Abstract
A feasibility study has been carried out to assess the potentialof an Artificial Neural Network (ANN) for determiningthe direction of incidence of an Atmospheric Cerenkov Event(ACE) from the arrival-time information registered by aspaced-array of wide-angle Cerenkov detectors. Theresults obtained so far, using both, simulated and experimental data, indicate that a properly-trained net can yield a degree of accuracy which is comparable with what is achieved through the conventional χ2-minimization, wavefront-fitting procedure.
Similar content being viewed by others
References
Bhat, C. L. et al.: 1994, Proc. Int. Workshop ‘Towards a Major Atmospheric Cerenkov Detector-III’, Tokyo, pp. 347.
Bhat, C. L. et al.: 1995, Proc. 24th ICRC, Roma 3, 400.
Dai, R. W.: 1992, Proc. 17th Int. Nathiagali summer college on Physics and contemporary Needs, pp. 3.
Hertz, J. et al.: 1991, Introduction to the theory of Neural computation, Addison-Wesley, Reading.
Karle, A. et al.: 1995, Astropart. Phys. 3, 321.
Koch, C.: 1997, Nature 385, 207.
Lahav, O.: 1994, Vistas in Astronomy 38, 251.
Naim, A.: 1994, Vistas in Astronomy 38, 265.
Rumelhart, O. E.: 1986, Nature 323, 533.
Sembroski, G. and Kertzman, M. P.: 1991, Proc. 22nd ICRC, Dublin, 1, 500.
Tickoo, A. K. et al.: 1999, Proc. 26th ICRC, Utah, O.G 4.3.19.
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Dhar, V.K., Tickoo, A.K., Koul, R. et al. Artificial Neural Network Approach for Reconstruction of Event Arrival-Direction in Wide-Angle Atmospheric Cerenkov Detector Arrays: A Feasibility Study. Experimental Astronomy 10, 487–498 (2000). https://doi.org/10.1023/A:1008121205995
Issue Date:
DOI: https://doi.org/10.1023/A:1008121205995