21. Second large-scale Monte Carlo study for the Cherenkov Telescope ArrayMarko Zavrtanik, Danilo Zavrtanik, Gabrijela Zaharijas, Lili Yang, Serguei Vorobiov, Samo Stanič, Gašper Kukec Mezek, Andrej Filipčič, T. Hassan, 2015, published scientific conference contribution Found in: ključnih besedah
Keywords: Cherenkov Telescope Array (CTA), CTA design optimization, Monte Carlo simulations
Published: 16.02.2017; Views: 2700; Downloads: 168
 Fulltext (341,65 KB) |
22. Monte Carlo Performance Studies of Candidate Sites for the Cherenkov Telescope ArrayMarko Zavrtanik, Danilo Zavrtanik, Gabrijela Zaharijas, Lili Yang, Serguei Vorobiov, Samo Stanič, Gašper Kukec Mezek, Andrej Filipčič, G. Maier, 2015, published scientific conference contribution Found in: ključnih besedah
Keywords: Cherenkov Telescope Array (CTA), CTA candidate sites, Monte Carlo performance studies
Published: 16.02.2017; Views: 2469; Downloads: 0
Fulltext (297,46 KB) |
23. Layout design studies for medium-sized telescopes within the Cherenkov Telescope ArrayMarko Zavrtanik, Danilo Zavrtanik, Gabrijela Zaharijas, Lili Yang, Serguei Vorobiov, Samo Stanič, Gašper Kukec Mezek, Andrej Filipčič, T. Hassan, 2015, published scientific conference contribution Found in: ključnih besedah
Summary of found: ...TA),
medium-sized telescopes (MST) CTA sub-array,
MST layout design studies,
Monte Carlo performance studies...
Keywords: Cherenkov Telescope Array (CTA), medium-sized telescopes (MST) CTA sub-array, MST layout design studies, Monte Carlo performance studies
Published: 16.02.2017; Views: 2669; Downloads: 202
Fulltext (1,59 MB) |
24. Monte Carlo Studies of the GCT Telescope for the Cherenkov Telescope ArrayMarko Zavrtanik, Danilo Zavrtanik, Gabrijela Zaharijas, Lili Yang, Serguei Vorobiov, Samo Stanič, Gašper Kukec Mezek, Andrej Filipčič, Thomas Armstrong, 2015, published scientific conference contribution Found in: ključnih besedah
Keywords: Cherenkov Telescope Array (CTA), GCT: a dual-mirror small-size telescope (SST-2M) design for CTA, Monte Carlo performance studies
Published: 16.02.2017; Views: 2441; Downloads: 169
Fulltext (752,33 KB) |
25. Simulations of a Distributed Intelligent Array Trigger for the Cherenkov Telescope ArrayMarko Zavrtanik, Danilo Zavrtanik, Gabrijela Zaharijas, Lili Yang, Serguei Vorobiov, Samo Stanič, Gašper Kukec Mezek, Andrej Filipčič, Hugh Dickinson, 2015, published scientific conference contribution Found in: ključnih besedah
Summary of found: ...Cherenkov Telescope Array (CTA),
distributed intelligent array trigger,
Monte-Carlo performance evaluation...
Keywords: Cherenkov Telescope Array (CTA), distributed intelligent array trigger, Monte-Carlo performance evaluation
Published: 16.02.2017; Views: 2925; Downloads: 138
Fulltext (366,72 KB) |
26. Performance of the Cherenkov Telescope ArrayMarko Zavrtanik, Danilo Zavrtanik, Gabrijela Zaharijas, Lili Yang, Serguei Vorobiov, Samo Stanič, Gašper Kukec Mezek, Christopher Eckner, G. Maier, 2017, published scientific conference contribution Found in: ključnih besedah
Summary of found: ...CTA,
Monte Carlo simulations,
gamma rays...
Keywords: CTA, Monte Carlo simulations, gamma rays
Published: 16.02.2018; Views: 1962; Downloads: 109
Fulltext (321,78 KB) |
27. A Monte Carlo simulation study for cosmic-ray chemical composition measurement with Cherenkov Telescope ArrayMarko Zavrtanik, Danilo Zavrtanik, Gabrijela Zaharijas, Lili Yang, Serguei Vorobiov, Samo Stanič, Gašper Kukec Mezek, Christopher Eckner, Michiko Ohishi, 2017, published scientific conference contribution Found in: ključnih besedah
Keywords: CTA, Monte Carlo simulation, cosmic-ray chemical composition
Published: 16.02.2018; Views: 2200; Downloads: 113
Fulltext (448,16 KB) |
28. Charge carrier transport in polycrystalline CH3NH3PbI3 perovskite thin films in a lateral direction characterized by time-of-flight photoconductivityGvido Bratina, Matjaž Valant, Egon Pavlica, Hasan Okuyucu, Saim Emin, 2018, original scientific article Found in: ključnih besedah
Summary of found: ...CH3NH3PbI3, Time-of-flight photoconductivity, Monte Carlo simulation, Carrier mobility...
Keywords: CH3NH3PbI3, Time-of-flight photoconductivity, Monte Carlo simulation, Carrier mobility
Published: 04.09.2018; Views: 2368; Downloads: 0
Fulltext (1,53 MB) |
29. Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layoutMarko Zavrtanik, Danilo Zavrtanik, Lili Yang, Serguei Vorobiov, Samo Stanič, A. Acharyya, 2019, original scientific article Found in: ključnih besedah
Keywords: very-high energy gamma-ray astronomy, Cherenkov Telescope Array, array layout optimisation, Monte Carlo studies
Published: 18.04.2019; Views: 1773; Downloads: 0
Fulltext (3,46 MB) |
30. Search for Anisotropy in the Ultra High Energy Cosmic Ray Spectrum using the Telescope Array Surface DetectorJ. P. Lundquist, R.U. Abbasi, 2017, other component parts Abstract: The Telescope Array (TA) experiment is located in the western desert of Utah, USA, and observes ultra high energy cosmic rays (UHECRs) in the Northern hemisphere. At the highest energies, E>10~EeV, the shape of cosmic ray energy spectrum may carry an imprint of the source density distribution along the line of sight different in different directions of the sky. In this study, we search for such directional variations in the shape of the energy spectrum using events observed with the Telescope Array's surface detector. We divide the TA field of view into two nearly equal-exposure regions: the "on-source" region which we define as ±30∘ of the supergalactic plane containing mostly nearby structures, and the complementary "off-source" region where the sources are further away on average. We compare the UHECR spectra in these regions by fitting them to the broken power law and comparing the resulting parameters. We find that the off-source spectrum has an earlier break at highest energies. The chance probability to obtain such or larger difference in statistically equivalent distributions is estimated as 6.2±1.1×10−4 (3.2σ) by a Monte-Carlo simulation. The observed difference in spectra is in a reasonable quantitative agreement with a simplified model that assumes that the UHECR sources trace the galaxy distribution from the 2MRS catalogue, primary particles are protons and the magnetic deflections can be neglected.
Found in: ključnih besedah
Summary of found: ...is estimated as 6.2±1.1×10−4 (3.2σ) by a Monte-Carlo simulation. The observed difference in spectra is...
Keywords: cosmic radiation: UHE, detector: surface, cosmic radiation: spectrum, cosmic radiation: energy spectrum, deflection: magnetic, numerical calculations: Monte Carlo, anisotropy
Published: 27.04.2020; Views: 1505; Downloads: 52
Fulltext (169,05 KB) |
