Gael Chauvin mainly investigates Astrophysics, Astronomy, Planetary system, Planet and Brown dwarf. His study in Astrophysics focuses on Exoplanet, Photometry, Effective temperature and Very Large Telescope. A large part of his Astronomy studies is devoted to Stars.
His Planetary system research integrates issues from Spectral line and Spectral energy distribution. His research in Giant planet and Beta Pictoris are components of Planet. His Brown dwarf research includes themes of Planetary mass and Low Mass.
His primary areas of study are Astrophysics, Astronomy, Planet, Stars and Brown dwarf. His work in the fields of Astrophysics, such as Planetary system, Exoplanet, Low Mass and Radial velocity, intersects with other areas such as Context. As a part of the same scientific study, Gael Chauvin usually deals with the Exoplanet, concentrating on Field of view and frequently concerns with Point source.
In general Stars study, his work on Stellar mass and Kepler-47 often relates to the realm of Polarimetry and Luminosity, thereby connecting several areas of interest. The study incorporates disciplines such as Metallicity, Effective temperature, Adaptive optics, Radius and Planetary mass in addition to Brown dwarf. His work in Effective temperature tackles topics such as Surface gravity which are related to areas like Atmospheric models.
Gael Chauvin focuses on Planet, Astrophysics, Stars, Planetary system and Exoplanet. To a larger extent, Gael Chauvin studies Astronomy with the aim of understanding Planet. His biological study spans a wide range of topics, including Pixel and Radiative transfer.
Gael Chauvin performs integrative study on Astrophysics and Context in his works. His work on Circumbinary planet as part of general Stars study is frequently connected to Polarimetry, therefore bridging the gap between diverse disciplines of science and establishing a new relationship between them. The concepts of his Exoplanet study are interwoven with issues in Field of view, Stellar mass and Radial velocity.
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.
A Giant Planet Candidate near a Young Brown Dwarf
G. Chauvin;A. M. Lagrange;C. Dumas;B. Zuckerman.
arXiv: Astrophysics (2004)
A Giant Planet Imaged in the Disk of the Young Star β Pictoris
A.-M. Lagrange;M. Bonnefoy;G. Chauvin;D. Apai.
Science (2010)
A probable giant planet imaged in the β Pictoris disk. VLT/NaCo deep L'-band imaging
A.-M. Lagrange;D. Gratadour;G. Chauvin;T. Fusco.
Astronomy and Astrophysics (2009)
A giant planet candidate near a young brown dwarf - Direct VLT/NACO observations using IR wavefront sensing
G. Chauvin;A.-M. Lagrange;C. Dumas;B. Zuckerman.
Astronomy and Astrophysics (2004)
Discovery of a planetary-mass companion within the gap of the transition disk around PDS 70
M. Keppler;M. Benisty;A. Müller;Th. Henning.
arXiv: Earth and Planetary Astrophysics (2018)
SPHERE: the exoplanet imager for the Very Large Telescope
J.-L. Beuzit;A. Vigan;D. Mouillet;K. Dohlen.
arXiv: Instrumentation and Methods for Astrophysics (2019)
Giant planet companion to 2MASSW J1207334-393254
G. Chauvin;A.-M. Lagrange;C. Dumas;B. Zuckerman.
Astronomy and Astrophysics (2005)
Spiral Arms in the Asymmetrically Illuminated Disk of MWC 758 and Constraints on Giant Planets
C. A. Grady;T. Muto;J. Hashimoto;M. Fukagawa.
arXiv: Solar and Stellar Astrophysics (2012)
Discovery of a planetary-mass companion within the gap of the transition disk around PDS 70
M. Keppler;M. Benisty;M. Benisty;A. Müller;Th. Henning.
Astronomy and Astrophysics (2018)
Discovery of a probable 4-5 Jupiter-mass exoplanet to HD 95086 by direct-imaging
J. Rameau;G. Chauvin;A.-M. Lagrange;A. Boccaletti.
arXiv: Earth and Planetary Astrophysics (2013)
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