2/tabled?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/441/2/tabled?GETtext/xml+votable180.050000true149.470993061.741410.0055555555555555565/6814 6/6047 6069 27245 272477.447298006782415e-19 1.4134638842407062e-18https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/441/2?format=asciiUVInfrareddefaultJ/MNRAS/441/2/tabledProperties of SDSS-DR7/POP galaxiesID[108993/313793] Identification number (1)meta.id;meta.mainintprimaryRAJ2000Right ascension (J2000)degpos.eq.ra;meta.mainDEJ2000Declination (J2000)degpos.eq.dec;meta.mainz[0.01/0.34] Redshiftsrc.redshiftfloatClass[-1/5] Spectral class (2)src.spTypeintlogMStellar masslog(solMass)phys.massfloatlogSFRStar formation ratelog(solMass.yr**-1)phys.SFRfloatZ[8.46/9.26]? Metallicity Z=12+log(O/H)phys.abund.ZfloatnullablelogLIRInfrared luminositylog(solLum)phys.luminosity;em.IRfloatsep1[0/3] Separation SDSS-PEP (J/A+A/532/A90)arcsecpos;arith.difffloatpE[0/1]? Probability of E morphology (3)stat.fit.goodnessfloatnullablepS0[0/1]? Probability of S0 morphology (3)stat.fit.goodnessfloatnullablepSab[0/1]? Probability of Sab morphology (3)stat.fit.goodnessfloatnullablepScd[0/1]? Probability of Scd morphology (3)stat.fit.goodnessfloatnullablesep2[0/2]? Separation SDSS-Morphology (J/A+A/525/A157)arcsecpos;arith.difffloatnullableFNUV? NUV flux from GALEX DIS DR6/7uJyphot.flux.density;em.UV.200-300nmfloatnullablee_FNUV? rms uncertainty on FNUVuJystat.errorfloatnullableFFUV? FUV flux from GALEX DIS DR6/7uJyphot.flux.density;em.UV.100-200nmfloatnullablee_FFUV? rms uncertainty on FFUVuJystat.errorfloatnullablesep3[0/4]? Separation GALEX-SDSSarcsecpos;arith.difffloatnullableFHaH{alpha} flux from SDSS DR7 (in 10^-17^erg/s/cm^2^)1e-20W.m**-2phot.flux;em.line.Halphafloate_FHarms uncertainty on FHa1e-20W.m**-2stat.errorfloatFHbH{beta} flux from SDSS DR7 (in 10^-17^erg/s/cm^2^)1e-20W.m**-2phot.flux;em.line.Hbetafloate_FHbrms uncertainty on FHb1e-20W.m**-2stat.errorfloatApCor[0/1.7] Aperture correction from Salim et al. (2007ApJS..172...86S)instr.paramfloatlogSFR1Star formation rate derived from IR luminositylog(solMass.yr**-1)phys.SFRfloatlogSFR2Star formation rate derived from H{alpha} luminosity (4)log(solMass.yr**-1)phys.SFRfloatlogSFR3Star formation rate derived from UV luminosity (5)log(solMass.yr**-1)phys.SFRfloatlogSFR4Extinction uncorrected star formation rate derived from UV luminosity (6)log(solMass.yr**-1)phys.SFRfloatE(B-V)1? Redenning from IRX=LIR/LUV (Hao et al., 2011ApJ...741..124H)magphot.color.excessfloatnullableE(B-V)2? Redenning from R=Ha/Hbmagphot.color.excessfloatnullableE(B-V)3? Redenning from {beta}=UV slope (Takeuchi et al., 2012ApJ...755..144T)magphot.color.excessfloatnullablesrcDetails from the sources catalogs (SDSS-DR7, GALEX-DR5, Hershecl-PEP, Morphologymeta.ref.urlcharSloanDisplay the SDSS data for this galaxymeta.ref.urlcharPEPDisplay the PEP DR1 (Lutz et al., 2011, Cat. J/A+A/532/A90) datameta.ref.urlchar