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The Slewing Mirror Telescope and the Data-Acquisition System for the UFFO-Pathfinder
Author(s) -
H. Lim,
S. Ahmad,
P. Barrillon,
S. Brandt,
C. BudtzJørgensen,
A. J. Castro–Tirado,
Pisin Chen,
Yeonju Choi,
P. Connell,
S. Dagoret-Campagne,
C. J. Eyles,
B. Grossan,
M. Huang,
A. Jung,
S. Jeong,
H.S. Kim,
M.B. Kim,
S.-W. Kim,
Y.W. Kim,
A.S. Krasnov,
J. Lee,
Eric V. Linder,
T.-C. Liu,
N. Lund,
K. W. Min,
G.W. Na,
J. W. Nam,
M. I. Panasyuk,
I.H. Park,
J. Řípa,
V. Reglero,
J.M. Rodrigo,
George F. Smoot,
J. E. Suh,
С. И. Свертилов,
N. Vedenkin,
M.-Z. Wang,
I. V. Yashin
Publication year - 2013
Publication title -
eas publications series
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.199
H-Index - 24
eISSN - 1638-1963
pISSN - 1633-4760
DOI - 10.1051/eas/1361087
Subject(s) - pathfinder , physics , telescope , gamma ray burst , observatory , aperture (computer memory) , field of view , photon , optics , detector , optical telescope , astronomy , computer science , library science , acoustics
The Ultra-Fast Flash Observatory (UFFO) aims to detect the earliest moment of Gamma-Ray Bursts (GRBs) which is not well known, resulting into the enhancement of GRB mechanism understand- ing. The pathfinder mission was proposed to be a scaled-down version of UFFO, and only contains the UFFO Burst Alert & Trigger Telescope (UBAT) measuring the X-ray/gamma-ray with the wide-field of view and the Slewing Mirror Telescope (SMT) with a rapid-response for the UV/optical photons. Once the UBAT detects a GRB candidate with the position accuracy of 10 arcmin, the SMT steers the UV/optical pho- tons from the candidate to the telescope by the fast rotatable mirror and provides the early UV/optical photons measurements with 4 arcsec

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