Numerical Likelihood Analysis of Cosmic Ray Anisotropies

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dc.creatorHojvat, Carlos
dc.creatorMcCauley, Thomas P.
dc.creatorReucroft, Stephen
dc.creatorSwain, John D.
dc.date2003-05-12
dc.date.accessioned2026-07-07T02:08:28Z
dc.date.available2026-07-07T02:08:28Z
dc.descriptionA numerical likelihood approach to the determination of cosmic ray anisotropies is presented which offers many advantages over other approaches. It allows a wide range of statistically meaningful hypotheses to be compared even when full sky coverage is unavailable, can be readily extended in order to include measurement errors, and makes maximum unbiased use of all available information.
dc.descriptionTo be published in the Proceedings of the 28th International Cosmic Ray Conference http://www.icrr.u-tokyo.ac.jp/icrc2003/
dc.identifierhttps://arxiv.org/abs/astro-ph/0305206
dc.identifierhttp://arxiv.org/abs/astro-ph/0305206
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6061
dc.subjectAstrophysics
dc.titleNumerical Likelihood Analysis of Cosmic Ray Anisotropies
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