MILES base models & new line index system (Vazdekis+, 2010)
We present synthetic spectral energy distributions (SEDs) for single-age, single-metallicity stellar populations (SSPs) covering the full optical spectral range at moderately high resolution [full width at half-maximum (FWHM)=2.3Å]. These SEDs constitute our base models, as they combine scaled-solar isochrones with an empirical stellar spectral
Vazdekis, A. et al.
Fecha de publicación:
11
2010