Sreekumar T. Balan, Ofer Lahav
Published 2009-07-21Version 1
We introduce EXOFIT, a Bayesian tool for estimating orbital parameters of extrasolar planets from radial velocity measurements. EXOFIT can search for either one or two planets at present. EXOFIT employs Markov Chain Monte Carlo method implemented in an object oriented manner. As an example we re-analyze the orbital solution of HD155358 and the results are compared with that of the published orbital parameters. In order to check the agreement of the EXOFIT orbital parameters with the published ones we examined radial velocity data of 30 stars taken randomly from www.exoplanet.eu. We show that while orbital periods agree in both methods, EXOFIT prefers lower eccentricity solutions for planets with higher (e >=0.5) orbital eccentricities.
Comments: To appear in the Proceedings of Molecules in the Atmospheres of Extrasolar Planets. 7 pages, 2 tables and 4 Figures
Finding binaries from phase modulation of pulsating stars with Kepler: V. Orbital parameters, with eccentricity and mass-ratio distributions of 341 new binaries
The orbital parameters of the binary BLAP HD133729 : advantages of the frequency modulation method
Markov Chain Monte Carlo applied to the Double Stars of Miller and Pitman
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