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@INPROCEEDINGS{Berlea:611550,
      author       = {Berlea, Vlad Dumitru and Asif, Arooj and Barschke, Merlin
                      and Berge, David and Crespo, Juan Maria Haces and Giavitto,
                      Gianluca and Kumar, Shashank and Porelli, Andrea and De
                      Simone, Nicola and Watson, Jason John and Steve, Worm and
                      Zappon, Francesco and Birman, Adi and Alfassi, Shay and
                      Fenigstein, Amos and Waxmann, Eli and Netzer, Udi and Liran,
                      Tuvia and Lapid, Ofer and Algranatti, Vikto M. and
                      Schvartzvald, Yossi},
      title        = {{P}reliminary results of the {S}ingle {E}vent {E}ffect
                      testing for the {ULTRASAT} sensors},
      journal      = {Nuclear instruments $\&$ methods in physics research /
                      Section A},
      volume       = {1068},
      issn         = {0168-9002},
      address      = {[Amsterdam]},
      publisher    = {Elsevier},
      reportid     = {PUBDB-2024-04968, arXiv:2407.03789},
      pages        = {169754},
      year         = {2024},
      abstract     = {ULTRASAT (ULtra-violet TRansient Astronomy SATellite) is a
                      wide-angle space telescope that will perform a deep
                      time-resolved all-sky survey in the near-ultraviolet (NUV)
                      spectrum. The science objectives are the detection of
                      counterparts to short-lived transient astronomical events
                      such as gravitational wave sources and supernovae. The
                      mission is led by the Weizmann Institute of Science and is
                      planned for launch in 2026 in collaboration with the Israeli
                      Space Agency and NASA. DESY will provide the UV camera,
                      composed by the detector assembly located in the telescope
                      focal plane and the remote electronics unit. The camera is
                      composed out of four back-metallized CMOS Image Sensors
                      (CIS) manufactured in the 4T, dual gain Tower process. As
                      part of the radiation qualification of the camera, Single
                      Event Effect (SEE) testing has been performed by irradiating
                      the sensor with heavy ions at the RADEF, Jyvaskyla facility.
                      Preliminary results of both Single Event Upset (SEU) and
                      Single Event Latch-up (SEL) occurrence rate in the sensor
                      are presented. Additionally, an in-orbit SEE rate simulation
                      has been performed in order to gain preliminary knowledge
                      about the expected effect of SEE on the mission.},
      month         = {May},
      date          = {2024-05-26},
      organization  = {PM2024 - 16th Pisa Meeting on Advanced
                       Detectors, Isola de Elba (Italy), 26
                       May 2024 - 1 Jun 2024},
      cin          = {$Z_DET$},
      ddc          = {530},
      cid          = {$I:(DE-H253)Z_DET-20201126$},
      pnm          = {622 - Detector Technologies and Systems (POF4-622) /
                      RADNEXT - RADiation facility Network for the EXploration of
                      effects for indusTry and research (101008126)},
      pid          = {G:(DE-HGF)POF4-622 / G:(EU-Grant)101008126},
      experiment   = {EXP:(DE-H253)ULTRASAT-20211201},
      typ          = {PUB:(DE-HGF)16 / PUB:(DE-HGF)8},
      eprint       = {2407.03789},
      howpublished = {arXiv:2407.03789},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:2407.03789;\%\%$},
      UT           = {WOS:001301406000001},
      doi          = {10.1016/j.nima.2024.169754},
      url          = {https://bib-pubdb1.desy.de/record/611550},
}