Stellar populations and their kinematics from high and medium resolution spectra: mixed inversions

Astronomy and Astrophysics – Astrophysics

Scientific paper

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2 pages, 2 figures, poster presented at SF2A 2003 conference in Bordeaux

Scientific paper

We present inversion techniques aiming at recovering the stellar content
(age, metallicity, extinction) and kinematics of a stellar population from its
absorption line spectrum. These techniques use new synthetic high resolution
spectra produced by PEGASE_HR and minimization algorithms. Application to SDSS
data and to a simulated disc-bulge system are presented as examples.

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