224 K
7 pp.
 
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TitleMAXIMA-1: A Measurement of the Cosmic Microwave Background Anisotropy on Angular Scales of 10' to 5 degrees
Author(s)Ade, P.; Balbi, A.; Bock, J.; Borrill, J.; Boscaleri, A.; de Bernardis, P.; Ferreira, P. G.; Hanany, S.; Hristov, V. V.; Jaffe, A. H.; Lange, A. E.; Lee, A. T.; Mauskopf, P. D.; Netterfield, C. B.; Oh, S.; Pascale, E.; Rabii, B.; Richards, P. L.; Smoot, G. F.; Stompor, R.; Winant,C. D.; Wu, J. H. P.
Publication DateJune 04, 2005
Report NumberLBNL--60038
Unique IdentifierACC0186
Other NumbersKX0410; KJ0102000; OSTI ID: 886077
Research OrgErnest Orlando Lawrence Berkeley National Laboratory [LBNL], Berkeley, CA (US)
Contract NoAC03-76SF00098
Sponsoring OrgU. S. Department of Energy (USDOE) Office of Science. Office of Advanced Scientific Computing Research; National Aeronautics and Space Administration Grants NAG5-3941 and NAG5-6552 and NAG5-4454 and GSRP-031 and GSRP-032, National Science Foundation AST-9120005; KDI Precision Products Inc Grant 9872979, Particle Physics and Astronomy Research Council UK
Other InformationAstrophysics Journal, Vol. 545, Issue 1, 12/10/2000
Subject71 Classical and Quantum Mechanics, General Physics; 99 General and Miscellaneous//Mathematics, Computing, and Information Science; Amplitudes; Anisotropy; Dipoles; Photometers; Relict Radiation; Resolution; Sky
KeywordsCosmic Microwave Background; Cosmology
Related Web PagesGeorge Smoot, Blackbody, and Anisotropyof the Cosmic Microwave Background Radiation
AbstractWe present a map and an angular power spectrum of the anisotropy of the cosmic microwave background (CMB) from the first flight of MAXIMA. MAXIMA is a balloon-borne experiment with an array of 16 bolometric photometers operated at 100 mK. MAXIMA observed a 124 deg{sup 2} region of the sky with 10' resolution at frequencies of 150, 240 and 410 GHz. The data were calibrated using in-flight measurements of the CMB dipole anisotropy. A map of the CMB anisotropy was produced from three 150 and one 240 GHz photometer without need for foreground subtractions.
224 K
7 pp.
 
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