[daip] outline for talk
Eric Greisen
egreisen at nrao.edu
Thu Sep 1 19:01:56 EDT 2005
Below is an outline (PowerPoint bullets) for the NSF software review
that I will almost certainly not give. But I offer it for comments
anyway to see if other important things should be on the list.
AIPS Group
Eric Greisen - Scientist, 75%
Amy Mioduszewski - Asst. Scientist, <= 75% (really ~ 50%)
Leonia Kogan - Scientis, 40% (+ 35% EVLA planning)
Wes Young - Software Engineer, 15% AIPS
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Lorant Sjouwerman - Assoc. Scientist, <= 50 %
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Major accomplishments in last 2 years (since proposal)
0. Support AIPS users world-wide, helping with installation and usage
problems, fixing bugs and inconveniences
1. VLBI:
APCAL - estimate opacity with weather tables
VLA as VLBA station - calibration transfer
Earth orientation Parameter - correction for poor estimates
2. VLA:
FILLM - read archive data from disk, avoid bad concatenations
Models for primary flux calibrators - Claire Chandler models
at high frequency, Amy now doing lower frequencies
3. Calibration:
DELZN - fit calibrators for clock, atmosphere
ATMCA - interpolate multiple calibrators to target
CALIB, FRING - overlapping intervals
CALIB - robust solution methods added, allows auto-flagging
4. Work toward pipelines:
VLARUN - VLA pipeline procedure, good first start
SYSTEM - new verb to do system commands from inside AIPS
FLAGR/FINDR - auto-editing tasks
RLDIF - new task to return parameter for pol. calibration
IMFIT/SETFC,others - return results to AIPS
5. Plotting - full color control of line drawing:
separate contours by spectral channel
color polarization vectors by angle
separate IFs, polarizations in point plots
6. Documentation:
CookBook kept up to date
CookBook now available in cross-linked html and pdf forms
XHELP links help files using browser also with the html and pdf
CookBook
6. Systems:
Mac OS/X - AIPS port
Binary installation: Mac w IBM, Solaris w SUN, Linux w Intel
Read-only file systems for DATs, security purposes
MNJ - updates systems area, POPS automatically
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Slide showing the shipping data
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Current VLA Pipeline "VLARUN"
calvlarun: (SNPLT between steps)
SETJY - clear then calculate for flux calibrators
CALIB - P solution on all calibrators
CLCAL - move above to CL table
CALIB - apply previous cal, average, do A&P
GETJY - convert gains of all cals to same scale
CLCAL - apply above to CL table
If (line work) then
copy tables to line data
BPASS - find bandpass calibration
POSSM - plot bandpass calibration
TASAV - save tables to null file
imavlarun:
SPLIT - apply calibration
For each source in dataset (read SU table to find)
IMAGR - each IF separately in line data
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