AstroImageJ specializes in improving LCs for an assumed standard transit structure, or flat line structure in the case of comps. However, there appear to be some functions of the software that could probably improve the LC of an undetermined shape and periodicity. For example, on the Data set 3 Fit Settings window, the use of Outlier Removal, Comp Star selection, and Detrend Parameter selection might improve the reliability of the raw data.
Could you please provide some advice on how best to modify the use of the Multi-plot Main, Multi-plot Y Data, and Data set 3 Fit Settings screens to improve raw data of an LC as described above?
What I mean by that is, for example, on the Multi-plot Y Data screen, I would assume that fit mode would be set off and on the Data set 3 Fit Settings window LDCs would not be used, etc. What other differences would you recommend?