J/ApJS/255/6ivo://CDS.VizieR/J/ApJS/255/6doi:10.26093/cds/vizier.22550006CDSDong J.Huang C.X.Dawson R.I.Foreman-Mackey D.Collins K.A.,Quinn S.N.Lissauer J.J.Beatty T.Quarles B.Sha L.Shporer A.,Guo Z.Kane S.R.Abe L.Barkaoui K.Benkhaldoun Z.Brahm R.,Bouchy F.Carmichael T.W.Collins K.I.Conti D.M.Crouzet N.,Dransfield G.Evans P.Gan T.Ghachoui M.Gillon M.Grieves N.,Guillot T.Hellier C.Jehin E.Jensen E.L.N.Jordan A.Kamler J.,Kielkopf J.F.Mekarnia D.Nielsen L.D.Pozuelos F.J.Radford D.J.,Schmider F.-X.Schwarz R.P.Stockdale C.Tan T.-G.Timmermans M.,Triaud A.H.M.J.Wang G.Ricker G.Vanderspek R.Latham D.W.Seager S.,Winn J.N.Jenkins J.M.Mireles I.Yahalomi D.A.Morgan E.H.Vezie M.,Quintana E.V.Rose M.E.Smith J.C.Shiao B.2021-12-06T19:57:22Z2021-11-24T12:38:36ZCDS support team

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

cds-question@unistra.frexoplanetsstellar-radiisurveysWarm Jupiters-defined here as planets larger than 6 Earth radii with orbital periods of 8-200 days-are a key missing piece in our understanding of how planetary systems form and evolve. It is currently debated whether Warm Jupiters form in situ, undergo disk or high-eccentricity tidal migration, or have a mixture of origin channels. These different classes of origin channels lead to different expectations for Warm Jupiters' properties, which are currently difficult to evaluate due to the small sample size. We take advantage of the Transiting Exoplanet Survey Satellite (TESS) survey and systematically search for Warm Jupiter candidates around main-sequence host stars brighter than the TESS-band magnitude of 12 in the full-frame images in Year 1 of the TESS Prime Mission data. We introduce a catalog of 55 Warm Jupiter candidates, including 19 candidates that were not originally released as TESS objects of interest by the TESS team. We fit their TESS light curves, characterize their eccentricities and transit-timing variations, and prioritize a list for ground-based follow-up and TESS Extended Mission observations. Using hierarchical Bayesian modeling, we find the preliminary eccentricity distributions of our Warm-Jupiter-candidate catalog using a beta distribution, a Rayleigh distribution, and a two-component Gaussian distribution as the functional forms of the eccentricity distribution. Additional follow-up observations will be required to clean the sample of false positives for a full statistical study, derive the orbital solutions to break the eccentricity degeneracy, and provide mass measurements.2021ApJS..255....6Dhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/255/6CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toI/345 : Gaia DR2 (Gaia Collaboration, 2018)IV/38 : TESS Input Catalog - v8.0 (TIC-8) (Stassun+, 2019)J/A+A/517/L1 : Radial velocities of WASP-8b planet (Queloz+, 2010)J/A+A/568/A81 : WASP-117b photometry and radial velocities (Lendl+, 2014)J/ApJ/790/146 : Planets in Kepler's multi-transiting systems (Fabrycky+, 2014)J/A+A/570/A64 : WASP-104b and WASP-106b photometry (Smith+, 2014)J/A+A/587/A64 : Physical properties of giant exoplanets (Santerne+, 2016)J/ApJ/831/64 : Mass-metallicity relation for giant planets (Thorngren+, 2016)J/ApJ/834/17 : Mass & radius of planets, moons, low mass stars (Chen+, 2017)J/MNRAS/465/3693 : 7 WASP-South transiting exoplanets (Hellier+, 2017)J/AJ/156/18 : Binary companions of evolved stars (Price-Whelan+, 2018)J/AJ/156/102 : TESS Input Catalog and Candidate Target List (Stassun+, 2018)J/AJ/156/234 : KELT transit false positive catalog for TESS (Collins+, 2018)J/AJ/157/191 : Light curve & radial velocities for TOI-172 (Rodriguez+, 2019)J/AJ/158/25 : Automated triage and vetting of TESS candidates (Yu+, 2019)J/AJ/158/45 : TESS light curve & radial velocities for HD 1397 (Brahm+, 2019)J/AJ/158/239 : Metal-rich host stars abundances & EWs (Teske+, 2019)J/AJ/159/145 : RVs & opt. photometry of the host star TOI-677 (Jordan+, 2020)J/AJ/160/235 : Opt. photometry and RVs of TOI-481b and TOI-892b (Brahm+, 2020)J/AJ/160/239 : Cluster difference imaging phot. survey. II. (Bouma+, 2020)J/AJ/161/97 : Radial Velocities of TOI-811 and TOI-852 (Carmichael+, 2021)J/AJ/161/194 : LCs & RVs of 5 exoplanets discovered by TESS (Rodriguez+, 2021)J/AJ/161/235 : Radial velocity of TOI-201 (Hobson+, 2021)J/ApJS/254/39 : Exoplanet candidates from TESS first 2yr obs (Guerrero+, 2021)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/255/6https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/255/6http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/255/6https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/255/6https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/255/6http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/255/6GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJS/255/6/table4 (Warm Jupiter candidates discovered in Year 1 TESS Full-Frame Images)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/255/6/table4?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/255/6/table4?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/255/6/table4?GETtext/xml+votable180.050000true4.4464678-66.35890670.0055555555555555566/16432 21614 21893 21912 22034 23027 23384 23600 24697 24889 25283 26918 32826 33145 33449 33723 33733 33875 33892 34068 34268 36965 37263 37426 37448 37656 37751 37770 38026 38287 38582 38950 38982 39016 39075 39140 39181 39281 39489 40668 41769 41875 42065 43038 43378 43432 43553 45354 45382 47106 47717 47737 47756 48327https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/255/6?format=asciidefaultJ/ApJS/255/6/table4Warm Jupiter candidates discovered in Year 1 TESS Full-Frame ImagesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTIC[4598935/464300749] TESS Input Catalog IDmeta.id;meta.mainlongPlTESS Objects of Interest namemeta.id.assoccharRs[0.68/2.3] Stellar radius derived from the isochrone fittingsolRadphys.size.radiusfloate_Rs[0.016/0.15] Rs downwards uncertaintysolRadstat.errorfloatE_Rs[0.016/0.15] Rs upwards uncertaintysolRadstat.error;stat.maxfloatRho[0.08/2.2] Stellar mean density in solar units derived from the isochrone fittingSunphys.densityfloate_Rho[0.007/1.55] Rho downwards uncertaintySunstat.errorfloatE_Rho[0.007/1.55] Rho upwards uncertaintySunstat.error;stat.maxfloatRhoc[0.059/4.9] Stellar mean density inferred from light curves (1)Sunphys.densityfloate_Rhoc[0.007/2.3] Rhoc downwards uncertaintySunstat.errorfloatE_Rhoc[0.009/2.2] Rhoc upwards uncertaintySunstat.error;stat.maxfloatdelta[1.28/35.7] Transit depth in parts per thousand, derived from the light-curve fittingsrc.var.amplitudefloate_delta[0.057/17] Delta downwards uncertaintystat.error;pos.eq.decfloatE_delta[0.076/77] Delta upwards uncertaintystat.error;stat.maxfloatRp[5.83/17.75] Planet radius derived from the light-curve fitting(6.3781x10+6m)phys.size.radiusfloate_Rp[0.18/3.9] Rp downwards uncertainty(6.3781x10+6m)stat.errorfloatE_Rp[0.2/11.3] Rp upwards uncertainty(6.3781x10+6m)stat.error;stat.maxfloatb[0.13/0.99] Impact parameter, b, derived from the light-curve fittingsrc.impactParamfloate_b[0.05/0.4] B downwards uncertaintystat.errorfloatE_b[0.033/0.31] B upwards uncertaintystat.error;stat.maxfloatPer[7.87/139.31] Orbital period derived from the light-curve fittingdtime.periodfloate_Per[0/1.5] Per downwards uncertaintydstat.errorfloatE_Per[0/1.5] Per upwards uncertaintydstat.error;stat.maxfloatTc[1243.91/1652.83] Conjunction time, T_c_, derived from the light-curve fittingdtime.epochdoublee_Tc[0/0.019] Tc downwards uncertaintydstat.errorfloatE_Tc[0/0.019] Tc upwards uncertaintydstat.error;stat.maxfloatecc[0.052/0.78] Eccentricity inferred from light curvessrc.orbital.eccentricityfloate_ecc[0.05/0.3] 68% lower HPD interval in eccstat.errorfloatE_ecc[0.09/0.4] 68% upper HPD interval in eccstat.error;stat.maxfloatomegaThe 68% highest posterior density (HPD) argument of periapse inferred from light curvesdegsrc.orbital.periastroncharelit[0.0046/0.43]? Median eccentricity from literature (see Ref)src.orbital.eccentricityfloatnullablee_elit[0.001/0.065]? 68% lower interval in elitstat.errorfloatnullableE_elit[0.0027/0.04]? 68% upper interval in elitstat.error;stat.maxfloatnullableolit[35/358]? Median of the argument of periapse from literature (see Ref)src.orbital.periastronintnullablee_olit[0/130]? 68% lower interval in olitstat.errorintnullableE_olit[0/120]? 68% upper interval in olitstat.error;stat.maxintnullableSig[0.1/27.1]? Significance level of the TTV signal (2)stat.snrfloatnullableTSM[1/100]? Transmission Spectroscopy Metric score (3)stat.fit.paramintnullableONameOther name (4)meta.idcharRefReference(s) (5)meta.ref;pos.framecharSimbadSimbad column added by the CDSmeta.ref.urlchar_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.main