Proceedings of 35th International Cosmic Ray Conference — PoS(ICRC2017) 2017
DOI: 10.22323/1.301.0759
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TAIGA-HiSCORE: results from the first two operation seasons

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Cited by 8 publications
(14 citation statements)
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“…The advantage of the Cherenkov telescope as part of the complex of wide-angle timing Cherenkov stations is a possibility to obtain additional information about position of the shower axis, direction to the source, and the primary particle energy [4]. All these parameters are determined by the wide-angle Cherenkov stations instead of the IACT.…”
Section: Introductionmentioning
confidence: 99%
“…The advantage of the Cherenkov telescope as part of the complex of wide-angle timing Cherenkov stations is a possibility to obtain additional information about position of the shower axis, direction to the source, and the primary particle energy [4]. All these parameters are determined by the wide-angle Cherenkov stations instead of the IACT.…”
Section: Introductionmentioning
confidence: 99%
“…The reconstruction of the shower parameters is performed by using the algorithms developed for the Tunka-133 [1], [11] and for the TAIGA-HiSCORE arrays [12]. The accuracy of the reconstruction procedure was checked by comparing of the MC simulation results with experimental data [13]. About 20 millions EAS with simultaneous hits of 4 or more stations were recorded during the 55 clean moonless nights of the 2016-2017 winter season.…”
Section: Pos(icrc2017)768mentioning
confidence: 99%
“…Main HiSCORE results are the energy spectrum of cosmic rays, a search for an event excess from the Crab Nebula and the first detection of the CATS-LIDAR onboard the ISS [14], used for precision pointing verification , see 3 . For details see [13], [15], [16].…”
Section: Pos(icrc2017)768mentioning
confidence: 99%
“…• calibrate the HiSCORE-station relative time-offsets using ISS-events ("time-offset calibration", as discussed in [2,8]). See Fig.8(b) for a comparison with other calibration methods,…”
Section: Application Of the Iss-lidarmentioning
confidence: 99%
“…• measure the time jitter for each station, see [2], • perform low level technical checks, like: array performance at large illumination, optimization of raw data extraction procedures (pulse extraction, amplitude definition), identification of small systematic effects (masked by stochastics dominated EAS analysis),…”
Section: Application Of the Iss-lidarmentioning
confidence: 99%