VS03m Results
Submitted checklist.txt and checklist.tex is also available |
[Summary | AIPS | Difmap ] |
Abstract
Good fringes were found to Halca as well as ground antennas. Amplitude self-calibration was not carried out since there was no co-observing time for all 4 stations. As a result, imaging was done with phase self-calibration only. A three Gaussian components model was used to fit the calibrated data. Calibrator (1334-127) was only detected on one ground baseline (HartRAO -- Mop) of 9,000km with a correlated flux density of 0.75Jy, too low compared to the PLS results of 5.0Jy at 7,200km. |
AIPS Input Files
INDXR.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
|
Image | ||||
Ampl, Phase vs (u,v) Distance PS (42 kb) GIF (7 kb) |
Ampl, Phase vs Time PS (132 kb) GIF 1, 2 |
(u,v) Coverage PS (23 kb) GIF (4 kb) | Closure Phase vs Time PS (93 kb) GIF 1 |
Clean Image PS (38 kb) GIF (52 kb) |
Modelfit | ||||
Ampl, Phase vs (u,v) Distance PS (42 kb) GIF (7 kb) |
Ampl, Phase vs Time PS (131 kb) GIF 1, 2 |
(u,v) Coverage PS (23 kb) GIF (4 kb) | Closure Phase vs Time PS (93 kb) GIF 1 |
Image with model components PS (39 kb) GIF (9 kb) |
More details on the Images and Modelfits are found in this page.