Free access article
Astronomy and Astrophysics Supplement Series, Vol. 119, October II 1996, 373-390
ELODIE: A spectrograph for accurate radial velocity measurements
A. Baranne
,
D. Queloz
, M. Mayor
, G. Adrianzyk
, G.
Knispel
, D. Kohler
, D. Lacroix
, J.-P.
Meunier
, G. Rimbaud
and A. Vin
Send offprint requests to: D. Queloz
Observatoire de Marseille, 2 Place Le Verrier, F--13248 Marseille, France
Observatoire de Genève, CH--1290 Sauverny, Switzerland
Observatoire de Haute--Provence, F--04870 Saint Michel l'Observatoire, France
Received September 28, 1995; accepted February 15, 1996
Abstract:
The fibre--fed echelle spectrograph of Observatoire de Haute--Provence, ELODIE, is presented. This instrument has been in operation since the end of 1993 on the 1.93 m telescope. ELODIE is designed as an updated version of the cross--correlation spectrometer CORAVEL, to perform very accurate radial velocity measurements such as needed in the search, by Doppler shift, for brown--dwarfs or giant planets orbiting around nearby stars. In one single exposure a spectrum at a resolution of 42000 (
) ranging from
3906 Å to 6811 Å is recorded on a 1024
1024 CCD. This
performance is achieved by using a
echelle
grating and a combination of a prism and a grism as
cross--disperser. An automatic on--line data treatment reduces
all the ELODIE echelle spectra and computes cross--correlation
functions. The instrument design and the data reduction
algorithms are described in this paper. The efficiency and
accuracy of the instrument and its long term instrumental
stability allow us to measure radial velocities with an accuracy
better than 15ms
for stars up to 9th magnitude in less than 30
minutes exposure time. Observations of 16th magnitude stars are
also possible to measure velocities at about 1kms
accuracy. For
classic spectroscopic studies (
>100) 9th magnitude stars
can be observed in one hour exposure time.
Key words: instrumentation: spectrographs --- methods: data analysis --- techniques: spectroscopic --- radial velocities
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