Rmodel: Determining Stellar Population Parameters

Details Rmodel: Determining Stellar Population Parameters Rmodel: Determining Stellar Population Parameters

Apr 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ascl.soft04008c&link_type=abstract

Astrophysics Source Code Library, record ascl:1104.008

Astronomy and Astrophysics

Astrophysics

Scientific paper

This program determines stellar population parameters (e.g. age,
metallicity, IMF slope,...), using as input a pair of line-strength
indices, through the interpolation in SSP model predictions. Both linear
and bivariate fits are computed to perform the interpolation.

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