We describe a Bayesian rejection-sampling algorithm designed to efficiently compute posterior distributions of orbital elements for data covering short fractions of long-period exoplanet orbits. Our implementation of this method, Orbits for the Impatient (OFTI), converges up to several orders of magnitude faster than two implementations of Markov Chain Monte Carlo (MCMC) in this regime. We illustrate the efficiency of our approach by showing that OFTI calculates accurate posteriors for all existing astrometry of the exoplanet 51 Eri b up to 100 times faster than a Metropolis\u2013Hastings MCMC. We demonstrate the accuracy of OFTI by comparing our results for several orbiting systems with those of various MCMC implementations, finding the ou...
We propose a new approach to Bayesian prior probability distributions (priors) that can improve orbi...
Astrometric discovery of sub-stellar mass companions orbiting stars is exceedingly hard due to the r...
Are we on the threshold of discovering life elsewhere in the universe? With the mounting discoveries...
The Gaia mission is expected to make a significant contribution to the knowledge of exoplanet system...
The Gaia mission is expected to make a significant contribution to the knowledge of exoplanet system...
International audienceA principal scientific goal of the Gemini Planet Imager (GPI) is obtaining mil...
A principal scientific goal of the Gemini Planet Imager (GPI) is obtaining milliarcsecond astrometry...
Transit timing variations (TTVs) are a valuable tool to determine the masses and orbits of transitin...
A principal scientific goal of the Gemini Planet Imager (GPI) is obtaining milliarcsecond astrometry...
Precise radial velocity measurements have led to the discovery of ~170 extrasolar planetary systems....
To date nearly 300 exoplanets have been discovered, most of them through measurements of the wobble ...
International audienceContext. Ground-based observing time is precious in the era of exoplanet follo...
When fitting transiting exoplanet lightcurves, it is usually desirable to have ranges and/or priors ...
orbitize! is an open-source, object-oriented software package for fitting the orbits of directly ima...
Transiting exoplanets in multiplanet systems exhibit non-Keplerian orbits as a result of the gravita...
We propose a new approach to Bayesian prior probability distributions (priors) that can improve orbi...
Astrometric discovery of sub-stellar mass companions orbiting stars is exceedingly hard due to the r...
Are we on the threshold of discovering life elsewhere in the universe? With the mounting discoveries...
The Gaia mission is expected to make a significant contribution to the knowledge of exoplanet system...
The Gaia mission is expected to make a significant contribution to the knowledge of exoplanet system...
International audienceA principal scientific goal of the Gemini Planet Imager (GPI) is obtaining mil...
A principal scientific goal of the Gemini Planet Imager (GPI) is obtaining milliarcsecond astrometry...
Transit timing variations (TTVs) are a valuable tool to determine the masses and orbits of transitin...
A principal scientific goal of the Gemini Planet Imager (GPI) is obtaining milliarcsecond astrometry...
Precise radial velocity measurements have led to the discovery of ~170 extrasolar planetary systems....
To date nearly 300 exoplanets have been discovered, most of them through measurements of the wobble ...
International audienceContext. Ground-based observing time is precious in the era of exoplanet follo...
When fitting transiting exoplanet lightcurves, it is usually desirable to have ranges and/or priors ...
orbitize! is an open-source, object-oriented software package for fitting the orbits of directly ima...
Transiting exoplanets in multiplanet systems exhibit non-Keplerian orbits as a result of the gravita...
We propose a new approach to Bayesian prior probability distributions (priors) that can improve orbi...
Astrometric discovery of sub-stellar mass companions orbiting stars is exceedingly hard due to the r...
Are we on the threshold of discovering life elsewhere in the universe? With the mounting discoveries...