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The TopHat Experiment: A Balloon‐borne Instrument for Mapping Millimeter and Submillimeter Emission
Author(s) -
R. F. Silverberg,
E. S. Cheng,
James E. Aguirre,
J. J. Bezaire,
T. M. Crawford,
S. S. Meyer,
A. Bier,
Barbara Campano,
T. C. Chen,
D. A. Cottingham,
Elmer Sharp,
P. R. Christensen,
S. Cordone,
Peter T. Timbie,
Richard E. Dame,
D. J. Fixsen,
R. J. K. Kristensen,
H. U. Nørgaard-Nielsen,
G. W. Wilson
Publication year - 2005
Publication title -
the astrophysical journal supplement series
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 3.546
H-Index - 277
eISSN - 1538-4365
pISSN - 0067-0049
DOI - 10.1086/432117
Subject(s) - cassegrain reflector , cosmic microwave background , physics , sky , telescope , millimeter , bolometer , dichroic glass , radiometer , remote sensing , astronomy , optics , astrophysics , detector , anisotropy , geology
The TopHat experiment was designed to measure the anisotropy in the cosmic microwave background radiation onangularscalesfrom0N3to30 andthethermalemissionfrombothGalacticandextragalacticdust.Theballoon-borne instrument had five spectral bands spanning frequencies from 175 to 630 GHz. The telescope was a compact, 1 m, on- axisCassegraintelescopedesignedtoscantheskyatafixedelevationof 78 .Theradiometerusedcryogenicbolometers coupled to a single feed horn via a dichroic filter system. The observing strategy was intended to efficiently cover a region 48 in diameter centered on the south polar cap with a highly cross-linked and redundant pattern with nearly uniform sky coverage. The Long Duration Balloon flight over Antarctica in 2001 January surveyed about 6% of the sky.Herewedescribethedesignoftheinstrumentandtheachievedin-flightperformanceandprovideabriefdiscussion of the data analysis. Subject headinggs: balloons — cosmic microwave background — cosmology: observations — galaxies: general

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