Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004a%26a...414..699c&link_type=abstract
Astronomy and Astrophysics, v.414, p.699-706 (2004)
Astronomy and Astrophysics
Astrophysics
18
Atlases, Stars: Late-Type
Scientific paper
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 (R=λ/δ λ ≈ 26 400). 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.
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 δ λ ≈ 0.15 Å.
Table 2 is also available in electronic form at the CDS via anonymous
Cincunegui Carolina
Mauas Pablo J. D.
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