The stellar component of the galaxy as seen by the AFGL Infrared Sky Survey. (original) (raw)

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Abstract

The noise-limited magnitudes for the Air Force Geophysical Laboratory (AFGL) Infrared Sky Survey have been estimated by direct comparison with ground-based observations. Using these limiting magnitudes, 'pruned' versions of the AFGL catalog have been generated. Infrared observations of all the stellar objects seen at 11, 20, or 27 microns and a statistical sample of the stars seen only at 4 microns are reported. Analysis of the observations leads to estimates of the absolute 4 and 10 microns magnitudes and space densities for the two clases of objects. The expected results from the Infrared Astronomical Satellite are reexamined.

Publication:

The Astrophysical Journal Supplement Series

Pub Date:

October 1983

DOI:

10.1086/190897

Bibcode:

1983ApJS...53..413G

Keywords: