J/AJ/167/233ivo://CDS.VizieR/J/AJ/167/233doi:10.26093/cds/vizier.51670233CDSHord B.J.Kempton E.M.-R.Evans-Soma T.M.Latham D.W.Ciardi D.R.,Dragomir D.Colon K.D.Ross G.Vanderburg A.de Beurs Z.L.,Collins K.A.Watkins C.N.Bean J.Cowan N.B.Daylan T.Morley C.V.,Ih J.Baker D.Barkaoui K.Batalha N.M.Behmard A.Belinski A.,Benkhaldoun Z.Benni P.Bernacki K.Bieryla A.Binnenfeld A.,Bosch-Cabot P.Bouchy F.Bozza V.Brahm R.Buchhave L.A.Calkins M.,Chontos A.Clark C.A.Cloutier R.Cointepas M.Collins K.I.,Conti D.M.Crossfield I.J.M.Dai F.de Leon J.P.Dransfield G.,Dressing C.Dustor A.Esquerdo G.Evans P.Fajardo-Acosta S.B.,Fiolka J.Fores-Toribio R.Frasca A.Fukui A.Fulton B.Furlan E.,Gan T.Gandolfi D.Ghachoui M.Giacalone S.Gilbert E.A.Gillon M.,Girardin E.Gonzales E.Grau Horta F.Gregorio J.Greklek-McKeon M.,Guerra P.Hartman J.D.Hellier C.Helm I.Helminiak K.G.Henning T.,Hill M.L.Horne K.Howard A.W.Howell S.B.Huber D.Isopi G.,Jehin E.Jenkins J.M.Jensen E.L.N.Johnson M.C.Jordan A.Kane S.R.,Kielkopf J.F.Krushinsky V.Lasota S.Lee E.Lewin P.,Livingston J.H.Lubin J.Lund M.B.Mallia F.Mann C.R.Marino G.,Maslennikova N.Massey B.Matson R.Matthews E.Mayo A.W.Mazeh T.,McLeod K.K.Michaels E.J.Mocnik T.Mori M.Mraz G.Munoz J.A.,Narita N.Natarajan K.Dyregaard Nielsen L.Osborn H.Palle E.,Panahi A.Papini R.Plavchan P.Polanski A.S.Popowicz A.,Pozuelos F.J.Quinn S.N.Radford D.J.Reed P.A.Relles H.M.Rice M.,Robertson P.Rodriguez J.E.Rosenthal L.J.Rubenzahl R.A.Schanche N.,Schlieder J.Schwarz R.P.Sefako R.Shporer A.Sozzetti A.Srdoc G.,Stockdale C.Tarasenkov A.Tan T.-G.Timmermans M.Ting E.B.,Van Zandt J.Vignes JPWaite I.Watanabe N.Weiss L.M.Wittrock J.,Zhou G.Ziegler C.Zucker S.2024-11-06T20:20:10Z2024-06-28T07:00:02ZCDS support team

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

cds-question@unistra.frexoplanetseffective-temperaturestellar-massesstellar-radiiinfrared-photometryvisible-astronomybroad-band-photometryJWST has ushered in an era of unprecedented ability to characterize exoplanetary atmospheres. While there are over 5000 confirmed planets, more than 4000 Transiting Exoplanet Survey Satellite (TESS) planet candidates are still unconfirmed and many of the best planets for atmospheric characterization may remain to be identified. We present a sample of TESS planets and planet candidates that we identify as "best-in-class" for transmission and emission spectroscopy with JWST. These targets are sorted into bins across equilibrium temperature Teq and planetary radius Rp and are ranked by a transmission and an emission spectroscopy metric (TSM and ESM, respectively) within each bin. We perform cuts for expected signal size and stellar brightness to remove suboptimal targets for JWST. Of the 194 targets in the resulting sample, 103 are unconfirmed TESS planet candidates, also known as TESS Objects of Interest (TOIs). We perform vetting and statistical validation analyses on these 103 targets to determine which are likely planets and which are likely false positives, incorporating ground-based follow-up from the TESS Follow-up Observation Program to aid the vetting and validation process. We statistically validate 18 TOIs, marginally validate 31 TOIs to varying levels of confidence, deem 29 TOIs likely false positives, and leave the dispositions for four TOIs as inconclusive. Twenty-one of the 103 TOIs were confirmed independently over the course of our analysis. We intend for this work to serve as a community resource and motivate formal confirmation and mass measurements of each validated planet. We encourage more detailed analysis of individual targets by the community.2024AJ....167..233Hhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/167/233CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toIV/34 : K2 Ecliptic Plane Input Catalog (EPIC) (Huber+, 2017)IV/38 : TESS Input Catalog - v8.0 (TIC-8) (Stassun+, 2019)VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)J/A+A/337/403 : Low-mass stars evolutionary models (Baraffe+ 1998)J/ApJ/720/1118 : i-band photometry of HAT-P-16 (Buchhave+, 2010)J/AJ/142/19 : Speckle observations of KOI (Howell+, 2011)J/other/Nat/486.375 : Stellar parameters of KOI stars (Buchhave+, 2012)J/AJ/147/119 : Cat of sources in the Kepler field of view (Coughlin+, 2014)J/ApJ/834/17 : Mass & radius of planets, moons, low mass stars (Chen+, 2017)J/AJ/153/71 : Kepler follow-up observation program I Imaging (Furlan+, 2017)J/ApJ/836/77 : Library of high-S/N optical spectra of FGKM stars (Yee+, 2017)J/AJ/157/43 : WASP-161b, WASP-163b and WASP-170b (Barkaoui+, 2019)J/AJ/157/124 : DAVE. I. Benchmarking K2 vetting tools (Kostov+, 2019)J/A+A/630/A89 : WASP-12b and WASP-43b griz light curves (Parviainen+, 2019)J/AJ/158/141 : Diff photometry & RVs of HAT-P-69 & HAT-P-70 (Zhou+, 2019)J/AJ/161/24 : TRICERATOPS predictions for 384 TOIs (Giacalone+, 2021)J/ApJS/254/39 : Exoplanet candidates from TESS first 2yr obs (Guerrero+, 2021)J/AJ/162/263 : TESS nearby planetary companions to hot Jupiters (Hord+, 2021)J/AJ/162/176 : The solar neighborhood. XLVIII. (Paredes+, 2021)J/ApJS/260/3 : 25 hot-Jupiter properties from HST & Spitzer (Changeat+, 2022)J/A+A/666/A155 : TOI-1468 photometry and radial velocities (Chaturvedi+, 2022)J/AJ/164/15 : Exoplanets Ariel's potential targets (Edwards+, 2022)J/A+A/668/A158 : HD 20329 Radial velocity and activity indices (Murgas+, 2022)J/A+A/667/A14 : Gaia-TESS transit candidates (Panahi+, 2022)J/A+A/669/A109 : TOI-969 light and RV curves (Lillo-Box+, 2023)J/AJ/166/33 : The TESS-Keck Survey. XV. 108 TESS Planets (MacDougall+, 2023)J/A+A/675/A39 : TOI-615, TOI-622, TOI-2641 RVs + ground phot. (Psaridi+, 2023)J/ApJS/265/1 : TESS Grand Unified Hot Jupiter Surveys. II. (Yee+, 2023)J/A+A/684/A83 : Wolf327b RV and spectral line activity indices (Murgas+, 2024)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/167/233https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/167/233http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/167/233https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/167/233https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/167/233http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/167/233GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/AJ/167/233/table4 (Our full best-in-class sample)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/167/233/table4?https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/167/233/table4?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/167/233/table4?GETtext/xml+votable180.050000true153.7090696-47.15493580.0055555555555555566/156 215 712 728 1024 1083 1202 1292 1585 2335 2532 2730 3900 3934 4309 4432 4651 4720 5170 5186 5212 5354 5657 6181 6974 7238 7241 7632 8035 8538 9459 9653 10028 10491 10593 10699 10730 11382 11487 11542 11658 11672 11686 11923 12251 12270 12644 12652 12983 13916 14446 14595 14709 14767 14914 15159 15226 15707 15769 15973 15977 16162 16306 16317 16395 16662 16847 17149 17240 17283 17559 17784 17851 18147 18220 18398 18640 18726 18785-18786 19791 20667 21271 22242 23529 23854 23867 23932 24246 24326 24373 24437 24816 25132 25312 25373 25427 25463 25885 26062 26318 26727 26751 26771 26844 26920 27358 27847 28548 29956 30009 30481 31216 32184 32838 33516 33598 33908 34002 34419 34440 34468 34499 35057 35210 35696 35922 36643 36794 37039 37157 37172 37207 37453 37929 38067 38260 38376 38401 38452 38464 39068 39148 39198 39542 40119 40220 40251 40554 40673 40772 40833 41034 41786 41995 42106 42131 42267 42520 42989 43393 43437 45041 45372 45527 45660 45964 46002 46333 46394 46429 46771 47089 47717 48178 491038.650015785639275e-20 3.852589004194616e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/167/233?format=asciiOpticalInfrareddefaultJ/AJ/167/233/table4Our full best-in-class samplerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintPer[0.17/749] Planet orbital perioddtime.perioddoubleSimbadSimbad column added by the CDSmeta.ref.urlcharMasspJ[0.001/10.2]? Planet mass, Jovian units(1.898187x10+27kg)phys.massdoublenullableE_MasspJUpper uncertainty, MasspJ(1.898187x10+27kg)stat.error;stat.maxchara[0.005/2] Planet semi-major axisauphys.angSize.smajAxis;src.orbitaldoublee[0.0/0.42]? Planet eccentricitysrc.orbital.eccentricitydoublenullablei[69.7/93.1]? Planet inclinationdegsrc.orbital.inclinationdoublenullableb[-0.14/1]? impact parametersrc.impactParamdoublenullableDist[-0.5/372]? Distance, Earth to Planetpcpos.distancedoublenullableS[0.007/19309]? Insolation flux, Sgeophot.flux;arith.ratiodoublenullableTDur[0.3/8.33]? Transit durationhtime.durationdoublenullablea/Rad*[1.6/415] Ratio, planet semi-major axis to stellar radiusphys.size.axisRatiodoubleTeff[2566/9219] Host Star Effective Temperature, starKphys.temperature.effectivefloatMass*[0.05/2.33] Host star masssolMassphys.massdoubleVmag[6.59/18.9]? V band (Vega) magnitudemagphot.mag;em.opt.VdoublenullableJmag[6.07/13.8] 2MASS J band (Vega) magnitudemagphot.mag;em.IR.JdoubleHmag[5.58/13.3] 2MASS H band (Vega) magnitudemagphot.mag;em.IR.HdoubleKsmag[5.54/13] 2MASS Ks band (Vega) magnitudemagphot.mag;em.IR.KdoubleFacFacility that discovered this targetmeta.id;instr.telcharDate.Y[1999/2023] year this target was discoveredyrtime.epochintTESS?[0/1] 1 means the target was discovered by TESSmeta.codeintRadp[0.75/23.4] Planet radius(6.3781x10+6m)phys.size.radiusdoubleE_Radp[0.01/4] Upper uncertainty on Radp(6.3781x10+6m)stat.error;stat.maxdoublee_Radp[0.01/4]? Lower uncertainty, Radp(6.3781x10+6m)stat.errordoublenullableMassp[0.32/3214] Planet mass(5.97236x10+24kg)phys.massdoubleE_Massp[0.01/80]? Upper uncertainty, Massp(5.97236x10+24kg)stat.error;stat.maxdoublenullablee_Massp[0.01/67]? Lower uncertainty, Massp(5.97236x10+24kg)stat.errordoublenullableRp/R*[0.0121/0.50849398] Ratio, planet to stellar radiiarith.ratio;phys.size.radiusdoubleE_Rp/R*Upper uncertainty, Rp/R*stat.error;stat.maxchare_Rp/R*Lower uncertainty, Rp/R*stat.errorcharE_Teff[7/150]? Upper uncertainty, TeffKstat.error;stat.maxfloatnullablee_Teff[7/150]? Lower uncertainty, TeffKstat.error;phys.temperature.effectivefloatnullableRad*[0.12/2.69] Stellar radiussolRadphys.size.radiusdoubleE_Rad*[0.0/0.12]? Upper uncertainty, Rad*solRadstat.error;stat.maxfloatnullablee_Rad*[0.0/0.12]? Lower uncertainty, Rad*solRadstat.errorfloatnullableRAJ2000[1/359] Right Ascension (J2000)degpos.eq.ra;meta.mainDEJ2000[-82/86] Declination (J2000)degpos.eq.dec;meta.mainRAhmsRight Ascension, hms (J2000)pos.eq.racharDEhmsDeclination, dms (J2000)pos.eq.deccharMass*SIStellar Mass, SI unitskgphys.masscharRad*SI? Stellar Radius, SI unitsmmeta.unit;phys.size.radiusnullableRadpSI? Planet radius, SI unitsmmeta.unit;phys.size.radiuslongnullableE_RadpSI[63710/24993433]? Upper uncertainty, RadpSImstat.error;stat.maxintnullablee_RadpSI[70081/24993433]? Lower uncertainty, RadpSImstat.errorintnullableRadpJ[0.06/2.09]? Planet radius, Jovian units(7.1492x10+7m)phys.size.radiusdoublenullableE_RadpJ[0.0008/0.4]? Upper uncertainty, RadpJ(7.1492x10+7m)stat.error;stat.maxdoublenullablee_RadpJ[0.0009/0.4]? Lower uncertainty, RadpJ(7.1492x10+7m)stat.errordoublenullableMasspSIMass of the planet in SI unitskgphys.masscharE_MasspSIUpper uncertainty, MasspSIkgstat.error;stat.maxchare_MasspSILower uncertainty, MasspSIkgstat.errorchare_MasspJLower uncertainty, MasspJ(1.898187x10+27kg)stat.errorchargpSI[1.89/296]? Surface gravity of the planet, SI unitsm.s**-2phys.gravitydoublenullableTeq[161/2997] Planetary equilibrium temperatureKphys.temperaturedoubleTSM[3.23/963] Transmission spectroscopy metric valuephys.transmission;instr.filterdoubleESM[0.005/1140] Emission spectroscopy metric valuephys.emissMeasuredoubleEDepthEstimated depth of secondary eclipsemagphys.absorption.opticalDepthcharSFsizeEstimated size of transmission spectra featuresphys.sizecharARVel[0.47/1618]? Predicted radial velocity semi-amplitudem.s**-1phys.veloc;pos.heliocentricdoublenullableTIC? TESS Input Catalog IDmeta.idlongnullableTeqK2[81/3230]? Equilibrium temperature reported by ExoFOPKphys.temperaturedoublenullable[g*][3.53/5.15]? log, surface gravity, host star, CGS unitslog(cm.s**-2)meta.unitdoublenullableTmag[7.62/15.8]? TESS magnitudemagphot.mag;em.optdoublenullableImag[10.2/15]? I band Vega magnitudemagphot.mag;em.opt.IfloatnullableTransm?[0/1] Flag denoting if the target is part of the transmission spectroscopy best-in-class listmeta.codeintEmiss?[0/1] Flag denoting if the target is part of the emission spectroscopy best-in-class listmeta.codeintDispDisposition assigned to it after our vetting and validationmeta.codecharvespaFPFalse positive probability from VESPA analysisstat.fit.goodnesscharTRIFPFalse positive probability from TRICERATOPS analysisstat.fit.goodnesscharTRINFPNearby false positive probability from TRICERATOPS analysisstat.fit.goodnesscharNamePlanet namemeta.id;meta.maincharMetMethod by which this target was discoveredmeta.code;obscharJ/AJ/167/233/table5Follow-up observations used in synthesis of TFOP dispositions that were incorporated into our vetting and validation analysisTypeObservation Type, Photometry, Spectroscopy, Speckle imagingmeta.notecharTOITESS Object of interestmeta.id;meta.mainfloatTelTelescope usedinstr.setupcharCamCamera/Instrument usedmeta.id;instrcharFiltFilter/Bandpass usedinstr.setupcharDateObservation Date (MM/DD/YY)time.epoch;obscharIndex[1/960] Indexmeta.id;meta.numberintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint