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Minimizing Radial-velocity Errors caused by Spectral-type Mismatch in Early-type Stars

Published online by Cambridge University Press:  12 April 2016

Werner Verschueren
Affiliation:
University of Antwerp (RUCA), Astrophysics Research Group, Groenenborgerlaan 171, 2020 Antwerpen, Belgium
Marc David
Affiliation:
University of Antwerp (RUCA), Astrophysics Research Group, Groenenborgerlaan 171, 2020 Antwerpen, Belgium
Myriam Vrancken
Affiliation:
Royal Observatory of Belgium, Ringlaan 3, 1180 Brussel, Belgium

Abstract

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We present the first results of a long-term study to increase the external accuracy of (relative and absolute) radial velocities of early-type stars below the 1 km/s level. The accuracy suffers mainly from important systematic errors caused by intrinsic object-template mismatch in cross-correlation. Based on synthetic spectra, the magnitude of these mismatch errors is shown in different spectral regions and for different rotational velocities around spectral-type mid-A. A line selection and combination scheme is proposed which optimizes the accuracy (systematic errors) in view of the precision (random errors) required.

Type
Part 2. Fundamental Concepts and Techniques
Copyright
Copyright © Astronomical Society of the Pacific 1999

References

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