Model Grid

[Fe/H]=0.5 [α/Fe]=0.2

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Photometric SystemIsochronesTracksBased on:
BV(RI)c0.25 - 1 Gyr1 - 15 GyrPreMS-RGBHB-AGBVC03
Stromgren uvby0.25 - 1 Gyr1 - 15 GyrPreMS-RGBHB-AGBClem et al. (2004)
UBV(RI)c JHKs0.25 - 1 Gyr1 - 15 GyrPreMS-RGBHB-AGBB90/2MASS
HST ACS-WFC0.25 - 1 Gyr1 - 15 GyrPreMS-RGBHB-AGBS05
HST WFPC20.25 - 1 Gyr1 - 15 GyrPreMS-RGBHB-AGBS05
HST WFC30.25 - 1 Gyr1 - 15 GyrN/AN/AK08
SDSS0.25 - 1 Gyr1 - 15 GyrPreMS-RGBHB-AGBSDSS DR6
ACS GGC EmpiricalN/A1 - 15 GyrPreMS-RGBHB-AGBVC03/S05
ACS GGC SyntheticN/A1 - 15 GyrPreMS-RGBHB-AGBB90/S05
TheoreticalN/AN/APreMS-RGBHB-AGBR,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.
Maintained by Aaron Dotter. Questions or Comments? Click here to send an email.