New readout and data-acquisition system in an electron-tracking Compton camera for MeV gamma-ray astronomy (SMILE-II)
Tetsuya Mizumoto, Yoshihiro Matsuoka, Yoshitaka Mizumura, Toru, Tanimori, Hidetoshi Kubo, Atsushi Takada, Satoru Iwaki, Tatsuya Sawano,, Kiseki Nakamura, Shotaro Komura, Shogo Nakamura, Tetsuro Kishimoto, Makoto, Oda, Shohei Miyamoto, Taito Takemura, Joseph D. Parker, Dai Tomono

TL;DR
This paper presents a new data-acquisition system for an electron-tracking Compton camera designed for MeV gamma-ray astronomy, significantly improving data handling and detection efficiency for balloon-borne observations.
Contribution
The paper introduces a novel data-acquisition system with parallel data flow and a new data-handling algorithm, enabling efficient management of large data volumes and improved track detection efficiency.
Findings
Achieved a 100-fold increase in detection area without added weight or power.
Enhanced TPC track detection efficiency from ~10% to ~100%.
Successfully managed increased data rates during balloon observations.
Abstract
For MeV gamma-ray astronomy, we have developed an electron-tracking Compton camera (ETCC) as a MeV gamma-ray telescope capable of rejecting the radiation background and attaining the high sensitivity of near 1 mCrab in space. Our ETCC comprises a gaseous time-projection chamber (TPC) with a micro pattern gas detector for tracking recoil electrons and a position-sensitive scintillation camera for detecting scattered gamma rays. After the success of a first balloon experiment in 2006 with a small ETCC (using a 101015 cm TPC) for measuring diffuse cosmic and atmospheric sub-MeV gamma rays (Sub-MeV gamma-ray Imaging Loaded-on-balloon Experiment I; SMILE-I), a (30 cm) medium-sized ETCC was developed to measure MeV gamma-ray spectra from celestial sources, such as the Crab Nebula, with single-day balloon flights (SMILE-II). To achieve this goal, a 100-times-larger…
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