| Issue |
A&A
Volume 422, Number 1, July IV 2004
|
|
|---|---|---|
| Page(s) | 205 - 215 | |
| Section | Stellar structure and evolution | |
| DOI | https://doi.org/10.1051/0004-6361:20040250 | |
| Published online | 06 July 2004 | |
Theoretical isochrones in several photometric systems
II. The Sloan Digital Sky Survey ugriz system
1
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
Corresponding author: L. Girardi, Lgirardi@ts.astro.it
Received:
11
February
2004
Accepted:
30
March
2004
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
© ESO, 2004
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