Output from grid_tests.py (described in section 5.2 of the memo)
The table below contains the output from the script grid_tests.py, which shows how the beamsize, peak intensity and flux densities vary with the number of pixels per beam for four different choices of support width for the gridding function.
Clicking on the thumbnail image for a Band/Antenna combination will take you to a separate page where all the images for that combination are displayed. Alternatively, you can view all plots collected in a 43-page PDF.
Mars Band 3
3c279 Band 3
Mars Band 6
Uranus Band 7
SF
GJINC
Comparison of TICRA models with astroholography images (described in section 3.3 of the memo)
The table below contains the XX polarization images from the 2013 astroholography campaign compared to the TICRA H-polarization model. The images were taken from the scops cluster in the directory: /mnt/scops/data/data/dgunawan/PrimaryBeams.
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DA
DV
PM
Band
TICRA image
holography image
TICRA image
holography image
TICRA image
holography image
3
6
7
Comparison of profiles from TICRA models and astroholography images (as described in section 3.3 of the memo)
Clicking on the thumbnail image for a Band/Antenna combination will take you to a separate page where all the images for that combination are displayed.