[Fe/H]=-2.5 [α/Fe]=0.4 Y=0.40
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Photometric System | Isochrones | Tracks | Based on: | |
BV(RI)c | 0.25 - 1 Gyr | 1 - 15 Gyr | PreMS-RGB | VC03 |
Stromgren uvby | 0.25 - 1 Gyr | 1 - 15 Gyr | PreMS-RGB | Clem et al. (2004) |
UBV(RI)c JHKs | 0.25 - 1 Gyr | 1 - 15 Gyr | PreMS-RGB | B90/2MASS |
HST ACS-WFC | 0.25 - 1 Gyr | 1 - 15 Gyr | PreMS-RGB | S05 |
HST WFPC2 | 0.25 - 1 Gyr | 1 - 15 Gyr | PreMS-RGB | S05 |
HST WFC3 | 0.25 - 1 Gyr | 1 - 15 Gyr | N/A | K08 |
SDSS | 0.25 - 1 Gyr | 1 - 15 Gyr | PreMS-RGB | SDSS DR6 |
ACS GGC Empirical | N/A | 1 - 15 Gyr | PreMS-RGB | VC03/S05 |
ACS GGC Synthetic | N/A | 1 - 15 Gyr | PreMS-RGB | B90/S05 |
Theoretical | N/A | N/A | PreMS-RGB | R,Yc,Zc,etc. |
B90=Bessell (1990); K08=Kalirai (2008, private communication); S05=Sirianni et al. (2005); VC03=Vandenberg & Clem (2003)
Synthetic= PHOENIX + Castelli & Kurucz synthetic fluxes
Empirical uses VC03 plus transformation equations.
More about the isochrones and color transformations can be found in the Reference section.