Okayama Planet Search Program: Difference between revisions
OPSP, http://adsabs.harvard.edu/abs/2005JKAS...38...81I |
removed Category:Exoplanetology; added Category:Exoplanet search projects using HotCat |
||
Line 11: | Line 11: | ||
* {{cite web | url=http://www.oao.nao.ac.jp/en/telescope/abouttel188/| title=telescope | work=http://www.oao.nao.ac.jp | accessdate=2008-10-11}} |
* {{cite web | url=http://www.oao.nao.ac.jp/en/telescope/abouttel188/| title=telescope | work=http://www.oao.nao.ac.jp | accessdate=2008-10-11}} |
||
[[Category: |
[[Category:Exoplanet search projects]] |
||
Revision as of 19:58, 23 November 2013
The Okayama Planet Search Program (OPSP) was started in 2001 with the goal of spectroscopically searching for planetary systems around stars. It reported on the detection of 3 new extrasolar planets: (18 Delphini b, ksi Aql b, and 41 Lyncis b), around intermediate-mass G and K giants 18 Delphini, Xi Aquilae, and HD 81688. Also, it updated the orbital parameters of HD 104985 b, the first planet discovered around the G giants from the survey, by using the data collected during the past six years. Since 2001, it has been conducting a precise Doppler survey of about 300 G and K giants using a 1.88m telescope, the High Dispersion Echelle Spectrograph (HIDES), and an iodine absorption cell I2 cell at the Okayama Astrophysical Observatory (OAO).
Observatory
- Okayama Astrophysical Observatory, Kurashiki in Japan
References
- "Okayama Astrophysical Observatory Homepage". http://www.oao.nao.ac.jp. Retrieved 2008-10-11.
{{cite web}}
: External link in
(help)|work=
- "Planetary Companions around Three Intermediate-Mass G and K Giants: 18 Delphini, Xi Aquilae, and HD81688" (PDF). http://www.oao.nao.ac.jp. Retrieved 2008-10-11.
{{cite web}}
: External link in
(help)|work=
- "telescope". http://www.oao.nao.ac.jp. Retrieved 2008-10-11.
{{cite web}}
: External link in
(help)|work=