dc.contributor.author |
Kamath, K |
|
dc.contributor.author |
Bhattacharyya, S |
|
dc.contributor.author |
Dhar, V. K |
|
dc.contributor.author |
Darzi, M. A |
|
dc.contributor.author |
Kaul, S. R |
|
dc.contributor.author |
Kaul, R. K |
|
dc.contributor.author |
Koul, R |
|
dc.contributor.author |
Sahayanathan, S |
|
dc.contributor.author |
Tickoo, A. K |
|
dc.contributor.author |
Wani, A. M |
|
dc.contributor.author |
Bhat, C. L |
|
dc.date.accessioned |
2008-06-19T07:27:17Z |
|
dc.date.available |
2008-06-19T07:27:17Z |
|
dc.date.issued |
2002 |
|
dc.identifier.citation |
BASI, Vol. 30, No. 1, pp. 377 - 380 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/2458 |
|
dc.description.abstract |
An ultra-sensitive, multidetector wide angle atmospheric Cerenkov telescope array is being set up at Mt. Abu for cosnic gamma-ray studies in tens of TeV energy region. The design features of the Cerenkov light detector, along with its efficiency, based on simulation and prototype testing studies, are presented in this paper. |
en |
dc.format.extent |
354096 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of India |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/2002BASI...30..377K |
en |
dc.subject |
Gamma-Ray |
en |
dc.subject |
MYSTIQUE Telescope |
en |
dc.subject |
LAWA detector |
en |
dc.title |
Large-Area Wide Angle (LAWA) cerenkov detector for MYSTIQUE array |
en |
dc.type |
Article |
en |