J/A+AS/109/293ivo://CDS.VizieR/J/A+AS/109/293CDSGREBEL E.K.ROBERTS W.J.1999-03-01T15:30:28Z1999-03-01T16:29:54ZCDS support team

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

cds-question@unistra.frextinctioninterstellar-mediumstellar-atmospheres(no description available)1995A&AS..109..293Ghttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/109/293CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+AS/109/293https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/109/293http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/109/293https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+AS/109/293https://vizier.iucaa.in/viz-bin/votable?-source=J/A+AS/109/293http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+AS/109/293GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/A+AS/109/293/coeff2*Actual coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintBandQuantity, e.g., filter or colourmeta.code;instr.filtercharlogg[]? Surface gravitylog(cm.s**-2)phys.gravityfloatnullablen_logg[m ] Lowest surface gravity model when there is no value for logg (1)meta.notechar[Fe/H]Metallicitylog(Sun)phys.abund.Fefloata0Coefficient a0 in the numeratorstat.fit.paramdoublea1Coefficient a1 in the numeratorstat.fit.paramdoublea2[]? Coefficient a2 in the numeratorstat.fit.paramdoublenullablea3[]? Coefficient a3 in the numeratorstat.fit.paramdoublenullablea4[]? Coefficient a4 in the numeratorstat.fit.paramdoublenullablea5[]? Coefficient a5 in the numeratorstat.fit.paramdoublenullablea6[]? Coefficient a6 in the numeratorstat.fit.paramdoublenullablea7[]? Coefficient a7 in the numeratorstat.fit.paramdoublenullablea8[]? Coefficient a8 in the numeratorstat.fit.paramdoublenullableb1[]? Coefficient b1 in the denominatorstat.fit.paramdoublenullableb2[]? Coefficient b2 in the denominatorstat.fit.paramdoublenullableb3[]? Coefficient b3 in the denominatorstat.fit.paramdoublenullableb4[]? Coefficient b4 in the denominatorstat.fit.paramdoublenullableb5[]? Coefficient b5 in the denominatorstat.fit.paramdoublenullableb6[]? Coefficient b6 in the denominatorstat.fit.paramdoublenullableb7[]? Coefficient b7 in the denominatorstat.fit.paramdoublenullableJ/A+AS/109/293/diffbDifferential interstellar extinction in UBVRIStarStar type (1)src.classcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint[Fe/H]MetallicitySunphys.abund.FefloatTeffeffective temperatureKphys.temperature.effectivefloatU-B(U-B) colour indexmagphot.color;em.opt.U;em.opt.BfloatE(U-B)differential interstellar extinction in (U-B)magphot.color.excessfloatR1E(U-B)/E(B-V) ratiophys.absorptionfloatB-V(B-V) colour indexmagphot.color;em.opt.B;em.opt.VfloatE(B-V)differential interstellar extinction in (B-V)magphot.color.excessfloatR2E(B-V)/E(B-V) ratiophys.absorptionfloatV-R(V-R) colour indexmagphot.color;em.opt.V;em.opt.RfloatE(V-R)differential interstellar extinction in (V-R)magphot.color.excessfloatR3E(V-R)/E(B-V) ratiophys.absorptionfloatR-I(R-I) colour indexmagphot.color;em.opt.R;em.opt.IfloatE(R-I)differential interstellar extinction in (R-I)magphot.color.excessfloatR4E(R-I)/E(B-V) ratiophys.absorptionfloatV-I(V-I) colour indexmagphot.color;em.opt.V;em.opt.IfloatE(V-I)differential interstellar extinction in (V-I)magphot.color.excessfloatR5E(V-I)/E(B-V) ratiophys.absorptionfloatJ/A+AS/109/293/diffwDifferential interstellar extinction in CMT1T2T1-T2(T1-T2) colour indexmagphot.colorfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintStarStar type (1)src.classchar[Fe/H]MetallicitySunphys.abund.FefloatTeffeffective temperatureKphys.temperature.effectivefloatC-M(C-M) colour indexmagphot.colorfloatE(C-M)differential interstellar extinction in (C-M)magphot.color.excessfloatR1E(C-M)/E(M-T2) ratiophys.absorptionfloatM-T1(M-T1) colour indexmagphot.colorfloatE(M-T1)differential interstellar extinction in (M-T1)magphot.color.excessfloatR2E(M-T1)/E(M-T2) ratiophys.absorptionfloatE(T1-T2)differential interstellar extinction in (T1-T2)magphot.color.excessfloatR3E(T1-T2)/E(M-T2) ratiophys.absorptionfloatM-T2(M-T2) colour indexmagphot.colorfloatE(M-T2)differential interstellar extinction in (M-T2)magphot.color.excessfloatR4E(M-T2)/E(M-T2) ratiophys.absorptionfloatJ/A+AS/109/293/coeff1*Rational polynomial coefficientsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintFilterFilters or quantity involved (1)meta.code;instr.filtercharBandQuantity, e.g., filter or colourmeta.code;instr.filtercharlogg[]? Surface gravitylog(cm.s**-2)phys.gravityfloatnullablen_logg[m ] Lowest surface gravity model when there is no value for logg (2)meta.notechar[Fe/H]Metallicitylog(Sun)phys.abund.FefloatnumNumerator degree (3)stat.fit.paramintdenDenominator degree (3)stat.fit.paramintMaxDevLargest deviation (4)stat.fit.paramdoubleTCminLower boundary of the valid range of temperature colour for that fit (5)stat.fit.paramfloatTCmaxUpper boundary of the valid range of temperature colour for that fit (5)stat.fit.paramfloatJ/A+AS/109/293/totbTotal interstellar extinction in UBVRIrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintStarStar type (1)src.classchar[Fe/H]MetallicitySunphys.abund.FefloatTeffEffective temperatureKphys.temperature.effectivefloatA(U)XTotal interstellar extinction in U for airmass 1 (because U filter is defined by atmospheric cutoff)magphys.absorptiondoubleA(B)XTotal interstellar extinction in B for airmass 1 (to allow calculation of U-B.)magphys.absorptiondoubleA(B)Total interstellar extinction in B for airmass 0magphys.absorptiondoubleA(V)Total interstellar extinction in V for airmass 0magphys.absorptiondoubleA(R)Total interstellar extinction in R for airmass 0magphys.absorptiondoubleA(I)Total interstellar extinction in I for airmass 0magphys.absorptiondoubleR(V)Ratio of total to differential extinctionphys.absorptiondoubleR(V)/R(V0)R(V0): same ratio as R(V) but for star with standard spectrum, i.e. T_eff=17000, log(g)=5.0, and [Fe/H]=0.phys.absorptiondoubleJ/A+AS/109/293/totwTotal interstellar extinction in CMT1T2recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintStarStar type (1)src.classchar[Fe/H]MetallicitySunphys.abund.FefloatTeffEffective temperatureKphys.temperature.effectivefloatA(C)Total interstellar extinction in C for airmass 0magphys.absorptiondoubleA(M)Total interstellar extinction in M for airmass 0magphys.absorptiondoubleA(T1)Total interstellar extinction in T1 for airmass 0magphys.absorptiondoubleA(T2)Total interstellar extinction in T2 for airmass 0magphys.absorptiondoubleR(T2)Ratio of total to differential extinctionphys.absorptiondoubleR(T2)/R(V0)R(V0): same ratio as R(T2) but for star with standard spectrum, i.e. T_eff=17000, log(g)=5.0, and [Fe/H]=0.0phys.absorptiondouble