| VS07g Results
Submitted checklist.txt and checklist.tex is also available |
[Summary | AIPS | Difmap ] |
| Abstract
Strong fringes were easily detected on ground-ground baselines except those to Kashima. Only small part of Kashima data was used for imaging. Hobart gains were multiplied by a factor of ~0.6 to match the adopted DPFU of 0.1 and the measured Tsys of ~300K. There were delay gaps when the tracking stations changed each time. For ground-space baselines, good fringes were found up to ~22:30 (UT) which included part of the TZ pass and an entire GZ pass. For NZ pass from 22:33 (UT) to 22:50 (UT), only some very weak fringes were detected (consistent with the correlator report) and these data were eventually flagged. Both imaging and modelfitting were made to the survey source J1658+07. A single elliptical Gaussian model was applied to fit the calibrator 1622-253. |
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 (100 kb) GIF (8 kb) |
Ampl, Phase vs Time PS (429 kb) GIF 1, 2, 3, 4 |
(u,v) Coverage PS (52 kb) GIF (5 kb) | Closure Phase vs Time PS (617 kb) GIF 1, 2, 3 |
Clean Image PS (55 kb) GIF (66 kb) |
| Modelfit | ||||
| Ampl, Phase vs (u,v) Distance PS (100 kb) GIF (8 kb) |
Ampl, Phase vs Time PS (429 kb) GIF 1, 2, 3, 4 |
(u,v) Coverage PS (52 kb) GIF (5 kb) | Closure Phase vs Time PS (617 kb) GIF 1, 2, 3 |
Image with model components PS (64 kb) GIF (8 kb) |
More details on the Images and Modelfits are found in this page.