PoS - Proceedings of Science
Volume 301 - 35th International Cosmic Ray Conference (ICRC2017) - Session Gamma-Ray Astronomy. GA-instrumentation
In-Situ Calibration of UFFO/Lomonosov for Observation of GRBs
S. Jeong*, I.H. Park, V. Bogomolov, S. Brandt, C. Budtz-Jørgensen, A.J. Castro-Tirado, Y. Chang, P. Chen, C.R. Chen, H.S. Choi, P. Connell, C. Eyles, G. Gaikov, G. Garipov, J.J. Huang, H.M. Jeong, J.E. Kim, M.B. Kim, S.W. Kim, H.K. Kim, E.J. Lee, H. Lim, J.W. Nam, M.I. Panasyuk, V.V. Petrov, V. Reglero, J. Ripa, J.M. Rodrigo, S. Svertilov, I.I. Yashin, M.Z. Wang, M.H.A. Huang, C.W. Chen and H.K. Leeet al. (click to show)
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Pre-published on: August 30, 2017
Published on: August 03, 2018
The UFFO/Lomonosov has been successfully launched into Sun synchronous orbit and is operational through tests and calibrations since its launch on Apr. 28, 2016. As a pathfinder of UFFO, it will be the first space instrument to use a fast slewing mirror which reduce the trigger latency of optical telescope, less than a second, to explore early time domain of GRB evolution. In this article, we will report in detail the first mission, UFFO/Lomonosov, for the rapid response to observe early photons from GRBs in orbit.
DOI: https://doi.org/10.22323/1.301.0821
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