Spectrophotometry of 26 supergiants in the LMC Virtual Observatory Resource

Authors

1. Oestreicher M.O.
2. Schmidt-Kaler T.

Published by

CDS

Abstract

New spectrophotometric data for 3 galactic and 23 LMC F to G supergiants are presented. The wavelength range of the spectra is 3400 to 6400{AA}, the resolution about 10{AA}. The mean transformational error of the fluxes is 0.03mag. The S/N ratio is about 100 and 30 for galactic and LMC stars, respectively. Details about the reduction one may found in Oestreicher & Schmidt-Kaler (1998MNRAS.299..625O) and Malyuto et al. (1997MNRAS.286..500M). The fluxes are given in magnitudes according to the system of Hayes & Latham (1975ApJ...197..593H). For each star an ASCII file is given with the name of the first identifier. In the first column the wavelength, in the second column the flux is given.

Keywords

1. spectrophotometry
2. supergiant-stars
3. magellanic-clouds

Bibliographic source Bibcode

1999AN....320..105O

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