J/AJ/159/44 RV curve of the metal-rich exoplanet host star XO-7 (Crouzet+, 2020)

XO-7b: a transiting hot Jupiter with a massive companion on a wide orbit. Crouzet N., Healy B.F., Hebrard G., McCullough P.R., Long D., Montanes- Rodriguez P., Ribas I., Vilardell F., Herrero E., Garcia-Melendo E., Conjat M., Foote J., Garlitz J., Vo P., Santos N.C., de Bruijne J., Osborn H.P., Dalal S., Nielsen L.D. <Astron. J., 159, 44 (2020)> =2020AJ....159...44C 2020AJ....159...44C
ADC_Keywords: Radial velocities; Stars, G-type; Exoplanets; Optical Keywords: Exoplanet astronomy ; Exoplanets ; Extrasolar gas giants ; Hot Jupiters ; Transits ; Transit photometry ; Transit instruments ; Exoplanet systems ; High resolution spectroscopy ; Surveys ; Visible astronomy ; Radial velocity Abstract: Transiting planets orbiting bright stars are the most favorable targets for follow-up and characterization. We report the discovery of the transiting hot Jupiter XO-7b and of a second, massive companion on a wide orbit around a circumpolar, bright, and metal-rich G0 dwarf (V=10.52, Teff=6250±100K, [Fe/H]=0.432±0.057dex). We conducted photometric and radial velocity follow-up with a team of amateur and professional astronomers. XO-7b has a period of 2.8641424±0.0000043days, a mass of 0.709±0.034MJ, a radius of 1.373±0.026RJ, a density of 0.340±0.027g/cm3, and an equilibrium temperature of 1743±23K. Its large atmospheric scale height and the brightness of the host star make it well suited to atmospheric characterization. The wide-orbit companion is detected as a linear trend in radial velocities with an amplitude of ∼100m/s over two years, yielding a minimum mass of 4MJ; it could be a planet, a brown dwarf, or a low-mass star. The hot Jupiter orbital parameters and the presence of the wide-orbit companion point toward a high-eccentricity migration for the hot Jupiter. Overall, this system will be valuable to understand the atmospheric properties and migration mechanisms of hot Jupiters and will help constrain the formation and evolution models of gas giant exoplanets. Description: Radial velocity (RV) measurements were obtained between 2016 July 23 and 2018 July 4 with the SOPHIE spectrograph at the 193cm telescope of Observatoire de Haute-Provence (OHP), France. We used its High-Resolution mode (resolving power R=75000). Exposure times were around 13min allowing signal-to-noise ratios of around 27 per pixel at 550nm to be reached on most of the exposures. Objects: ------------------------------------------------------------ RA (ICRS) DE Designation(s) ------------------------------------------------------------ 18 29 54.93 +85 13 59.6 XO-7 = TYC 4652-1593-1 ------------------------------------------------------------ File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table5.dat 32 49 Radial velocity measurements of the host star XO-7 obtained with the SOPHIE spectrograph -------------------------------------------------------------------------------- See also: I/259 : The Tycho-2 Catalogue (Hog+, 2000) II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+, 2003) III/231 : The Tycho-2 Spectral Type Catalog (Wright+, 2003) II/328 : AllWISE Data Release (Cutri+, 2013) I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018) I/345 : Gaia DR2 (Gaia Collaboration, 2018) VI/135 : All-sky spectrally matched Tycho2 stars (Pickles+, 2010) J/ApJ/622/1102 : The planet-metallicity correlation. (Fischer+, 2005) J/A+A/487/373 : Spectroscopic parameters of 451 HARPS-GTO stars (Sousa+, 2008) J/A+A/505/853 : HD16760 radial velocity curve (Bouchy+, 2009) J/ApJ/707/446 : HAT-P-13 photometry follow-up (Bakos+, 2009) J/A+A/513/A69 : HD9446 radial velocity curve (Hebrard+, 2010) J/A+A/523/A88 : A Jupiter-mass companion around HD 109246 (Boisse+, 2010) J/other/A+ARV/18.67 : Accurate masses and radii of normal stars (Torres+, 2010) J/A+A/538/A113 : Extrasolar planets Radial velocities of 8 stars (Diaz+ 2012) J/A+A/545/A55 : Extrasolar planets Radial velocities 5 stars (Boisse+, 2012) J/ApJ/757/18 : Radial velocities 16 hot Jupiter host stars (Albrecht+, 2012) J/A+A/556/A150 : SWEETCat I. Stellar parameters for host stars (Santos+, 2013) J/A+A/563/A22 : Radial velocities of 3 new hot Jupiters (Moutou+, 2014) J/ApJ/785/126 : HIRES radial velocity measurements (Knutson+, 2014) J/ApJ/809/77 : Transiting Exoplanet Survey Satellite (TESS) (Sullivan+, 2015) J/A+A/585/A46 : Extrasolar planets Radial velocities 5 stars (Bouchy+, 2016) J/A+A/588/A145 : Radial velocities 8 stars with giant planets (Hebrard+, 2016) J/A+A/591/A55 : Five transiting Jupiters discovered using WASP (Maxted+, 2016) J/A+A/600/A30 : Limb-darkening for TESS satellite (Claret, 2017) J/A+A/601/A9 : HD17674, HD29021, and HD42012 radial velocities (Rey+, 2017) J/A+A/618/A103 : Gl617A and Gl96 radial velocity curves (Hobson+, 2018) J/AJ/156/216 : Differential photometry & RVs of HATS-59 (Sarkis+, 2018) Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 F10.4 --- BJD [57593/58304] Reduced Barycentric Julian Date; BJD-2400000 12- 18 F7.5 --- Phase [0.05/0.95] Orbital phase (1) 20- 26 F7.3 km/s RV [-13.2/-12.8] Radial velocity 28- 32 F5.3 km/s e_RV [0.008/0.03] Error on RV (σ) -------------------------------------------------------------------------------- Note (1): The orbital phase is 0 at mid-transit. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by Coralie Fix [CDS], 31-Mar-2020
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line