Simulating surveys of the high-z mm Universe

Details Simulating surveys of the high-z mm Universe Simulating surveys of the high-z mm Universe

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..17..268c&link_type=abstract

Galaxy Evolution: Theory & Observations (Eds. Vladimir Avila-Reese, Claudio Firmani, Carlos S. Frenk & Christine Allen) Revista

Astronomy and Astrophysics

Astronomy

Cosmology: Large Scale Structure, Galaxies: Clusters, Igm: Quasar Absorption Lines, Quasars: Space Distribution

Scientific paper

The next generation of large single-dish mm and sub-mm (hereafter mm)
telescopes (ground-based, balloon-borne, satellites) and
interferometers, using new large-format fully-sampled focal-plane
arrays, will provide greatly improved mapping speed, sensitivity,
wavelength coverage, and resolution.

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