ACIS_Exposure_Time (make it small)
ACIS_Frame_Transfer_Time (make it large)
While only a small number of Chandra observations are done in CC mode, they would often profit from MARX modelling because there is not image that helps with seeing what we see.
At a certain level, this could be done as a post-processing step similar to pile-up. However, CC mode and pile-up are possible at the same time. Maybe the easiest approach would be to turn "marx2fits" into a post-processing module that has "--pileup" and "--CC-mode" flags. On the other hand, this would deprecate the use of the MARX binary output (because one could not get CC mode binary output).
I don't think that's a problem, but it should be considered.
Currently can maybe fake cc-mode by adjusting:
While only a small number of Chandra observations are done in CC mode, they would often profit from MARX modelling because there is not image that helps with seeing what we see.
At a certain level, this could be done as a post-processing step similar to pile-up. However, CC mode and pile-up are possible at the same time. Maybe the easiest approach would be to turn "marx2fits" into a post-processing module that has "--pileup" and "--CC-mode" flags. On the other hand, this would deprecate the use of the MARX binary output (because one could not get CC mode binary output). I don't think that's a problem, but it should be considered.