Initially this could be done just for frames that are used for astrometric solutions, and applied to the entire session, or alternatively, provide the option to evaluate every image.
I assume that the metric of "star count" would have to be empirically determined by the user, perhaps with a config lookup-table.
Initially this could be done just for frames that are used for astrometric solutions, and applied to the entire session, or alternatively, provide the option to evaluate every image.
I assume that the metric of "star count" would have to be empirically determined by the user, perhaps with a config lookup-table.