| 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 | |
| dc.format.mimetype | application/pdf | |
| 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 |