Hostname: page-component-788cddb947-m6qld Total loading time: 0 Render date: 2024-10-19T07:51:24.291Z Has data issue: false hasContentIssue false
  • English
  • Français

First thoughts on stellar variability from Kepler commissioning data

Published online by Cambridge University Press:  26 February 2010

Lucianne M. Walkowicz  and
Gibor Basri
Lucianne M. Walkowicz
Affiliation:
University of California Berkeley, 601 Campbell Hall, Berkeley CA 94720USA email: lucianne@astro.berkeley.edu
Gibor Basri
Affiliation:
University of California Berkeley, 601 Campbell Hall, Berkeley CA 94720USA email: lucianne@astro.berkeley.edu
Rights & Permissions [Opens in a new window]

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.

The Kepler mission will obtain high precision, continuous lightcurves for more than ~150,000 stars over the next four years. Prior to primary mission operations, ten days of commissioning data were obtained for the ~52,000 brightest targets in the Kepler field. While Kepler's main goal is the discovery of transiting low mass planets, it will also provide a rich dataset for studies of variable stars. These commissioning data give a first glimpse of the amazing diversity of stellar variability Kepler will observe. Here, we discuss the tools we are currently developing to quantify variability in the Kepler data, and show initial results on the distribution of target stars in these metrics. Ultimately these measures will be used both to characterize the data and to select active rotationally modulated stars for rotation period determination.

Keywords

stars: activitystars: statistics
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S264: Solar and Stellar Variability: Impact on Earth and Planets , August 2009 , pp. 469 - 474
Copyright
Copyright © International Astronomical Union 2010

References

Basri, G., Borucki, W. J., & Koch, D. G., 2005, New Astron. Revs, 49, 478Google Scholar
Batalha, N. M., et al. 2007, Bulletin of the American Astronomical Society, 38, 974Google Scholar
Eyer, L. & Grenon, M., 1997, ESA-SP 402 (Hipparcos Venice Workshop), p. 467Google Scholar
Gilliland, R. L. 2008, AJ, 136, 566Google Scholar
Horne, J. H. & Baliunas, S. L., 1986, ApJ 302, 757CrossRefGoogle Scholar
Pizzolato, N., Maggio, A., Micela, G., Sciortino, S., & Ventura, P., 2003, A&A, 397, 147Google Scholar
Strassmeier, K. G., 2002, AN 323, 309Google Scholar