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 |
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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 |