VS05h Results
Submitted checklist.txt and checklist.tex is also available |
[Summary | AIPS | Difmap ] |
Observation code | : | VS05h | AIPS Version | : | 15OCT99 | |
Date of Observation | : | 1998/72 | Difmap Version | : | 2.3c | |
Source Name | : | J1058-80 | vsop_difmap used | : | Yes | |
Calibration Source(s) | : | None | ||||
Ground telescopes | : | Hart (Mopra and Hobart not available?) | Model Fitted to data | : | No | |
Tracking Station(s) | : | TZ and GZ (not available?) | Image made | : | No | |
Correlator | : | Penticton |
Abstract
Strong fringes were easily found between Hart and HALCA. But, Mopra and Hobart data were not available. Checking on this. Also, GZ between 18:00 and 20:40 not available. TZ track from 22:12 to 01:00 was okay. Unless another ground telescope can be found, this observations should be rescheduled. Correlated flux density is about 0.7 Jy and this source becomes stronger at longer spacings!! Maybe a calibration problem or just caused by a fortuitous position angle at long spacings. ACCOR did not work for some reason. This might have helped possible amplitude problem. |
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KRING |
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1 |
AIPS Input Files
ANTAB.TXT | Comments No light-curve data available for this source. No INDXR.TXT needed as there were no gain jumps during this experiment. |
AIPS Output Files
LISTR.LIS PRTAN.LIS SNAPCAL_1.PS |
UVPLOT_UV.PS UVPLOT_UVD.PS UVPLOT_UVPA.PS |
Phase selfcal applied? | No |
Global amplitude selfcal (gscal) applied? | No |
Amplitude selfcal on non-global timescales used? | No |
Modelfit made and saved? | No |
Image Made and saved? | No |
Comments on Difmap processing
SNVER = 2 |