Hi, I am working on a project to determine the possible presence of periodicities in the LC of a star surrounded by dust/rubble/etc. The occultations are not predictable and they do not result in a normal exoplanet LC. I would like to use AstroImageJ and the "Dataset 3 Fit Settings" screen to optimize the LC before further analysis. In what ways should I use the "Dataset 3 Fit Settings" screen differently for such an LC than I would use it for a conventional exoplanet occultation (if any)? Thanks!
Ed
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