ABSOLUTE FLUX CALIBRATION OF OPTICAL SPECTROPHOTOMETRIC STANDARD STARS

被引：49
|
作者：
COLINA, L
BOHLIN, RC
机构：
[1] Space Telescope Science Institute, Baltimore, MD 21218
来源：
ASTRONOMICAL JOURNAL | 1994年 / 108卷 / 05期
关键词：
D O I：
10.1086/117206
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
A method based on Landolt photometry in B and V is developed to correct for a wavelength independent offset of the absolute flux level of optical spectrophotometric standards. The method is based on synthetic photometry techniques in B and V and is accurate to similar to 1%. The correction method is verified by Hubble Space Telescope Faint Object Spectrograph absolute fluxes for five calibration stars, which agree with Landolt photometry to 0.5% in B and V.
引用
收藏
页码：1931 / 1935
页数：5
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