Changes between Version 5 and Version 6 of Changes/gpcal


Ignore:
Timestamp:
08/22/07 12:39:10 (17 years ago)
Author:
MarkWieringa
Comment:

--

Legend:

Unmodified
Added
Removed
Modified

  • Changes/gpcal

    v5 v6  
    33 ||gpcal                     ||            ||          ||           ||      ||
    44 ||Item                      || Complexity || Research || Milestone || Time ||
    5  ||XYPhase                   || easy    ||  some    || 6  ||   2d   ||
     5 ||~~XYPhase ~~              || easy    ||  some    || 6  ||   ~~2d ~~  ||
    66 ||Wide band calibration     || hard    || moderate || 10 || 20d ||
    77
    88== Things to Change ==
    9  * potential XYPhase issue
     9 * ~~potential XYPhase issue~~
    1010 * wide band calibration option - add option to split wide frequency band in a number of sub-bands for gain and leakage calibration and derive spline fits across the frequency range instead of scalars.
    1111
    … …  
    1313 * check whether gpcal reads xyphase from input uv data.
    1414 At present this is in a variable?
    15     * ''No, xyphase from RPFITS syscal records can be applied in atlod and is stored in a uv variable (xyphase), but is not read by the calibration tasks.''
     15    * ''No, xyphase from RPFITS syscal records can be applied in atlod and is stored in a uv variable (xyphase), but is not read by the calibration tasks. This eliminates this item from the table above.''
    1616 * Study how miriad stores calibration tables and how we can extend these to store additional variation in frequency for complex antenna gains and leakages.
    1717    * see MiriadCalibrationTables for some reverse engineered formats and possible extensions.