J/AJ/159/173ivo://CDS.VizieR/J/AJ/159/173doi:10.26093/cds/vizier.51590173CDSHartman J.D.Jordan A.Bayliss D.Bakos G.A.Bento J.Bhatti W.,Brahm R.Csubry Z.Espinoza N.Henning T.Mancini L.Penev K.,Rabus M.Sarkis P.Suc V.de Val-Borro M.Zhou G.Crane J.D.,Shectman S.Teske J.K.Wang S.X.Butler R.P.Lazar J.Papp I.,Sari P.Anderson D.R.Hellier C.West R.G.Barkaoui K.Pozuelos F.J.,Jehin E.Gillon M.Nielsen L.Lendl M.Udry S.Ricker G.R.,Vanderspek R.Latham D.W.Seager S.Winn J.N.Christiansen J.,Crossfield I.J.M.Henze C.E.Jenkins J.M.Smith J.C.Ting E.B.2021-12-07T21:07:28Z2020-07-20T08:15:23ZCDS support team

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

cds-question@unistra.frk-starsexoplanetsinfrared-photometryvisible-astronomyWide-band photometryspectroscopyradial-velocitystellar-agesstellar-massesWe report the discovery of four transiting giant planets around K-dwarfs. The planets HATS-47b, HATS-48Ab, HATS-49b, and HATS-72b have masses of 0.369_-0.021_^+0.031^M_J_, 0.243_-0.030_^+0.022^M_J_, 0.353_-0.027_^+0.038^M_J_, and 0.1254{+/-}0.0039M_J_, respectively, and radii of 1.117{+/-}0.014R_J_, 0.800{+/-}0.015R_J_, 0.765{+/-}0.013R_J_, and 0.7224{+/-}0.0032R_J_, respectively. The planets orbit close to their host stars with orbital periods of 3.9228days, 3.1317days, 4.1480days, and 7.3279days, respectively. The hosts are main-sequence K-dwarfs with masses of 0.674_-0.012_^+0.016^M_{odot}_, 0.7279{+/-}0.0066M_{odot}_, 0.7133{+/-}0.0075M_{odot}_, and 0.7311{+/-}0.0028, and with V-band magnitudes of V=14.829{+/-}0.010, 14.35{+/-}0.11, 14.998{+/-}0.040 and 12.469{+/-}0.010. The super-Neptune HATS-72b (a.k.a. WASP-191b and TOI294.01) was independently identified as a transiting planet candidate by the HATSouth, WASP, and TESS surveys, and we present a combined analysis of all of the data gathered by each of these projects (and their follow-up programs). An exceptionally precise mass is measured for HATS-72b thanks to high-precision radial velocity (RV) measurements obtained with VLT/ESPRESSO, FEROS, HARPS, and Magellan/PFS. We also incorporate TESS observations of the warm Saturn-hosting systems HATS-47 (a.k.a. TOI1073.01), HATS-48A, and HATS-49. HATS-47 was independently identified as a candidate by the TESS team, while the other two systems were not previously identified from the TESS data. The RV orbital variations are measured for these systems using Magellan/PFS. HATS-48A has a resolved 5.4" neighbor in Gaia DR2, which is a common-proper-motion binary star companion to HATS-48A with a mass of 0.22M_{odot}_ and a current projected physical separation of ~1400au.2020AJ....159..173Hhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/159/173CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toI/345 : Gaia DR2 (Gaia Collaboration, 2018)J/ApJ/710/1724 : Follow-up photometry for HAT-P-11 (Bakos+, 2010)J/ApJ/724/866 : Follow-up observations of HAT-P-15 (Kovacs+, 2010)J/ApJ/742/59 : HAT-P-32 and HAT-P-33 follow-up (Hartman+, 2011)J/ApJ/750/84 : Follow-up photometry and velocity of Qatar 2 (Bryan+, 2012)J/A+A/546/A14 : Limb-darkening for CoRoT, Kepler, Spitzer (Claret+, 2012)J/AJ/146/113 : Differential griz photometry of HATS-3 (Bayliss+, 2013)J/A+A/552/A16 : Limb-darkening for CoRoT, Kepler, Spitzer.II. (Claret+,2013)J/A+A/552/A82 : WASP-64b and WASP-72b light curves (Gillon+, 2013)J/AJ/145/5 : Follow-up photometry of HATS-1 (Penev+, 2013)J/A+A/551/A80 : WASP-80 photometric and radial velocity data (Triaud+, 2013)J/MNRAS/440/1470 : Ji light curves of WTS-2 (Birkby+, 2014)J/AJ/148/29 : Spectro. & differential photometry of HATS-4 (Jordan+, 2014)J/AJ/149/166 : Photometry and spectroscopy of HATS-6 (Hartman+, 2015)J/AJ/152/108 : i filter photom. HATS-25 through HATS-30 (Espinoza+, 2016)J/ApJ/831/64 : Mass-metallicity relation giant planets (Thorngren+, 2016)J/AJ/153/136 : Planets & their host with Gaia parallaxes (Stassun+, 2017)J/A+A/618/A20 : Limb-darkening for TESS, Kepler, Corot, MOST (Claret, 2018)J/AJ/156/259 : Robo-AO detected close binaries in Gaia DR2 (Ziegler+, 2018)J/AJ/157/55 : RVs and light curves for HATS-60-HATS-69 (Hartman+, 2019)J/AJ/159/19 : SOAR TESS survey. I. (Ziegler+, 2020)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/159/173https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/159/173http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/159/173https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/159/173https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/159/173http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/159/173GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/AJ/159/173/table6 (*Adopted derived stellar parameters for HATS-47, HATS-48A, HATS-49, and HATS-72)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/159/173/table6?https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/159/173/table6?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/159/173/table6?GETtext/xml+votable180.050000true287.4843767-49.66496330.0055555555555555566/18437 34957 47168 47310https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/159/173?format=asciiOpticalInfrareddefaultJ/AJ/159/173/table6*Adopted derived stellar parameters for HATS-47, HATS-48A, HATS-49, and HATS-72recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDObject identifiermeta.id;meta.maincharprimaryM[0.67/0.74] Object masssolMassphys.massfloate_M[0.002/0.02] Minimum error on MsolMassstat.errorfloatE_M[0.016]? Maximum error on M, if different from minimum errorsolMassstat.error;stat.maxfloatnullableR[0.65/0.73] RadiisolRadphys.size.radiusfloate_R[0.002/0.006] Error on RsolRadstat.errorfloatlogg[4.58/4.64] Surface gravitylog(cm.s**-2)phys.gravityfloate_logg[0.002/0.02] Error on logglog(cm.s**-2)stat.errorfloatrho[2.74/3.36] Density ({rho})g.cm**-3phys.densityfloate_rho[0.02/0.1] Minimum error on rhog.cm**-3stat.errorfloatE_rho[0.13]? Maximum error on rho, if different from minimum errorg.cm**-3stat.error;stat.maxfloatnullableL[0.15/0.22] LuminositysolLumphys.luminosityfloate_L[0.002/0.005] Error on LsolLumstat.errorfloatTeff[4405/4657] Effective temperatureKphys.temperature.effectivefloate_Teff[8.9/19] Minimum error on TeffKstat.error;phys.temperature.effectivefloatE_Teff[23]? Maximum error on Teff, if different from minimum errorKstat.error;stat.maxintnullable[Fe/H][-0.12/0.21] Metallicityphys.abund.Zfloate_[Fe/H][0.01/0.06] Error on [Fe/H]stat.error;phys.abund.FefloatAge[8.1/12.2] AgeGyrtime.agefloate_Age[0.45/4.3] Minimum error on AgeGyrstat.error;time.agefloatE_Age[0.24/2.9] Maximum error on AgeGyrstat.error;stat.maxfloatAV[0.02/0.12] V band extinctionmagphys.absorptionfloate_AV[0.008/0.04] Error on AVmagstat.errorfloatDist[127.6/324.6] Distancepcpos.distancefloate_Dist[0.52/2.2] Error on Distpcstat.errorfloatl_McompLimit flag on Mcompmeta.code.errorcharMcomp[0.22/0.36] Companion mass (1)solMassphys.massfloatPer[3.13/7.33] Period as found in the abstract (added by CDS)dmeta.abstract;time.periodfloatLCInteractive Plot; Light Curvemeta.ref.urlcharRVInteractive Plot; Radial Velocitymeta.ref.urlcharSimbadSimbad column added by the CDSmeta.ref.urlchar_RAPosition from Simbad (right ascension part)degpos.eq.ra;meta.main_DEPosition from Simbad (declination part)degpos.eq.dec;meta.mainJ/AJ/159/173/table1Summary of Photometric ObservationsFiltFilter usedinstr.setup;instr.filtercharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDObject identifiermeta.id;meta.maincharInstInstrument and field used (1)instr.setup;obs.fieldcharstart[2006/2019] Year of the beginning of the observationtime.epochend[2011/2019]? Year of the end of the observation, only if different from the beginning yeartime.epochnullableNphot[30/24431] Number of images, excluding any outliers or other data not included in the modelingmeta.numberintCad[21/1798] The median time between consecutive images rounded to the nearest second (2)stime.intervalintrms[0.66/21.8] The rms of the residuals from the best-fit model (3)mmaginstr.det.noisefloatJ/AJ/159/173/table2Light curve data for HATS-47, HATS-48A, HATS-49, and HATS-72InstInstrument used (3)instr.setupcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDObject identifiermeta.id;meta.maincharBJD[2453862/2458683] Barycentric Julian Date (1)dtime.epochdoublemag[-6.86/14.5] Observed magnitude in Filtermagphot.magdoublee_mag[0.0007/4] The 1{sigma} uncertainty in magmagstat.error;phot.magdoubleOmag[-0.11/16]? Original magnitude (2)magphot.magdoublenullableFiltFilter used (I+, T, i, r and un)instr.setup;instr.filtercharObsDetails of photometric observations for this source (link to table1)meta.ref.urlcharJ/AJ/159/173/table3Summary of Spectroscopy ObservationsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDObject identifiermeta.id;meta.maincharInstInstrument usedinstr.setupcharstart[2013/2019] Year of the beginning of the observationtime.epochend? Year of the end of the observation, only if different from the year of beginningtime.epochnullableNspec[1/12] Number of spectrameta.numberintR[3/140] Resolution/1000spect.resolutionintS/Nmin[9/52]? Minimum S/N per resolution element near 5180{AA}stat.snrintnullableS/Nmax[31/68]? Maximum S/N per resolution element near 5180{AA}, if different from minimumstat.snrintnullablegRV[-23/68]? Zero-point RV from the best-fit orbit ({gamma}RV) (1)km/sstat.fit;arith.zpfloatnullablepRV[10.5/4000]? Scatter in the RV residuals from the best-fit orbit (2)m/sstat.fit.residualfloatnullableJ/AJ/159/173/table5Relative radial velocities and bisector spans for HATS-47, HATS-48A, HATS-49 and HATS-72InstInstrument used (3)instr.setupcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDObject identifiermeta.id;meta.maincharBJD[7023/86387] Barycentric Julian Date BJD-2450000dtime.epochdoubleRVel[-93.65/78.44]? Radial velocity (1)m/sphys.veloc;pos.heliocentricfloatnullablee_RVel[0.6/35]? The 1{sigma} uncertainty in RVel (2)m/sstat.error;spect.dopplerVelocfloatnullableBS[-379.5/698.2]? Spectral line bisector spanm/sphys.velocfloatnullablee_BS[10/286]? Uncertainty in BSm/sstat.errorfloatnullablePhase[0.014/0.951] Orbital phasem/stime.phasefloatObsDetails of spectroscopic observations for this source (link to table3)meta.ref.urlchar