Measuring Gamma-Ray Energy Spectra with the HEGRA IACT System

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dc.creatorHofmann, W.
dc.date1997-10-27
dc.date.accessioned2026-07-07T02:24:50Z
dc.date.available2026-07-07T02:24:50Z
dc.descriptionThe stereoscopic reconstruction of air showers viewed by multiple imaging atmospheric Cherenkov telescopes (IACTs) allows a more precise reconstruction of shower energies and hence an improved determination of energy spectra. Reconstruction techniques and in particular new systematic checks are discussed on the basis of the large sample of gamma-rays from Mkn 501 detected with the HEGRA IACT system. (Talk presented at the Workshop ``Towards a Major Atmospheric Cherenkov Detector V'', Kruger Park, South Africa, 1997)
dc.description10 Pages, 11 figures, Latex, uses epsfig
dc.identifierhttps://arxiv.org/abs/astro-ph/9710297
dc.identifierhttp://arxiv.org/abs/astro-ph/9710297
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11702
dc.subjectAstrophysics
dc.titleMeasuring Gamma-Ray Energy Spectra with the HEGRA IACT System
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