The trispectrum of the cosmic microwave background on subdegree angular scales: An analysis of the BOOMERanG data

Monthly Notices of the Royal Astronomical Society

Volumn 343, Issue 1, 2003, Pages 284-292

  De Troia, G ^a,g   Ade, P A R ^b   Bock, J J ^c   Bond, J R ^d   Boscaleri, A ^e   Contaldi, C R ^d   Crill, B P ^f   De Bernardis, P ^a   Ferreira, P G ^g   Giacometti, M ^a   Hivon, E ^h   Hristov, V V ^f   Kunz, M ^g,i   Lange, A E ^f   Masi, S ^a   Mauskopf, P D ^b   Montroy, T ^j   Natoli, P ^k   Netterfield, C B ^l   Pascale, E ^e   Piacentini, F ^a   Polenta, G ^a   Romeo, G ^m   Ruhl, J E ^j   more..

^a UNIVERSITÀ DI ROMA LA SAPIENZA   (Italy)

^b CARDIFF UNIVERSITY   (United Kingdom)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^d UNIVERSITY OF TORONTO   (Canada)

^e CNR   (Italy)

^f CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^g UNIVERSITY OF OXFORD   (United Kingdom)

^h CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

ⁱ UNIVERSITY OF SUSSEX   (United Kingdom)

^j CASE WESTERN RESERVE UNIVERSITY   (United States)

^k UNIVERSITY OF ROME TOR VERGATA   (Italy)

^l UNIVERSITY OF TORONTO   (Canada)

^m ISTITUTO NAZIONALE DI GEOFISICA E VULCANOLOGIA   (Italy)

more..

Author keywords

Cosmic microwave background; Methods: statistical

Indexed keywords

ANGULAR DISTRIBUTION; MICROWAVES;

ANGULAR SCALE; COSMIC MICROWAVES BACKGROUND; COSMOLOGICAL SCALE; DATA SET; FOURTH ORDER MOMENTS; METHODS:STATISTICAL; NONGAUSSIANITY; PRIMORDIAL NON-GAUSSIANITY; PROBABILITY DISTRIBUTION FUNCTIONS; TRISPECTRUM;

COSMOLOGY;

EID: 0142118265     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06665.x     Document Type: Article

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