Searching for Non-Gaussian Signals in the BOOMERANG 2003 CMB Maps
Author(s) -
G. De Troia,
P. A. R. Ade,
J. J. Bock,
J. R. Bond,
J. Borrill,
A. Boscaleri,
P. Cabella,
Carlo Contaldi,
B. P. Crill,
P. de Bernardis,
G. de Gasperis,
A. de OliveiraCosta,
Giuseppe Di Stefano,
Pedro G. Ferreira,
E. Hivon,
A. H. Jaffe,
T. S. Kisner,
M. Kunz,
W. C. Jones,
A. E. Lange,
M. Liguori,
S. Masi,
S. Matarrese,
P. Mauskopf,
C. J. MacTavish,
A. Melchiorri,
T. E. Montroy,
P. Natoli,
C. B. Netterfield,
E. Pascale,
F. Piacentini,
D. Pogosyan,
G. Polenta,
S. Prunet,
S. Ricciardi,
G. Romeo,
J. E. Ruhl,
P. Santini,
Max Tegmark,
M. Veneziani,
N. Vittorio
Publication year - 2007
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/524402
Subject(s) - physics , cosmic microwave background , gaussian , estimator , minkowski space , non gaussianity , amplitude , parameter space , cosmic background radiation , astrophysics , statistical physics , statistics , optics , mathematical physics , quantum mechanics , anisotropy , mathematics
We analyze the BOOMERANG 2003 (B03) 145 GHz temperature map to constrain the amplitude of a non-Gaussian, primordial contribution to CMB fluctuations. We perform a pixel-space analysis restricted to a portion of the map chosen in view of high-sensitivity, very low foreground contamination and tight control of systematic effects. We set up an estimator based on the three Minkowski functionals which relies on high-quality simulated data, including non-Gaussian CMB maps. We find good agreement with the Gaussian hypothesis and derive the first limits based on BOOMERANG data for the nonlinear coupling parameter fNL as -300
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