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l-space spectroscopy of the cosmic microwave background with the BOOMERanG experiment

Authors :
K. Coble
Alessandro Melchiorri
P. de Bernardis
Peter A. R. Ade
Calvin B. Netterfield
B. P. Crill
A. Boscaleri
Nicola Vittorio
L. Martinis
T. E. Montroy
J. Borrill
Peter Mason
F. Piacentini
Andrew E. Lange
Philip Daniel Mauskopf
Francesco Scaramuzzi
J. J. Bock
Silvia Masi
E. Hivon
F. Pongetti
Andrew H. Jaffe
A. Iacoangeli
Carlo R. Contaldi
W. C. Jones
P. C. Farese
G. De Troia
M. Giacometti
G. de Gasperis
K. Ganga
V. V. Hristov
Dmitry Pogosyan
Enzo Pascale
J. E. Ruhl
P. Natoli
G. Polenta
J. R. Bond
G. Romeo
Simon Prunet
DePetris, M.
Gervasi, M.
Source :
ResearcherID
Publication Year :
2002

Abstract

The BOOMERanG experiment has recently produced detailed maps of the Cosmic Microwave Background, where sub-horizon structures are resolved with good signal to noise ratio. A power spectrum (spherical harmonics) analysis of the maps detects three peaks, at multipoles ℓ = (213_(-13)^(+10)),(541_(-32)^(+20))(845_(-25)^(+12)). In this paper we discuss the data analysis and the implications of these results for cosmology.

Details

Language :
English
Database :
OpenAIRE
Journal :
ResearcherID
Accession number :
edsair.doi.dedup.....362f01a1a08ad3785db0bef0c4ea3572