000576674 001__ 576674
000576674 005__ 20231023210341.0
000576674 0247_ $$2INSPIRETeX$$aSpencer:2022cqu
000576674 0247_ $$2inspire$$ainspire:2632897
000576674 0247_ $$2arXiv$$aarXiv:2302.07611
000576674 0247_ $$2datacite_doi$$a10.3204/PUBDB-2023-00867
000576674 037__ $$aPUBDB-2023-00867
000576674 041__ $$aEnglish
000576674 088__ $$2arXiv$$aarXiv:2302.07611
000576674 1001_ $$0S.T.Spencer.1$$aSpencer, Samuel Timothy$$b0$$eCorresponding author
000576674 245__ $$aAdvanced Analysis of Night Sky Background Light for SSTCAM
000576674 260__ $$c2022
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000576674 500__ $$aPoS(Gamma2022)218. 6 pages, 3 figures. From proceedings of the 7th Heidelberg International Symposium on High-Energy Gamma-Ray Astronomy (Gamma2022) in Barcelona (Spain) on 4-8 July 2022. This version with corrected acknowledgements
000576674 520__ $$aNight Sky Background (NSB) is a complex phenomenon, consisting of all light detected by Imaging Atmospheric Cherenkov Telescopes (IACTs) not attributable to Cherenkov light emission. Understanding the effect of NSB on cameras for the next-generation Cherenkov Telescope Array (CTA) is important, as it affects the systematic errors on observations, the energy threshold, the thermal control of the cameras and the ability of the telescopes to operate under partial moonlight conditions. This capacity to observe under partial moonlight conditions is crucial for the CTA transient science programme, as it substantially increases the potential observing time. Using tools initially developed for H.E.S.S. (in combination withthe prototype CTA analysis package ctapipe) we will present predictions for the NSB present in images taken by the CTA Small Sized Telescope Camera (SSTCAM), showing that SSTCAM will likely be able to meet the associated CTA requirements. Additionally, we calculate the potential observing time gain by operating under high NSB conditions.
000576674 536__ $$0G:(DE-HGF)POF4-613$$a613 - Matter and Radiation from the Universe (POF4-613)$$cPOF4-613$$fPOF IV$$x0
000576674 588__ $$aDataset connected to INSPIRE
000576674 650_7 $$2INSPIRE$$aradiation, Cherenkov
000576674 650_7 $$2INSPIRE$$aenergy, threshold
000576674 650_7 $$2INSPIRE$$aCherenkov Telescope Array
000576674 650_7 $$2INSPIRE$$abackground
000576674 650_7 $$2INSPIRE$$aCherenkov counter
000576674 650_7 $$2INSPIRE$$athermal
000576674 650_7 $$2INSPIRE$$aimaging
000576674 650_7 $$2INSPIRE$$aHESS
000576674 693__ $$0EXP:(DE-H253)CTA-20150101$$5EXP:(DE-H253)CTA-20150101$$eCherenkov Telescope Array$$x0
000576674 7001_ $$0P:(DE-H253)PIP1091973$$aWatson, Jason John$$b1
000576674 7001_ $$0P:(DE-H253)PIP1018949$$aGiavitto, Gianluca$$b2
000576674 7001_ $$0G.Cotter.4$$aCotter, Garret$$b3
000576674 7001_ $$aWhite, Richard$$b4
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