Pulse Brain · Growing Health Evidence Index
Peer-reviewed

Early results from GRBAlpha and VZLUSAT-2

J. Řípa, András Pál, M. Ohno, Norbert Werner, László Mészáros, B. Csák, Marianna Dafcikova, Vladimír Dániel, Juraj Dudáš, Marcel Frajt, Péter Hanák, Ján Hudec, Milan Junas, Jakub Kapus, Miroslav Kasal, Martin Koleda, Robert László, Pavol Lipovský, F. Münz, Maksim Rezenov, Miroslav Šmelko, Petr Svoboda, H. Takahashi, M. Topinka, Tomáš Urbanec, Jean-Paul Breuer, Teruaki Enoto, Z. Frei, Y. Fukazawa, Gábor Galgóczi, Filip Hroch, Yuto Ichinohe, L. L. Kiss, Hiroto Matake, Tsunefumi Mizuno, Kazuhiro Nakazawa, Hirokazu Odaka, H. Poon, Nagomi Uchida, Yuusuke Uchida

Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray · 2022

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Summary

We present the detector performance and early science results from <i>GRBAlpha</i>, a 1U CubeSat mission, which is a technological pathfinder to a future constellation of nanosatellites monitoring gamma-ray bursts (GRBs). <i>GRBAlpha</i> was launched in March 2021 and operates on a 550 km altitude sun-synchronous orbit. The gamma-ray burst detector onboard <i>GRBAlpha</i> consists of a 75×75×5 mm CsI(Tl) scintillator, read out by a dual-channel multi-pixel photon counter (MPPC) setup. It is sensitive in the ∼30−900 keV range. The main goal of <i>GRBAlpha</i> is the in-orbit demonstration of the detector concept, verification of the detector’s lifetime, and measurement of the background level on low-Earth orbit, including regions inside the outer Van Allen radiation belt and in the South At

Source type
Peer-reviewed study
DOI
10.1117/12.2629332
Catalogue ID
SNmoic298q-inhnhq
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