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@ARTICLE{Spencer:596804,
      author       = {Spencer, Samuel Timothy and Watson, Jason John and
                      Giavitto, Gianluca and Cotter, Garret and White, Richard},
      title        = {{A}dvanced {A}nalysis of {N}ight {S}ky {B}ackground {L}ight
                      for {SSTCAM}},
      journal      = {Proceedings of Science / International School for Advanced
                      Studies},
      volume       = {(Gamma2022)},
      issn         = {1824-8039},
      address      = {Trieste},
      publisher    = {SISSA},
      reportid     = {PUBDB-2023-06291, arXiv:2302.07611},
      series       = {2632897},
      pages        = {218},
      year         = {2023},
      note         = {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},
      abstract     = {Night 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.},
      month         = {Jul},
      date          = {2022-07-04},
      organization  = {7th Heidelberg International Symposium
                       on High-Energy Gamma-Ray Astronomy,
                       Barcelona (Spain), 4 Jul 2022 - 8 Jul
                       2022},
      keywords     = {radiation: Cherenkov (INSPIRE) / energy: threshold
                      (INSPIRE) / Cherenkov Telescope Array (INSPIRE) / background
                      (INSPIRE) / Cherenkov counter (INSPIRE) / thermal (INSPIRE)
                      / imaging (INSPIRE) / gamma ray: VHE (INSPIRE) / HESS
                      (INSPIRE)},
      cin          = {ZEU-EL},
      ddc          = {530},
      cid          = {I:(DE-H253)ZEU-EL-20120731},
      pnm          = {613 - Matter and Radiation from the Universe (POF4-613)},
      pid          = {G:(DE-HGF)POF4-613},
      experiment   = {EXP:(DE-H253)CTA-20150101},
      typ          = {PUB:(DE-HGF)8 / PUB:(DE-HGF)16},
      eprint       = {2302.07611},
      howpublished = {arXiv:2302.07611},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:2302.07611;\%\%$},
      doi          = {10.22323/1.417.0218},
      url          = {https://bib-pubdb1.desy.de/record/596804},
}