Spectrum radial velocity analyser (SERVAL). High-precision radial velocities and two alternative spectral indicators
M. Zechmeister, A. Reiners, P. J. Amado, M. Azzaro, F. F. Bauer, V. J., S. B\'ejar, J. A. Caballero, E. W. Guenther, H.-J. Hagen, S. V. Jeffers, A., Kaminski, M. K\"urster, R. Launhardt, D. Montes, J. C. Morales, A., Quirrenbach, S. Reffert, I. Ribas, W. Seifert, L. Tal-Or

TL;DR
SERVAL is a high-precision, publicly available Python tool that measures stellar radial velocities and introduces spectral diagnostics like the chromatic index and differential line width to identify stellar activity effects.
Contribution
We developed the SERVAL algorithm, providing high-precision RV measurements and novel spectral indicators to analyze stellar activity in high-resolution spectra.
Findings
SERVAL achieves 1 m/s RV precision with HARPS data.
The chromatic index effectively identifies activity-induced RV variations.
Differential line width serves as an alternative stellar activity indicator.
Abstract
Context: The CARMENES survey is a high-precision radial velocity (RV) programme that aims to detect Earth-like planets orbiting low-mass stars. Aims: We develop least-squares fitting algorithms to derive the RVs and additional spectral diagnostics implemented in the SpEctrum Radial Velocity Analyser (SERVAL), a publicly available python code. Methods: We measured the RVs using high signal-to-noise templates created by coadding all available spectra of each star.We define the chromatic index as the RV gradient as a function of wavelength with the RVs measured in the echelle orders. Additionally, we computed the differential line width by correlating the fit residuals with the second derivative of the template to track variations in the stellar line width. Results: Using HARPS data, our SERVAL code achieves a RV precision at the level of 1m/s. Applying the chromatic index to…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Astrophysics and Star Formation Studies
