Estimation of expected performance for the MACE γ-ray telescope in low zenith angle range

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dc.contributor.authorBorwankar, C.
dc.contributor.authorSharma, M.
dc.contributor.authorBhatt, N.
dc.contributor.authorBhattacharyya, S.
dc.contributor.authorRannot, R. C.
dc.contributor.authorTickoo, A. K.
dc.date.accessioned2021-04-12T06:57:37Z
dc.date.available2021-04-12T06:57:37Z
dc.date.issued2020
dc.description.divisionApSDen
dc.format.extent5831 bytes
dc.format.mimetypetext/html
dc.identifier.sourceNuclear Instruments & Methods in Physics Research-A, 2020. Vol. 953: Article no. 163182en
dc.identifier.urihttp://hdl.handle.net/123456789/22738
dc.language.isoenen
dc.subjectCherenkov telescopesen
dc.subjectCosmic raysen
dc.subjectGamma raysen
dc.titleEstimation of expected performance for the MACE γ-ray telescope in low zenith angle rangeen
dc.typeArticleen

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