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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1571
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dc.contributor.authorRannot, R. C-
dc.contributor.authorBhat, C. L-
dc.contributor.authorSenecha, V. K-
dc.contributor.authorSapru, M. L-
dc.contributor.authorTickoo, A. K-
dc.contributor.authorKaul, R. K-
dc.contributor.authorRawat, H. S-
dc.date.accessioned2007-05-10T06:00:23Z-
dc.date.available2007-05-10T06:00:23Z-
dc.date.issued1993-
dc.identifier.citationBASI, Vol. 21, pp. 627-630en
dc.identifier.urihttp://hdl.handle.net/2248/1571-
dc.description.abstractAn 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 systemen
dc.format.extent284166 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectGamma rayen
dc.titleA search for TeV photons from 4U0115 + 63en
dc.typeArticleen
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