Numerical likelihood analysis of cosmic ray anisotropies

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Description

A 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.

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102 Kilobytes pages

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al., Carlos Hojvat et July 2, 2003.

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Description

A 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.

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102 Kilobytes pages

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  • 28th International Cosmic Ray Conferences (ICRC 2003), Tsukuba (JP), 07/31/2003--08/07/2003

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  • Report No.: FERMILAB-Conf-03/185-A
  • Grant Number: AC02-76CH03000
  • Office of Scientific & Technical Information Report Number: 812144
  • Archival Resource Key: ark:/67531/metadc736578

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  • July 2, 2003

Added to The UNT Digital Library

  • Oct. 18, 2015, 6:40 p.m.

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  • Aug. 5, 2016, 3:43 p.m.

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al., Carlos Hojvat et. Numerical likelihood analysis of cosmic ray anisotropies, article, July 2, 2003; Batavia, Illinois. (digital.library.unt.edu/ark:/67531/metadc736578/: accessed September 22, 2017), University of North Texas Libraries, Digital Library, digital.library.unt.edu; crediting UNT Libraries Government Documents Department.