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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. Grebel2, 3, M. Odenkirchen3 and C. Chiosi41 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
SIMBAD Objects
© ESO 2004
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