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Subsections
- Scientific completeness
- This remains the primary driver in
synthesis development. Significant synthesis capabilities exist within
the package at present, and are being more widely used in the
scientific community with each release. This process can be aided by
continued improvement in vertical integration of synthesis
applications, and in the addition of scientific completeness beyond
current capabilities.
- Time-critical local priorities
- It is important that the project
meet time-critical targets required for successful AIPS++ use at
consortia sites, particularly where the use of AIPS++ is closely
integrated into the critical path required for instrument use or
operation.
- Basic automated imaging
- Significant work in this area took
place in v1.4, but needs to continue in this development cycle to
include the highest level tools in this area.
- Automated testing
- Expanding the automated testing of synthesis
capabilities using simulated data is a priority during this cycle,
both at the C++ and Glish level. This has benefits in speeding up
release testing, and in daily and weekly checks of system integrity
for end-users and user test groups.
- BIMA filler migration
- Migrate the BIMA filler to MS v2. (PT, H, 3 wk).
- MS v2 FITS definition
- Complete definition of MS v2 in an
external FITS binary table format. (GM, H, 2 wk).
- Additional VLA filler features
- Add: (i) shadowing; (ii) Tsys
and weighting; (iii) complete output filtering; (iv) new weights
scheme currently adopted by FILLM. (RM, H, 4 wk).
- MS data volume control
- Implement initial solution to the MS data volume
problem caused by the MODEL_DATA, CORRECTED_DATA and IMAGING_WEIGHT
scratch columns. (AK, H, 1 wk).
- Automated editing
- Complete initial automated editing
algorithms, including spectral rejection. (OS, H, 8 wk).
- Investigate coupled solver for ATCA
- Complete investigate a coupled
solver for ATCA data. Includes a comparison with MIRIAD. (AK, H, 2 wk).
- Complete integration of calibration table re-gridding
- Complete
integration of existing table smoothing and re-gridding tool. (AK, H, 2 wk, HR, H, 2 wk, DM, H, 1 wk).
- Ephemeris-based planet flux density calibration
- Enable flux
density calibration based on planet observations, as currently done in
Miriad. (RP, M, 4wk).
- Holography support in imager
- Complete general holography support
in imager, excluding near-field corrections. (JB, H, 4 wk).
- Optimal-sized FFT's for mosaicing
- Complete the implementation
of optimal-sized FFT's for mosaiced imaging. (MH, H, 2 wk).
- Simulator error models
- Expand the analytic error models in the
simulator for use in correctness testing. Also, complete initial
support of pointing errors(MH, H, 3 wk).
- Automated imaging prototype
- Provide an initial automated
imaging utility, automap.g. (AK, H, 2 wk).
- Pipeline scientific requirements
- Complete the scientific
requirements document for common pipeline architectures. (AK, H, 1 wk).
- New Getting Results chapters
- Add new Getting Results chapters
for synthesis reduction for specific instruments, including VLA and
BIMA. (AK H, 1 wk, RP, H, 1 wk, DM, H, 1 wk).
- Synthesis tests
- Expand test scripts for all consortium
connected-element instruments (VLA, ATNF). (GM, H, 2 wk, DM, H, 6
wk, RP, H, 2 wk).
- Errors in componentlist tables
- Add support for simple errors
(one per existing parameter) in componentlist tables. (RM, H, 1
wk).
- Ionosphere support in calibrater
- Complete FJones support in
calibrater, including: i) finalize FVisJones classes; ii) test
PIM-based corrections with WSRT data; and, iii) add secondary PIM
corrections. (OS, H, 6 wk).
- imager tests against simulated data
- Add imager tests against
simulated data for all imaging modes to imagertest, and assay. (GM, H, 3 wk).
- VLBI FITS-IDI filler
- Finalize existing FITS IDI filler. (BM, H, 6 wk).
- Initial fringe-fitter
- Complete initial single-band, coherent
fringe fitter. (GM, H, 4 wk).
- Mosaic and wide-field demonstrations
- Complete demonstration
scripts for mosaic, and wide-field imaging. (MH, H, 2 wk).
- Improved total-power support in mosaicing
- (MH, H, 4wk).
- calibrater infrastructure
- Complete calibrater infrastructure
development in interpolation and parametrized solvers (AK, H, 4 wk).
- Custom synthesis GUI
- Initial custom synthesis GUI. Includes
variants for individual instruments (AK, H, 2 wk, DM, M, 2 wk).
- ATCA filler enhancements
- i) birdies; ii) syscal flagging; iii)
Hanning smoothing; iv) shadowing; v) documentation (MW, M, 3
wk).
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Up: AIPS++ DEVELOPMENT PLAN: Release 1.5
Previous: Single-dish
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2006-08-01