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Blue and Red Brightnesses of the Integrated Starlight Obtained by Star-Counts in 24 Regions

Published online by Cambridge University Press:  08 February 2017

H. Tanabe
Affiliation:
National Astronomical Observatory Mitaka Tokyo 181, Japan
K. Mori
Affiliation:
National Astronomical Observatory Mitaka Tokyo 181, Japan

Abstract

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Star-counts on the Palomar Sky Survey Atlas were made in 1968-87 in order to estimate the background brightness in zodiacal light and airglow observations. Measured diameters of blue and red images of each star were converted to the magnitude with empirical diameter-magnitude relations. The resultant blue and red brightnesses and colors of the integrated starlight are presented for 24 sky regions, including 4 polar (North Celestial, North Ecliptic, North and South Galactic) and 10 ecliptic regions.

Type
II. Galactic Background Starlight from UV to IR: Observations and Models
Copyright
Copyright © Kluwer 1990 

References

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