MID-IR Surveys - The Next Generations
Abstract
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.
Cite
@article{arxiv.astro-ph/0007085,
title = {MID-IR Surveys - The Next Generations},
author = {Chris Pearson},
journal= {arXiv preprint arXiv:astro-ph/0007085},
year = {2007}
}
Comments
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)