Beyond HDF - Searching for Early Star Formation in the Infrared
arXiv:astro-ph/9702062
Abstract
The success of the Hubble Deep Field (HDF) data in identifying galaxies at redshifts up to ~3 has been quite spectacular. It is possible to extend this to even higher redshifts using infrared techniques, several of which are briefly described in this paper.
3 pages, LaTeX, no figures, uses World Scientific Press style file. To appear in the proceedings from the 18th Texas Symposium (1996)