Caroline Soubiran focuses on Astrophysics, Stars, Metallicity, Astronomy and Galaxy. Her Astrophysics study is mostly concerned with Milky Way, Astrometry, Globular cluster, Open cluster and Stellar population. Caroline Soubiran combines subjects such as Data release, Payload, Photometry and Data processing with her study of Astrometry.
The various areas that Caroline Soubiran examines in her Photometry study include Vista Variables in the Via Lactea, Apparent magnitude and Proper motion. Her Stars study frequently draws connections between related disciplines such as Spectral line. Her Metallicity research is multidisciplinary, relying on both Astronomical spectroscopy and Stellar classification.
Her scientific interests lie mostly in Astrophysics, Stars, Astronomy, Metallicity and Galaxy. Caroline Soubiran studied Astrophysics and Spectral line that intersect with Stellar evolution. Her Stars research is multidisciplinary, incorporating perspectives in Disc, Spectrograph and Thick disk.
Her work in the fields of Observatory, Magnitude, Star cluster and Sky overlaps with other areas such as Benchmark. Her study in Metallicity is interdisciplinary in nature, drawing from both Line, Spectral resolution, Surface gravity and Globular cluster. Her Astrometry research includes elements of Data release, Photometry and Proper motion.
Caroline Soubiran mostly deals with Astrophysics, Stars, Open cluster, Astronomy and Astrometry. Her work on Astrophysics deals in particular with Milky Way, Radial velocity, Galaxy, Data release and Metallicity. The study incorporates disciplines such as Magnitude and Phase space in addition to Radial velocity.
Her work carried out in the field of Stars brings together such families of science as Spectral line, Planet, Calibration and Chemical composition. Her Open cluster study which covers Binary star that intersects with Stellar structure. Her research investigates the connection between Astrometry and topics such as RR Lyrae variable that intersect with problems in Cepheid variable.
Her primary scientific interests are in Astrophysics, Stars, Astrometry, Data release and Radial velocity. Her Open cluster, Milky Way, Galaxy and Metallicity study in the realm of Astrophysics connects with subjects such as Context. Caroline Soubiran interconnects Stellar population and Stellar classification in the investigation of issues within Metallicity.
Her Stars study is focused on Astronomy in general. Her Astrometry study combines topics in areas such as Variable star, RR Lyrae variable, Parallax, Photometry and Proper motion. She interconnects Effective temperature and Payload in the investigation of issues within Data release.
This overview was generated by a machine learning system which analysed the scientist’s body of work. If you have any feedback, you can contact us here.
Gaia Data Release 2 Summary of the contents and survey properties
A. G. A. Brown;A. Vallenari;T. Prusti.
Astronomy and Astrophysics (2018)
The Gaia mission
T. Prusti;J. H. J. de Bruijne;A. G. A. Brown.
Astronomy and Astrophysics (2016)
Gaia Data Release 1 Summary of the astrometric, photometric, and survey properties
A. G. A. Brown;A. Vallenari;T. Prusti.
Astronomy and Astrophysics (2016)
The Gaia-ESO Public Spectroscopic Survey
G. Gilmore;S. Randich;M. Asplund;J. Binney.
The Messenger (2012)
Gaia Data Release 2: Catalogue validation
F. Arenou;X. Luri;C. Babusiaux;C. Fabricius.
arXiv: Astrophysics of Galaxies (2018)
Gaia Data Release 2: Observational Hertzsprung-Russell diagrams
C. Babusiaux;F. van Leeuwen;M.A. Barstow.
arXiv: Solar and Stellar Astrophysics (2018)
STELIB: A library of stellar spectra at R 2000 ?;??
J.-F. Le Borgne;G. Bruzual;R. Pelló;A. Lançon.
Astronomy and Astrophysics (2003)
A database of high and medium-resolution stellar spectra ?;??
Ph. Prugniel;C. Soubiran.
Astronomy and Astrophysics (2001)
Gaia Data Release 2. Catalogue validation
F. Arenou;X. Luri;C. Babusiaux;C. Fabricius.
Astronomy and Astrophysics (2018)
Evolutionary synthesis of galaxies at high spectral resolution with the code PEGASE-HR
Damien Le Borgne;Damien Le Borgne;Brigitte Rocca-Volmerange;Philippe Prugniel;Ariane Lancon.
arXiv: Astrophysics (2004)
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