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- 1.
- Complete the FITS-IDI filler: Including: i) support for all
required MS sub-tables; ii) VLBA correlator quantization corrections;
iii) testing with SMA and VLBA data. Work with SMA in these
tasks. (GM, H, 2 wk).
- 2.
- BIMA filler revisions: Continued improvements in the BIMA
filler. (RP, H, 1 wk).
- 3.
- Multi-MS support in imager and calibrater: Make existing
multi-MS support available in the calibrater and imager tools. (KG, H, 3 wk).
- 4.
- Support for variable spw: Ensure proper functioning of the
synthesis tools with variable-shaped spectral windows. Includes
resolution of all current defects in this area (KG, H, 2 wk).
- 5.
- Implement initial compressed data format: Implement initial
solution to the MS data volume problem caused by the MODEL_DATA,
CORRECTED_DATA and IMAGING_WEIGHT scratch columns. (GvD, H, 2
wk, AK, H, 1 wk).
- 6.
- msplot defect correction: Fix all current, high-severity msplot
defects. (RM, H, 2 wk).
- 7.
- Autoflag interface revisions: Change autoflag.g Glish interface
to be compatible with AIPS++ user interface conventions. (OS, H,
1 wk).
- 8.
- Autoflag C++ code review: Complete preparation of autoflag C++
code for AIPS++ code review. (OS, H, 2 wk, AK, H, 1 wk).
- 9.
- Requirements for uv-component fitting: Finalize requirements and
implementation document for full uv-component fitting. Including list
of required changes to component models. (WB, H, 1 wk).
- 10.
- Analytic errors in simulator: Add basic analytic errors to
simulator, including: i) Chebyshev polynomial in amplitude, phase,
rate and delay (G Jones); ii) polynomial bandpass (B Jones); iii)
Chebyshev polynomial in instrumental polarization (D Jones). Requires
Chebyshev polynomial implementation. (RP, H, 2 wk).
- 11.
- calibrater enhancements: Includes: i) identified improvements in
the MS access classes; ii) full interpolation and parametrization
modes. (GM, H, 4 wk).
- 12.
- Ionosphere C++ code review: Prepare Ionosphere C++ code for code
review. (OS, H, 2 wk).
- 13.
- Ionsophere correction testing: Test first-order FJones
correction on WSRT and other data. (OS, H, 3 wk).
- 14.
- Second-order ionosphere corrections: Derive initial second-order
FJones corrections to the PIM model. (OS, H, 6 wk).
- 15.
- Automated wide-field imaging: Refine the packaging of the
existing wide-field imaging capabilities. Includes: i) improved mask
setting, including automated options; ii) improvements to
dragon.g. (KG, H, 3 wk).
- 16.
- SD mosaic combinations: Improved single-dish mosaicing data
combination options. (KG, H, 3 wk).
- 17.
- Planet flux density calibration: Develop flux density calibration
using planets. (RP, H, 2 wk).
- 18.
- imager test scripts: Revise all imager test scripts to use
simulated data for test generation and verification. Includes coverage
of all observing contexts (single-field, multi-field, mosaiced, and
wide-field), and all available deconvolution algorithms. (DM, H,
4 wk, KG, H, 1 wk).
- 19.
- ATCA test scripts: Test scripts and associated data
demonstrating ATCA reduction for continuum, continuum polarimetry and
spectral line reduction modes. (MW, H, 3 wk).
- 20.
- WSRT test scripts: Test scripts and associated data
demonstrating WSRT reduction for continuum, continuum polarimetry and
spectral line reduction modes. (JN, H, 4 wk).
- 21.
- BIMA test scripts: Additions to the existing BIMA test scripts
to cover new observing modes. (DM, H, 2 wk).
- 22.
- VLA test scripts: Expand the existing VLA test scripts to cover spectral-line modes and additional data sets. (AK, H, 1 wk).
- 23.
- IRAM AIPS++ test: Verify AIPS++ reduction using IRAM test
data. (AK, H, 5 wk, KG, M, 2 wk).
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Previous: Single-dish
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