fixms 0.1.3

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FixMS

WARNING FOR USERS: These scripts are still being verified for complete correctness. Please use at your own risk.

ASKAP utilities for updating MeasurementSets for external imagers.

ASKAP MSs are produced in a way that breaks compatibility with most other imagers (e.g. CASA, WSclean). Here we provide two modules (with CLI hooks) that perform the fixes that need to be applied in order to produce astronomically correct imagers with non-YandaSoft imagers:

1. fix_ms_dir : ASKAP MeasurementSets are phased towards the centre of field, but not the centre of its given beam. This utility reads the appropriate offsets to the beam centre from the BEAM_OFFSET and updates the FIELD table, as well as the phase and delay reference columns.

2. fix_ms_corrs : ASKAP MeasurementSets, as calibrated by the obervatory, provide correlations in the instrument frame. ASKAP has a unique 'roll' axis which means, in principle, the instrument frame can be at any arbitrary rotation on the sky. This utility applies the appropriate rotation matrix to the visibilities such the 'X' is aligned North-South and 'Y' is aligned East-West (IAU convention). Further, ASKAPsoft defines Stokes I as $I=XX+YY$, whereas most other telescopes use $I=\frac{1}{2}(XX+YY)$ (note this also applies to all other Stokes paramters). This factor is also corrected for here at the same time as the rotation.

For convenience, we also provide fix_ms which does both of the above!

Full documentation on Read The Docs.

Installation

Obtain and install Python 3 (I recommend Miniforge or Miniconda).

Install the Python scripts:

Latest:

pip install git+https://github.com/AlecThomson/FixMS.git

Stable:

pip install FixMS

Usage

❯ fix_ms -h
usage: fix_ms [-h] [--chunksize CHUNKSIZE] [--data-column DATA_COLUMN] [--corrected-data-column CORRECTED_DATA_COLUMN] [ms]

Utility to correct the ASKAP beam positions and apply a rotation to apply a change of the reference frame of the visibilities

positional arguments:
  ms                    Measurement set to update (default: None)

options:
  -h, --help            show this help message and exit
  --chunksize CHUNKSIZE
                        The chunksize to use when reading the MS (default: 1000)
  --data-column DATA_COLUMN
                        The column to fix (default: DATA)
  --corrected-data-column CORRECTED_DATA_COLUMN
                        The column to write the corrected data to (default: CORRECTED_DATA)

❯ fix_ms_corrs -h
usage: fix_ms_corrs [-h] [--chunksize CHUNKSIZE] [--data-column DATA_COLUMN] [--corrected-data-column CORRECTED_DATA_COLUMN] ms

Fix the correlation rotation of ASKAP MSs. Converts the ASKAP standard correlations to the 'standard' correlations This will make them compatible with most imagers (e.g. wsclean, CASA) The new correlations are placed in a new column called 'CORRECTED_DATA'

positional arguments:
  ms                    The MS to fix

options:
  -h, --help            show this help message and exit
  --chunksize CHUNKSIZE
                        The chunksize to use when reading the MS (default: 1000)
  --data-column DATA_COLUMN
                        The column to fix (default: DATA)
  --corrected-data-column CORRECTED_DATA_COLUMN
                        The column to write the corrected data to (default: CORRECTED_DATA)

❯ fix_ms_dir -h
usage: fix_ms_dir [-h] [ms]

ASKAP utility - update the pointing centre of a beam in an MS. - Allows imaging by CASA or wsclean.

positional arguments:
  ms          Measurement set to update (default: None)

optional arguments:
  -h, --help  show this help message and exit

Contribution

Contributions are very welcome! Please open an issue first to discuss any bugs or updates you might have.