Statistical properties of exoplanets
Since the detection a decade ago of the planetary companion of 51 Peg, more than 200
extrasolar planets have been unveiled, mostly by radial-velocity measurements but also in a …
extrasolar planets have been unveiled, mostly by radial-velocity measurements but also in a …
M stars as targets for terrestrial exoplanet searches and biosignature detection
The changing view of planets orbiting low mass stars, M stars, as potentially hospitable
worlds for life and its remote detection was motivated by several factors, including the …
worlds for life and its remote detection was motivated by several factors, including the …
How to constrain your M dwarf. II. The mass–luminosity–metallicity relation from 0.075 to 0.70 solar masses
The mass–luminosity relation for late-type stars has long been a critical tool for estimating
stellar masses. However, there is growing need for both a higher-precision relation and a …
stellar masses. However, there is growing need for both a higher-precision relation and a …
How to constrain your M dwarf: measuring effective temperature, bolometric luminosity, mass, and radius
Precise and accurate parameters for late-type (late K and M) dwarf stars are important for
characterization of any orbiting planets, but such determinations have been hampered by …
characterization of any orbiting planets, but such determinations have been hampered by …
CARMENES input catalogue of M dwarfs-V. Luminosities, colours, and spectral energy distributions
C Cifuentes, JA Caballero, M Cortés-Contreras… - Astronomy & …, 2020 - aanda.org
Context. The relevance of M dwarfs in the search for potentially habitable Earth-sized
planets has grown significantly in the last years. Aims. In our on-going effort to …
planets has grown significantly in the last years. Aims. In our on-going effort to …
[HTML][HTML] The HARPS search for southern extra-solar planets-XXXI. The M-dwarf sample
Context. Searching for planets around stars with different masses helps us to assess the
outcome of planetary formation for different initial conditions. The low-mass M dwarfs are …
outcome of planetary formation for different initial conditions. The low-mass M dwarfs are …
New constraints on the chemical evolution of the solar neighbourhood and Galactic disc (s)-Improved astrophysical parameters for the Geneva-Copenhagen Survey
L Casagrande, R Schönrich, M Asplund… - Astronomy & …, 2011 - aanda.org
We present a re-analysis of the Geneva-Copenhagen survey, which benefits from the
infrared flux method to improve the accuracy of the derived stellar effective temperatures and …
infrared flux method to improve the accuracy of the derived stellar effective temperatures and …
Giant planet occurrence in the stellar mass-metallicity plane
Correlations between stellar properties and the occurrence rate of exoplanets can be used
to inform the target selection of future planet-search efforts and provide valuable clues about …
to inform the target selection of future planet-search efforts and provide valuable clues about …
Friends of hot Jupiters. I. A radial velocity search for massive, long-period companions to close-in gas giant planets
In this paper we search for distant massive companions to known transiting gas giant
planets that may have influenced the dynamical evolution of these systems. We present new …
planets that may have influenced the dynamical evolution of these systems. We present new …
SWEET-Cat: A catalogue of parameters for Stars With ExoplanETs-I. New atmospheric parameters and masses for 48 stars with planets
Context. Thanks to the importance that the star-planet relation has to our understanding of
the planet formation process, the precise determination of stellar parameters for the ever …
the planet formation process, the precise determination of stellar parameters for the ever …