Library of medium-resolution Fiber Optic Echelle spectra of
F, G, K and M field dwarfs to giants stars
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D. Montes1,2,, L.W. Ramsey2, A.D. Welty3,
1
Departamento de Astrofísica, Univerdidad Complutense de Madrid
2
The Pennsylvania State University,
Dept. of Astronomy & Astrophysics
3
Space Telescope Science Institute
(accepted November 1998)
1999, Astrophysical Journal Supplement Series, 123, 283 (July 1999 Vol. 123 #1)
PS_file
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PDF file
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HTML
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Available at CDS (J/ApJS/123/283/)
to H_epsilon),
Ca II H & K,
Mg I b triplet,
Na I D1,D2,
He I D3,
and Ca II IRT lines, as well as a large number of
photospheric lines, which can also be affected by chromospheric activity,
and temperature sensitive photospheric features such
as TiO bands.
The spectra have been compiled with the aim of providing a set of
standards observed at medium-resolution.
We have extensively used such data for the study of active chromosphere
stars by
applying a spectral subtraction technique.
However, the data set presented here can also be utilized in a wide
variety of
ways ranging from radial velocity templates to study of variable stars
and stellar population synthesis.
This library can also be used for spectral classification purposes,
and determination of atmospheric parameters (T_eff}, log{g},
[Fe/H]).
A digital version with all the fully reduced spectra is available
via ftp and the
World Wide Web (WWW) in FITS format.
Echelle Spectra
H
line region
spectra
NaI D1,
D2,
and HeI D3 line region
spectra
H
This page is under construction
