His primary areas of investigation include Astrophysics, Radial velocity, Planet, Astronomy and Exoplanet. Many of his research projects under Astrophysics are closely connected to High resolution and Humanities with High resolution and Humanities, tying the diverse disciplines of science together. He interconnects Amplitude, Stellar mass and Radius in the investigation of issues within Radial velocity.
His Radius research incorporates themes from Spectral line and Transit. A. P. Hatzes regularly links together related areas like Stellar classification in his Planet studies. His Exoplanet research includes themes of Light curve, Telescope, Spectrograph and Binary star.
A. P. Hatzes mostly deals with Astrophysics, Planet, Astronomy, Exoplanet and Radial velocity. His biological study deals with issues like Radius, which deal with fields such as Star. A. P. Hatzes combines subjects such as Orbital period and Transit with his study of Planet.
His research in the fields of Giant planet, Photometry, Solar-like oscillations and Jupiter overlaps with other disciplines such as Field. His Exoplanet research incorporates elements of Telescope, Brown dwarf, Effective temperature, Spectrograph and Terrestrial planet. In his study, Stellar rotation and Starspot is strongly linked to Rotation period, which falls under the umbrella field of Radial velocity.
His primary scientific interests are in Astrophysics, Planet, Exoplanet, Radial velocity and Astronomy. His Super-Earth, Star and Hot Jupiter study in the realm of Astrophysics interacts with subjects such as European union. His Planet study integrates concerns from other disciplines, such as Radius, Orbital period and Photometry.
To a larger extent, A. P. Hatzes studies Stars with the aim of understanding Exoplanet. His research on Radial velocity also deals with topics like
The scientist’s investigation covers issues in Planet, Astrophysics, Exoplanet, Radial velocity and Radius. Planet is a subfield of Astronomy that A. P. Hatzes studies. His studies deal with areas such as Spectral line and Computational physics as well as Astrophysics.
His work deals with themes such as Hot Neptune and Hot Jupiter, which intersect with Radial velocity. As a member of one scientific family, A. P. Hatzes mostly works in the field of Radius, focusing on Neptune and, on occasion, Outer planets and Planetary science. His Planetary system research focuses on subjects like Accretion, which are linked to Jupiter.
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.
The PLATO 2.0 Mission
H. Rauer;C. Catala;C. Aerts;T. Appourchaux.
arXiv: Earth and Planetary Astrophysics (2013)
The PLATO 2.0 mission
H. Rauer;H. Rauer;C. Catala;C. Aerts;T. Appourchaux.
Experimental Astronomy (2014)
Transiting exoplanets from the CoRoT space mission VIII. CoRoT-7b: the first Super-Earth with measured radius
A. Leger;D. Rouan;J. Schneider;P. Barge.
arXiv: Earth and Planetary Astrophysics (2009)
Transiting exoplanets from the CoRoT space mission VIII. CoRoT-7b: the first Super-Earth with measured radius
A. Léger;D. Rouan;J. Schneider;P. Barge.
Astronomy and Astrophysics (2009)
The CoRoT-7 planetary system: two orbiting super-Earths
D. Queloz;F. Bouchy;F. Bouchy;C. Moutou;A. Hatzes.
Astronomy and Astrophysics (2009)
Oscillating red giants in the CoRoT exofield: asteroseismic mass and radius determination
T. Kallinger;T. Kallinger;W. W. Weiss;C. Barban;F. Baudin.
Astronomy and Astrophysics (2010)
Transiting exoplanets from the CoRoT space mission . VI. CoRoT-Exo-3b: the first secure inhabitant of the brown-dwarf desert
M. Deleuil;H. J. Deeg;R. Alonso;F. Bouchy.
Astronomy and Astrophysics (2008)
The CARMENES search for exoplanets around M dwarfs: High-resolution optical and near-infrared spectroscopy of 324 survey stars
A. Reiners;M. Zechmeister;J.A. Caballero;I. Ribas.
arXiv: Solar and Stellar Astrophysics (2017)
CARMENES instrument overview
A. Quirrenbach;P. J. Amado;J. A. Caballero;R. Mundt.
Proceedings of SPIE (2014)
Evolved stars suggest an external origin of the enhanced metallicity in planet-hosting stars
L. Pasquini;M. P. Döllinger;A. Weiss;L. Girardi.
Astronomy and Astrophysics (2007)
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