A library of synthetic galaxy spectra for GAIA. Comparison with SDSS.

Astronomy and Astrophysics – Astronomy

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Introduction: The ESA cornerstone mission GAIA will acquire spectrophotometric observations of a large number of unresolved galaxies. An integral part of the data analysis task is the preparation of a library of galaxy spectra, suitable for the classification and parameterization of the observed objects. Methods: An extended grid of synthetic galaxy spectra has been created, using the code PEGASE.2, which is based on models of galaxy evolutionary synthesis and the BaSeL stellar spectral library. Results: The library contains about 4000 zero-redshift spectra, in the wavelength range 250 to 1050 nm and at one nm or less resolution, and covers the main morphological (Hubble) types of galaxies, at a regular grid of four key astrophysical parameters for each type and at intermediate random values of the same parameters. In addition, the library is produced for various redshifts. Discussion: This synthetic library has been compared with real spectra obtained from SDSS. We have produced two-color diagrams computed from both the synthetic PEGASE.2 and the real SDSS spectra. The agreement is very good at the full range of morphological types.

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