18 | | Place project meeting minutes here. |
19 | | |
20 | | Preferably write them as you go! |
| 18 | * CABB systemps can be affected by RFI and/or problem channels, can't currently fix this problem |
| 19 | * systemps most important when imaging |
| 20 | * ATLOD can now revert to raw counts instead of online-calculated tsys, and can then recalculate after flux calibration with attsys before imaging |
| 21 | * recalculation of XY phases on reference antenna is still troublesome |
| 22 | * perhaps get online calculations to be more robust to interference to mitigate this problem |
| 23 | * pgflag bug reports have been acted upon and fixed |
| 24 | * mirflag binary and doc files can just be "dropped in" to the correct places in Miriad tree and will hence be distributed in standard distribution |
| 25 | * would be useful if mirflag can work with phases, Emil thinks this is possible |
| 26 | * polarisation with CABB: |
| 27 | * imrm can't work with cubes, would be handy if it could work |
| 28 | * Dave finds that at 6cm over 2 GHz, the leakages change across the band, but impact of this is uncertain |
| 29 | * it may be desirable for gp tasks to be transferred to mf tasks, but how much effort should be invested in this? |
| 30 | * working panel will deliberate on questions re: Miriad's future |
| 31 | * write a discussion paper for the next ATUC meeting |
| 32 | * astro group will be consulted after 23rd November |
| 33 | * Miriad is becoming a CABB calibration engine, and less useful for wideband imaging |
| 34 | * CASA has plenty of issues still, needs testing and debugging |
| 35 | * ASKAPsoft may also be useful, but needs to be accessible |