SOPHIE: the successor of the spectrograph ELODIE for extrasolar planet search and characterization

Details SOPHIE: the successor of the spectrograph ELODIE for extrasolar planet search and characterization SOPHIE: the successor of the spectrograph ELODIE for extrasolar planet search and characterization

Feb 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006tafp.conf..319b&link_type=abstract

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

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The SOPHIE echelle spectrograph is presently built at the Haute Provence Observatory (OHP). It will replace and upgrade the ELODIE spectrograph, well known for the discovery of the first hot Jupiter 51Peg-b ten years ago. This new spectrograph is going to be installed at the 1.93-cm telescope and be commissioned beginning of 2006. Primarily based on the experiment acquired on HARPS (3.6-m ESO), SOPHIE should be considered as its North counter part. Its main characteristics and expected performances are described. Some exoplanet programs which will be conducted these next years are presented.

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