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Pulsed emission of TeV gamma rays from Vela pulsarThe Ooty atmospheric Cerenkov array, consisting of 10 parabolic mirrors of 0.9 m diameter and 8 of 1.5 m diameter, was used for observations on the Vela pulsar to see if it emits gamma rays in the TeV energy range. During the winter of 1984-85, the array was split into two parts: (1) consisting wholly of the smaller mirrors, and (2) wholly of the bigger mirrors. The two arrays were operated at two different sites to distinguish a marginally significant genuine pulsar signal from spurious signals produced trivially by chance fluctuations in the background rates. All the mirrors were pointed at the celestial object to track it for durations of the order of 1 to 6 hours during clear moonless nights. The event time data is analyzed to detect a possible pulsed emission of TeV gamma rays using the contemporaneous pulsar elements on the basis of their radio observations on the Vela pulsar. Results from the analyses of observations made during the winters of 1982-83 and 1984-85 on steady pulsed emission and on possible transient emission is presented.
Document ID
19850025634
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Bhat, P. N.
(Tata Inst. of Fundamental Research Bombay, India)
Gupta, S. K.
(Tata Inst. of Fundamental Research Bombay, India)
Ramanamurthy, P. V.
(Tata Inst. of Fundamental Research Bombay, India)
Sreekantan, B. V.
(Tata Inst. of Fundamental Research Bombay, India)
Vishwanath, P. R.
(Tata Inst. of Fundamental Research Bombay, India)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 1
Subject Category
Space Radiation
Accession Number
85N33947
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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