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000600671 0247_ $$2doi$$a10.22323/1.444.0594
000600671 0247_ $$2datacite_doi$$a10.3204/PUBDB-2023-08094
000600671 0247_ $$2arXiv$$aarXiv:2309.11315
000600671 0247_ $$2openalex$$aopenalex:W4385304783
000600671 037__ $$aPUBDB-2023-08094
000600671 041__ $$aEnglish
000600671 082__ $$a530
000600671 088__ $$2arXiv$$aarXiv:2309.11315
000600671 088__ $$2Other$$aCTA-ICRC/2023/12
000600671 1001_ $$aAbe, Kazuki$$b0
000600671 1112_ $$a38th International Cosmic Ray Conference$$cNagoya$$d2023-07-26 - 2023-08-03$$gICRC2023$$wJapan
000600671 245__ $$aPerformance of the Large-Sized Telescope prototype of the Cherenkov Telescope Array
000600671 260__ $$aTrieste$$bSISSA$$c2023
000600671 300__ $$a10
000600671 3367_ $$2ORCID$$aCONFERENCE_PAPER
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000600671 3367_ $$0PUB:(DE-HGF)8$$2PUB:(DE-HGF)$$aContribution to a conference proceedings$$bcontrib$$mcontrib$$s1707124297_3708073
000600671 3367_ $$0PUB:(DE-HGF)7$$2PUB:(DE-HGF)$$aContribution to a book$$mcontb
000600671 4900_ $$2Author$$a2681608
000600671 500__ $$aPresented at the 38th International Cosmic Ray Conference (ICRC 2023), 2023 (arXiv:2309.08219) Pre-published
000600671 520__ $$aThe next-generation ground-based gamma-ray Cherenkov Telescope Array Observatory (CTAO) will consist of imaging atmospheric Cherenkov telescopes (IACTs) of three different sizes distributed in two sites. The Large-Sized Telescopes will cover the low-energy end of the CTA energy range, starting at about 20 GeV. After its first years of operation at the CTA northern site, the Large-Sized Telescope prototype (LST-1) is in the final stage of its commissioning phase, having collected a significant amount of scientific data to date.In this contribution, we present the physics performance of the telescope using low-zenith Crab Nebula observations and Monte Carlo simulations fine-tuned accordingly. We show performance figures of merit such as the energy threshold, effective area, energy and angular resolution, and sensitivity based on the standard Hillas-parameters approach and following the source-independent and dependent analysis methods. The analysis threshold is estimated at 30 GeV. The energy resolution is around 30%, and the angular resolution is 0.3 degrees at 100 GeV.The best integral sensitivity of LST-1 is about 1.1% of the Crab Nebula flux above 250 GeV for 50 hours of observations. We also show the spectral energy distribution and light curve from Crab Nebula observations, which agree with results from other IACTs and link smoothly with Fermi-LAT when considering statistical and systematic uncertainties near the energy threshold.
000600671 536__ $$0G:(DE-HGF)POF4-613$$a613 - Matter and Radiation from the Universe (POF4-613)$$cPOF4-613$$fPOF IV$$x0
000600671 588__ $$aDataset connected to CrossRef Conference
000600671 650_7 $$2INSPIRE$$aenergy: threshold
000600671 650_7 $$2INSPIRE$$adetector: performance
000600671 650_7 $$2INSPIRE$$anumerical calculations: Monte Carlo
000600671 650_7 $$2INSPIRE$$aCherenkov counter: atmosphere
000600671 650_7 $$2INSPIRE$$aGeV
000600671 650_7 $$2INSPIRE$$aCherenkov Telescope Array
000600671 650_7 $$2INSPIRE$$aangular resolution
000600671 650_7 $$2INSPIRE$$asensitivity
000600671 650_7 $$2INSPIRE$$asite
000600671 650_7 $$2INSPIRE$$aobservatory
000600671 650_7 $$2INSPIRE$$aflux
000600671 650_7 $$2INSPIRE$$astatistical
000600671 650_7 $$2INSPIRE$$aspectral energy distribution
000600671 650_7 $$2INSPIRE$$aGLAST
000600671 650_7 $$2INSPIRE$$aenergy resolution
000600671 650_7 $$2INSPIRE$$aimaging
000600671 650_7 $$2INSPIRE$$agamma ray
000600671 693__ $$0EXP:(DE-H253)CTA-20150101$$5EXP:(DE-H253)CTA-20150101$$eCherenkov Telescope Array$$x0
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000600671 7001_ $$0P:(DE-H253)PIP1080676$$aMorcuende, Daniel$$b181$$eCorresponding author
000600671 7001_ $$aMorselli, Aldo$$b182
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