Photometric Redshifts in Hubble Deep Field South
Astrophysics
2007-05-23 v1
Abstract
We apply both a traditional `dropout' approach and a photometric redshift estimation technique to the Hubble Deep Field South data. We give a list of dropout selected z3 objects, and show their images. We then discuss our photometric redshift estimation technique, demonstrate both its effectiveness and the role played by near-IR data, and then apply it to HDF-S to obtain an estimated redshift distribution.
Keywords
Cite
@article{arxiv.astro-ph/9909045,
title = {Photometric Redshifts in Hubble Deep Field South},
author = {D. L. Clements},
journal= {arXiv preprint arXiv:astro-ph/9909045},
year = {2007}
}
Comments
To appear in "Photometric Redshifts and High Redshift Galaxies", eds. R. Weymann, L. Storrie-Lombardi, M. Sawicki & R. Brunner