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Title: | Pachmarhi array of Cerenkov telescopes |
Authors: | Bhat, P. N Acharya, B. S Chitnis, V. R D'Souza, A. I Francis, P. J Gothe, K. S John, A. V Mazumdar, P Nagesh, B. K Purohit, P. N Rahman, M. A Rao, S. K Rao, K. K Sharma, S. K Stanislaus, A. J Sudershanan, P. V Swamy, M. R. K Upadhyaya, S. S Murty, B. L. V |
Keywords: | VHE γ-rays Atmospheric Cerenkov Technique PACT |
Issue Date: | 2000 |
Publisher: | Astronomical Society of India |
Citation: | BASI, Vol. 28, No. 2, pp. 455 - 457 |
Abstract: | Pachmarhi Array of Cerenkov Telescopes (PACT) consisting of 25 telescopes has been installed at Pachmarhi (longitude : 76d 26' E, latitude : 22d 28' N and altitude : 1075m) recently. The telescopes are deployed in the form of a 5 - 5 matrix spread over an area of 80m - 100m. The array is designed to detect celestial TeV gamma-rays by wavefront sampling technique as against the standard imaging technique used at other ?-ray observatories elsewhere in the world. Each telescope consists of 7 parabolic reflectors of 90 cm diameter and an f/d ~1. Each telescope is independently steerable on separate equatorial mounts operated through a computer based control system capable of orienting them with an angular accuracy better than 0.2d. The pointing is monitored in real time to maintain a source tracking accuracy of better than 0.1d. We will discuss the array design, its suitability for wavefront sampling and its pointing capabilities. |
URI: | http://hdl.handle.net/2248/2176 |
Appears in Collections: | BASI Publications |
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Bhat_PN.pdf | 207.54 kB | Adobe PDF | View/Open |
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