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Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/87266
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dc.contributor.authorYoshikoshi, T.-
dc.contributor.authorClay, R.W.-
dc.contributor.authorDawson, B.R.-
dc.contributor.authorMatsubara, Y.-
dc.contributor.authorMori, M.-
dc.contributor.authorNaito, T.-
dc.contributor.authorNishijima, K.-
dc.contributor.authorOhishi, M.-
dc.contributor.authorRowell, G.P.-
dc.contributor.authorToyama, T.-
dc.date.issued2011-
dc.identifier.citationProceedings of the 32nd International Cosmic Ray Conference, ICRC 2011, 2011, vol.9, pp.231-234-
dc.identifier.urihttp://hdl.handle.net/2440/87266-
dc.description.abstractIn spite of more than 100 discoveries of TeV gamma-ray sources by the current imaging atmospheric Cherenkov telescope (IACT) arrays, Galactic cosmic ray accelerators up to the knee energies (∼ PeV) still remain unclear. PeV Explorer (or PeX) is a future project of a relatively small IACT array, optimized to detect gamma rays of energies greater than 10 TeV and aiming to explore Galactic accelerators up to PeV energies. We present the status of our hardware R & D studies for this project and some extension plans.-
dc.description.statementofresponsibilityT. Yoshikoshi, R. W. Clay, B. R. Dawson, Y. Matsubara, M. Mori, T. Naito, K. Nishijima, M. Ohishi, G. P. Rowell, T. Toyama-
dc.language.isoen-
dc.publisherInstitute of High Energy Physics-
dc.rightsCopyright status unknown-
dc.titleR&D studies for very high energy gamma-ray astrophysics at energies greater than 10 TeV-
dc.typeConference paper-
dc.contributor.conference32nd International Cosmic Ray Conference (ICRC) (11 Aug 2011 - 18 Aug 2011 : Beijing, China)-
dc.identifier.doi10.7529/ICRC2011/V09/1260-
pubs.publication-statusPublished-
dc.identifier.orcidClay, R.W. [0000-0002-9040-9648]-
dc.identifier.orcidDawson, B.R. [0000-0002-4271-3055]-
dc.identifier.orcidRowell, G.P. [0000-0002-9516-1581]-
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Chemistry and Physics publications

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