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Published 1998 | public
Book Section - Chapter

Lines and Lenses on the Hubble Deep Field

Abstract

In this contribution I describe progress on and preliminary results from a redshift survey on the Hubble Deep Field (HDF) that is being carried out using the Low Resolution Imaging Spectrograph on the Keck Telescope. The primary goal of this research (which involves the combined effort and cooperation of several research groups) is to assemble a uniform redshift sample for about 500 galaxies and use it to probe the spatial distribution, the birth rate and the evolution of field galaxies. There are various secondary goals, one of which - the investigation of strong and weak gravitational lensing - I will also discuss here.

Additional Information

© 1998 Springer Science+Business Media Dordrecht. I thank Tereasa Brainerd, Chris Fassnacht, David Hogg, Tomislav Kundic, Sangeeta Malhotra, Mike Pahre and especially Judith Cohen, who has led the Caltech portion of the redshift survey discussed here, for their collaboration. I thank Don Hamilton for financial assistance to attend this meeting and his patience. Support by STScI/NASA grant AR-06337.12-94A and NSF grant AST 95-29170 is also greatly appreciated.

Additional details

Created:
August 22, 2023
Modified:
January 14, 2024