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Layout design studies for medium-sized telescopes within the Cherenkov Telescope Array
Marko 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
.pdf Fulltext (1,59 MB)

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Simulations of a Distributed Intelligent Array Trigger for the Cherenkov Telescope Array
Marko 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
.pdf Fulltext (366,72 KB)

26.
Performance of the Cherenkov Telescope Array
Marko 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
.pdf Fulltext (321,78 KB)

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Charge carrier transport in polycrystalline CH3NH3PbI3 perovskite thin films in a lateral direction characterized by time-of-flight photoconductivity
Gvido 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
.pdf Fulltext (1,53 MB)

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Search for Anisotropy in the Ultra High Energy Cosmic Ray Spectrum using the Telescope Array Surface Detector
J. 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
.pdf Fulltext (169,05 KB)

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