# The data for each MRA can be found in each folder starting with MRA*

# The data for MRAs are saved in the correlated visibility measurement format which can be fed into
  CASA radio astronomy software

# Each measurement set is bandpass calibrated, bright sources peeled, near-field corrected, background visibility subtracted

# Imaging will allow to see a bright source in the middle of the field of view

# Each dataset is named as diff[mra_number/integration]_[subband no].ms
# mra_number goes from 1-5
# integration goes from a-f
# subband number goes from [01, 03, 05, 07] for [30-32.6, 35.2-37.8, 40.4-43, 45.6-48.2] MHz