This page describes some known issues.
The following is a list of known issues with the cosmic rays analysis pipeline.
The relative gain calibration (on the galactic noise) is not centered around 1.0 but rather on roughly 1.1.
The task Galaxy is used to perform the calibration based on a two component Fourier transform fit to the data that was calculated from the antennas_cleaned_power parameter of the :clas:`~pycrtools.tasks.FindRFI`.