As fakes are planted into the images, we need a catalog (flat file, maybe FITS or an AstroPy table) or a database (SQL?) to track the information about the fake sources, their host galaxies, the results of the detection algorithms, and the results of the classfication algorithms.
Choose a flat ascii text file for simplicity and ease of visualization, unless features of a SQL db are needed.
As fakes are planted into the images, we need a catalog (flat file, maybe FITS or an AstroPy table) or a database (SQL?) to track the information about the fake sources, their host galaxies, the results of the detection algorithms, and the results of the classfication algorithms.
Choose a flat ascii text file for simplicity and ease of visualization, unless features of a SQL db are needed.