Beyond HDF - Searching for Early Star Formation in the Infrared
| dc.creator | Thompson, D. | |
| dc.date | 1997-02-06 | |
| dc.date.accessioned | 2026-07-07T02:22:53Z | |
| dc.date.available | 2026-07-07T02:22:53Z | |
| dc.description | 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. | |
| dc.description | 3 pages, LaTeX, no figures, uses World Scientific Press style file. To appear in the proceedings from the 18th Texas Symposium (1996) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9702062 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9702062 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/11047 | |
| dc.subject | Astrophysics | |
| dc.title | Beyond HDF - Searching for Early Star Formation in the Infrared | |
| dc.type | text |