Method of stellar population synthesis dedicated to the IR range

Details Method of stellar population synthesis dedicated to the IR range Method of stellar population synthesis dedicated to the IR range

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sf2a.conf..605f&link_type=abstract

SF2A-2004: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 14-18, 2004. Edited by F. Combes, D. Barret

Astronomy and Astrophysics

Astrophysics

Scientific paper

The importance of the IR domain in determining stellar populations from the integrated light of galaxies will be shown. A new code dedicated to these investigations and based on flux measurement, including emission by dust, will be presented. The method used is a revival of the quadratic programming first intraduced by Faber (1972). It is required to perform proper error analysis, both for the statistical and the systematic errors.

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