Article (Scientific journals)
Gaia Data Release 3. Properties of the line-broadening parameter derived with the Radial Velocity Spectrometer (RVS)
Frémat, Y.; Royer, F.; Marchal, O. et al.
2023In Astronomy and Astrophysics, 674, p. 8
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Keywords :
stars: rotation; catalogs; Astrophysics - Solar and Stellar; Astrophysics; Astrophysics - Astrophysics of Galaxies
Abstract :
[en] Context. The third release of the Gaia catalogue contains radial velocities for 33 812 183 stars with effective temperatures ranging from 3100 K to 14 500 K. The measurements are based on the comparison of the spectra observed with the Radial Velocity Spectrometer (RVS; wavelength coverage: 846-870 nm, median resolving power: 11 500) to synthetic data broadened to the adequate along-scan line spread function. The additional line-broadening, fitted as it would only be due to axial rotation, is also produced by the pipeline and is available in the catalogue (field name vbroad). <BR /> Aims: We describe the properties of the line-broadening information extracted from the RVS and published in the catalogue, and analyse the limitations imposed by the adopted method, wavelength range, and instrument. <BR /> Methods: We used simulations to express the link between the line-broadening measurement provided in Gaia Data Release 3 and V sin i. We then compared the observed values to the measurements published by various catalogues and surveys (GALAH, APOGEE, LAMOST, etc.). <BR /> Results: While we recommend caution in the interpretation of the vbroad measurement, we also find a reasonable general agreement of the Gaia Data Release 3 line-broadening values and values in other catalogues. We discuss and establish the validity domain of the published vbroad values. The estimate tends to be overestimated at the lower V sin i end, and at T<SUB>eff</SUB> > 7500 K its quality and significance degrade rapidly when G<SUB>RVS</SUB> > 10. Despite all the known and reported limitations, the Gaia Data Release 3 line-broadening catalogue contains measurements obtained for 3 524 677 stars with T<SUB>eff</SUB> ranging from 3500 to 14 500 K, and G<SUB>RVS</SUB> < 12. It gathers the largest stellar sample ever considered for the purpose, and allows a first mapping of the Gaia line-broadening parameter across the Hertzsprung-Russel diagram.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Frémat, Y.;  Royal Observatory of Belgium
Royer, F.;  Observatoire de Paris, Laboratoire Galaxies Etoiles Physiques et Instrumentation
Marchal, O.;  Centre de Donnees Astronomiques, Strasbourg
Blomme, R.;  Royal Observatory of Belgium
Sartoretti, P.;  Observatoire de Paris, Laboratoire Galaxies Etoiles Physiques et Instrumentation
Guerrier, A.;  Centre National d'Etudes Spatiales, Toulouse
Panuzzo, P.;  Observatoire de Paris, Laboratoire Galaxies Etoiles Physiques et Instrumentation
Katz, D.;  Observatoire de Paris, Laboratoire Galaxies Etoiles Physiques et Instrumentation
Seabroke, G. M.;  University College London, Mullard Space Science Laboratory
Thévenin, F.;  Observatoire de la Cote d'Azur, France
Cropper, M.;  University College London, Mullard Space Science Laboratory
Benson, K.;  University College London, Mullard Space Science Laboratory
Damerdji, Yassine ;  Université de Liège - ULiège > Département d'astrophysique, géophysique et océanographie (AGO) > Groupe d'astrophysique des hautes énergies (GAPHE)
Haigron, R.;  Observatoire de Paris, Laboratoire Galaxies Etoiles Physiques et Instrumentation
Lobel, A.;  Royal Observatory of Belgium
Smith, M.;  University College London, Mullard Space Science Laboratory
Baker, S. G.;  University College London, Mullard Space Science Laboratory
Chemin, L.;  University of Antofagasta, Chile
David, M.;  University of Antwerpen, Belgium
Dolding, C.;  University College London, Mullard Space Science Laboratory
Gosset, Eric ;  Université de Liège - ULiège > Département d'astrophysique, géophysique et océanographie (AGO) > Groupe d'astrophysique des hautes énergies (GAPHE)
Janßen, K.;  Leibniz Institute for Astrophysics, Potsdam
Jasniewicz, G.;  Laboratoire Univers et Particules de Montpellier
Plum, G.;  Observatoire de Paris, Laboratoire Galaxies Etoiles Physiques et Instrumentation
Samaras, N.;  Royal Observatory of Belgium, Charles University, Astronomical Institute
Snaith, O.;  Observatoire de Paris, Laboratoire Galaxies Etoiles Physiques et Instrumentation
Soubiran, C.;  Observatoire de Bordeaux
Vanel, O.;  Observatoire de Paris, Laboratoire Galaxies Etoiles Physiques et Instrumentation
Zorec, J.;  Institut d'Astrophysique de Paris
Zwitter, T.;  University of Ljubljana, Faculty of Mathematics and Physics
Brouillet, N.;  Observatoire de Bordeaux
Caffau, E.;  Observatoire de Paris, Laboratoire Galaxies Etoiles Physiques et Instrumentation
Crifo, F.;  Observatoire de Paris, Laboratoire Galaxies Etoiles Physiques et Instrumentation
Fabre, C.;  Centre National d'Etudes Spatiales, Toulouse
Fragkoudi, F.;  Durham University, Department of Physics, European Southern Observatory, Germany
Huckle, H. E.;  University College London, Mullard Space Science Laboratory
Lasne, Y.;  Centre National d'Etudes Spatiales, Toulouse
Leclerc, N.;  Observatoire de Paris, Laboratoire Galaxies Etoiles Physiques et Instrumentation
Mastrobuono-Battisti, A.;  Observatoire de Paris, Laboratoire Galaxies Etoiles Physiques et Instrumentation
Jean-Antoine Piccolo, A.;  Centre National d'Etudes Spatiales, Toulouse
Viala, Y.;  Observatoire de Paris, Laboratoire Galaxies Etoiles Physiques et Instrumentation
More authors (31 more) Less
Language :
English
Title :
Gaia Data Release 3. Properties of the line-broadening parameter derived with the Radial Velocity Spectrometer (RVS)
Publication date :
01 June 2023
Journal title :
Astronomy and Astrophysics
ISSN :
0004-6361
eISSN :
1432-0746
Publisher :
EDP Sciences, Les Ulis, Fr
Volume :
674
Pages :
A8
Peer reviewed :
Peer Reviewed verified by ORBi
Available on ORBi :
since 30 June 2023

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