ELODIE spectrograph

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ELODIE was an echelle spectrograph installed on the 1.93m reflector at the Observatoire de Haute-Provence in south-eastern France. Its optical instrumentation was developed by André Baranne from the Marseille Observatory. The purpose of the instrument was extrasolar planet detection by the radial velocity method.

ELODIE's first light was achieved in 1993. The instrument was decommissioned in August 2006 and replaced in September 2006 by SOPHIE, a new instrument of the same type but with improved features.[1][2]

Characteristics

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The instrument could observe the electromagnetic spectrum over a wavelength range of 389.5 nm to 681.5 nm in a single exposure, split into 67 spectral orders. The instrument, which was located in a temperature-controlled room, was fed with optical fibers from the Cassegrain focus. The observatory provided an integrated data reduction pipeline which fully reduced the spectra immediately after acquisition and allowed the user to measure radial velocities to an accuracy as good as ±7 m/s.

Over 34,000 spectra were taken with ELODIE, over 20,000 of which are publicly available through a dedicated on-line archive.[3] The instrument was the result of a collaboration between the observatories of Haute-Provence, Geneva and Marseille. A publication describing the instrument appeared in Astronomy & Astrophysics Supplements.[4]

Discovered planets

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The first extrasolar planet to be discovered orbiting a Sun-like star, 51 Pegasi b, was discovered in 1995 using ELODIE.[5] Michel Mayor and Didier Queloz received the Nobel Prize in Physics in 2019 for their achievement. [6] Over twenty such planets have been found with ELODIE.

The instrument was also used to find a planet by the transit method.[7]

Planet Announced in Ref
51 Pegasi b 1995 [5]
Gliese 876 b 1998 [8]
14 Herculis b 1998 [9]
HD 209458 b 1999 [7]

See also

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References

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  1. ^ The ELODIE-SOPHIE Archive in the Virtual Observatory, S. Ilovaisky, Ph. Prugniel, C. Soubiran, M. Koleva, and H. Le Coroller, in Astronomical spectroscopy and the Virtual Observatory, Madrid (Spain), March 21–23, 2007, Madrid, 2007.
  2. ^ A user's guide to Elodie archive data products, Elodie archive, Observatoire de Haute Provence. Accessed on line June 15, 2008.
  3. ^ The ELODIE archive. Accessed on line June 15, 2008.
  4. ^ ELODIE: A spectrograph for accurate radial velocity measurements, A. Baranne et al., Astronomy and Astrophysics Supplement 119 (October 1996), pp.373–390. Bibcode:1996A&AS..119..373B
  5. ^ a b Mayor; Queloz, Didier (1995). "A Jupiter-mass companion to a solar-type star". Nature. 378 (6555): 355–359. Bibcode:1995Natur.378..355M. doi:10.1038/378355a0.
  6. ^ "The Nobel Prize in Physics 2019". Nobel Media AB. Retrieved 8 October 2019.
  7. ^ a b Queloz; et al. (2000). "Detection of a spectroscopic transit by the planet orbiting the star HD209458". Astronomy and Astrophysics Letters. 359: L13–L17. arXiv:astro-ph/0006213. Bibcode:2000A&A...359L..13Q.
  8. ^ Delfosse, Xavier; Forveille, Thierry; Mayor, Michel; Perrier, Christian; Naef, Dominique; Queloz, Didier (1998). "The closest extrasolar planet. A giant planet around the M4 dwarf GL 876". Astronomy and Astrophysics. 338: L67–L70. arXiv:astro-ph/9808026. Bibcode:1998A&A...338L..67D.
  9. ^ Naef, Dominique; Mayor, Michel; Beuzit, Jean-Luc; Perrier, Christian; Queloz, Didier; Sivan, Jean-Pierre; Udry, Stéphane (2004). "The ELODIE survey for northern extra-solar planets. III. Three planetary candidates detected with ELODIE" (PDF). Astronomy and Astrophysics. 414 (1): 351–359. arXiv:astro-ph/0310261. Bibcode:2004A&A...414..351N. doi:10.1051/0004-6361:20034091.
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