(Q58322918)

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Maximum likelihood analysis of clusters of ultrahigh energy cosmic rays

article by Günter Sigl et al published 15 October 1997 in Physical Review D

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Maximum likelihood analysis of clusters of ultrahigh energy cosmic rays (English)

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Martin Lemoine

2

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author name string

Günter Sigl

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1

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Angela V. Olinto

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3

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language of work or name

English

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publication date

15 October 1997

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published in

Physical Review D

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volume

56

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issue

8

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page(s)

4470-4479

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cites work

End to the Cosmic-Ray Spectrum?

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21 January 2018

Detection of a cosmic ray with measured energy well beyond the expected spectral cutoff due to cosmic microwave radiation

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21 January 2018

On the origin of highest energy cosmic rays

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https://api.crossref.org/works/10.1103%2FPHYSREVD.56.4470

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21 January 2018

In search of a source for the 320 EeV Fly's Eye cosmic ray

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21 January 2018

The Origin of Ultra-High-Energy Cosmic Rays

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21 January 2018

Cosmological Gamma-Ray Bursts and the Highest Energy Cosmic Rays

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21 January 2018

Possible Association of Ultra–High-Energy Cosmic-Ray Events with Strong Gamma-Ray Bursts

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21 January 2018

Grand unified theories, topological defects, and ultrahigh-energy cosmic rays.

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21 January 2018

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https://api.crossref.org/works/10.1103%2FPHYSREVD.56.4470

retrieved

21 January 2018

Topological defects and highest energy cosmic and gamma rays

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Crossref

reference URL

https://api.crossref.org/works/10.1103%2FPHYSREVD.56.4470

retrieved

21 January 2018

Influence of the universal microwave background radiation on the extragalactic cosmic-ray spectrum.

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retrieved

21 January 2018

Ultra–high-Energy Cosmic-Ray Sources and Large-Scale Magnetic Fields

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https://api.crossref.org/works/10.1103%2FPHYSREVD.56.4470

retrieved

21 January 2018

Detecting intergalactic magnetic fields using time delays in pulses of γ-rays

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stated in

Crossref

reference URL

https://api.crossref.org/works/10.1103%2FPHYSREVD.56.4470

retrieved

21 January 2018

Identifiers

DOI

10.1103/PHYSREVD.56.4470

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(Q58322918)

Maximum likelihood analysis of clusters of ultrahigh energy cosmic rays

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