Hostname: page-component-cd9895bd7-jkksz Total loading time: 0 Render date: 2024-12-12T10:43:06.599Z Has data issue: false hasContentIssue false
  • English
  • Français

Identification of Infrared Sources in “Empty” Fields

Published online by Cambridge University Press:  14 August 2015

G. H. Rieke  and
M. J. Lebofsky
G. H. Rieke
Affiliation:
Steward Observatory, University of Arizona, Tucson, AZ 85721
M. J. Lebofsky
Affiliation:
Steward Observatory, University of Arizona, Tucson, AZ 85721

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

From infrared observation of a radio selected sample of QSOs, it is shown that optical identification programs produce samples biased against very red sources, even if identifications are made without regard to color.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 92: Objects of High Redshift , 1980 , pp. 263 - 268
Copyright
Copyright © Reidel 1980 

References

Condon, J. J., Hicks, P. D., and Jauncey, D. L. 1977, A. J., 82, 692.CrossRefGoogle Scholar
Condon, J. J., Jauncey, D. L., and Wright, A. E. 1978, A. J., 83, 1036.CrossRefGoogle Scholar
Neugebauer, G., Oke, J. B., Becklin, E. E., and Matthews, K. 1979, Ap. J., 230, 79.CrossRefGoogle Scholar
Rieke, G. H., Lebofsky, M. J. 1979, Ann. Rev. Astron. Ap., in press.Google Scholar
Rieke, G. H., Lebofsky, M. J., and Kinman, T. D. 1979, Ap. J. (Letters), in press.Google Scholar