Development of the imaging system of the balloon-borne gamma-ray telescope Máscara Codificada (MASCO)
Author(s) -
J. Braga,
F. D’Amico,
T. Villela,
Jorge Mejı́a,
R.A. Fonseca,
E. Rinke
Publication year - 2002
Publication title -
review of scientific instruments
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.605
H-Index - 165
eISSN - 1089-7623
pISSN - 0034-6748
DOI - 10.1063/1.1505841
Subject(s) - physics , coded aperture , optics , telescope , angular resolution (graph drawing) , detector , aperture (computer memory) , rotation (mathematics) , gamma ray , gamma ray astronomy , gamma camera , computer science , astrophysics , acoustics , mathematics , combinatorics , artificial intelligence
We report laboratory imaging results of a balloon-borne gamma-ray imaging telescope, Mascara Codificada (Portuguese for “coded mask,”) designed to obtain high angular resolution (∼14 arcmin) images of the sky in the 50 keV–1.8 MeV energy range. The instrument incorporates a coded mask with an aperture pattern based on a 19×19-element modified uniformly redundant array (MURA). This pattern belongs to a subclass of MURAs that are almost completely antisymmetrical for 90° rotations with respect to the lower-right corner of the central element, which allows the implementation of an antimask by a single rotation of the whole mask by 90°. The symmetry properties of the MURAs are discussed. The algorithm for determining the position of the gamma-ray interactions on the instrument’s main detector is described and the results of laboratory tests of the imaging system are presented. The mask–antimask subtraction, applied after a flat-fielding procedure, produced a 60% increase in the signal-to-noise ratio of a stro...
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