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A&A 402, 433-442 (2003)
DOI: 10.1051/0004-6361:20030243
STELIB: A library of stellar spectra at
J.-F. Le Borgne1, G. Bruzual2, R. Pelló1, A. Lançon3, B. Rocca-Volmerange4, B. Sanahuja5, D. Schaerer1, C. Soubiran6 and R. Vílchez-Gómez7
1 Laboratoire d'Astrophysique, UMR 5572, Observatoire Midi-Pyrénées, 14 Avenue E. Belin, 31400 Toulouse, France
2 Centro de Investigaciones de Astronomía, AP 264, 5101-A Mérida, Venezuela
3 Observatoire de Strasbourg, UMR 7550, 11 rue de l'Université, 67000 Strasbourg, France
4 Institut d'Astrophysique de Paris, UMR 7095, 98 bis Boulevard Arago, 75014 Paris, France
5 Departament d'Astronomia i Meteorologia, Universitat de Barcelona, Martí i Franquès 1, 08028 Barcelona, Spain
6 Observatoire de Bordeaux, UMR 5804, BP 89, 33270 Floirac, France
7 Departamento de Física, Universidad de Extremadura, Avda. de la Universidad, s/n 10071 Cáceres, Spain
(Received 11 September 2002 / Accepted 14 February 2003 )
Abstract
We present STELIB, a new spectroscopic stellar library,
available at http://webast.ast.obs-mip.fr/stelib. STELIB consists of an
homogeneous library of 249 stellar spectra in the visible range (3200 to
9500 Å), with an intermediate spectral resolution (
3 Å) and sampling
(1 Å). This library includes stars of various spectral types and luminosity
classes, spanning a relatively wide range in metallicity. The spectral
resolution, wavelength and spectral type coverage of this library represents a
substantial improvement over previous libraries used in population synthesis
models. The overall absolute photometric uncertainty is 3%.
Key words: atlases -- stars: fundamental parameters -- galaxies: stellar content.
Offprint request: J.-F. Le Borgne, leborgne@ast.obs-mip.fr
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