Clustering in Deep (submillimetre) Surveys

Details Clustering in Deep (submillimetre) Surveys Clustering in Deep (submillimetre) Surveys

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001dms..conf..131g&link_type=abstract

DEEP MILLIMETER SURVEYS Implications for Galaxy Formation and Evolution. Held 19-21 June 2000 in University of Massachusetts, Am

Astronomy and Astrophysics

Astronomy

Scientific paper

Hughes & Gaztañaga (2001, see article in these proceedings) have presented realistic simulations to address key issues confronting existing and forthcoming submm surveys. An important aspect illustrated by the simulations is the effect induced on the counts by the sampling variance of the large-scale galaxy clustering. We find factors of up to ~ 2 - 4 variation (from the mean) in the extracted counts from deep surveys identical in area (~ 6 arcmin2) to the SCUBA surveys of the Hubble Deep Fields (HDF) 4. Here we present a recipe to model the expected degree of clustering as a function of sample area and redshift.

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