INT monitoring of Local Grp. VII. IC 10 photometry

We created a photometric catalog for 53,579 stars within the area of CCD4 of WFC (~0.07deg^2^ corresponding to 13.5kpc^2^ at the distance of IC 10), of which we classified 536 and 380 stars as LPV candidates, mostly asymptotic giant branch (AGBs) stars and red supergiants, within CCD4 and two half-light radii of IC 10, respectively.

By comparing our output catalog to the catalogs from Pan-STARRS, Spitzer Space Telescope, Hubble Space Telescope (HST), and carbon stars from the Canada- France-Hawai'i Telescope survey, we determined the success of our detection method. We recovered ~73% of Spitzer's sources in our catalog and demonstrated that our survey successfully identified 43% of the variable stars found with Spitzer, and also retrieved 40% of the extremely dusty AGB stars among the Spitzer variables.