Elodie metallicity-biased search for transiting hot Jupiters

Details Elodie metallicity-biased search for transiting hot Jupiters Elodie metallicity-biased search for transiting hot Jupiters

Feb 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006tafp.conf..135d&link_type=abstract

"Tenth Anniversary of 51 Peg-b: Status of and prospects for hot Jupiter studies. Colloquium held at Observatoire de Haute Proven

Other

Scientific paper

Star hosting planets have been shown to be more metal rich than single stars of the solar neighborhood. We present here a metallicity-biased planet-search program on-going since 18 months at Haute-Provence Observatory with the ELODIE spectrograph, where the target sample are high metallicity stars. We use a cross-correlation technique for radial-velocity estimates, together with a photometric transit search performed with the 120-cm telescope at the Haute-Provence Observatory. This program has already conducted to the discovery of two new planets candidates orbiting HD 118203 and HD 189733, and to the confirmation of another one orbiting HD 149143.

Affiliated with

Also associated with

No associations

Rating

Elodie metallicity-biased search for transiting hot Jupiters does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Elodie metallicity-biased search for transiting hot Jupiters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Elodie metallicity-biased search for transiting hot Jupiters will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1165679