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000596804 088__ $$2arXiv$$aarXiv:2302.07611
000596804 1001_ $$0P:(DE-HGF)0$$aSpencer, Samuel Timothy$$b0$$eCorresponding author
000596804 1112_ $$a7th Heidelberg International Symposium on High-Energy Gamma-Ray Astronomy$$cBarcelona$$d2022-07-04 - 2022-07-08$$gGamma 2022$$wSpain
000596804 245__ $$aAdvanced Analysis of Night Sky Background Light for SSTCAM
000596804 260__ $$aTrieste$$bSISSA$$c2023
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000596804 500__ $$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
000596804 520__ $$aNight Sky Background (NSB) is a complex phenomenon, consisting of all light detected byImaging Atmospheric Cherenkov Telescopes (IACTs) not attributable to Cherenkov light emission.Understanding the effect of NSB on cameras for the next-generation Cherenkov Telescope Array(CTA) is important, as it affects the systematic errors on observations, the energy threshold, thethermal control of the cameras and the ability of the telescopes to operate under partial moonlightconditions. This capacity to observe under partial moonlight conditions is crucial for the CTAtransient science programme, as it substantially increases the potential observing time. Usingtools initially developed for H.E.S.S. (in combination with the prototype CTA analysis packagectapipe) we will present predictions for the NSB present in images taken by the CTA Small SizedTelescope Camera (SSTCAM), showing that SSTCAM will likely be able to meet the associatedCTA requirements. Additionally, we calculate the potential observing time gain by operatingunder high NSB conditions.
000596804 536__ $$0G:(DE-HGF)POF4-613$$a613 - Matter and Radiation from the Universe (POF4-613)$$cPOF4-613$$fPOF IV$$x0
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000596804 650_7 $$2INSPIRE$$aradiation: Cherenkov
000596804 650_7 $$2INSPIRE$$aenergy: threshold
000596804 650_7 $$2INSPIRE$$aCherenkov Telescope Array
000596804 650_7 $$2INSPIRE$$abackground
000596804 650_7 $$2INSPIRE$$aCherenkov counter
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000596804 650_7 $$2INSPIRE$$agamma ray: VHE
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000596804 693__ $$0EXP:(DE-H253)CTA-20150101$$5EXP:(DE-H253)CTA-20150101$$eCherenkov Telescope Array$$x0
000596804 7001_ $$0P:(DE-H253)PIP1091973$$aWatson, Jason John$$b1$$udesy
000596804 7001_ $$0P:(DE-H253)PIP1018949$$aGiavitto, Gianluca$$b2$$udesy
000596804 7001_ $$aCotter, Garret$$b3
000596804 7001_ $$aWhite, Richard$$b4
000596804 773__ $$0PERI:(DE-600)2642026-0$$a10.22323/1.417.0218$$p218$$tProceedings of Science / International School for Advanced Studies$$v(Gamma2022)$$x1824-8039$$y2023
000596804 7870_ $$0PUBDB-2023-00867$$aSpencer, Samuel Timothy et.al.$$dSissa Medialab Trieste, Italy, 2022$$iIsParent$$rarXiv:2302.07611$$tAdvanced Analysis of Night Sky Background Light for SSTCAM
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000596804 9141_ $$y2023
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