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Two kinds of restoration algorithms for wobbler switched data are
available: The EKH [Emerson et al. 1979] and shift-and-add algorithms. EKH is
much more elaborated and it enables to recover all the source structure as
long as the source stays undetected at the edges of the map along the
scanning direction. However, it works well only for relatively small source
size (i.e.
). Now, there are scientific projects
which search for point sources (at least sources whose size is smaller than
the half wobbler throw) on much larger sky areas. For these (i.e. search
for point sources on very large field of views), the shift-and-add
restoration method works well.
We thus offer the user the following choice:
- EKH restoration
- The PI must give the source size in both
perpendicular directions:
. The PI can
request
unrelated sources in this mode (the sources must share
the same pointing calibrator...).
- Shift-and-add restoration
- The PI must give the sizes of the final
mosaic:
. We then assume that this area will
be observed in square submaps, whose typical duration is set to
so that
is an integer number. If we define
, we then find the size
through the following equation:
|
(15) |
This second order equation has a single physical solution
|
(16) |
There are then two cases:
- If
, then we use the user
inputs:
- Else we use:
We note that in this case,
is not a real number of sources
in this case. It is a number of submap and it thus does not need to be
an integer.
Next: Associated noise
Up: Mapping
Previous: Observing strategy
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Gildas manager
2014-07-01