4.6 Article

An extensive library of synthetic spectra covering the far red, RAVE and GAIA wavelength ranges

Journal

ASTRONOMY & ASTROPHYSICS
Volume 417, Issue 3, Pages 1055-1062

Publisher

EDP SCIENCES S A
DOI: 10.1051/0004-6361:20034324

Keywords

astronomical data bases : miscellaneous; stars : fundamental parameters; surveys; stars : atmospheres

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A library of 183 588 synthetic spectra based on Kurucz's ATLAS9 models is presented for the far red spectral interval (7653-8747 Angstrom). It is characterized by 3500 K less than or equal to T(eff) less than or equal to 47 500 K, 0.0 less than or equal to log g less than or equal to 5.0, -3.0 less than or equal to [M/H] less than or equal to +0.5, 0 less than or equal to V(rot) less than or equal to 500 km s(-1), xi = 2 km s(-1). The whole grid of spectra is calculated for resolving powers 8500, 11500 and 20000. A section of the grid is also computed for [alpha/Fe] = +0.4 and for microturbulent velocities 0 and 4 km s(-1). The library covers the wavelength ranges and resolutions of the two ambitious spectroscopic surveys by the ground experiment RAVE and the space mission GAIA. Cross-sections across the multi-dimensional data-cube are used to illustrate the behaviour of the strongest spectral lines. Interpretation of real data will have to include interpolation to grid substeps. We present a simple estimate of the accuracy of such a procedure.

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