Spectrophotometry of stars of intermediate brightness

Details Spectrophotometry of stars of intermediate brightness Spectrophotometry of stars of intermediate brightness

Aug 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pasp..100..973g&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 100, Aug. 1988, p. 973-985. Research supported by Unive

Astronomy and Astrophysics

Astronomy

24

Brightness, Stellar Magnitude, Stellar Spectrophotometry, Atmospheric Attenuation, Photomultiplier Tubes, Stellar Spectra

Scientific paper

Spectrophotometric observations of 15 stars in a magnitude range m of between 8.0 and 10.9, located mostly near the equator and covering all the range of right ascensions, are presented. The energy distributions have been obtained in Hayes' (1970) system as revised by Hayes and Latham (1975), and in the augmented system presented by Taylor (1984). Comments about some of the standard stars are presented as well as a comparison of the results obtained with both systems.

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