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III/153 An Atlas of Near Infrared Stellar Spectra (Arnaud+ 1989)
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Beginning of ReadMe :III/153 An Atlas of Near Infrared Stellar Spectra (Arnaud+ 1989)
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An Atlas of Stellar Spectra between 2.00 and 2.45 micrometers
Arnaud K.A., Gilmore G., Collier C.A.
<Mon. Not. Roy. Astron. Soc. 237, 495, (1989)>
=1989MNRAS.237..495A
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ADC_Keywords: Spectra, infrared; Spectrophotometry
Abstract:
The atlas represents a collection of spectra in the wavelength range
2.00 to 2.45 micrometers having a resolution of approximately 0.02
micrometers. The sample of 73 stars includes a supergiant, giants,
dwarfs, and subdwarfs with a chemical abundance range of about -2 to
+0.5 dex.
Introduction:
An Atlas of Stellar Spectra between 2.00 and 2.45 micrometers contains
digital spectra for a sample of 73 stars of various temperature
classes of F and later, most luminosity classifications, and a range
of abundances. A majority of the spectra were obtained with the UKIRT,
while some observations were collected with the Mount Hopkins MMT. The
UKIRT provided a 59-point spectrum from 2.004 to 2.451 micrometers and
the MMT gave a 30-point spectrum from 2.001 to 2.431 micrometers.
This documentation should be used only to supplement the information
contained in the source reference, which should be consulted for
details regarding the impetus for the work, the selection of standard
stars, the observational procedures, and the technique of data
reduction. The source reference also contains a full listing of the
observed stars and a table of flux standards used. Graphical
presentations of all spectra are also given in the body of the paper,
while the digital spectra are listed on a microfiche card accompanying
the journal issue. (Note: The labels on the two microfiche cards in
the issue are reversed.) In any case, the published paper should be
consulted by all users of the machine-readable data.