An extensive library of 2500–10 500 Å synthetic spectra

We present a complete library of synthetic spectra based on Kurucz’s codes that covers the 2500–10 500 A wavelength range at resolving powers RP = 20 000, 11 500 (≡GAIA), 8500 (≡RAVE), 2000 (≡SLOAN) and uniform dispersions of 1 and 10 A/pix. The library maps the whole HR diagram, exploring 51 288 combinations of atmospheric parameters spanning the ranges: 3500 ≤ Teff ≤ 47 500 K, 0.0 ≤ log g ≤ 5.0, −2.5 ≤ [M/H] ≤ 0.5, [α/Fe] = 0.0,+0.4, ξ = 1, 2, 4 km s −1 ,0 ≤ Vrot ≤ 500 km s −1 . The spectra are available both as absolute fluxes as well as continuum normalized. Performance tests and spectroscopic applications of the library are discussed, including automatic classification of data from spectroscopic surveys like RAVE, SLOAN, GAIA. The entire library of synthetic spectra is accessible via the web.

[1]  R. Kurucz,et al.  Is missing Fe I opacity in stellar atmospheres a significant problem , 2004 .

[2]  U. Munari,et al.  Asiago eclipsing binaries program I. V432 Aurigae , 2004 .

[3]  E. al.,et al.  The Sloan Digital Sky Survey: Technical summary , 2000, astro-ph/0006396.

[4]  A. Buzzoni,et al.  ATLAS Versus NextGen Model Atmospheres: A Combined Analysis of Synthetic Spectral Energy Distributions , 2004, astro-ph/0406215.

[5]  U. Munari,et al.  High resolution spectroscopy over $\lambda\lambda$ 8500-8750 Å for GAIA , 1999 .

[6]  Astrophysics,et al.  On the Anomaly of Balmer Line Profiles of A-Type Stars. Fundamental binary systems , 2002, astro-ph/0209239.

[7]  P. Treanor Stellar Evolution , 1951, Nature.

[8]  U. Munari,et al.  High resolution spectroscopy over $\mathsf{\lambda\lambda}$ 8500-8750 Å for GAIA - IV. Extending the cool MK stars sample , 2003 .

[9]  A library of high-resolution Kurucz spectra in the range λλ3000–10 000 , 2004, astro-ph/0404010.

[10]  M. Bessell The Temperature Scale for Cool Dwarfs , 1995 .

[11]  C. Leitherer,et al.  A high-resolution stellar library for evolutionary population synthesis , 2005, astro-ph/0501225.

[12]  E. al.,et al.  Spectroscopic survey of the Galaxy with Gaia– I. Design and performance of the Radial Velocity Spectrometer , 2004, astro-ph/0409709.

[13]  Nancy Houk,et al.  University of Michigan Catalogue of two-dimensional spectral types for the HD stars. Volume I. Declinations -90_ to -53_f0. , 1975 .

[14]  Robert L. Kurucz,et al.  SYNTHE Spectrum Synthesis Programs and Line Data. , 1993 .

[15]  M. Perryman,et al.  The Three-Dimensional Universe with Gaia , 2005 .

[16]  G. Paltoglou,et al.  The Calibration of Synthetic Colours , 1994 .

[17]  U.Munari,et al.  The distance to the Pleiades from orbital solution of the double-lined eclipsing binary HD 23642 , 2004, astro-ph/0403444.

[18]  Faraday Discuss , 1985 .

[19]  C. Morossi,et al.  An Atlas of high resolution synthetic spectra in the wavelength region $\bf 4850-5400 \AA$ , 1997 .

[20]  Dept. of Physics,et al.  An extensive library of synthetic spectra covering the far red, RAVE and GAIA wavelength ranges , 2004, astro-ph/0401069.

[21]  Nikolai Piskunov,et al.  Modelling of Stellar Atmospheres , 2003 .

[22]  Nancy Houk,et al.  Michigan catalogue of two-dimensional spectral types for the HD stars , 1975 .

[23]  J. Christensen-Dalsgaard,et al.  Theory of Stellar Pulsation , 1982 .

[24]  V. Straižys,et al.  Fundamental stellar parameters derived from the evolutionary tracks , 1981 .

[25]  D. A. Banks,et al.  The Three-Dimensional Universe. , 1992 .

[26]  A. Bijaoui,et al.  Spectroscopic Survey of the Galaxy with Gaia II. The expected science yield from the Radial Velocity Spectrometer , 2005, astro-ph/0506083.

[27]  D. Schwenke Opacity of TiO from a coupled electronic state calculation parametrized by abinitio and experimental data , 1998 .

[28]  N. Grevesse,et al.  Abundances of the elements: Meteoritic and solar , 1989 .

[29]  F. Castelli,et al.  Round Table Summary: Problems in Modelling Stellar Atmospheres , 2003 .

[30]  Jianmin Yuan Atomic Data for Opacity Calculations , 2007 .

[31]  V. Straižys Multicolor Stellar Photometry , 1992 .