Database of Geneva stellar evolution tracks and isochrones for (UBV)(J)(RI)(C) JHKLL ' M, HST-WFPC2, Geneva and Washington photometric systems

We have used an updated version of the empirically and semi-empirically cal ibrated BaSeL library of synthetic stellar spectra of Lejeune et al. (1997, 1998) and Westera ct al. (1911'3) to calculate synthetic photometry in the (UBV)(J)(RI)(C) JHKLL'M, HST-WFPC2, Geneva, and Washington systems for the entire set of non-rotating Geneva stellar evolution models covering masses front 0.4-0.8 to 120 150 M., and metallicities Z = 0.0004 (1/50 Z.) to 0.1 (5 Z.) The results are provided in a database which includes all individua l stellar tracks and the corresponding isochrones covering ages from 10(3) yr to 16-20 Gyr in time steps of Delta log t = 0.05 dex. The database also includes a new grid of stellar tracks of very metal-poor stars (Z = 0.0004) from 0.8-150 M. calculated with the Geneva stellar evolution code.