vs03o Results
Submitted checklist.txt and checklist.tex is also available |
[Summary | AIPS | Difmap ] |
Abstract
This survey dataset is an extraction of the GOT experiment v085q. The extraction was received on tape from Socorro containing data from the EB, HN, NL, and SC GRTs plus HALCA, over a 3 hour time range. The NL data was flagged before imaging in Difmap. 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. 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 this source was difficult with only 3 GRTs. Fringes were found to HALCA over only ~1/2 of the 3 hour time range. While an image with all 4 GRTs recovers the source structure, flagging any of the remaining GRTs significantly worsens the image. |
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 (27 kb) GIF (6 kb) |
Ampl, Phase vs Time PS (200 kb) GIF 1, 2, 3 |
(u,v) Coverage PS (16 kb) GIF (4 kb) | Closure Phase vs Time PS (239 kb) GIF 1, 2 |
Clean Image PS (38 kb) GIF (62 kb) |
Modelfit | ||||
Ampl, Phase vs (u,v) Distance PS (27 kb) GIF (6 kb) |
Ampl, Phase vs Time PS (202 kb) GIF 1, 2, 3 |
(u,v) Coverage PS (16 kb) GIF (4 kb) | Closure Phase vs Time PS (237 kb) GIF 1, 2 |
Image with model components PS (37 kb) GIF (7 kb) |
More details on the Images and Modelfits are found in this page.