J/A+A/664/A94       8 TOI RV curves and 2 TOI light curves      (Psaridi+, 2022)

Three new brown dwarfs and a massive hot Jupiter revealed by TESS around early-type stars. Psaridi A., Bouchy F., Lendl M., Grieves N., Stassun K.G., Carmichael T., Gill S., Pena Rojas P.A., Gan T., Shporer A., Bieryla A., Christiansen J.L., Crossfield I.J.M., Galland F. Hooton M.J., Jenkins J.M., Jenkins J.S, Latham D.W, Lund M.B, Rodriguez J.E, Ting E.B, Udry S., Ulmer-Moll S., Wittenmyer R.A, Zhang Y., Zhou G., Addison B., Cointepas M., Collins K.A., Collins K.I., Deline A., Dressing C.D., Evans P., Giacalone S., Heitzmann A., Mireles I., Mounzer D., Otegi J., Radford D.J., Rudat A., Schlieder J.E., Schwarz R.P., Srdoc G., Stockdale C., Suarez O., Wright D.J., Zhao Y. <Astron. Astrophys. 664, A94 (2022)> =2022A&A...664A..94P 2022A&A...664A..94P (SIMBAD/NED BibCode)
ADC_Keywords: Stars, double and multiple ; Stars, brown dwarf ; Exoplanets ; Photometry ; Radial velocities ; Optical Keywords: brown dwarfs - planetary systems - techniques: photometric - techniques: radial velocities - stars: early-type - binaries: eclipsing Abstract: The detection and characterization of exoplanets and brown dwarfs around massive AF-type stars is essential to investigate and constrain the impact of stellar mass on planet properties. However, such targets are still poorly explored in radial velocity (RV) surveys because they only feature a small number of stellar lines and those are usually broadened and blended by stellar rotation as well as stellar jitter. As a result, the available information about the formation and evolution of planets and brown dwarfs around hot stars is limited. We aim to increase the sample and precisely measure the masses and eccentricities of giant planets and brown dwarfs transiting early-type stars detected by the Transiting Exoplanet Survey Satellite (TESS). We followed bright (V<12mag) stars with Teff>6200K that host giant companions (R>7R) using ground-based photometric observations as well as high precision radial velocity measurements from the CORALIE, CHIRON, TRES, FEROS, and MINERVA-Australis spectrographs. In the context of the search for exoplanets and brown dwarfs around early-type stars, we present the discovery of three brown dwarf companions, TOI-629b, TOI-1982b, and TOI-2543b, and one massive planet, TOI-1107b. From the joint analysis of TESS and ground-based photometry in combination with high precision radial velocity measurements, we find the brown dwarfs have masses between 66 and 68MJup, periods between 7.54 and 17.17 days, and radii between 0.95 and 1.11RJup. The hot Jupiter TOI-1107b has an orbital period of 4.08 days, a radius of 1.30RJup, and a mass of 3.35MJup. As a by-product of this program, we identified four low-mass eclipsing components (TOI-288b, TOI-446b, TOI-478b, and TOI-764b). Both TOI-1107b and TOI-1982b present an anomalously inflated radius with respect to the age of these systems. TOI-629 is among the hottest stars with a known transiting brown dwarf. TOI-629b and TOI-1982b are among the most eccentric brown dwarfs. The massive planet and the three brown dwarfs add to the growing population of well-characterized giant planets and brown dwarfs transiting AF-type stars and they reduce the apparent paucity. Description: Ground-based photometric fluxes for the observation of TOI-1107 and TOI-1982 with El Sauce, ASTEP, Brierfield, Hazelwood and LCOGT. The first column corresponds to the time of the observation in BJD_TDB. The second and third columns correspond respectively to the flux and flux_error on the raw light curves. The fourth column corresponds to the name of the instrument. The fifth column corresponds to the name of the target. We obtained radial velocity measurements for TOI-1107, TOI-629, TOI-1982 and TOI-2543 with different spectrographs, CORALIE, CHIRON, TRES, FEROS, and MINERVA-Australis, in order to identify the nature of the candidate, determine its mass and measure its orbital parameters. We obtained radial velocity measurements as a by-product of this RV follow-up and identified four low mass, single-lined spectral eclipsing binaries, TOI-288, TOI-446, TOI-478 and TOI-764. Objects: ----------------------------------------------------- RA (2000) DE Designation(s) ----------------------------------------------------- 10 22 25.82 -82 13 07.97 TOI-1107 = TIC 394561119 06 23 18.69 +00 53 00.11 TOI-629 = TIC 293853437 13 50 20.36 -23 23 00.16 TOI-1982 = TIC 437329044 09 06 23.26 +03 34 03.61 TOI-2543 = TIC 270604417 22 41 13.85 -28 01 57.57 TOI-288 = TIC 47316976 05 00 41.18 -35 12 09.63 TOI-446 = TIC 1449640 06 40 38.13 -27 34 16.54 TOI-478 = TIC 172464366 11 37 12.68 -38 18 25.89 TOI-764 = TIC 181159386 ----------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file stars.dat 65 8 List of studied stars lcs1.dat 48 1617 Ground based photometric fluxes for TOI-1107 from ASTEP, Brierfield and LCOGT lcs2.dat 48 870 Ground based photometric fluxes for TOI-1982 from El Sauce, Hazelwood and LCOGT rvs1.dat 49 156 Radial velocity time series of TOI-1107, TOI-629, TOI-1982 and TOI-2543 from CORALIE, MINERVA, TRES, FEROS and CHIRON rvs2.dat 48 57 Radial velocity time series of TOI-288, TOI-446, TOI-478 and TOI-764 from CORALIE -------------------------------------------------------------------------------- See also: IV/38 : TESS Input Catalog - v8.0 (TIC-8) (Stassun+, 2019) Byte-by-byte Description of file: stars.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Name Star name (TOI-NNNN) 10- 11 I2 h RAh Right ascension (J2000) 13- 14 I2 min RAm Right ascension (J2000) 16- 20 F5.2 s RAs Right ascension (J2000) 22 A1 --- DE- Declination sign (J2000) 23- 24 I2 deg DEd Declination (J2000) 26- 27 I2 arcmin DEm Declination (J2000) 29- 33 F5.2 arcsec DEs Declination (J2000) 35- 47 A13 --- OName Other name (TIC NNNNNNNNN) 49- 56 A8 --- FileName1 Name of file with photometric data 58- 65 A8 --- FileName2 Name of file with radial velocity data -------------------------------------------------------------------------------- Byte-by-byte Description of file: lcs1.dat lcs2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 F13.5 d BJD Time of observation in BJD_TDB 15- 21 F7.5 --- Flux Normalized raw flux 23- 29 F7.5 --- e_Flux Error on Flux 31- 39 A9 --- Inst Instrument used 41- 48 A8 --- Target Name of the target -------------------------------------------------------------------------------- Byte-by-byte Description of file: rvs1.dat rvs2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 14 F14.6 d BJD Time of observation in BJD_TDB 16- 24 F9.5 km/s RV Radial velocity 26- 32 F7.5 km/s e_RV Uncertainty in RV 34- 40 A7 --- Inst Instrument used 42- 49 A8 --- Target Name of the target -------------------------------------------------------------------------------- Acknowledgements: Angelica Psaridi, angeliki.psaridi(at)unige.ch
(End) Patricia Vannier [CDS] 13-May-2022
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