@article{3c682d038260471aa1261b0ec5ae7de1,
title = "Searching for non-Gaussian signals in the BOOMERanG 2003 CMB map: Preliminary results",
abstract = "We analyse the 145 GHz temperature map produced from the 2003 flight of BOOMERanG in search for deviations from Gaussianity. We perform a pixel space analysis computing the map's skewness, kurtosis and Minkowski functionals, as well as a Fourier space analysis computing the diagonal part the of angular bispectrum. The preliminary results presented here suggest that the data are fully consistent with the Gaussian hypothesis.",
author = "{De Troia}, G. and Ade, {P. A.R.} and Bock, {J. J.} and Bond, {J. R.} and J. Borrill and A. Boscaleri and P. Cabella and Contaldi, {C. R.} and Crill, {B. P.} and {de Bernardis}, P. and {de Gasperis}, G. and {de Oliveira-Costa}, A. and {Di Stefano}, G. and Ferreira, {P. G.} and E. Hivon and A. Jaffe and T. Kisner and M. Kunz and Jones, {W. C.} and Lange, {A. E.} and S. Masi and Mauskopf, {P. D.} and C. MacTavish and A. Melchiorri and T. Montroy and P. Natoli and Netterfield, {C. B.} and E. Pascale and F. Piacentini and D. Pogosyan and G. Polenta and S. Prunet and S. Ricciardi and G. Romeo and Ruhl, {J. E.} and P. Santini and M. Tegmark and M. Veneziani and N. Vittorio",
note = "Funding Information: The BOOMERanG collaboration acknowledges support from CIAR, CSA and NERSC in Canada, ASI, University La Sapienza and PNRA in Italy, PPARC and the Leverhulme Trust in the UK, and NASA (awards NAG5-9251 and NAG5-12723) and NSF (awards OPP-9980654 and OPP-0407592) in the USA. Additional support for detector development was provided by CIT and JPL. CBN acknowledges support from a Sloan Foundation Fellowship; WCJ and TEM were partially supported by NASA GSRP Fellowships. Field, logistical, and flight support was outstandingly supplied by USAP and NSBF; data recovery was especially appreciated. This research used resources at NERSC, supported by the DOE under Contract No. DE-AC03-76SF00098, and the MacKenzie cluster at CITA, funded by the Canada Foundation for Innovation. We thank the CASPUR (Rome-ITALY) and NERSC/LBL (US) computational facilities. Some of the results in this paper have been derived using the HEALPix ( G{\'o}rski et al., 2005 ) package and nearly all have benefited from the FFTW3 implementation of Fast Fourier Transform ( Frigo and Johnson, 2005 ). ",
year = "2007",
month = mar,
doi = "10.1016/j.newar.2006.11.064",
language = "English (US)",
volume = "51",
pages = "250--255",
journal = "New Astronomy Reviews",
issn = "1387-6473",
publisher = "Elsevier B.V.",
number = "3-4",
}