• makeRMErrorMap.py:
  For a given Stokes-Q or U cube and corresponding polarized intensity map, the script outputs the theoretical Rotation Measure error map.

• getRMSF.py:
  Plots the Rotation Measure Spread Function for a given list of frequencies.

• makeFitsCube.py:
  Concats a list of 2D fits images into a 4D cube. Handy for running RM Synthesis.

• listDataCols.py:
  List all the data columns containing visibilities in a measurement set.

• tgss2bbs.py:
  Extract a TGSS skymodel in a BBS compatible format.

• plotWSCleanWeights.py:
  Plot azimuthally averaged visibility weights from WSClean.

• getSpecIndex.py
  Place holder

• stackWSCleanImages.py
  Script to stack lofar images.

• fitSpectralProfile.py
  Fit curved spectra to input images.

• plotVisibilityDensity.py
  Plots the visibility density for a given measurement set.

• findDistance.py
  Print angular distances between two astronomical sources.