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The MAXIMA and MAXIPOL Experiments

Authors :
De Petris, Marco
Gervasi, Massimo
Richards, P. L.
Abroe, M.
Ade, P.
Balbi, A.
Bock, J.
Borrill, J.
Boscaleri, A.
de Bernardis, P.
Collins, J.
Ferreira, P. G.
Hanany, S.
Hristov, V. V.
Jaffe, A. H.
Johnson, B.
Lee, A. T.
Matsumura, T.
Mauskopf, P. D.
Netterfield, C. B.
Pascale, E.
Rabii, B.
Smoot, G. F.
Stompor, R.
Winant, C. D.
Wu, J. H. P.
De Petris, Marco
Gervasi, Massimo
Richards, P. L.
Abroe, M.
Ade, P.
Balbi, A.
Bock, J.
Borrill, J.
Boscaleri, A.
de Bernardis, P.
Collins, J.
Ferreira, P. G.
Hanany, S.
Hristov, V. V.
Jaffe, A. H.
Johnson, B.
Lee, A. T.
Matsumura, T.
Mauskopf, P. D.
Netterfield, C. B.
Pascale, E.
Rabii, B.
Smoot, G. F.
Stompor, R.
Winant, C. D.
Wu, J. H. P.
Publication Year :
2002

Abstract

MAXIMA is a balloon-based bolometric experiment to measure the temperature anisotropy of the CMB over spatial frequency range 36 ≤ l ≤ 1235. The MAXIMA-1 flight produced a 124 square degree temperature anisot0ropy map with a beam diameter of 10 arcmin. These data have been used to produce a power spectrum which is in excellent agreement with data from BOOMERANG and DASI, but covers a wider range of angular scales. The MAXIMA power spectrum is consistent with the prediction of Lambda CDM models and has been used to constrain cosmological models. The MAXIMA experiment is described and an outline is given of the contents and significance of papers written by the MAXIMA team. MAXIMA is being modified to measure the polarization anisotropy of the CMB. A brief description of this MAXIPOL experiment is also given.

Details

Database :
OAIster
Notes :
application/pdf, The MAXIMA and MAXIPOL Experiments, English
Publication Type :
Electronic Resource
Accession number :
edsoai.on1005054123
Document Type :
Electronic Resource

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