Fig. 10
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Light curve of GRB 1901l4C with the data of all SPI detectors summed. The filled area marks the active time of the GRB. Due to the detection of this GRB by MAGIC in the TeV energy range (MAGIC Collaboration 2019), this would be a very interesting source to analyse with the SPI data, if an out-oſ-cFoV response will be constructed in the future.
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