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III/196 Near-IR stellar spectra from 1.428 to 2.5 um (Lancon+ 1996)
The following files can be converted to FITS (extension .fit .fiz or .fiZ)
stars.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=III/196
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drwxr-xr-x 259 cats archive 8192 Dec 5 19:00 [Up]
drwxr-xr-x 3 cats archive 4096 May 26 2023 [TAR file]
-rw-r--r-- 1 cats archive 464 Dec 19 2022 .message
-r--r--r-- 1 cats archive 5973 Oct 26 2012 ReadMe
-rw-r--r-- 1 cats archive 419 Oct 2 2018 +footg5.gif
-rw-r--r-- 1 cats archive 4234 Oct 2 2018 +footg8.gif
drwxr-xr-x 2 cats archive 4096 Oct 2 2018 fits
-r--r--r-- 1 cats archive 11520 May 24 1996 rawspec.fit
-r--r--r-- 1 cats archive 13742 Apr 14 1997 stars.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-rw-r--r-- 1 cats archive 22596 Feb 27 2005 stars.ps.gz [Uncompressed]
-r--r--r-- 1 cats archive 11733 Apr 14 1997 stars.tex Beginning of ReadMe :III/196 Near-IR stellar spectra from 1.428 to 2.5 um (Lancon+ 1996)
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A library of near-IR stellar spectra from 1.428 to 2.5 mum.
Lancon A., Rocca-Volmerange B.
<Astron. Astrophys. Suppl. Ser. 96, 593 (1992)>
=1992A&AS...96..593L
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ADC_Keywords: Spectra, infrared
Keywords: stars: atlas - stars: infrared spectroscopy -
stars: temperature and colours
Description:
This library is an EXTENDED VERSION of the library published by
A.Lancon and B.Rocca-Volmerange in 1992.
The catalog contains near-IR spectra of 84 stars, obtained with the
Fourier Transform Spectrograph at the Canada-France-Hawaii Telescope
on Mauna Kea, Hawaii. The spectra cover the H and K atmospheric
windows, i.e. wavelengths from 1.43 to 2.5 microns, with a typical
resolving power of 500.
The spectra have all been reduced again in 1996. The general procedure
was as described in the original article, except that the intrinsic
energy distributions of the stars used as references were assumed to
be well represented by the models of Kurucz, 1993. Making extensive
use of the Simbad data base, we have searched the literature on each
of these stars, looking for effective temperature and extinction
determinations. The new reduction improves the reliability of the
continua, and reduces possible systematic differences between
observing runs.
The files contain the reduced spectra in FITS format, with fluxes in
arbitrary units of energy per unit frequency (normalised to
approximately 1 in the K band) and frequencies in cm^-1^, the
natural units of Fourier Transform spectroscopy.