Detection of anisotropy in the Cosmic Microwave Background at horizon and sub-horizon scales with the BOOMERanG experiment

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dc.creatorde Bernardis, P.
dc.creatorAde, P. A. R.
dc.creatorBock, J. J.
dc.creatorBond, J. R.
dc.creatorBorrill, J.
dc.creatorBoscaleri, A.
dc.creatorCoble, K.
dc.creatorCrill, B. P.
dc.creatorDe Gasperis, G.
dc.creatorDe Troia, G.
dc.creatorFarese, P. C.
dc.creatorFerreira, P. G.
dc.creatorGanga, K.
dc.creatorGiacometti, M.
dc.creatorHivon, E.
dc.creatorHristov, V. V.
dc.creatorIacoangeli, A.
dc.creatorJaffe, A. H.
dc.creatorLange, A. E.
dc.creatorMartinis, L.
dc.creatorMasi, S.
dc.creatorMason, P.
dc.creatorMauskopf, P. D.
dc.creatorMelchiorri, A.
dc.creatorMiglio, L.
dc.creatorMontroy, T.
dc.creatorNetterfield, C. B.
dc.creatorPascale, E.
dc.creatorPiacentini, F.
dc.creatorPogosyan, D.
dc.creatorPongetti, F.
dc.creatorPrunet, S.
dc.creatorRao, S.
dc.creatorRomeo, G.
dc.creatorRuhl, J. E.
dc.creatorScaramuzzi, F.
dc.creatorSforna, D.
dc.creatorVittorio, N.
dc.date2000-11-25
dc.date.accessioned2026-07-07T01:56:42Z
dc.date.available2026-07-07T01:56:42Z
dc.descriptionBOOMERanG has recently resolved structures on the last scattering surface at redshift $\sim$ 1100 with high signal to noise ratio. We review the technical advances which made this possible, and we focus on the current results for maps and power spectra, with special attention to the determination of the total mass-energy density in the Universe and of other cosmological parameters.
dc.identifierhttps://arxiv.org/abs/astro-ph/0011468
dc.identifierhttp://arxiv.org/abs/astro-ph/0011468
dc.identifierProc. of the IAU symposium 201: New Cosmological Data and the Values of the Fundamental Parameters, Manchester, 7-11 Aug. 2000
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2095
dc.subjectAstrophysics
dc.titleDetection of anisotropy in the Cosmic Microwave Background at horizon and sub-horizon scales with the BOOMERanG experiment
dc.typetext

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