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Paper Abstract

EDGE is a Long Duration Balloon (LDB) borne instrument designed to measure the large-scale anisotropy of the Cosmic Infrared Background (CIB). The goal is to use this signal as a new observational tool to measure the character of the spatial distribution of galaxies at the largest spatial scales. With a 6\arcmin\ beam mapping more than 400 square degrees of sky at 8 frequency bands between 250GHz and 1.5 THz the experiment can determine the variation of galaxy density on spatial scales ranging from >200h-1 Mpc, where dark matter variations are determined directly from Cosmic Microwave Background Radiation (CMBR) anisotropy, to <5h-1 Mpc where the distribution of dark matter and galaxies is determined from galaxy redshift surveys and the underlying dynamics of structure growth is non-linear. The instrument consists of a 1-meter class off-axis telescope and a Frequency Selective Bolometer (FSB) array radiometer. The FSB design provides the compact, multi-chromatic, high sensitivity focal plane needed for this measurement.

Paper Details

Date Published: 3 March 2003
PDF: 13 pages
Proc. SPIE 4857, Airborne Telescope Systems II, (3 March 2003); doi: 10.1117/12.458648
Show Author Affiliations
Stephan S. Meyer, Univ. of Chicago (United States)
Edward S. Cheng, NASA Goddard Space Flight Ctr. (United States)
David A. Cottingham, Global Space and Technology Corp. and NASA Goddard Space Flight Ctr. (United States)
Dale J. Fixsen, Science Systems and Applications, Inc. and NASA Goddard Space Flight Ctr. (United States)
Lloyd Knox, Univ. of California/Davis (United States)
Robert F. Silverberg, NASA Goddard Space Flight Ctr. (United States)
Peter T. Timbie, Univ. of Wisconsin/Madison (United States)
Grant Wilson, Univ. of Massachusetts/Amherst (United States)


Published in SPIE Proceedings Vol. 4857:
Airborne Telescope Systems II
Ramsey K. Melugin; Hans-Peter Roeser, Editor(s)

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