dc.contributor.author |
Rannot, R. C |
|
dc.contributor.author |
Yadav, K. K |
|
dc.contributor.author |
Dhar, V. K |
|
dc.contributor.author |
Tickoo, A. K |
|
dc.contributor.author |
Bhatt, N |
|
dc.contributor.author |
Bhattacharyya, S |
|
dc.contributor.author |
Chandra, P |
|
dc.contributor.author |
Goyal, H. C |
|
dc.contributor.author |
Kaul, C. L |
|
dc.contributor.author |
Kaul, R. K |
|
dc.contributor.author |
Kothari, M |
|
dc.contributor.author |
Kotwal, S |
|
dc.contributor.author |
Koul, R |
|
dc.contributor.author |
Sahayanathan, S |
|
dc.contributor.author |
Sapru, M. L |
|
dc.contributor.author |
Sharma, M |
|
dc.contributor.author |
Venugopal, K |
|
dc.contributor.author |
Bhat, C. L |
|
dc.date.accessioned |
2008-07-22T09:09:52Z |
|
dc.date.available |
2008-07-22T09:09:52Z |
|
dc.date.issued |
2002-09 |
|
dc.identifier.citation |
BASI, Vol. 30, No. 3, pp. 699 - 700 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/2796 |
|
dc.description.abstract |
The TACTIC Imaging Element has observed Crab Nebula/pulsar
for a total. of about 40 hours during Jan.- Mar. 2001. Preliminary results do
not show any evidence of the 33 ms pulsations from the pulsar direction at an
energy threshold of 1 TeV. The 99.9% confidence level upper limit for pulsed
emission has been derived to be ~ 22% of the steady flux from the Crab Nebula. |
en |
dc.format.extent |
73748 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.subject |
TeV Gamma Rays |
en |
dc.subject |
The Crab Nebula |
en |
dc.title |
Search for pulsed Te V gamma- rays from Crab pulsar with the TACTIC Imaging gamma-ray Telescope |
en |
dc.type |
Article |
en |