Hi,
If you're using master calibration frames to run the BPP script, the state of these frames should be as shown below:
- Master bias: A simple integration.
- Master dark: Also a simple integration. We don't remove the bias from the dark. This is very convenient since you preserve the bias signal in the master dark. That allows you to run BPP without biases, if you're not scaling your darks.
- Master flat: Completely calibrated.
If you manually generate your masters and you calibrate the dark frames before integrating them, then you'll have problems when running BPP.
On the other hand, I think BPP is a powerful tool in its current state. I still remember when I gave my first US workshop at the Adler Planetarium, many years ago. I was teaching how to manually calibrate everything. I was deeply wrong (although at that time we didn't have the BPP script!). Right now, if you care about the critical step in the automation (the integration of the master light), BPP will give you very good results with a big benefit: it will optimize your working time! This is really important. Our time is always limited. A combination of automation and manual control of the critical parts is almost always the best option IMO. Think about this: you can have really bad results even by running a completely manual procedure if you don't know what to look at the rejection maps.
Best regards,
Vicent.