Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4795
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dc.contributor.authorChitnis, V. R-
dc.contributor.authorAcharya, B. S-
dc.contributor.authorBhat, P. N-
dc.contributor.authorCowsik, R-
dc.contributor.authorPrabhu, T. P-
dc.contributor.authorSrinivasan, R-
dc.contributor.authorSrivatsan, R-
dc.contributor.authorVishwanath, P. R-
dc.date.accessioned2009-09-08T14:11:13Z-
dc.date.available2009-09-08T14:11:13Z-
dc.date.issued2005-
dc.identifier.citationSripathi Acharya, B. eds., [et al.]... Proceedings of the 29th International Cosmic Ray Conference. August 3 - 10, 2005, Pune, India. pp. 235 - 238en
dc.identifier.urihttp://hdl.handle.net/2248/4795-
dc.description.abstractA 7 telescope array is planned to be constructed at Hanle in the Himalayas at an altitude of about 4200m above mean sea level for detecting celestial gamma-rays. The atmospheric Cerenkov light pool created by the primary gamma-rays is sampled through wave-front sampling technique to infer the direction and energy of the incident gamma-rays. Monte Carlo simulation calculations were performed to understand the energy threshold and event trigger rates. One telescope is fabricated and shifted to Hanle after extensive tests at CREST, Hosakote. The current schedule for the fabrication of remaining telescopes, experiment and the energy threshold will be discussed.en
dc.language.isoenen
dc.publisherTata Institute of Fundamental Researchen
dc.relation.ispartofseriesInternational Cosmic Ray Conference;No. 29-
dc.relation.urihttp://adsabs.harvard.edu//abs/2005ICRC....5..235Cen
dc.subjectStatus of HAGARen
dc.subjectHigh Altitude Gamma Ray Observatoryen
dc.subjectA 7 Telescope Arrayen
dc.subjectCelestial Gamma Raysen
dc.titleStatus of HAGAR, the high altitude gamma ray observatory at Hanleen
dc.typeArticleen
Appears in Collections:Publications based on data from IAO, Hanle
IIAP Publications

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