J/ApJ/636/1098ivo://CDS.VizieR/J/ApJ/636/1098doi:10.26093/cds/vizier.16361098CDSBryden G.Beichman C.A.Trilling D.E.Rieke G.H.Holmes E.K.,Lawler S.M.Stapelfeldt K.R.Werner M.W.Gautier T.N.Blaylock M.,Gordon K.D.Stansberry J.A.Su K.Y.L.2017-10-09T13:34:44Z2007-06-17T11:28:14ZCDS support team

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

cds-question@unistra.frf-starsinfrared-sourcesdwarf-starsWe have searched for infrared excesses around a well-defined sample of 69 FGK main-sequence field stars. These stars were selected without regard to their age, metallicity, or any previous detection of IR excess; they have a median age of 4Gyr.2006ApJ...636.1098Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/636/1098CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/MNRAS/325/1365 : Solar neighbourhood metallicity distributionJ/A+AS/129/237 : G and K dwarfs abundances (Feltzing+ 1998)J/A+A/377/911 : Age-metallicity relation in solar neighbourhoodJ/ApJ/555/932 : IR fluxes of solar-type stars (Spangler+, 2001)J/ApJS/152/261 : Chromospheric Ca II emission in nearby stars (Wright+ 2004)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/636/1098https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/636/1098http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/636/1098https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/636/1098https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/636/1098http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/636/1098GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/636/1098/table1 (FGK survey stars)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/636/1098/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/636/1098/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/636/1098/table1?GETtext/xml+votable180.050000true1.653266429.02150170.0055555555555555566/137 679 684 706 934 1341 1875 2472 3102 3932 4854 5009 5304 5522 5836 5853 6066 6308 6523 6926 6941 7763 8094 8476 8790 8985 8995 9403 9476 9835 10375 10598 10812 11403 11691 11834 12238 12592 13763 13778 14278 14573 15174 15356 15962 16069 16679 16883 17171 18139 18614 19585 19912 20127 20145 20328 20440 20701 21177 21185 23190 23230 23342 23369 24028 24160 24729 24777 24924 25231 26521 26575 26975 28122 28605 30176 30878 30965 31130 32192 32757 32812 32848 32930 33552 33717 33849 34817 34864 35064 35079 35353 36365 36379 36564 36664 37408 37585 40242 40692 40932 41143 42845 43595 43639 43688 43804 43989 45143 45364 45485 45535 45564 45668 45669 45865 46640 46681 46925 46982 47589 47910 47997 48355 487052.4016587514425055e-21 1.000830682546041e-20https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/636/1098?format=asciiInfrareddefaultJ/ApJ/636/1098/table1FGK survey starsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintHDThe HD number (Cat. III/135)meta.id;meta.mainintprimaryn_HD[ab] a = Observed, b = Known planet-bearing star.meta.notecharIRSimbad column added by the CDSmeta.ref.urlcharSpTypeSIMBAD MK spectral typesrc.spTypecharVmagSIMBAD visual magnitude (2)magphot.mag;em.opt.VfloatAge? The Wright et al. (2004, Cat. J/ApJS/152/261) age (3)Gyrtime.agefloatnullableAgeMin? Minimum ageGyrtime.age;stat.minfloatnullableAgeMax? Maximum ageGyrtime.age;stat.maxfloatnullabler_AgeReference(s) for Agemeta.ref;pos.framechar[Fe/H]? The average [Fe/H] abundancelog(Sun)phys.abund.Fe;stat.meanfloatnullablee_[Fe/H]? Dispersion in Abundlog(Sun)stat.error;phys.abund.Fefloatnullableo_[Fe/H]Number of estimates in Abundmeta.numberintRefsAdditional reference(s)meta.ref;pos.framecharWrightDisplay data from Wright et al., Cat. J/ApJS/152/261meta.ref.urlcharSimbadSimbad column added by the CDSchar_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.main_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainJ/ApJ/636/1098/refsReferencesComCommentmeta.notecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRefReference codemeta.notecharBibcodeBibcodemeta.bib.bibcodecharAutAuthor's namemeta.bib.authorcharJ/ApJ/636/1098/table2Measured and predicted fluxes at 24 and 70{mu}mrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintHDThe HD numbermeta.id;meta.mainintn_HD[de] Note on IR excess (1)meta.notecharMIPS24umMeasured MIPS 24{mu}m flux densitymJyphot.flux.density;em.IR.15-30umfloatStar24umPredicted 24{mu}m flux densitymJyphot.flux.density;em.IR.15-30umfloatRat24umThe MIPS/predicted 24{mu}m flux density ratiostat.fit.omcfloatMIPS70umMeasured MIPS 70{mu}m flux densitymJyphot.flux.density;em.IR.30-60umfloate_MIPS70umUncertainty in MIPS70ummJystat.errorfloatStar70umPredicted 70{mu}m flux densitymJyphot.flux.density;em.IR.30-60umfloatRat70umThe MIPS/predicted 70{mu}m flux density ratiostat.fit.omcfloatS/NThe 70{mu}m signal-to-noise ratiostat.snrfloatchi70Significance of excess (Eq. 1)stat.fit.goodnessfloatFDust? Dust flux density at 70{mu}m (2)mJyphot.flux.density;em.IR.30-60umfloatnullablel_LDustLimit flag on LDustmeta.code.errorcharLDustDust luminosity from 70{mu}m emission (3)phys.luminosity;em.IRdoubleSimbadSimbad column added by the CDSchar