A Deep UBVRI Imaging Survey with the WFC
PI: Dr Gavin Dalton
Summary of Programme
We propose to survey four contiguous regions of
10 deg² each in broad band BVRI filters to a limiting depth
of B=26, I=24.5 (5 sigma). The primary scientific goals of the
survey are the evolution of galaxy clustering as a function of colour
at faint magnitudes, a well-defined catalogue of rich galaxy clusters
at intermediate redshifts, and the detection of a significant number
of quasars with z>5. We propose to make use of the small fraction of
the required survey time which is likely to have very good seeing
conditions to observe two sub-areas of 5 deg² each to U=26
(3 sigma) to investigate the large-scale clustering of the
Lyman-break galaxies at z>3 and investigate the hypothesis
that these objects trace the formation sites of present day rich
clusters of galaxies. The survey will provide an invaluable resource
for the new generation of 8-m class telescopes.
This page last updated: 16 Jun 1998 by Nic Walton
( naw@ing.iac.es )
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