Probing The High Redshift Universe with the NGST
| dc.creator | Madau, Piero | |
| dc.date | 1998-08-14 | |
| dc.date.accessioned | 2026-07-07T02:27:37Z | |
| dc.date.available | 2026-07-07T02:27:37Z | |
| dc.description | Through a combination of deep wide-field imaging and multi-object spectroscopy, the Next Generation Space Telescope will be able to chart with unprecedented accuracy the evolution of cosmic structures after the `dark ages' (z<5), when galaxies are thought to assemble and form the bulk of their stars. In this talk I will discuss how NGST observations might determine the history of the stellar birthrate in the universe and reveal the character of cosmological ionizing sources at high redshifts. | |
| dc.description | LaTeX, 9 pages, esapub.sty, 6 figures. Invited Review at the 34th Liege International Astrophysics Colloquium ``The Next Generation Space Telescope: Science Drivers and Technological Challenges'', June 1998, ESA Publications | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9808150 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9808150 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/12772 | |
| dc.subject | Astrophysics | |
| dc.title | Probing The High Redshift Universe with the NGST | |
| dc.type | text |