Bayesian Kepler periodogram
- Bayesian Kepler periodogram
Bayesian Kepler periodogram is an automatic instrument installed in Markov chain Monte Carlo observatory in British Columbia, Canada. It is designed to find more planets in single or multiple planetary systems. P.C. Gregory operates this instrument to find evidence for any new planets. In September 2006, the formally unconfirmed planet HD 208487 c was confirmed. [cite journal | url=http://arxiv.org/abs/astro-ph/0609229 | author=Gregory "et al" | title=A Bayesian Kepler periodogram detects a second planet in HD 208487 | journal=Monthly Notices of the Royal Astronomical Society | format=abstract | month=September | day=8 | year=2006 | volume=374 | issue=4 | pages=1321-1333 | accessdate=2008-09-03] In September 2007, it found a third planet orbiting around HD 11964. [cite journal | url=http://arxiv.org/abs/0709.0970 | author=Gregory "et al" | title=A Bayesian periodogram finds evidence for three planets in HD 11964 | journal=Astrophysics | format=abstract | month=September | day=6 | year=2007 | volume= | issue= | pages= | accessdate=2008-09-03]
See also
* HARPS
References
Wikimedia Foundation.
2010.
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HD 11964 — Starbox begin name = HD 11964 Starbox observe epoch = J2000.0 constell = Cetus ra = RA|1|57|09.6064 dec = DEC| 10|14|32.739 appmag v = +6.42 Starbox character class = G5IV b v = +0.82 u b = variable = Suspected Starbox astrometry radial v = 6.9… … Wikipedia
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