Large-Scale Structure in the Hubble Deep Field -- South: Near-Infrared Imaging

Details Large-Scale Structure in the Hubble Deep Field -- South: Near-Infrared Imaging Large-Scale Structure in the Hubble Deep Field -- South: Near-Infrared Imaging

Aug 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999noao.prop..171g&link_type=abstract

NOAO Proposal ID #1999B-0171

Physics

Scientific paper

We propose to image 1/2 square degree around and including the Hubble Deep Field - South in the near-infrared K band. These data will be used with our existing uBVRI Big Throughput Camera image to improve photometric redshifts of galaxies at z< 1, and to extend them to z> 1. We will measure the galaxy-galaxy correlation function as a function of photometric redshift, and for the first time as a function of K magnitude at 16< K< 19. In the spirit of the HDF project, we will add reduced images and catalogs from these observations to the BTC data we have made publically available through our web site: http://hires.gsfc.nasa.gov/~gardner/hdfs.

Affiliated with

Also associated with

No associations

Rating

Large-Scale Structure in the Hubble Deep Field -- South: Near-Infrared Imaging 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-Scale Structure in the Hubble Deep Field -- South: Near-Infrared Imaging, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Large-Scale Structure in the Hubble Deep Field -- South: Near-Infrared Imaging will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1015898