Special NAUG - 2007-Jan-03
Progress/Status EVLA TST
-
calibrator models - high frequency images are available; currently, the images are stored and are scaled appropriately for their band - we will work on enabling an OTF scaling to the appropriate frequency:
Calibrator |
Q |
K |
U |
C |
X |
L |
3C48 0137+331 (J2000) 0134+329 (B1950) |
X |
X |
X |
X |
X |
X |
3C138 0521+166 (J2000) 0518+165 (B1950) |
X |
X |
X |
X |
X |
X |
3C147 0542+498 (J2000) 0538+498 (B1950) |
X |
X |
X |
- |
- |
X |
3C286 1331+305 (J2000) 1328+307 (B1950) |
X |
X |
X |
X |
X |
X |
- data selection - Will keep the index specifiers (fieldid, etc) for now.
fieldid:---> field: takes a single string (spaces separate the names of the fields)
it does a minimum match on each string so:
field='133'
field='1331+305'
field='1331+30500002_0' (Field Name reported in listobs)
are all equivalent
Multiple fields are specified as:
field='133 144'
will get you fields: 1331+30500002_0, 1445_09900002_0
Implemented in: clean, contsub, exportuvfits, flagdata, flagxy, ft, invert,
mosaic, plotxy, setjy, split
-
-
- added field,spwid (to eventually replace msselect) in:
- bandpass, blcal, correct, fringecal, gaincal, pointcal, uvmodelfit
- Refant now refers to antenna name; Note: still needs calplot to use antenna names not indices
- bandpass, blcal, fringecal, gaincal, pointcal
-
error trapping within tasks 20070105
- makemask task - support for clean boxes - Do we still need a makemask task?
- added cleanbox parameter to clean, mosaic;
- this will take a list (or list of lists):
- cleanbox=[blcx,blcy,trcx,trcy]
- cleanbox=[[blcx,blcy,trcx,trcy],[blcx,blcy,trcx,trcy],...]
- cleanbox=filename
- compliant with clean boxes in AIPS BOXFILE parameter - Note: can not currently handle the different 'cards' (C,F,W, etc).
- accepts a file like:
# fieldname blc-x blc-y trc-x trc-y -- as in AIPS BOXFILE
0 60 60 75 75 # or
0 18:30:24.0 -05.15.00 18:30:26.0 -05:15:15
- Task History
- remove tool level history (okay?)
- add task level history
- ms - clearcal, contsub, correct, flagautocorr, flagdata, fluxscale, ft, importvla, importasdm, importuvfits, setjy, split,
- image - clean, feather, invert, mosaic
CASA 2007 Calendar
- Update: Crystal will be in Socorro from Feb 4 to Feb
- Question: Does this cover your flagging interactions; if not, please state it.
- Question: What algorithms should be ported from AIPS first?
- Interface
- data selection by:
- antennanames (antennaid), spwid, fieldnames (fieldid), uvdist, time, correlation, (nchan, start, width)
- any other parameters needed?
- manual flagging:
- antenna, autocorrelation, baseline, fieldnames, spwid, channels, freqs, timerange, timeslot, clip, quack, unflag
- other parameters?
- algorithms
- timemedian, freqmedian, spectralrejection, uvbin
- what others first?
- summary/statistics
- get percentage of data flagged vs antenna, baseline, spwid, channel, correlations, time
- other statistics?
- queries
- return list of antennas, channels, baselines, times with more or less than a specified percentage of flagged data.
- extend flags
- use queries to extend flags (e.g, flag all channels that have more than 70% of the data flagged)
- extend flag scope
- extend by time, channel, baseline, polarization, spwid, spectral/time averages
- other functions
- flag history - append to history file
- flag reset - reset flags
--
JosephMcMullin - 10 Jan 2007