A Bayesian Kepler periodogram detects a second planet in HD 208487

Monthly Notices of the Royal Astronomical Society

Volumn 374, Issue 4, 2007, Pages 1321-1333

  Gregory, P C ^a  

^a UNIVERSITY OF BRITISH COLUMBIA   (Canada)

Author keywords

Methods: numerical; Methods: statistical; Stars: individual: HD 208487; Stars: Planetary systems; Techniques: radial velocities

Indexed keywords

MARKOV PROCESSES; ORBITS; STARS;

BAYESIAN; METHOD: NUMERICAL; METHODS:STATISTICAL; PERIODOGRAMS; PLANETARY ORBITS; SEMIMAJOR AXIS; STAR: INDIVIDUAL: HD 208487; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: PLANETARY SYSTEM; TECHNIQUES: RADIAL VELOCITIES;

NUMERICAL METHODS;

EID: 33846450614     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.11240.x     Document Type: Article

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