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VI/50 Intensity Distribution of Normal Stars (Sviderskiene, 1988)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
data.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=VI/50
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Beginning of ReadMe :VI/50 Intensity Distribution of Normal Stars (Sviderskiene, 1988)
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Mean Intensity Distributions in the Stellar Spectra of different Spectral Types
and Luminosities. V. Normal Stars
Sviderskiene Z.
<Bull.Vilnius Obs. 80 (1988)>
=1988VilOB..80....7S
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ADC_Keywords: Spectrophotometry
Description:
Mean energy distributions are given for 98 normal stars in the
spectral range from O to M and luminosity classes V, IV, III, II, and
I. The points cover the wavelength range from 1200A to 10500A and a
include a point at 12500A.
Introduction:
The energy distributions were based on photometric and
spectrophotometric data from many authors. All stars are dereddened.
The zero point for each wavelength is based on a Vega model atmosphere
by Mihalas (1966ApJS...13....1M) with theta effective = 0.525 (9600K)
and log.g = 4. It has been extended into the ultraviolet using the
OAO-2 results. This energy distribution is given in the last column
of file "data.dat", and can be used to change to another system if
desired. The ultraviolet portions are based on the IUE calibrations.
The energy distributions are given in intensities per unit wavelength
interval normalized to 100AA (100nm) at 5500AA (550nm). Each value
given in the catalog is the intensity in the interval
Deltalambda = 50AA (5nm) centered on the given wavelength.