We should have a diverse sample of WFPC2, ACS, and WFC3 images to test the pipeline on, once we finish adding in the necessary additions. We should have plenty of images from each detector, preferably in even proportions. We need to make sure that settings which work well for an ACS HRC image of Mars don't end up eating an ACS WFC image of a comet, for instance.
We should have a diverse sample of WFPC2, ACS, and WFC3 images to test the pipeline on, once we finish adding in the necessary additions. We should have plenty of images from each detector, preferably in even proportions. We need to make sure that settings which work well for an ACS HRC image of Mars don't end up eating an ACS WFC image of a comet, for instance.