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.