Modelling and interpreting optical spectra of galaxies at R=10000

Ariane Lancon; Pierre Ocvirk; Damien Le Borgne; Christophe Pichon; Philippe Prugniel; Michel Fioc; Brigitte Rocca-Volmerange; Caroline Soubiran

doi:10.1063/1.1913917

arXiv · astro-ph/0501278

Modelling and interpreting optical spectra of galaxies at R=10000

Ariane Lancon·Pierre Ocvirk·Damien Le Borgne·Christophe Pichon·Philippe Prugniel·Michel Fioc·Brigitte Rocca-Volmerange·Caroline Soubiran

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Abstract

One way to extract more information from the integrated light of galaxies is to improve the spectral resolution at which observations and analysis are carried out. The population synthesis code currently providing the highest spectral resolution is Pegase-HR, which was made available by D. Le Borgne et al. in 2004. Based on an empirical stellar library, it provides synthetic spectra between 4000 and 6800 A at lambda/d(lambda)=10000 for any star formation history, with or without chemical evolution. Such a resolution is particularly useful for the study of low mass galaxies, massive star clusters, or other galaxy regions with low internal velocity dispersions. After a summary of the main features of Pegase-HR and comparisons with other population synthesis codes, this paper focuses on the inversion of optical galaxy spectra. We explore the limits of what information can or can not be recovered, based on theoretical principles and extensive simulations. First applications to extragalactic objects are shown.

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Ariane Lancon, Pierre Ocvirk, Damien Le Borgne, Christophe Pichon, Philippe Prugniel, Michel Fioc, Brigitte Rocca-Volmerange, Caroline Soubiran. 2005-01-14. Modelling and interpreting optical spectra of galaxies at R=10000. https://doi.org/10.1063/1.1913917

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