Physical Parameters for RR Lyrae Stars in the SDSS Filter System
arXiv:1301.5626 · doi:10.1017/S1743921312021230
Abstract
We present a calibration of the metallicity and physical parameters (temperature, luminosity, gravity, mass, radius) for RR Lyrae stars using the ugriz SDSS photometric system. Our work is based on calculations of synthetic horizontal branches (HBs), fully taking into account evolutionary effects for a wide range in metallicities and HB morphologies. We provide analytical fits that are able to provide all quantities mentioned with very high (internal) precision, based solely on mean SDSS magnitudes and colors.
4 pages, contributed paper, proceedings IAU Symp. 289
References in corpus (9)
- The Eighth Data Release of the Sloan Digital Sky Survey: First Data from SDSS-III
- The Milky Way Tomography with SDSS: II. Stellar Metallicity
- SkyMapper Filter Set: Design and Fabrication of Large Scale Optical Filters
- Towards More Precise Survey Photometry for PanSTARRS and LSST: Measuring Directly the Optical Transmission Spectrum of the Atmosphere
- The Period-Luminosity Relation of RR Lyrae Stars in the SDSS Photometric System
- Identifying Blue Horizontal Branch Stars Using the z Filter
- Characterisation of Sloan Digital Sky Survey Stellar Photometry
- Predicted properties of RR Lyrae stars in the SDSS photometric system
- Exploring the Variable Sky with the Sloan Digital Sky Survey