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• W2154554007 abstract "The GRAINE project (Gamma-Ray Astro-Imager with Nuclear Emulsion) has been developed for the observation of cosmic |$gamma$|-rays in the energy range 10 MeV–100 GeV with a precise (0.08|$^{circ }$| at 1–2 GeV), polarization-sensitive, large-aperture-area (⁠|$sim$|10 m|$^2$|⁠) emulsion telescope by repeated long-duration balloon flights. In 2011, the first balloon-borne experiment was successfully performed with a |$12.5 times 10$|cm|$^2$| aperture area and 4.6 hour flight duration for a feasibility and performance test. Systematic detection, energy reconstruction, and timestamping of |$gamma$|-ray events were performed across the whole area of the emulsion film, up to 45|$^{circ }$| incident zenith angle, down to 50 MeV |$gamma$|-ray energy, with 97% detection reliability, 0.2 sec timestamp accuracy, and 98% timestamp reliability. A |$gamma$|-ray data checking and calibration method was created using the |$gamma$|-rays produced in the converter. We measured the atmospheric |$gamma$|-ray flux in the energy range 50–300 MeV and obtained a first understanding of the cosmic |$gamma$|-ray background. By combining the attitude data, we established a procedure for determining the |$gamma$|-ray arrival direction in celestial coordinates. The first flight of the balloon-borne emulsion telescope confirmed its potential as a high-performance cosmic |$gamma$|-ray detector." @default.
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• W2154554007 date "2015-04-01" @default.
• W2154554007 modified "2023-10-11" @default.
• W2154554007 title "GRAINE project: The first balloon-borne, emulsion gamma-ray telescope experiment" @default.
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• W2154554007 doi "https://doi.org/10.1093/ptep/ptv046" @default.
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