Using the catalog we created two interactive plots which allows users to explore our results. The plot is similar in appearance to the anomaly map in figure 8. Each point represents a star in or near an ACS/WFC observation and the black lines represent the ACS/WFC chips. Users can hover over each point and see the image in which it caused scattering. Above the image there is also information about the star including the guide star name, the name of the image, the filter used, the filter magnitude, and the magnitude corrected to 500 seconds. There is also a slider which selects stars based on their exposure time corrected detector magnitudes. This slider allows the user to view stars withing 1 magnitude of the selected magnitude. This is a great tool for exploring examples of scattered light appearing in multiple dithered observations, in multiple filters, and how magnitude can determine the length of the scattering.