Description
Perform a test. The dataset used is an observation of 3C273 at 8GHz
using the C-configuration of the VLA. It is part of the
AIPS++ distribution.
Note that if doshift is set to T then the imaging is done in
Galactic coordinates.
The test does the following:
- The uvfits file that is to be read in is
in a standard place in the AIPS++ code source area.
- The MeasurementSet is read from the uvfits file.
- A summary of what exists is logged.
- The data are weighted using the Briggs algorithm.
- An initial CLEAN-only deconvolution is performed, and then restored.
- A CLEAN mask is constructed by thresholding I > 0.015
- The deconvolution is repeated with
masks enabled.
- Residual images are calculated for the North Celestial pole,
on the Sun, and for azimuth elevation (0d, 0d).
Returns
Bool
Arguments
| size |
|
Number of pixels on a side |
|
|
Allowed: |
Int |
|
|
Default: |
128 |
| cleanniter |
|
Number of clean iterations |
|
|
Allowed: |
Int |
|
|
Default: |
1000 |
| cleangain |
|
Clean loop gain |
|
|
Allowed: |
Float |
|
|
Default: |
0.1 |
| doshift |
|
Shift the phase center |
|
|
Allowed: |
Bool |
|
|
Default: |
T |
| doplot |
|
Plot? |
|
|
Allowed: |
Bool |
|
|
Default: |
T |
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