Data processing proceeded in the usual manner. The data were overscan-subtracted, and then bias subtracted using a median filtered bias from each night. Primary flat fielding was done using sky flats obtained each evening. The atmospheric extinction was determined using the Landolt standards and found to be similar to the standard CTIO extinction coefficients. A B image of one of the newly discovered Cen A dwarfs, H I PASS1321-31.
North is up and east is to the left.
The image is 2.7 across.