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- W2068192481 abstract "During the last decade ground-based very high-energy γ-ray astronomy achieved a remarkable advancement in the development of the observational technique for the registration and study of γ-ray emission above 100 GeV. It is widely believed that the next step in its future development will be the construction of telescopes of substantially larger size than the currently used 10 m class telescopes. This can drastically improve the sensitivity of the ground-based detectors for γ-rays of energy from 10 to 100 GeV. Based on Monte Carlo simulations of the response of a single stand-alone 30 m imaging atmospheric Cherenkov telescope (IACT), the maximal rejection power against background cosmic ray showers for low-energy γ-rays was investigated in great detail. An advanced Bayesian multivariate analysis has been applied to the simulated Cherenkov light images of the γ-ray- and proton-induced air showers. The results obtained here quantitatively testify that the separation between the signal and background images degrades substantially at low energies, and consequently the maximum overall quality factor can only be about 3.1 for γ-rays in the 10–30 GeV energy range. Various selection criteria as well as optimal combinations of the standard image parameters utilized for effective image separation have also been evaluated." @default.
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- W2068192481 date "2006-10-09" @default.
- W2068192481 modified "2023-10-18" @default.
- W2068192481 title "Study on cosmic ray background rejection with a 30 m stand-alone IACT using non-parametric multivariate methods in a sub-100 GeV energy range" @default.
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- W2068192481 doi "https://doi.org/10.1088/0954-3899/32/11/019" @default.
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