I recommend always collect 360 degrees with "oscillation" not more than 0.2 deg.  
Ideally this should be less than 1/3 of your mosaic spread, whatever that is.  
Be mindful of the "wedge" size, this defines the shutterless sweep size, 
and if it is "1" collection will not be faster than with the old detector.  
Exposure times should not be less than 0.1s.  Although the detector can go faster 
than this, we are seeing noisier data that way, so for now, keep it above 0.1s.  
Note that with full beam this is 25 MGy: pretty close to the dose limit.  
So, if you want to do MAD, you are going to have to attenuate.  I recommend 
attenuating the beam by lowering the divergence to 0.2x0.2 so that each
 180-deg pass is about 1.5 MGy of dose.  
Then collect 8 pairs of (peak+infl)/2 and remote wavelengths.

This will be a lot of data, and that is a hallmark of Pilatus data collection. 
 We have cleared out /data so now there is plenty of room.  Your old files will 
be on /data2.  We have also (finally) ordered a new processing and storage computer, 
which will hopefully be here in a few more weeks.  This will have 72 cores, 
1 TB of RAM and 170 TB of /data.