SARG Extra Solar Planet Search

Details SARG Extra Solar Planet Search SARG Extra Solar Planet Search

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.485..265g&link_type=abstract

In: Proceedings of the First Eddington Workshop on Stellar Structure and Habitable Planet Finding, 11 - 15 June 2001, Córdoba, S

Computer Science

Stars: Asteroseismology, Planets: Exoplanets

Scientific paper

SARG (Spettrografo Alta Risoluzione Galileo) is the high resolution spectrograph of TNG (Telescopio Nazionale Galileo), the Italian National Telescope in operation at La Palma (Canary Island, Spain). The spectrograph is equipped with an iodine cell in order to perform high precision radial velocity measurements. It is used by the SARG Extra Solar Planet Search: this quest (started from September 2000) is devoted to find planets around individual components of wide binary systems with a parallax larger than 10.0 mas and declination greater than 20 degree. In this contribution we describe the spectrograph, the survey criterion and some preliminary results.

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