Predicted lens redshifts and magnitudes for gravitational lenses


If we know something about the mass distribution of the lens then, for a given cosmological model, we can predict the lens redshift and magnitude from the image separation. I did this for a poster at the IAU Symposium 173: The Astrophysics of Gravitational Lensing in July 1995 in Melbourne: for those lens systems with unknown lens redshifts and for some representative cosmological models.

The links below point to one file containing the complete text and a separate file containing the figures, not individually but as included figures in LaTeX---6 pages with several small figures, caption etc. on each page (one page for each lens system).

As are most of my publications this is available in more than one form:

directory of individual short descriptions of papers
Phillip Helbig's publications
Phillip Helbig's research
Phillip Helbig's home page
last modified on Monday, February 22, 2021 at 08:53:39 PM by (remove animal to reply)