Right now we are deprojecting a map of all objects in the source catalog classified as stars (as a template for possible star contamination). We should probably also deproject any contribution that looks like the distribution of bright stars, since those will also have an impact on the density field.
@anicola has had some experience doing this and could help in this task. Can you give us a few more details here?
Right now we are deprojecting a map of all objects in the source catalog classified as stars (as a template for possible star contamination). We should probably also deproject any contribution that looks like the distribution of bright stars, since those will also have an impact on the density field. @anicola has had some experience doing this and could help in this task. Can you give us a few more details here?