vs01a Results
Submitted checklist.txt and checklist.tex is also available |
[Summary | AIPS | Difmap ] |
Abstract
This survey dataset is an extraction of the GOT experiment v081b. The extraction was received on tape from Socorro containing data for five GRTs plus HALCA. All but 3 GRTs at any one time were flagged before imaging in Difmap. BR,PT,SC are used during the RZ tracking pass, and MK,PT,SC during the NZ tracking pass. In order to find weak HALCA fringes, the ground telescopes were fringed first. These solutions were applied and the resulting data was averaged in frequency and time using SPLAT. This helped increase the SNR for the weak HALCA fringes. Because of this, the GRTs in the final fringe plots have zero delays and rates, and there are two TASAV files: the final version and the tables as they were before SPLAT was applied. Suggested parameters for all AIPS tasks were used. CALIB was not run so the final SN and CL tables have non-zero phases in them. Imaging and model-fitting both went very well and produced good results. |
AIPS Input Files
UVFLG.TXT ANTAB.TXT |
Comments - None - |
AIPS Output Files
Phase selfcal applied? | No |
Global amplitude selfcal (gscal) applied? | No |
Amplitude selfcal on non-global timescales used? | No |
Modelfit made and saved? | Yes |
Image Made and saved? | Yes |
Comments on Difmap processing
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Image | ||||
Ampl, Phase vs (u,v) Distance PS (67 kb) GIF (9 kb) |
Ampl, Phase vs Time PS (311 kb) GIF 1, 2, 3, 4 |
(u,v) Coverage PS (35 kb) GIF (5 kb) | Closure Phase vs Time PS (335 kb) GIF 1, 2 |
Clean Image PS (73 kb) GIF (114 kb) |
Modelfit | ||||
Ampl, Phase vs (u,v) Distance PS (67 kb) GIF (9 kb) |
Ampl, Phase vs Time PS (312 kb) GIF 1, 2, 3, 4 |
(u,v) Coverage PS (35 kb) GIF (5 kb) | Closure Phase vs Time PS (336 kb) GIF 1, 2 |
Image with model components PS (81 kb) GIF (9 kb) |
More details on the Images and Modelfits are found in this page.