Searches for Ultra–High‐Energy Gamma Rays from SN 1987A and Centaurus X‐3

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dc.contributor.authorH. Yoshii
dc.contributor.authorT. Baba
dc.contributor.authorT. Kaneko
dc.contributor.authorK. Suga
dc.contributor.authorF. Kakimoto
dc.contributor.authorS. Ogio
dc.contributor.authorY. Shirasaki
dc.contributor.authorN. Gironda
dc.contributor.authorM. Teshima
dc.contributor.authorY. Toyoda
dc.coverage.spatialBolivia
dc.date.accessioned2026-03-22T15:44:27Z
dc.date.available2026-03-22T15:44:27Z
dc.date.issued1996
dc.descriptionCitaciones: 5
dc.description.abstractSearches for gamma rays above 100 TeV from SN 1987A and above 50 TeV from Cen X-3 were carried out with an air shower array at Mount Chacaltaya over a period of 3 years. The array, which consists of 13 4 m2 and 28 1 m2 scintillation detectors, was located on a slope of about 30 facing southward to e ectively observe air showers coming from the directions of these sources. In the analysis, a selection by shower age parameter was applied to reduce the background due to showers initiated by protons or nuclei.
dc.identifier.doi10.1086/178108
dc.identifier.urihttps://doi.org/10.1086/178108
dc.identifier.urihttps://andeanlibrary.org/handle/123456789/54134
dc.language.isoen
dc.publisherIOP Publishing
dc.relation.ispartofThe Astrophysical Journal
dc.sourceEhime University
dc.subjectPhysics
dc.subjectCentaurus A
dc.subjectAir shower
dc.subjectGamma ray
dc.subjectAstrophysics
dc.subjectSupernova
dc.subjectHigh energy
dc.subjectScintillation
dc.subjectAstronomy
dc.subjectSemiconductor detector
dc.titleSearches for Ultra–High‐Energy Gamma Rays from SN 1987A and Centaurus X‐3
dc.typearticle

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