GCN Circular 32815
Subject
GRB 221020A: Detection by GRBAlpha
Date
2022-10-22T14:20:07Z (2 years ago)
From
Jakub Ripa at Masaryk University <245487@mail.muni.cz>
J. Ripa (Masaryk U.), A. Pal (Konkoly Observatory), N. Werner (Masaryk
U.), M. Ohno, H. Takahashi (Hiroshima U.), L. Meszaros, B. Csak (Konkoly
Observatory), M. Dafcikova, F. Munz, N. Husarikova, J.-P. Breuer, M.
Topinka, F. Hroch (Masaryk U.), T. Urbanec, M. Kasal,�� A. Povalac (Brno
U. of Technology), J. Hudec, J. Kapus, M. Frajt (Spacemanic s.r.o), R.
Laszlo, M. Koleda (Needronix s.r.o), M. Smelko, P. Hanak, P. Lipovsky
(Technical U. of Kosice), G. Galgoczi (Wigner Research Center/Eotvos
U.), Y. Uchida, H. Poon, H. Matake (Hiroshima U.), N. Uchida
(ISAS/JAXA), T. Bozoki (Eotvos U.), G. Dalya (Eotvos U.), T. Enoto
(Kyoto U.), Zs. Frei (Eotvos U.), G. Friss (Eotvos U.), Y. Fukazawa, K.
Hirose (Hiroshima U.), S. Hisadomi (Nagoya U.), Y. Ichinohe (Rikkyo U.),
K. Kapas (Eotvos U.), L. L. Kiss (Konkoly Observatory),�� T. Mizuno
(Hiroshima U.), K. Nakazawa (Nagoya U.), H. Odaka (Univ of Tokyo), J.
Takatsy (Eotvos U.), K. Torigoe (Hiroshima U.), N. Kogiso, M. Yoneyama
(Osaka Metropolitan U.), M. Moritaki (U. Tokyo), T. Kano (U. Michigan)
-- the GRBAlpha collaboration.
The long-duration GRB 221020A (Fermi-GBM detection: Fermi GBM Team, GCN
Circ. 32806) was detected by the GRBAlpha 1U CubeSat (Pal et al. Proc.
SPIE 2020).
The 11.3 sigma detection was confirmed at the peak time 2022-10-20
05:23:59.8 UTC. The GRB has a T90 duration of 15 s.
The light curve obtained by GRBAlpha is available here:
https://grbalpha.konkoly.hu/static/share/GRB221020A_GCN_GRBAlpha.pdf
GRBAlpha, launched on 2021 March 22, is a demonstration mission for a
future CubeSat constellation (Werner et al. Proc. SPIE 2018). Its
detector consists of a 75 x 75 x 5 mm^3 CsI(Tl) scintillator read out by
a SiPM array, covering the energy range from ~50 keV to ~1000 keV. To
increase the duty cycle and the downlink rate, we are continuously
upgrading the on-board data acquisition software stack. The ground
segment is also supported by the radio amateur community and it takes
advantage of the SatNOGS network for increased data downlink volume.