Theoretical isochrones in several photometric systems II. The Sloan Digital Sky Survey ugriz system
Astrophysics
2011-05-05 v1
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.
Cite
@article{arxiv.astro-ph/0404358,
title = {Theoretical isochrones in several photometric systems II. The Sloan Digital Sky Survey ugriz system},
author = {L. Girardi and E. K. Grebel and M. Odenkirchen and C. Chiosi},
journal= {arXiv preprint arXiv:astro-ph/0404358},
year = {2011}
}
Comments
11 pages, to appear in Astronomy & Astrophysics, data files are available in http://pleiadi.pd.astro.it/isoc_photsys.01/isoc_photsys.01.html