Spectrophotometry of stars of intermediate brightness

• DOI: 10.1086/132259
• Publication Date: 2002-07-26T17:56:22Z
• Authors: A. Gutierrez-Moreno; H. Moreno; G. Cortes; E. Wenderoth
• Keywords: 0103 physical sciences; 01 natural sciences

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.