PASTIS: Bayesian extrasolar planet validation. I. General framework, models, and performance
@article{Diaz2014PASTISBE, title={PASTIS: Bayesian extrasolar planet validation. I. General framework, models, and performance}, author={R. Diaz and J. M. Almenara and A. Santerne and C. Moutou and A. Lethuillier and Magali Deleuil 1. Aix Marseille Universit'e and Cnrs and Lam and France and 2. O. A. D. L. D. Geneve and Switzerland.}, journal={Monthly Notices of the Royal Astronomical Society}, year={2014}, volume={441}, pages={983-1004} }
A large fraction of the smallest transiting planet candidates discovered by the Kepler and CoRoT space missions cannot be confirmed by a dynamical measurement of the mass using currently available observing facilities. To establish their planetary nature, the concept of planet validation has been advanced. This technique compares the probability of the planetary hypothesis against that of all reasonably conceivable alternative false positive (FP) hypotheses. The candidate is considered as… CONTINUE READING
Figures and Tables from this paper
99 Citations
PASTIS: Bayesian extrasolar planet validation II. Constraining exoplanet blend scenarios using spectroscopic diagnoses
- Physics
- 2015
- 55
- PDF
Stellar and Planetary Properties of K2 Campaign 1 Candidates and Validation of 17 Planets, Including a Planet Receiving Earth-like Insolation
- Physics
- 2015
- 90
- PDF
Low False-Positive Rate of Kepler Candidates Estimated From a Combination of Spitzer and Follow-Up Observations
- Physics
- 2015
- 36
- PDF
References
SHOWING 1-10 OF 96 REFERENCES
PLANETARY CANDIDATES OBSERVED BY KEPLER. III. ANALYSIS OF THE FIRST 16 MONTHS OF DATA
- Physics
- 2013
- 774
- PDF
TRANSIT TIMING OBSERVATIONS FROM KEPLER. II. CONFIRMATION OF TWO MULTIPLANET SYSTEMS VIA A NON-PARAMETRIC CORRELATION ANALYSIS
- Physics
- 2012
- 75
- PDF
Homogeneous studies of transiting extrasolar planets – IV. Thirty systems with space-based light curves
- Physics
- 2011
- 245
- PDF
Kepler-10 c: a 2.2 Earth Radius Transiting Planet in a Multiple System
- Physics
- 2011
- 85
- Highly Influential
- PDF