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  1. It would be good to have a table of content here or an introduction, e.g. explaining that here we aim at releasing the famous fields observed by Apertif and the first one is Bootes but Elais and LH will follow...or something like this. I would make very clear here that, while the initial calibration is the same as described in DR1,  the images of the famous fields are made using a new DD pipeline. It is important to have it upfront.