J/A+A/651/A70ivo://CDS.VizieR/J/A+A/651/A70doi:10.26093/cds/vizier.36510070CDSDesidera S.Chauvin G.Bonavita M.Messina S.LeCoroller H.Schmidt T.,Gratton R.Lazzoni C.Meyer M.Schlieder J.Cheetham A.Hagelberg J.,Bonnefoy M.Feldt M.Lagrange A-M.Langlois M.Vigan A.Tan T.G.,Hambsch F.-J.Millward M.Alcala J.Benatti S.Brandner W.Carson J.,Covino E.Delorme P.D'Orazi V.Janson M.Rigliaco E.Beuzit J.-L.,Biller B.Boccaletti A.Dominik F.Cantalloube C.Fontanive C.,Galicher R.Henning T.Lagadec E.Ligi R.Maire A-L.Menard F.,Mesa D.Mueller A.Samland M.Schmid H.M.Sissa E.Turatto M.Udry S.,Zurlo A.Asensio-Torres R.Kopytova T.Rickman E.Abe L.Antichi J.,Baruolo A.Baudoz P.Baudrand J.Blanchard P.Bazzon A.Buey T.,Carbillet M.Carle M.Charton J.Cascone E.Claudi R.Costille A.,Deboulbe A.De Caprio V.Dohlen K.Fantinel D.Feautrier P.Fusco T.,Gigan P.Giro E.Gisler D.Gluck L.Hubin N.Hugot E.Jaquet M.,Kasper M.Madec F.Magnard Y.Martinez P.Maurel D.Le Mignant D.,Moeller-Nilsson O.Llored M.Moulin T.Origne A.Pavlov A.Perret D.,Petit C.Pragt J.Puget P.Rabou P.Ramos J.Rigal F.Rochat S.,Roelfsema R.Rousset G.Roux A.Salasnich B.Sauvage J.-F.Sevin A.,Soenke C.Stadler E.Suarez M.Weber L.Wildi F.2024-08-06T20:01:17Z2021-07-14T08:45:30ZCDS support team

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

cds-question@unistra.frpre-main-sequence-starsphotometryeffective-temperaturestellar-massesstellar-agesLarge surveys with new-generation high-contrast imaging instruments are needed to derive the frequency and properties of exoplanet populations with separations from 5 to 300au. A careful assessment of the stellar properties is crucial for a proper understanding of when, where, and how frequently planets form, and how they evolve. The sensitivity of detection limits to stellar age makes this a key parameter for direct imaging surveys. We describe the SpHere INfrared survey for Exoplanets (SHINE), the largest direct imaging planet-search campaign initiated at the VLT in 2015 in the context of the SPHERE Guaranteed Time Observations of the SPHERE consortium. In this rst paper we present the selection and the properties of the complete sample of stars surveyed with SHINE, focusing on the targets observed during the rst phase of the survey (from February 2015 to February 2017). This early sample composed of 150 stars is used to perform a preliminary statistical analysis of the SHINE data, deferred to two companion papers presenting the survey performance, main discoveries, and the preliminary statistical constraints set by SHINE. We describe the SpHere INfrared survey for Exoplanets (SHINE), the largest direct imaging planet-search campaign initiated at the VLT in 2015 in the context of the SPHERE Guaranteed Time Observations of the SPHERE consortium. In this rst paper we present the selection and the properties of the complete sample of stars surveyed with SHINE, focusing on the targets observed during the first phase of the survey (from February 2015 to February 2017). This early sample composed of 150 stars is used to perform a preliminary statistical analysis of the SHINE data, deferred to two companion papers presenting the survey performance, main discoveries, and the preliminary statistical constraints set by SHINE. Based on a large database collecting the stellar properties of all young nearby stars in the solar vicinity (including kinematics, membership to moving groups, isochrones, lithium abundance, rotation, and activity), we selected the original sample of 800 stars that were ranked in order of priority according to their sensitivity for planet detection in direct imaging with SPHERE. The properties of the stars that are part of the early statistical sample were revisited, including for instance measurements from the GAIA Data Release 2. Rotation periods were derived for the vast majority of the late-type objects exploiting TESS light curves and dedicated photometric observations. The properties of individual targets and of the sample as a whole are presented.2021A&A...651A..70Dhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/651/A70CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+A/651/A71 : SHINE II (Langlois+, 2021)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/651/A70https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/651/A70http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/651/A70https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/651/A70https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/651/A70http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/651/A70GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/651/A70/table5 (Summary of target parameters: names, coordinates, and photometry (V, J, H and K magnitude, B-V and V-I colors))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/651/A70/table5?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/651/A70/table5?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/651/A70/table5?GETtext/xml+votable180.050000true1.46875-41.75305560.0055555555555555566/8717 12436 12592 12848 16393 17552 17887 18797 19509 20125 20505 21180 21289 21788 22146 22289 22773 22964 23230 23895 25015 25793 26924 27392 27735 27884 28784 29569 29993 30419 30477 30655 30793 30826 31281 32844 32891 33312 33361 33449 33818 33850 34054 34244-34245 34436 34683 34733 34823 34825 34830 34886 34909 34930 35077 35497 35861 36036 36308 36664 36969 37012 37175 37414 37968 37973 38272 38489 38687 38706 38800 38936 38950 39019 39044 39123 39162 39284 39489 39579 39735 40717 41641 41652 41759 42072 42096 42252 42401 42425 42493 42601 42677 42708 42714 42754 42808 42913 42923 43014 43073 43097 43130 43177 43259 43276 43377 43402 43510 43676-43677 44069 44139 44319 44363 44669 45152 45247 45351 45544 45746 45927 46113 46383 46692 46922 46925 46939 47120 47205 47209 47287 47366 47598 47626 47703 47740 47863 47941 47943 48045 48163 48274 48546 48559 486271.1166583743361574e-19 3.916500758235022e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/651/A70?format=asciidefaultJ/A+A/651/A70/table5Summary of target parameters: names, coordinates, and photometry (V, J, H and K magnitude, B-V and V-I colors)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/150] Sequential numbermeta.recordintNameNamemeta.id;meta.maincharONameOther namemeta.idcharSimbadNameSimbad column added by the CDSmeta.idcharnullableOName2Other namemeta.idcharRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainGmag? Gaia DR2 magnitudemagphot.mag;em.optfloatnullableBP-RP? Gaia DR2 BP-RP colour indexmagphot.color;em.opt.B;em.opt.RfloatnullableVmagV magnitudemagphot.color;em.opt.V;em.opt.RfloatB-V? B-V colour indexmagphot.color;em.opt.B;em.opt.VfloatnullableV-I? V-I colour indexmagphot.color;em.opt.V;em.opt.IfloatnullableJmag2MASS J magnitudemagphot.mag;em.IR.JfloatHmag2MASS H magnitudemagphot.mag;em.IR.HfloatKmag2MASS K magnitudemagphot.mag;em.IR.KfloatJ/A+A/651/A70/table6Summary of target parameters: name, trigonometric parallax , proper motion, radial velocity, U, V, W space velocities, moving group membershiprecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/150] Sequential numbermeta.recordintNameNamemeta.id;meta.maincharONameOther namemeta.idcharplxParallaxmaspos.parallaxfloate_plxParallax errormasstat.error;pos.parallaxfloatr_plxReference for plx (1)meta.ref;pos.framecharpmRAProper motion along RAmas/yrpos.pm;pos.eq.rafloate_pmRAProper motion along RA errormas/yrstat.error;pos.pm;pos.eq.rafloatpmDEProper motion along DEmas/yrpos.pm;pos.eq.decfloate_pmDEProper motion along DE errormas/yrstat.error;pos.pm;pos.eq.decfloatr_pmRAReference for proper motions (1)meta.ref;pos.pm;pos.eq.racharRV? Radial velocitykm/sphys.veloc;pos.heliocentricfloatnullablee_RV? Radial velocity errorkm/sstat.errorfloatnullabler_RVReference for RV (1)meta.ref;pos.framecharUvel? Galactic U velocitykm/sphys.veloc;pos.cartesian.xfloatnullableVvel? Galactic V velocitykm/sphys.veloc;pos.cartesian.yfloatnullableWvel? Galactic W velocitykm/sphys.veloc;pos.cartesian.zfloatnullableMembMoving group membershipmeta.code.membercharJ/A+A/651/A70/table7Summary of target parameters: name, X-ray luminosity, RX=logLX/Lbol, logRHK, rotation period, vsini, Lithium 6708 EW, effective temperature, and stellar massNameNamemeta.id;meta.maincharRX? X-ray-to-bolometric luminosity ratiophys.luminosity;arith.ratiofloatnullableS? S value (1)stat.valuefloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/150] Sequential numbermeta.recordintONameOther namemeta.idcharlogLX? X-ray luminositylog(1e-07W)phys.luminosity;em.X-rayfloatnullablelogRHK? Mount Wilson logR_HK_ indexphot.flux;arith.ratiofloatnullabler_logLXReference for logLX (2)meta.ref;pos.framecharProt? Rotational perioddtime.periodfloatnullablee_Prot? Rotational period errordstat.errorfloatnullableAmp? Amplitude of variationmagarith.rate;phot.magdoublenullabler_ProtRotational period references (2)meta.ref;pos.framecharvsini? Rotational velocitykm/sphys.veloc.rotatfloatnullabler_vsiniRotational velocity reference (2)meta.refcharEWLi? Lithium equivalent width0.1pmspect.line.eqWidthfloatnullabler_EWLiLithium equivalent width reference (2)meta.ref;pos.framecharJ/A+A/651/A70/table8Summary of target parameters: name, spectral type, effective temperature, stellar mass, and flag on the presence of disksrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/150] Sequential numbermeta.recordintNameNamemeta.id;meta.maincharONameOther namemeta.idcharSpTypeSpectral typesrc.spTypecharTeffEffective temperatureKphys.temperature.effectiveinte_TeffEffective temperature errorKstat.error;phys.temperature.effectiveintMassStar masssolMassphys.massfloate_MassStar mass errorsolMassstat.error;phys.massfloatDiskDisk flags (1)meta.codecharJ/A+A/651/A70/table9Summary of target parameters: stellar agesb_AgeMinimum ageMyrtime.age;stat.minintB_AgeMaximum ageMyrtime.age;stat.maxintr_AgeAge reference (1)meta.ref;pos.framecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/150] Sequential numbermeta.recordintNameNamemeta.id;meta.maincharONameOther namemeta.idcharOName2Other namemeta.idcharAgeAgeMyrtime.ageintJ/A+A/651/A70/table10Wide companions to targets in the samplerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameSPH target namemeta.id;meta.maincharCompCompanion namemeta.id.assoccharrho? Angular separationarcsecpos.angDistancefloatnullablerhol? Linear separationAUpos.distance;phys.sizeintnullableDmag? Magnitude difference (1)magphot.mag;arith.difffloatnullableBandBand for magnitude differenceinstr.bandpasscharMassT? Targert mass (2)solMassphys.massfloatnullableMassCCompanion mass (2)solMassphys.massfloatRemRemarksmeta.notecharSeqSequential number of targetmeta.recordintJ/A+A/651/A70/table11Parameters adopted in the original selectionrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/150] Sequential numbermeta.recordintNameNamemeta.id;meta.maincharONameOther namemeta.idcharOName2Other namemeta.idcharMass? MasssolMassphys.massfloatnullableDist? Distancepcpos.distancefloatnullableAge? AgeMyrtime.ageintnullableMembMoving group membershipmeta.code.membercharPrio? Prioritymeta.codeintnullableMF15? Merit function for cut-offs of planet distribution to 15austat.fit.goodnessfloatnullableMF30? Merit function for cut-offs of planet distribution to 30austat.fit.goodnessfloatnullableMF50? Merit function for cut-offs of planet distribution to 50austat.fit.goodnessfloatnullable