New! (05mar12) A few photometric systems/filters were added recently: Pan-STARRS1, Swift/UVOT, Kepler, VISIR.
Choose among the available photometric systems:
2MASS + Spitzer (IRAC+MIPS)
2MASS + Spitzer (IRAC+MIPS) + WISE
UBVRIJHK (cf. Maiz-Apellaniz 2006 + Bessell 1990)
UBVRIJHKLMN (cf. Bessell 1990 + Bessell & Brett 1988)
DMC 14 filters
DMC 15 filters
ESO/EIS (WFI UBVRIZ + SOFI JHK)
GALEX FUV+NUV (Vegamag) + Johnson's UBV
GALEX FUV+NUV + SDSS ugriz (all ABmags)
HST+GALEX+Swift/UVOT UV filters
HST/STIS imaging mode
HST/WFC3 IR channel (final throughputs)
HST/WFC3 UVIS channel, chip 1 (final throughputs)
HST/WFC3 UVIS channel, chip 2 (final throughputs)
HST/WFC3 medium filters (UVIS1+IR, final throughputs)
HST/WFC3 wide filters (UVIS1+IR, final throughputs)
HST/WFPC2 (Vegamag, cf. Holtzman et al. 1995)
Kepler + SDSS griz + DDO51 (in ABmags)
Kepler + SDSS griz + DDO51 (in ABmags) + 2MASS (~Vegamag)
SDSS ugriz + 2MASS JHKs
SDSS ugriz + UKIDSS ZYJHK
SWIFT/UVOT UVW2, UVM2, UVW1,u (Vegamag)
UKIDSS ZYJHK (Vegamag)
VISTA ZYJHKs (Vegamag)
Washington CMT1T2 + DDO51
They are briefly described here.
For Carbon stars, you can choose bolometric corrections based either on Loidl et al. (2001) (as in Marigo et al. (2008) and Girardi et al. (2008)) or on Aringer et al. (2009) (Note: The interpolation scheme has been slightly improved w.r.t. to the paper's Fig. 19.)
Warning: For the moment, interstellar extinction works only for isochrone tables, not for LFs or SSP integrated magnitudes.
WARNING: with the latest Girardi et al. (2010) TP-AGB tracks, the maximum age for a reliable interpolation in metallicity is 13.5 Gyr, or logt=10.13. Please avoid larger ages for the moment.
Single isochrone of t = yr, and Z = Sequence of isochrones of constant metallicity, Z = , from log(t/yr) = to at steps of Δ(logt) = Sequence of isochrones of constant age, t = , from Z = to at steps of ΔZ =
gzip the output file (Files above 2 Mby will always be gzipped!)