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Issue A&A Volume 422, Number 1, July IV 2004 Page(s) 205 - 215 Section Stellar structure and evolution DOI 10.1051/0004-6361:20040250

A&A 422, 205-215 (2004)
DOI: 10.1051/0004-6361:20040250

Theoretical isochrones in several photometric systems

II. The Sloan Digital Sky Survey ugriz system

L. Girardi¹, E. K. Grebel^{2, 3}, M. Odenkirchen³ and C. Chiosi<sup>4

1</sup>  Osservatorio Astronomico di Trieste - INAF, via G.B. Tiepolo 11, 34131 Trieste, Italy
²  Astronomisches Institut der Universität Basel, Venusstrasse 7, 4102 Binningen, Switzerland
³  Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany
⁴  Dipartimento di Astronomia, Università di Padova, Vicolo dell'Osservatorio 2, 35122 Padova, Italy

(Received 11 February 2004 / Accepted 30 March 2004)

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.

Key words: stars: fundamental parameters -- stars: Hertzprung-Russell (HR) and C-M diagrams -- galaxies: globular clusters: individual: Palomar 5 -- galaxies: globular clusters: individual: NGC 2419 -- galaxies: individual: Draco dSph

Offprint request: L. Girardi, Lgirardi@ts.astro.it

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