Abstract
Using data collected by the MACRO experiment during the years 1989–1996, we show evidence for the shadow of the Moon in the underground cosmic ray flux with a significance of 3.6σ. This detection of the shadowing effect is the first by an underground detector. A maximum-likelihood analysis is used to determine that the angular resolution of the apparatus is [Formula Presented] These results demonstrate MACRO’s capabilities as a muon telescope by confirming its absolute pointing ability and quantifying its angular resolution.
| Lingua originale | Inglese |
|---|---|
| Rivista | Physical Review D - Particles, Fields, Gravitation and Cosmology |
| Volume | 59 |
| Numero di pubblicazione | 1 |
| DOI | |
| Stato di pubblicazione | Pubblicato - 1999 |
| Pubblicato esternamente | Sì |
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