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Steps Towards Absolute Accuracy In Radial Velocities1
Published online by Cambridge University Press: 12 April 2016
Abstract
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We are developing methods to reach high absolute accuracy in spectroscopic radial velocities for stars of different spectral types. The basic idea is to remove the effects from convection and surface gravity that cause large systematic errors, in order to improve the absolute accuracy of radial velocities by one order of magnitude. This paper briefly describes observations and methodology in computing the radial velocities.
- Type
- Part 2. Fundamental Concepts and Techniques
- Information
- International Astronomical Union Colloquium , Volume 170: Precise Stellar Radial Velocities , 1999 , pp. 58 - 62
- Copyright
- Copyright © Astronomical Society of the Pacific 1999
Footnotes
1
Data were obtained at Observatoire de Haute-Provence, Prance
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