Evidence for non-Gaussianity in the CMB

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dc.creatorMagueijo, J.
dc.creatorFerreira, P.
dc.creatorGorski, K.
dc.date1998-10-26
dc.date.accessioned2026-07-07T02:28:44Z
dc.date.available2026-07-07T02:28:44Z
dc.descriptionIn a recent Letter we have shown how COBE-DMR maps may be used to disprove Gaussianity at a high confidence level. In this report we digress on a few issues closely related to this Letter. We present the general formalism for surveying non-Gaussianity employed. We present a few more tests for systematics. We wonder about the theoretical implications of our result.
dc.descriptionProceedings of the Planck meeting, Santender 98
dc.identifierhttps://arxiv.org/abs/astro-ph/9810414
dc.identifierhttp://arxiv.org/abs/astro-ph/9810414
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13185
dc.subjectAstrophysics
dc.titleEvidence for non-Gaussianity in the CMB
dc.typetext

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