Centre d'Etude Spatiale
des Rayonnements
Département
Hautes-Energies
The SIGMA imaging principle
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The elements of the coded mask have a transparency 0 or 1.
The position detector receives the flux from the sky modulated by the mask.
So a point-like source situed at infinity projects a gamma-ray light and shadow pattern
on the detector which is characteristic of the source position in the sky
The mask is built with a 31x29 Uniformly Redundant Array : The mask is limited
to 53x49 in order to avoid ambiguities.
* The part of the sky that projects the full mask pattern is named completely
coded field of view and its dimension is 4 degrees 45' x 4 degrees 20'.
* Beyond there is the partially coded field of view.
Its dimension is 18 degrees x 16 degrees.
A point-like source projects an incomplete mask pattern on the detector.
The sensitivity becomes weaker as the source is further from the axis of the telescope.
The position of a source is determined by comparing the observed pattern with all possible projections.
A pattern projected by a source in a given direction is completely different
from the one projected by any other source.
So it is possible to reconstruct mathematically the image of a source from the pattern
projected on the detector.
.Image projected on the detector
image:images/image.before.decoding.gif[]
.Image reconstructed
image:images/image.after.decoding.gif[]