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III/232 STELIB: A library of stellar spectra at R 2000 (Le Borgne+, 2003)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
table.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=III/232
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drwxr-xr-x 259 cats archive 8192 Dec 5 19:00 [Up]
drwxr-xr-x 4 cats archive 4096 Jul 25 2023 [TAR file]
-rw-r--r-- 1 cats archive 464 Jul 25 2023 .message
-r--r--r-- 1 cats archive 5989 May 17 2003 ReadMe
-rw-r--r-- 1 cats archive 516 Jul 25 2023 +footg5.gif
-rw-r--r-- 1 cats archive 4833 Jul 25 2023 +footg8.gif
drwxr-xr-x 2 cats archive 12288 Sep 25 2003 cor_sp
drwxr-xr-x 2 cats archive 12288 Oct 3 2017 obs_sp
-r--r--r-- 1 cats archive 4349438 Apr 22 2003 stelib.ps.gz [Uncompressed]
-r--r--r-- 1 cats archive 47771 Apr 28 2003 table.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe :III/232 STELIB: A library of stellar spectra at R 2000 (Le Borgne+, 2003)
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STELIB: A library of stellar spectra at R 2000.
Le Borgne J.-F., Bruzual G., Pello R., Lancon A., Rocca-Volmerange B.,
Sanahuja B., Schaerer D., Soubiran C., Vilchez-Gomez R.
<Astron. Astrophys. 402, 433 (2003)>
=2003A&A...402..433L
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ADC_Keywords: Atlases ; Spectroscopy
Keywords: atlases - stars: fundamental parameters - galaxies: stellar content
Description:
STELIB is a new spectroscopic stellar library, available at
http://webast.ast.obs-mip.fr/stelib . It consists in an homogeneous
library of stellar spectra in the visible range (3200 to 9500)AA),
with an intermediate spectral resolution (< 3AA) and sampling
(1AA), and corrected from interstellar absorption. This library
includes 255 stars of various spectral types and luminosity classes,
spanning a relatively wide range in metallicity. The spectral
resolution, wavelength and spectral type coverage of this library
represents a substantial improvement over previous libraries used in
population synthesis models. The overall absolute photometric
uncertainty is 3%.
The data were obtained during two runs, one at the 1m Jacobus Kaptein
Telescope (JKT), Roque de los Muchachos Observatory, La Palma, Canary
Islands, Spain, between 1994 March 28 and April 4, and a second one at
the 2.3m of the Australian National University at Siding Spring (SSO),
Australia, between 1994 December 25 and 31.