Observation of sub-TeV gamma-rays from RX J0852.0-4622 with the CANGAROO-II telescope

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dc.contributor.authorKatagiri, H.
dc.contributor.authorEnomoto, R.
dc.contributor.authorMori, M.
dc.contributor.authorAsahara, A.
dc.contributor.authorBicknell, G.
dc.contributor.authorClay, R.
dc.contributor.authorDoi, Y.
dc.contributor.authorEdwards, P.
dc.contributor.authorGunji, S.
dc.contributor.authorHara, S.
dc.contributor.authorHara, T.
dc.contributor.authorHattori, T.
dc.contributor.authorHayashi, S.
dc.contributor.authorItoh, C.
dc.contributor.authorKabuki, S.
dc.contributor.authorKajino, F.
dc.contributor.authorKawachi, A.
dc.contributor.authorKifune, T.
dc.contributor.authorKsenofontov, L.
dc.contributor.authorKubo, H.
dc.contributor.authoret al.
dc.contributor.conferenceInternational Cosmic Ray Conference (28th : 2003 : Tsukuba, Japan)
dc.date.issued2003
dc.description.abstractRX J0852.0−4622 (G266.2−1.2) is a Type-II Supernova Remnant (SNR) located along the line of sight to the Vela SNR. We observed RX J0852.0−4622 with the CANGAROO-II telescope from the middle of December, 2001, to the end of February, 2002, to search for sub-TeV gamma-rays. A preliminary analysis shows an apparent excess of gamma-ray-like events in alpha distribution from RX J0852.0−4622, which is to be examined in continued analyses and further observations.
dc.identifier.citation28th International Cosmic Ray Conference, 2003 / T. Kajita, Y. Asaoka, A. Kawachi, Y. Matsubara, M. Sasaki (eds.): pp. 2409-2412
dc.identifier.isbn4946443800
dc.identifier.issn0915-8502
dc.identifier.orcidClay, R. [0000-0002-9040-9648]
dc.identifier.urihttp://hdl.handle.net/2440/49634
dc.language.isoen
dc.publisherUniversal Academy Press
dc.relation.ispartofseriesFrontiers Science Series No. 41
dc.source.urihttp://www-rccn.icrr.u-tokyo.ac.jp/icrc2003/
dc.titleObservation of sub-TeV gamma-rays from RX J0852.0-4622 with the CANGAROO-II telescope
dc.typeConference paper
pubs.publication-statusPublished

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