The arrival direction of (4/3)e-lepton candidates in celestial coordinates

Details The arrival direction of (4/3)e-lepton candidates in celestial coordinates The arrival direction of (4/3)e-lepton candidates in celestial coordinates

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ncimc..11..229w&link_type=abstract

Nuovo Cimento C, Serie 1 (ISSN 0390-5551), vol. 11 C, Mar.-Apr. 1988, p. 229-235.

Astronomy and Astrophysics

Astrophysics

Astronomical Coordinates, Cosmology, Electrostatic Charge, Leptons, Nuclear Astrophysics, Abundance, Astronomical Models, Particle Telescopes, Quantum Chromodynamics, Quarks

Scientific paper

A cosmic-ray counter telescope (Okayama telescope) has been operated at several zenith angles at sea level. Several millions of clean single events have been analyzed. About thirty candidates of (4/3)e charged leptons were found at around 40-deg zenith angles. The distribution of the arrival directions of these candidates in the celestial sphere was found to be anisotropic.

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