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Journal article

Calibration and Simulation of the GRB trigger detector of the Ultra Fast Flash Observatory

From

National United University Taiwan1

University of Valencia2

Ewha Womans University3

Sungkyunkwan University4

Yonsei University5

Lomonosov Moscow State University6

University of Paris-Sud - University of Paris XI7

National Space Institute, Technical University of Denmark8

Astrophysics, National Space Institute, Technical University of Denmark9

Instituto de Astrofísica de Andalucía10

National Space Organization11

National Taiwan University12

Korea Institute of Industrial Technology13

Korea Advanced Institute of Science and Technology14

...and 4 more

The UFFO (Ultra-Fast Flash Observatory) is a GRB detector on board the Lomonosov satellite, to be launched in 2013. The GRB trigger is provided by an X-ray detector, called UBAT (UFFO Burst Alarm & Trigger Telescope), which detects X-rays from the GRB and then triggers to determine the direction of the GRB and then alerts the Slewing Mirror Telescope (SMT) to turn in the direction of the GRB and record the optical photon fluxes.

This report details the calibration of the two components: the MAPMTs and the YSO crystals and simulations of the UBAT. The results shows that this design can observe a GRB within a field of view of ±35° and can trigger in a time scale as short as 0.2 – 1.0 s after the appearance of a GRB X-ray spike.

Language: English
Year: 2013
Pages: 531-535
ISSN: 16381963 and 16334760
Types: Journal article
DOI: 10.1051/eas/1361086
ORCIDs: Brandt, Søren , Budtz-Jørgensen, Carl and Lund, Niels

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