| 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 | |
| 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 |