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2019-05-09
Search for Ultra-High-Energy Neutrinos with the Telescope Array Surface Detector
R. U. AbbasiM. AbeT. Abu-ZayyadM. AllenE. BarcikowskiJ. W. BelzD. R. BergmanS. A. BlakeR. CadyB. G. CheonJ. ChibaM. ChikawaA. di MatteoT. FujiiK. FujisueK. FujitaR. FujiwaraM. FukushimaG. FurlichW. HanlonM. HayashiY. HayashiN. HayashidaK. HibinoK. HondaD. IkedaN. InoueT. IshiiH. ItoD. IvanovH. M. JeongS. JeongC. C. H. JuiK. KadotaF. KakimotoO. KalashevK. KasaharaH. KawaiS. KawakamiS. KawanaK. KawataE. KidoH. B. KimJ. H. KimJ. H. KimS. KishigamiV. KuzminM. KuznetsovY. J. KwonK. H. LeeB. LubsandorzhievJ. P. LundquistK. MachidaK. MartensT. MatsuyamaJ. N. MatthewsR. MaytaM. MinaminoK. MukaiI. MyersK. NagasawaS. NagatakiK. NakaiR. NakamuraT. NakamuraT. NonakaH. OdaS. OgioM. OhnishiH. OhokaT. OkudaY. OmuraM. OnoR. OnogiA. OshimaS. OzawaI. H. ParkM. S. PshirkovJ. RemingtonD. C. RodriguezG. RubtsovD. RyuH. SagawaR. SaharaK. SaitoY. SaitoN. SakakiT. SakoN. SakuraiL. M. ScottT. SekiK. SekinoP. D. ShahF. ShibataT. ShibataH. ShimodairaB. K. ShinH. S. ShinJ. D. SmithP. SokolskyB. T. StokesS. R. StrattonT. A. StromanT. SuzawaY. TakagiY. TakahashiM. TakamuraM. TakedaR. TakeishiA. TaketaM. TakitaY. TamedaH. TanakaK. TanakaM. TanakaY. TanoueS. B. ThomasG. B. ThomsonP. TinyakovI. TkachevH. TokunoT. TomidaS. TroitskyY. TsunesadaY. UchihoriS. UdoF. UrbanT. WongK. YadaM. YamamotoH. YamaokaK. YamazakiJ. YangK. YashiroH. YoshiiY. ZhezherZ. Zundel
文献摘要
We present an upper limit on the flux of ultra-high-energy down-going neutrinos for derived with the nine years of data collected by the Telescope Array surface detector (05-11-2008 – 05-10-2017). The method is based on the multivariate analysis technique, so-called Boosted Decision Trees (BDT). Proton-neutrino classifier is built upon 16 observables related to both the properties of the shower front and the lateral distribution function.
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