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http://hdl.handle.net/2248/1571
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DC Field | Value | Language |
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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 |
Appears in Collections: | BASI Publications |
Files in This Item:
File | Description | Size | Format | |
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Paper_13.pdf | 277.51 kB | Adobe PDF | View/Open |
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