/ftp/cats/III/218



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III/218   ==OBSOLETE version of Catalogue==
11-Feb-2008: (by Francois Ochsenbein) See Version 3.1 = III/251
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=III/218
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drwxr-xr-x 259 cats archive 8192 Dec 5 19:00 [Up] drwxr-xr-x 4 cats archive 4096 Jan 12 2023 [TAR file] -rw-r--r-- 1 cats archive 408 Dec 19 2022 .message -r--r--r-- 1 cats archive 15983 Sep 17 2003 ReadMe -rw-r--r-- 1 cats archive 920 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 2047 Mar 5 2008 +footg8.gif drwxr-xr-x 2 cats archive 24576 Mar 19 2017 lh drwxr-xr-x 2 cats archive 24576 Mar 19 2017 ll -r--r--r-- 1 cats archive 258780 Jun 24 2001 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 1113 Jun 24 2001 table2.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : III/218 ELODIE archive (Prugniel+, 2001) ================================================================================ A database of high and medium-resolution stellar spectra Prugniel P., Soubiran, C. <Astron. Astrophys. 369, 1048 (2001)> =2001A&A...369.1048P ================================================================================ ADC_Keywords: Spectrophotometry ; Atlases ; Spectroscopy ; Populations, stellar Keywords: atlases - stars: abundances - stars: atmospheres - stars: fundamental parameters - galaxies: stellar content Abstract: We present a database of 908 stellar spectra of 709 stars in the wavelength range 410 to 680 nm obtained with the ELODIE spectrograph. The archive provides a large coverage of the space of stellar parameters: Spectral types O to M, luminosity classes V to I and metallicities [Fe/H] from -3.0 to +0.8. At the nominal resolution, R=42000, the mean signal-to-noise ratio is 150 per pixel. The spectra given at this resolution are normalized to their pseudo-continuum and are intended to serve for abundance studies, spectral classification and tests of stellar atmosphere models. A lower resolution version of the archive, R=10000, is calibrated in physical flux with a broad-band photometric precision of 2.5% and narrow-band precision of 0.5%. It is scoped for stellar population synthesis of galaxies and clusters, and for kinematical investigations of stellar systems. The archive is also distributed in FITS format through the HYPERCAT database http://www-obs.univ-lyon1.fr/hypercat/spectrophotometry.html .