2022
DOI: 10.1016/j.asr.2021.12.028
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Development of a cosmic ray oriented trigger for the fluorescence telescope on EUSO-SPB2

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Cited by 10 publications
(7 citation statements)
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“…Each PDM is covered with a BG3 filter 1 to limit its sensitivity to the UV region (290-430 nm) and reduce the background of photon counts outside this optimal frequency band. The trigger [4] operates individually on each PDM. The 6912-pixel camera consists of 3 such PDMs.…”
Section: The Fluorescence Telescope (Ft)mentioning
confidence: 99%
“…Each PDM is covered with a BG3 filter 1 to limit its sensitivity to the UV region (290-430 nm) and reduce the background of photon counts outside this optimal frequency band. The trigger [4] operates individually on each PDM. The 6912-pixel camera consists of 3 such PDMs.…”
Section: The Fluorescence Telescope (Ft)mentioning
confidence: 99%
“…Nine of these ECs are connected to xilinx FPGA to form a PDM with 36 MAPMTs and 2,304 total pixels. Each PDM has a square field of view of roughly 12 o x12 o and can trigger internally [6]. The three PDMs (shown in top panel of fig.…”
Section: The Instrumentmentioning
confidence: 99%
“…Due to limited telemetry, the identified event candidates will be prioritized using machine learning techniques. Details of the trigger and the prioritization can be found in [5,7]. Additionally, EUSO-SPB2 will search for the candidate upward-going events similar to the ones reported by the Antarctic Impulse Transient Antenna (ANITA) [8] but with even steeper emergence angles.…”
Section: Uhecr Via Fluorescence Techniquementioning
confidence: 99%