| dc.contributor.author | Rannot, R. C | |
| dc.contributor.author | Bhat, C. L | |
| dc.contributor.author | Senecha, V. K | |
| dc.contributor.author | Sapru, M. L | |
| dc.contributor.author | Tickoo, A. K | |
| dc.contributor.author | Kaul, R. K | |
| dc.contributor.author | Rawat, H. S | |
| dc.date.accessioned | 2007-05-10T06:00:23Z | |
| dc.date.available | 2007-05-10T06:00:23Z | |
| dc.date.issued | 1993 | |
| dc.identifier.citation | BASI, Vol. 21, pp. 627-630 | en |
| dc.identifier.uri | http://hdl.handle.net/2248/1571 | |
| dc.description.abstract | An analysis of 47 hours of data collected by the Gulmarg gamma-ray telescope during the period 1989 September 27-October 30, indicates absence of a statistically significant steady, persistent-pulsed or episodic pulsed signal from the X-ray binary pulsar, 4U0115 + 63, at photons energies greater than or = 4 TeV. An upper limit of 2.33 x 10-11 photons/sq cm/sec is placed at 99% confidence level on the steady gamma-ray flux from this transient X-ray binary system | en |
| dc.format.extent | 284166 bytes | |
| dc.format.mimetype | application/pdf | |
| dc.language.iso | en | en |
| dc.publisher | Astronomical Society of India | en |
| dc.subject | Gamma ray | en |
| dc.title | A search for TeV photons from 4U0115 + 63 | en |
| dc.type | Article | en |