Search for high-amplitude δ Scuti and RR Lyrae stars in Sloan Digital Sky Survey Stripe 82 using principal component analysis
Article first published online: 23 JUL 2012
© 2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS
Monthly Notices of the Royal Astronomical Society
Volume 424, Issue 4, pages 2528–2550, 21 August 2012
How to Cite
Süveges, M., Sesar, B., Váradi, M., Mowlavi, N., Becker, A. C., Ivezić, Ž., Beck, M., Nienartowicz, K., Rimoldini, L., Dubath, P., Bartholdi, P. and Eyer, L. (2012), Search for high-amplitude δ Scuti and RR Lyrae stars in Sloan Digital Sky Survey Stripe 82 using principal component analysis. Monthly Notices of the Royal Astronomical Society, 424: 2528–2550. doi: 10.1111/j.1365-2966.2012.21229.x
- Issue published online: 8 AUG 2012
- Article first published online: 23 JUL 2012
- Manuscript Accepted: 2 MAY 2012
- Manuscript Received: 27 APR 2012
- Swiss National Science Foundation MHV. Grant Number: PMPDP2_129178
- National Science Foundation
- US Department of Energy
- National Aeronautics and Space Administration
- Japanese Monbukagakusho
- Max Planck Society
- Higher Education Funding Council
Disclaimer: Supplementary materials have been peer-reviewed but not copyedited.
Table 1. RR Lyrae candidates in Stripe 82.
Table 2. Best-fitting templates of Sesar et al. (2010) for the new RR Lyrae candidates in Stripe 82.
Table 6. HADS candidates in Stripe 82.
Online figures. Summary plots for the complete final sample.
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