Hostname: page-component-cc8bf7c57-ksm4s Total loading time: 0 Render date: 2024-12-12T06:29:11.103Z Has data issue: false hasContentIssue false
  • English
  • Français

Towards 1 ms−1 RV Accuracy

Published online by Cambridge University Press:  26 May 2016

F. Pepe ,
M. Mayor ,
D. Queloz  and
S. Udry
F. Pepe
Affiliation:
Geneva Observatory, 51 ch. des Maillettes, 1290 Sauverny, Switzerland
M. Mayor
Affiliation:
Geneva Observatory, 51 ch. des Maillettes, 1290 Sauverny, Switzerland
D. Queloz
Affiliation:
Geneva Observatory, 51 ch. des Maillettes, 1290 Sauverny, Switzerland
S. Udry
Affiliation:
Geneva Observatory, 51 ch. des Maillettes, 1290 Sauverny, Switzerland

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Since the discovery of 51 Peg by Mayor & Queloz (1995) about 50 extra-solar planets have been discovered by means of the Doppler technique, and much more will follow. In future the goal will be to detect even lighter planets and/or planets with longer orbital periods, which may induce changes of only few m/s on the radial velocity of their parent star. Therefore very high performance instruments will be required. In view of the realization of HARPS (Pepe et al. 2000), the high-accuracy RV spectrograph for the ESO 3.6-m telescope dedicated to extra-solar planet search, we are investigating the accuracy limits and possible error sources. First results are presented in this paper.

Type
Part I: Discovery and study of extrasolar planets - current
Information
Symposium - International Astronomical Union , Volume 202: Planetary Systems in the Universe – Observation, Formation and Evolution , 2004 , pp. 103 - 105
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Baranne, A., Queloz, D., Mayor, , et al. 1996, A&A, 119, 373.Google Scholar
Mayor, M., Queloz, D. 1995, Nature, 378, 355.Google Scholar
Pepe, F., Mayor, M., Delabre, , et al. 2000, in SPIE conf. 4008, Optical and IR Telescope Instrumentation and Detectors.Google Scholar