/ftp/cats/3/166



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III/166  A New Library of Optical Spectra (Silva + 1992)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	stars.dat spectra.dat
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Query from: http://vizier.cds.unistra.fr/cgi-bin/VizieR?-source=III/166
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drwxr-xr-x 259 cats archive 8192 Dec 5 19:00 [Up] drwxr-xr-x 3 cats archive 4096 Jan 12 2023 [TAR file] -rw-r--r-- 1 cats archive 452 Dec 19 2022 .message -r--r--r-- 1 cats archive 8723 Apr 10 2002 ReadMe -rw-r--r-- 1 cats archive 444 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 3848 Mar 5 2008 +footg8.gif drwxr-xr-x 2 cats archive 4096 Sep 25 2003 sp -r--r--r-- 1 cats archive 1268 Sep 16 1999 spectra.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 4540 Sep 18 1999 stars.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : III/166 A New Library of Optical Spectra (Silva + 1992) ================================================================================ A New Library of Stellar Optical Spectra Silva D.R., Cornell M.E. <Astrophys. J. Suppl. 81, 865 (1992)> =1992ApJS...81..865S ================================================================================ ADC_Keywords: Spectrophotometry ; Spectral types Abstract: Silva and Cornell have compiled a new digital optical stellar spectra library, consisting of intensities at 5A intervals between 3510A and 8930A for 72 different spectral types. These types range from O to M and luminosities range from I to V. Some weak-line and strong-line spectra are also included. The intensities are in ergs/A, normalized to 100 at 5450A. Description: Newly acquired and previously published data have been combined to form a new digital optical library intended primarily for use in empirical population synthesis. Stellar data for a large number of individual stars were acquired during seven observing runs between December 1988 and May 1989. An effort was made to observe, primarily, stars with TZG parameters derived from stellar atmosphere models of high dispersion data. Observations of photometric calibration stars were made during each run, but absolute calibrations were not attempted. Composite spectra from different observations of each star were formed by multiplicatively scaling the individual sub-spectra and averaging. The resultant composite spectra were normalized to 100 at 5450A. Next, the effects of interstellar reddening were removed. Intensities in the spectral regions most affected by telluric absorption were set to zero. Finally, stars with similar TZG parameters and similar overall spectral characteristics were averaged to form the individual spectra in the library, also normalized to 100 at 5450A. Table 1 lists the individual types averaged to form each of the 72 entries in the catalog. The prefixes R and W refer to strong- and weak-line stars, respectively. The list of the observed stars (Table 2 of the paper), and the synthesized UBV colors (Tables 3 and 4 of the paper) were added to the electronic catalog in 1999.