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Predicted Lens Redshifts And Magnitudes

Published online by Cambridge University Press:  25 May 2016

P. Helbig*
Affiliation:
Hamburger Sternwarte, Gojenbergsweg 112, D-21029 Hamburg, Germany

Abstract

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For gravitational lens systems with unknown lens redshifts, the redshifts and brightnesses of the lenses are predicted for a variety of cosmological models. Besides providing hints as to which systems should be observed with a realistic chance of measuring the lens redshifts, which are needed for detailed lensing statistics and for modelling the lenses, these calculations give a visual impression of the influence of the cosmological model in gravitational lensing.

Type
Chapter 1: Classical Cosmology
Copyright
Copyright © Kluwer 1996 

References

Turner, E. L., Ostriker, J. P. & Gott, J. R., 1984, ApJ, 284, 1 Google Scholar
Schechter, P., 1976, ApJ, 203, 297 CrossRefGoogle Scholar
Tully, R. & Fisher, J., 1977, A&A, 54, 661 Google Scholar
Faber, S. M. & Jackson, R. E., 1976, ApJ, 204, 668 Google Scholar
Feige, B., 1992, Astr. Nachr., 313, 139 Google Scholar
Kochanek, C. S., 1992, ApJ, 384, 1 Google Scholar