J/A+A/674/A39       Gaia DR3. 95 extrasolar planets          (Gaia Coll.+, 2023)

Gaia Data Release 3: A golden sample of astrophysical parameters. Gaia Collaboration, Creevey O.L., Sarro L.M., Lobel A., Pancino E., Andrae R., Smart R.L., et al. <Astron. Astrophys. 674, A39 (2023)> =2023A&A...674A..39G 2023A&A...674A..39G (SIMBAD/NED BibCode)
ADC_Keywords: Stars, double and multiple ; Exoplanets ; Photometry, CCD ; Stars, masses ; Stars, diameters Keywords: catalogues - stars: fundamental parameters - stars: early-type - stars: low-mass - Galaxy: stellar content - Galaxy: kinematics and dynamics Abstract: Gaia Data Release 3 provides a wealth of new data products for the astronomical community to exploit, including astrophysical parameters for a half billion stars. In this work we demonstrate the high quality of these data products and illustrate their use in different astrophysical contexts. We have produced six homogeneous samples of stars with high quality astrophysical parameters across the HR diagram for the community to exploit. We first focus on three samples that span a large parameter space: young massive disk stars (OBA), FGKM spectral-type stars, and ultra-cool dwarfs (UCDs). We provide these sources along with additional information (either a flag or complementary parameters) as tables that are made available in the Gaia archive. We furthermore identify 15740 bone fide carbon stars, 5863 solar-analogues, and provide the first homogeneous set of stellar parameters of the Spectro Photometric Standard Stars. We demonstrate some applications of these samples in different astrophysical contexts. We use a subset of the OBA sample to illustrate its usefulness to analyse the Milky Way rotation curve. We then use the properties of the FGKM stars to analyse known exoplanet systems. We also analyse the ages of some unseen UCD-companions to the FGKM stars. We additionally predict the colours of the Sun in various passbands (Gaia, 2MASS, WISE) using the solar-analogue sample. Description: Radius, mass, and age of 95 known extra solar planets and their host stars, derived using the astrophysical parameters from Gaia Data Release 3 along with existing literature data of photometric transits and radial velocities from exoplanet.org and references therein. The stellar mass and age are inferred assuming a solar metallicity prior. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table8.dat 108 95 Planet and stellar properties -------------------------------------------------------------------------------- See also: I/355 : Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022) Byte-by-byte Description of file: table8.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 20 I19 --- GaiaDR3 Gaia DR3 SourceID (GaiaDR3SourceID) 23- 38 A16 --- Planet Extra solar planet name (Planet) 42- 46 F5.3 Rjup RadPl Radius of planet (PlanetRadius) 49- 53 F5.3 Rjup e_RadPl Error in radius of planet (PlanetRadiusError) 55- 60 F6.3 Mjup MassPl Mass of planet (PlanetMass) 64- 68 F5.3 Mjup e_MassPl Error in mass of planet (PlanetMassError) 71- 75 F5.3 Rsun RadStar Radius of star (StarRadius) 78- 82 F5.3 Rsun e_RadStar Error in radius of star (StarRadiusError) 85- 89 F5.3 Msun MassStar Mass of star (StarMass) (1) 92- 96 F5.3 Msun e_MassStar Error in mass of star (StarMassError) 98-102 F5.2 Ga AgeStar ?=-9.99 Age of star (StarAge) (1) 105-108 F4.2 Ga e_AgeStar ?=0 Error in age of star (StarAgeError) -------------------------------------------------------------------------------- Note (1): The stellar mass and age are inferred using the BASTI models (Hidalgo et al., 2018ApJ...856..125H 2018ApJ...856..125H) and assuming solar metallicity. -------------------------------------------------------------------------------- Acknowledgements: Orlagh L. Creevey, orlagh.creevey(at)oca.eu
(End) Orlagh Creevey [OCA, Nice, France], Patricia Vannier [CDS] 15-Jul-2022
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