001     576674
005     20231023210341.0
024 7 _ |a Spencer:2022cqu
|2 INSPIRETeX
024 7 _ |a inspire:2632897
|2 inspire
024 7 _ |a arXiv:2302.07611
|2 arXiv
024 7 _ |a 10.3204/PUBDB-2023-00867
|2 datacite_doi
037 _ _ |a PUBDB-2023-00867
041 _ _ |a English
088 _ _ |a arXiv:2302.07611
|2 arXiv
100 1 _ |a Spencer, Samuel Timothy
|0 S.T.Spencer.1
|b 0
|e Corresponding author
245 _ _ |a Advanced Analysis of Night Sky Background Light for SSTCAM
260 _ _ |c 2022
336 7 _ |a Preprint
|b preprint
|m preprint
|0 PUB:(DE-HGF)25
|s 1698049622_232149
|2 PUB:(DE-HGF)
336 7 _ |a WORKING_PAPER
|2 ORCID
336 7 _ |a Electronic Article
|0 28
|2 EndNote
336 7 _ |a preprint
|2 DRIVER
336 7 _ |a ARTICLE
|2 BibTeX
336 7 _ |a Output Types/Working Paper
|2 DataCite
500 _ _ |a PoS(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
520 _ _ |a Night 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.
536 _ _ |a 613 - Matter and Radiation from the Universe (POF4-613)
|0 G:(DE-HGF)POF4-613
|c POF4-613
|f POF IV
|x 0
588 _ _ |a Dataset connected to INSPIRE
650 _ 7 |a radiation, Cherenkov
|2 INSPIRE
650 _ 7 |a energy, threshold
|2 INSPIRE
650 _ 7 |a Cherenkov Telescope Array
|2 INSPIRE
650 _ 7 |a background
|2 INSPIRE
650 _ 7 |a Cherenkov counter
|2 INSPIRE
650 _ 7 |a thermal
|2 INSPIRE
650 _ 7 |a imaging
|2 INSPIRE
650 _ 7 |a HESS
|2 INSPIRE
693 _ _ |0 EXP:(DE-H253)CTA-20150101
|5 EXP:(DE-H253)CTA-20150101
|e Cherenkov Telescope Array
|x 0
700 1 _ |a Watson, Jason John
|0 P:(DE-H253)PIP1091973
|b 1
700 1 _ |a Giavitto, Gianluca
|0 P:(DE-H253)PIP1018949
|b 2
700 1 _ |a Cotter, Garret
|0 G.Cotter.4
|b 3
700 1 _ |a White, Richard
|b 4
856 4 _ |y OpenAccess
|u https://bib-pubdb1.desy.de/record/576674/files/2302.07611v2.pdf
856 4 _ |y OpenAccess
|x pdfa
|u https://bib-pubdb1.desy.de/record/576674/files/2302.07611v2.pdf?subformat=pdfa
909 C O |o oai:bib-pubdb1.desy.de:576674
|p openaire
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910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 1
|6 P:(DE-H253)PIP1091973
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 2
|6 P:(DE-H253)PIP1018949
913 1 _ |a DE-HGF
|b Forschungsbereich Materie
|l Matter and the Universe
|1 G:(DE-HGF)POF4-610
|0 G:(DE-HGF)POF4-613
|3 G:(DE-HGF)POF4
|2 G:(DE-HGF)POF4-600
|4 G:(DE-HGF)POF
|v Matter and Radiation from the Universe
|x 0
915 _ _ |a OpenAccess
|0 StatID:(DE-HGF)0510
|2 StatID
915 _ _ |a Published
|0 StatID:(DE-HGF)0580
|2 StatID
915 _ _ |a Creative Commons Attribution-NonCommercial-NoDerivs CC BY-NC-ND 4.0
|0 LIC:(DE-HGF)CCBYNCND4
|2 HGFVOC
920 1 _ |0 I:(DE-H253)Z_EL-20210408
|k Z_EL
|l Elektronik
|x 0
980 _ _ |a preprint
980 _ _ |a VDB
980 _ _ |a UNRESTRICTED
980 _ _ |a I:(DE-H253)Z_EL-20210408
980 1 _ |a FullTexts


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