J/A+A/653/A98ivo://CDS.VizieR/J/A+A/653/A98doi:10.26093/cds/vizier.36530098CDSMontalto M.Piotto G.Marrese P.M.Nascimbeni V.Prisinzano L.,Granata V.Marinoni S.Desidera S.Ortolani S.Aerts. C.Alei E.,Altavilla G.Benatti S.Borner A.Cabrera J.Claudi R.Deleuil M.,Frabrizio M.GizonL.Goupil M.J.Heras A.M.Magrin D.Malavolta L.,Mas-Hesse J.M.Pagano I.Paproth C.Pertenais M.Pollacco D.,Ragazzoni R. Ramsay G.Rauer H.Udry S.2023-11-24T09:24:13Z2021-09-15T08:09:13ZCDS support team

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

cds-question@unistra.frsurveysastrometryproper-motionsphotometryf-starsvisible-astronomytrigonometric-parallaxstellar-distancestellar-masseseffective-temperatureThe ESA PLAnetary Transits and Oscillations of stars (PLATO) mission will search for terrestrial planets in the habitable zone of solar-like stars. Because of telemetry limitations PLATO targets need to be pre-selected. In this paper we present an all sky catalog that will be fundamental to select the best PLATO fields and the most promising target stars, derive their fundamental parameters, analyze the instrumental performances and then plan and optimize follow-up observations. This catalog also represents a valuable resource for the general definition of stellar samples optimized for the search of transiting planets. We used Gaia Data Release 2 (DR2) astrometry and photometry and 3D maps of the local interstellar medium to isolate FGK (V<=13) and M(V<=16) dwarfs and subgiant stars. We present the first public release of the all sky PLATO Input Catalog (asPIC1.1) containing a total of 2675539 stars among which 2378177 FGK dwarfs and subgiants and 297362 M dwarfs. The median distance in our sample is 428pc for FGK stars and 146 pc for M dwarfs, respectively. We derived the reddening of our targets and developed an algorithm to estimate stellar fundamental parameters (Teff, radius, mass) from astrometric and photometric measurements. We show that our overall (internal+external) uncertainties on the stellar parameters determination is ~230K (4%) for the effective temperatures, ~0.1R_{sun}_ (9%) for the stellar radii and ~0.1M_{sun}_ (11%) for the stellar mass. We release a special target list containing all known planet hosts cross-matched with our catalog.2021A&A...653A..98Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/653/A98CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toI/345 : Gaia DR2 (Gaia Collaboration, 2018)I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/653/A98https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/653/A98http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/653/A98https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/653/A98https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/653/A98http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/653/A98GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/653/A98/aspic1_1 (All-sky PLATO input catalog (2675539 sources))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/653/A98/aspic1_1?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/653/A98/aspic1_1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/653/A98/aspic1_1?GETtext/xml+votable180.050000true109.83651272444-89.947237236550.0055555555555555560/0-11 6/3.322582951404819e-19 3.852589004194616e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/653/A98?format=asciiOpticaldefaultJ/A+A/653/A98/aspic1_1All-sky PLATO input catalog (2675539 sources)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintPICDR1idPLATO identifier for asPIC1.1meta.id;meta.mainintPICDR1PLATO identifier for asPIC1.1 with version number, PIC DR1 NNNNNNNNmeta.idcharGaiaDR2Gaia DR2 sourceIdmeta.idRAICRSBarycentric right ascension of the source in ICRS at Ep=2015.5degpos.eq.ra;meta.mainindexede_RAICRSStandard error e_RA*=e_RA x cosDE of the right ascension in ICRS at Ep=2015.5masstat.error;pos.eq.rafloatDEICRSBarycentric declination of the source in ICRS at Ep=2015.5degpos.eq.dec;meta.mainindexede_DEICRSStandard error of the declination in ICRS at Ep=2015.5masstat.error;pos.eq.decfloatPlxParallaxmaspos.parallaxdoublee_PlxStandard error on parallaxmasstat.error;pos.parallaxfloatpmRA*Proper motion in right ascension direction pmRA*=pmRAxcosDE in ICRS at Ep=2015.5mas/yrpos.pm;pos.eq.radoublee_pmRA*Standard error on proper motion in right ascension directionmas/yrstat.error;pos.pm;pos.eq.rafloatpmDEProper motion in declination direction in ICRS at Ep=2015.5mas/yrpos.pm;pos.eq.decdoublee_pmDEStandard error on proper motion in declination directionmas/yrstat.error;pos.pm;pos.eq.decfloatpmThe total proper motion calculated as pm = sqrt(pmRA^2^ + pmDE^2^)mas/yrpos.pm;pos.eq.dec;meta.modelleddoublee_pmError on the total proper motionmas/yrstat.errorfloatEpoch[2015.5] Reference epoch to which the astrometric source parameters are referredyrmeta.ref;time.epochfloatindexedFGMean flux in the G bandphot.flux.density;em.optdoublee_FGError on G band mean fluxstat.errordoubleGmagMean magnitude in the G bandmagphot.mag;em.optdoublee_GmagError on mean magnitude in the G bandmagstat.error;phot.magdoublee_FBPError on mean flux in the integrated BP bandstat.errordoubleBPmagMean magnitude in the integrated BP bandmagphot.mag;em.opt.Bdoublee_BPmagError in the mean magnitude in the integrated BP bandmagstat.error;phot.magdoubleFRPMean flux in the integrated RP bandphot.flux.density;em.opt.Rdoublee_FRPError on mean flux in the integrated RP bandstat.errordoubleRPmagMean magnitude in the integrated RP bandmagphot.mag;em.opt.Rdoublee_RPmagError in the mean magnitude in the integrated RP bandmagstat.error;phot.magdoubleE(BP/RP)BP/RP excess factorarith.factordoubleBP-RPGBP - GRP colormagphot.color;em.opt.B;em.opt.RdoubleBP-GGBP - G colormagphot.color;em.opt;em.optdoubleG-RPG - GRP colormagphot.color;em.opt;em.optdoubleGLONGalactic longitude of the object at Ep=2015.5degpos.galactic.lonGLATGalactic latitude of the object at Ep=2015.5degpos.galactic.latdoubleELONEcliptic longitude of the object at Ep=2015.5degpos.ecliptic.lonELATEcliptic latitude of the object at Ep=2015.5degpos.ecliptic.latdoublerestThe estimated distance (1)pcpos.distancedoublerloThe lower bound of the confidence interval of the estimated distance (1)pcstat.errordoublerhiThe higher bound of the confidence interval of the estimated distance (1)pcstat.errordoublee_restThe error in the estimated distance calculated as e_rest = 0.5(rhi - rlo)pcstat.errordoubleAGEstimate of the extinction AG in the G bandmagphys.absorptiondoublee_AGUncertainty on AG estimatemagstat.errordoubleE(BP-RP)Estimate of reddening E(GBP-GRP)magphot.color.excessdoublee_E(BP-RP)Uncertainty on reddening E(GBP - GRP)magstat.errordoubleE(B-V)Estimate of reddening E(B-V)magphot.color.excessdoublee_E(B-V)Uncertainty on E(B-V) reddeningmagstat.errordoubleextStatus[0/1] extStatus value. If extStatus=1 the star is outside the limits of the reddening map (2)meta.codeint(BP-RP)0Dereddened (GBP - GRP) colormagphot.color;em.opt.B;em.opt.Rdoublee_(BP-RP)0Error on dereddened (GBP - GRP) colormagstat.errordoublegaiaV0Dereddened apparent visual magnitude V in the Johnson-Cousin systemmagphot.mag;em.opt.Vdoublee_gaiaV0Error on intrinsic visual magnitudemagstat.errordoubleBJgaiaMV0Absolute intrinsic visual magnitude obtained as: BJgaiaMV0 = gaiaV0 -5log10rest + 5magphys.magAbsdoublee_BJgaiaMV0Error on absolute intrinsic visual magnitudemagstat.errordoublegaiaVVisual apparent magnitude in the Johnson-Cousin system obtained as: gaiaV = gaiaV0 + 3.1E(B-V)magphot.mag;em.opt.Vdoublee_gaiaVError on apparent visual magnitude Vmagstat.errordoubleBJgaiaMG0Absolute intrinsic G magnitude obtained as: BJgaiaMG0 = Gmag -5log10rest +5 -AGmagphys.magAbsdoublee_BJgaiaMG0Error on intrinsic absolute G magnitudemagstat.errordoubleTeff? Estimate of stellar effective temperatureKphys.temperature.effectivefloatnullablee_Teff? Uncertainty on Teff estimateKstat.error;phys.temperature.effectivefloatnullableRad? Estimate of stellar radiussolRadphys.size.radiusfloatnullablee_Rad? Uncertainty on stellar radius estimatesolRadstat.errorfloatnullableMass? Estimate of stellar masssolMassphys.massfloatnullablee_Mass? Uncertainty on mass estimatesolMassstat.error;phys.massfloatnullablesourceFlag[0/6] Bitmask indicating if the source is a FGK or M star and if the star hosts known planet(s) (3)meta.codeintcontGMag60? Total G magnitude of the Gaia contaminants within 60 arcsecmagphot.mag;em.optdoublenullablecontN60Total number of Gaia contaminants within 60 arcsecmeta.numberintcontGMag45? Total G magnitude of the Gaia contaminants within 45 arcsecmagphot.mag;em.optdoublenullablecontN45Total number of Gaia contaminants within 45 arcsecmeta.numberintcontGMag30? Total G magnitude of the Gaia contaminants within 30 arcsecmagphot.mag;em.optdoublenullablecontN30Total number of Gaia contaminants within 30 arcsecmeta.numberint_RA.icrsRight ascension (ICRS) at Epoch=J2000, proper motions taken into accountdegpos.eq.raindexed_DE.icrsDeclination (ICRS) at Epoch=J2000, proper motions taken into accountdegpos.eq.decindexedFBPMean flux in the integrated BP bandphot.flux.density;em.opt.Bdouble