Issue |
A&A
Volume 417, Number 3, April III 2004
|
|
---|---|---|
Page(s) | 1055 - 1062 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361:20034324 | |
Published online | 26 March 2004 |
An extensive library of synthetic spectra covering the far red, RAVE and GAIA wavelength ranges
1
University of Ljubljana, Department of Physics, Jadranska 19, 1000 Ljubljana, Slovenia
2
CNR - Istituto di Astrofisica Spaziale e Fisica Cosmica, Via del Fosso del Cavaliere, 00133 Roma, Italy
3
INAF - Osservatorio Astronomico di Trieste, Via G.B. Tiepolo 11, 34131 Trieste, Italy
4
Osservatorio Astronomico di Padova, Sede di Asiago, 36012 Asiago (VI), Italy
5
CISAS, Centro Interdipartimentale Studi ed Attività Spaziali dell'Università di Padova, Italy
Corresponding author: T. Zwitter, tomaz.zwitter@fmf.uni-lj.si
Received:
16
September
2003
Accepted:
24
December
2003
A library of 183 588 synthetic spectra based on Kurucz's ATLAS9
models is presented for the far red spectral interval (7653-8747 Å).
It is characterized by K,
,
,
km s-1,
km s-1.
The whole grid of spectra is calculated for resolving powers 8500, 11 500 and 20 000. A section of the grid is
also computed for [
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.
Key words: astronomical data bases: miscellaneous / stars: fundamental parameters / surveys / stars: atmospheres
© ESO, 2004
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