Theoretical isochrones in several photometric systems II. The Sloan Digital Sky Survey ugriz system
arXiv:astro-ph/0404358 · doi:10.1051/0004-6361:20040250
Abstract
Following Paper I, we provide extended tables of bolometric corrections, extinction coefficients, stellar isochrones, and integrated magnitudes and colours of single-burst stellar populations, for the Sloan Digital Sky Survey (SDSS) ugriz photometric system. They are tested on comparisons with DR1 data for a few stellar systems, namely the Palomar 5 and NGC 2419 globular clusters and the Draco dSph galaxy.
11 pages, to appear in Astronomy & Astrophysics, data files are available in http://pleiadi.pd.astro.it/isoc_photsys.01/isoc_photsys.01.html