MID-IR Surveys - The Next Generations
| dc.creator | Pearson, Chris | |
| dc.date | 2000-07-07 | |
| dc.date.accessioned | 2026-07-07T01:54:18Z | |
| dc.date.available | 2026-07-07T01:54:18Z | |
| dc.description | Using new cosmological models for galaxy evolution, predictions for the next generation of deep mid-IR surveys are presented for both the ASTRO-F space telescope (due for launch 2003) and the proposed HII/L2 mission (2010). Although ASTRO-F will be able to detect between 20,000-40,000 sources in the mid-IR, deep surveys will be severely constrained by confusion due to faint sources (due to the relatively small aperture of all IR space telescopes to date). However, HII/L2 with its larger 3.5m mirror will be able to observe to fluxes 10-100 times deeper below the present confusion limits. | |
| dc.description | Proceedings of ISAS International Workshop on Mid- & Far-Infrared Astromony and future Space Missions, April 17-18, 2000, ISAS, Japan, 8 pages, 3figures, style files included (please use dvips) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0007085 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0007085 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/1291 | |
| dc.subject | Astrophysics | |
| dc.title | MID-IR Surveys - The Next Generations | |
| dc.type | text |