BaSeL¶
- class beast.physicsmodel.stars.stellib.BaSeL(*args, **kwargs)[source]¶
Bases:
Stellib- BaSeL 2.2 (This library is used in Pegase.2)
This library is used in Pegase.2
The BaSeL stellar spectral energy distribution (SED) libraries are libraries of theoretical stellar SEDs recalibrated using empirical photometric data. Therefore, we call them semi-empirical libraries.
The BaSeL 2.2 library was calibrated using photometric data from solar metallicity stars.
References
Lejeune, Cuisiner, and Buser, 1998 A&AS, 130, 65
Contructor
Attributes Summary
Methods Summary
bbox([dlogT, dlogg])Boundary of Basel 2.2 library
Attributes Documentation
- NHI¶
- NHeI¶
- NHeII¶
- Teff¶
- Z¶
- logT¶
- logZ¶
- logg¶
Methods Documentation