Large Area/multicolor Survey - Cycle 4

Details Large Area/multicolor Survey - Cycle 4 Large Area/multicolor Survey - Cycle 4

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994hst..prop.5090g&link_type=abstract

HST Proposal ID #5090

Physics

Hst Proposal Id #5090 Galaxies &Amp, Clusters

Scientific paper

Deep high latitude observations will be made with the WFPC2 in order to study cosmology using as probes: the clustering of galaxies, galaxy counts as a function of magnitude, evolution of the galaxy luminosity function, evolution of galaxy colors, galaxy morphology, and the distribution of galaxies in redshift. The observations consist of a strip of 28 overlapping WFC exposures with the wide I and V filters. It is assumed that the observations will occur when the target is opposite the Sun and the strip is oriented so that at the nominal roll for this date, the WFPC2 fields overlap in a chevron pattern. These exposures will also be useful for star count studies bearing on galactic structure. This program is the combined GTO time of Groth and Schroeder and is coordinated with a WFPC1 GTO program.

Affiliated with

Also associated with

No associations

Rating

Large Area/multicolor Survey - Cycle 4 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Large Area/multicolor Survey - Cycle 4, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Large Area/multicolor Survey - Cycle 4 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1255287