dc.contributor.author |
Maneva, G. M |
|
dc.contributor.author |
Temnikov, P. P |
|
dc.date.accessioned |
2008-06-02T11:47:13Z |
|
dc.date.available |
2008-06-02T11:47:13Z |
|
dc.date.issued |
2002 |
|
dc.identifier.citation |
BASI, Vol. 30, No. 1, pp. 255 - 260 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/2388 |
|
dc.description.abstract |
Artificial Neural Network (ANN) method is applied for the analysis of raw data from the gamma ray CELESTE experiment. Our preliminary results show that, in the energy range 30-300 GeV, a good discrimination between showers generated by primary photons or hadrons could be obtained. |
en |
dc.format.extent |
481056 bytes |
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dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of India |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/2002BASI...30..255M |
en |
dc.subject |
Gamma Astronomy on the Ground |
en |
dc.subject |
Artificial Neural Network |
en |
dc.title |
Application of neural network for the gamma-hadron discrimination |
en |
dc.type |
Article |
en |