Issue |
A&A
Volume 414, Number 2, February I 2004
|
|
---|---|---|
Page(s) | 699 - 706 | |
Section | Stellar atmospheres | |
DOI | https://doi.org/10.1051/0004-6361:20031671 | |
Published online | 19 January 2004 |
Library of flux-calibrated echelle spectra of southern late-type dwarfs with different activity levels*,**
Instituto de Astronomía y Física del Espacio, CC. 67, suc. 28, 1428 Buenos Aires, Argentina Visiting Astronomers, Complejo Astronómico El Leoncito operated under agreement between the Consejo Nacional de Investigaciones Científicas y Técnicas de la República Argentina and the National Universities of La Plata, Córdoba and San Juan
Corresponding authors: C. Cincunegui, carolina@iafe.uba.ar pablo@iafe.uba.ar
Received:
24
April
2003
Accepted:
7
October
2003
We present Echelle spectra of 91 late-type dwarfs, of
spectral types from F to M and of different levels of
chromospheric activity, obtained with the 2.15 m telescope of the
CASLEO Observatory located in the Argentinean Andes. Our observations
range from 3890 to 6690 Å at a spectral resolution from 0.141 to
0.249 Å per pixel (). The
observations were flux calibrated with the aid of long slit spectra. A
version of the calibrated spectra is available via the World Wide
Web.
Key words: atlases / stars: late-type
Table 2 is also available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/414/699
The spectra are available as FITS and ascii-files at the URL:
http://www.iafe.uba.ar/cincunegui/spectra/Table2.html. They
are also available in electronic form at the CDS via anonymous ftp to
cdsarc.u-strasbg.fr (130.79.128.5) or via
http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/414/699. When converting the
fits to ascii, the spectra were oversampled to a constant Å.
© ESO, 2004
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