Theoretical isochrones in several photometric systems II. The Sloan Digital Sky Survey ugriz system

Details Theoretical isochrones in several photometric systems II. The Sloan Digital Sky Survey ugriz system Theoretical isochrones in several photometric systems II. The Sloan Digital Sky Survey ugriz system

2004-04-19

arxiv.org/abs/astro-ph/0404358v1

Astron.Astrophys.422:205-215,2004

Astronomy and Astrophysics

Astrophysics

11 pages, to appear in Astronomy & Astrophysics, data files are available in http://pleiadi.pd.astro.it/isoc_photsys.01/isoc_p

Scientific paper

10.1051/0004-6361:20040250

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.

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