The Hubble Deep Fields: North vs. South
天体物理学
2007-05-23 v1
摘要
Photometric redshifts have been calculated for the Hubble Deep Fields. The redshift distributions of the fields differ; there is a large excess of galaxies in the HDF-North in the redshift range 0.4<z<1.2. The difference is consistent with the presence of a weak cluster in the HDFN and is only slightly larger than the cosmic variance in other fields of similar depths and with models of large scale structure.
引用
@article{arxiv.astro-ph/9907336,
title = {The Hubble Deep Fields: North vs. South},
author = {Stephen D. J. Gwyn},
journal= {arXiv preprint arXiv:astro-ph/9907336},
year = {2007}
}
备注
6 pages 4 figures quires paspconf.sty. To be published in "Photometric Redshifts and High Redshift Galaxies", eds. R. Weymann, L. Storrie-Lombardi, M. Sawicki & R. Brunner, (San Francisco: ASP Conference Series)