Sérgio G. Sousa mainly investigates Astrophysics, Stars, Astronomy, Metallicity and Planet. His study focuses on the intersection of Astrophysics and fields such as Spectral line with connections in the field of Globular cluster. His study in the field of Planetary system, Milky Way and Stellar evolution also crosses realms of Context.
His studies examine the connections between Metallicity and genetics, as well as such issues in Effective temperature, with regards to Surface gravity and Accretion. His work on Terrestrial planet as part of general Planet study is frequently connected to Homogeneous, therefore bridging the gap between diverse disciplines of science and establishing a new relationship between them. Sérgio G. Sousa interconnects Astrometry, Stellar mass and Radial velocity in the investigation of issues within Exoplanet.
His primary areas of study are Astrophysics, Stars, Planet, Astronomy and Metallicity. His Astrophysics research focuses on Spectral line and how it connects with Line. His study on Asteroseismology and Effective temperature is often connected to Population, Thick disk and Homogeneous as part of broader study in Stars.
His research on Planet frequently links to adjacent areas such as Stellar mass. His work focuses on many connections between Metallicity and other disciplines, such as Star formation, that overlap with his field of interest in Supernova. His Habitability of orange dwarf systems and Planetary migration study in the realm of Planetary system interacts with subjects such as Lithium.
His primary areas of investigation include Stars, Astrophysics, Metallicity, Planet and Exoplanet. His study in the fields of Planetary system under the domain of Stars overlaps with other disciplines such as Chemical composition. He is involved in the study of Astrophysics that focuses on Asteroseismology in particular.
His work deals with themes such as Disc and Open cluster, which intersect with Metallicity. His research in Planet intersects with topics in Astrobiology and Solar System. His Exoplanet study combines topics from a wide range of disciplines, such as Star cluster and Field of view.
His primary scientific interests are in Astrophysics, Stars, Planet, Exoplanet and Metallicity. Astrophysics is a component of his Main sequence and Formation and evolution of the Solar System studies. Sérgio G. Sousa is interested in Planetary system, which is a branch of Stars.
His biological study spans a wide range of topics, including Asteroseismology, Orbital period, Giant planet and Subgiant. His Asteroseismology research incorporates elements of Saturn and Transit. His studies deal with areas such as Disc, Interstellar medium and Stellar evolution as well as Metallicity.
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The PLATO 2.0 Mission
H. Rauer;C. Catala;C. Aerts;T. Appourchaux.
arXiv: Earth and Planetary Astrophysics (2013)
The Gaia-ESO Public Spectroscopic Survey
G. Gilmore;S. Randich;M. Asplund;J. Binney.
The Messenger (2012)
The PLATO 2.0 mission
H. Rauer;H. Rauer;C. Catala;C. Aerts;T. Appourchaux.
Experimental Astronomy (2014)
Spectroscopic parameters for 451 stars in the HARPS GTO planet search program - Stellar [Fe/H] and the frequency of exo-Neptunes
S Sousa;N C Santos;M Mayor;S Udry.
Astronomy and Astrophysics (2008)
Chemical abundances of 1111 FGK stars from the HARPS GTO planet search program - Galactic stellar populations and planets
V. Zh. Adibekyan;S. G. Sousa;S. G. Sousa;N. C. Santos;E. Delgado Mena.
Astronomy and Astrophysics (2012)
A Mean Redshift of 2.8 for Swift gamma - ray bursts
P Jakobsson;A Levan;A Levan;Jpu Fynbo;R Priddey.
Astronomy and Astrophysics (2006)
Gaia FGK Benchmark Stars - Metallicity
Paula Jofre;U. Heiter;C. Soubiran;S. Blanco-Cuaresma.
arXiv: Astrophysics of Galaxies (2013)
A mean redshift of 2.8 for Swift gamma-ray bursts
P. Jakobsson;A. Levan;J. P. U. Fynbo;R. Priddey.
arXiv: Astrophysics (2005)
Ensemble Asteroseismology of Solar-Type Stars with the NASA Kepler Mission
W. J. Chaplin;H. Kjeldsen;J. Christensen-Dalsgaard;S. Basu.
A new code for automatic determination of equivalent widths: Automatic Routine for line Equivalent widths in stellar Spectra (ARES)
S. G. Sousa;S. G. Sousa;N. C. Santos;G. Israelian;M. Mayor.
Astronomy and Astrophysics (2007)
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