J/AJ/167/153  TESS-Keck Survey. XII. TOI-1347 radial velocity (Rubenzahl+, 2024)

The TESS-Keck Survey. XII. A Dense 1.8 R⊕ Ultra-short-period Planet Possibly Clinging to a High-mean-molecular-weight Atmosphere after the First Gigayear. Rubenzahl R.A., Dai F., Howard A.W., Lissauer J.J., Van Zandt J., Beard C., Giacalone S., Murphy J.M.A., Chontos A., Lubin J., Brinkman C.L., Tyler D., MacDougall M.G., Rice M., Dalba P.A., Mayo A.W., Weiss L.M., Polanski A.S., Blunt S., Yee S.W., Hill M.L., Angelo I., Turtelboom E.V., Holcomb R., Behmard A., Pidhorodetska D., Batalha N.M., Crossfield I.J.M., Dressing C., Fulton B., Huber D., Isaacson H., Kane S.R., Petigura E.A., Robertson P., Scarsdale N., Mocnik T., Fetherolf T., Malavolta L., Mortier A., Fiorenzano A., Pedani M. <Astron. J., 167, 153 (2024)> =2024AJ....167..153R 2024AJ....167..153R
ADC_Keywords: Exoplanets; Spectra, optical; Radial velocities Keywords: Exoplanet astronomy ; Radial velocity ; Transit photometry ; Exoplanet atmospheres ; Super Earths ; Exoplanet detection methods Abstract: The extreme environments of ultra-short-period planets (USPs) make excellent laboratories to study how exoplanets obtain, lose, retain, and/or regain gaseous atmospheres. We present the confirmation and characterization of the USP TOI-1347b, a 1.8±0.1R⊕ planet on a 0.85day orbit that was detected with photometry from the TESS mission. We measured radial velocities of the TOI-1347 system using Keck/HIRES and HARPS-N and found the USP to be unusually massive at 11.1±1.2M⊕. The measured mass and radius of TOI-1347b imply an Earth-like bulk composition. A thin H/He envelope (>0.01% by mass) can be ruled out at high confidence. The system is between 1 and 1.8Gyr old; therefore, intensive photoevaporation should have concluded. We detected a tentative phase-curve variation (3σ) and a secondary eclipse (2σ) in TESS photometry, which, if confirmed, could indicate the presence of a high-mean-molecular-weight atmosphere. We recommend additional optical and infrared observations to confirm the presence of an atmosphere and investigate its composition. Description: We collected 120 high-resolution optical spectra of TOI-1347 between UT 2019 November 28 and UT 2022 July 26 with HIRES on the Keck I telescope as part of TKS. We took exposures using the "C2" decker (R=45000). We also obtained 14 spectra with the HARPS-N , installed at the Telescopio Nazionale Galileo. Observations were taken with 1800s exposure times (average S/N is 42.3 in order 50) with simultaneous wavelength calibration provided by the Fabry-Perot etalon. Objects: --------------------------------------------------------------- RA (2000) DE Designation(s) (Period) --------------------------------------------------------------- 18 41 18.42 +70 17 23.7 TOI-1347 = TIC 229747848 (P<1d) --------------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3.dat 46 134 TOI-1347 radial velocities and S-Indices -------------------------------------------------------------------------------- See also: III/159 : Ca II H and K Measurements Made at MWO (Duncan+ 1991) J/ApJ/687/1264 : Age estimation for solar-type dwarfs (Mamajek+, 2008) J/ApJ/725/875 : Chromospheric activity for CPS stars (Isaacson+, 2010) J/AJ/142/19 : Speckle observations of KOI (Howell+, 2011) J/ApJ/790/146 : Planets Kepler's multi-transiting systems (Fabrycky+, 2014) J/ApJ/787/47 : 106 Kepler ultra-short-period planets (Sanchis-Ojeda+, 2014) J/AJ/154/109 : California-Kepler Survey. III. Planet radii (Fulton+, 2017) J/MNRAS/472/1618 : Kepler study of starspot lifetimes (Giles+, 2017) J/ApJ/844/102 : KIC parallaxes from asteroseismology vs Gaia (Huber+, 2017) J/ApJ/855/115 : Lithium abundances of KOIs from CKS spectra (Berger+, 2018) J/AJ/155/107 : HARPS-N obs of K2-141 planetary system (Malavolta+, 2018) J/AJ/159/280 : Gaia-Kepler stellar properties.I. KIC stars (Berger+, 2020) J/A+A/648/A103 : Thorium line list (Dumusque+, 2021) J/ApJS/254/39 : Exoplanet candidates from TESS 1st 2yr obs (Guerrero+, 2021) J/AJ/161/56 : The TESS-Keck Survey. II. RVs of TOI-561 (Weiss+, 2021) J/A+A/668/A158 : HD 20329 Radial velocity & activity indices (Murgas+, 2022) J/AJ/166/62 : New HIRES radial velocity data for V1298 Tau (Blunt+, 2023) J/AJ/166/33 : TESS-Keck Survey. XV. 108 TESS Planets (MacDougall+, 2023) Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 14 F14.6 d-- BJD [2e+06/3e+06] Barycentric Julian Date of Observation (BJD-2457000) 16- 22 F7.3 m/s RVel [-30/36] Radial velocity (1) 24- 27 F4.2 m/s e_RVel [1/5] Error on RVel 29- 33 F5.3 --- SHK [0/0.34]? SHK Index 35- 38 F4.3 --- e_SHK [0.001]? Error on SHK 40- 46 A7 --- Instr Instrument used (HARPS-N or HIRES) -------------------------------------------------------------------------------- Note (1): A median value of -13965.395km/s has been subtracted from the HARPS-N RVels -------------------------------------------------------------------------------- History: From electronic version of the journal References: Dalba+, Paper I: 2020AJ....159..241D 2020AJ....159..241D Cat. J/AJ/159/241 Weiss+, Paper II: 2021AJ....161...56W 2021AJ....161...56W Cat. J/AJ/161/56 Dai+, Paper III: 2020AJ....160..193D 2020AJ....160..193D Rubenzahl+, Paper IV: 2021AJ....161..119R 2021AJ....161..119R Cat. J/AJ/161/119 Scarsdale+, Paper V: 2021AJ....162..215S 2021AJ....162..215S Cat. J/AJ/162/215 MacDougall+, Paper VI: 2021AJ....162..265M 2021AJ....162..265M Cat. J/AJ/162/265 Dalba+, Paper VIII: 2022AJ....163...61D 2022AJ....163...61D Cat. J/AJ/163/61 Lubin+, Paper IX: 2022AJ....163..101L 2022AJ....163..101L Cat. J/AJ/163/101 Turtelboom+, Paper XI: 2022AJ....163..293T 2022AJ....163..293T Cat. J/AJ/163/293 MacDougall+, Paper XIII: 2022AJ....164...97M 2022AJ....164...97M Cat. J/AJ/164/97 Van Zandt+, Paper XIV: 2023AJ....165...60V 2023AJ....165...60V Cat. J/AJ/165/60 MacDougall+, Paper XV : 2023AJ....166...33M 2023AJ....166...33M Cat. J/AJ/166/33
(End) Prepared by Coralie fix [CDS], 04-Jun-2024
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