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Redshift Estimates for Distant Radio Galaxies Based on Broadband Photometry

Published online by Cambridge University Press:  14 August 2015

J. J. Puschell ,
F. N. Owen  and
R. Laing
J. J. Puschell
Affiliation:
University of California, San Diego
F. N. Owen
Affiliation:
National Radio Astronomy Observatory
R. Laing
Affiliation:
National Radio Astronomy Observatory

Extract

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Calculations modeling the effects of stellar evolution on elliptical galaxies (e.g., Bruzual and Kron 1980, Bruzual 1981) suggest that the shape of the spectral flux distribution should remain almost constant in the red and near-infrared out to at least z ∼ 2. Thus, it should be possible to derive the redshift of a distant elliptical galaxy by fitting a model galaxy spectrum to broadband near-infrared (RIJHK) photometry.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 97: Extragalactic Radio Sources , 1982 , pp. 423 - 424
Copyright
Copyright © Reidel 1982 

References

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