VizieR Online Data Catalog: M giant stars asteroseismology with Kepler and APOGEE (Auge+, 2020)

We utilize photometry from the Asteroid Terrestrial-impact Last Alert System (ATLAS) and All-Sky Automated Survey for Supernovae (ASAS-SN) for our analysis. ATLAS is primarily designed to detect small asteroids on their final approach to Earth. To achieve this ATLAS scans all of the accessible sky every few nights using fully robotic 0.5m f/2 Wright Schmidt telescopes with a 5.4x5.4° field of view. ATLAS began operations with one telescope on Haleakala on the Hawaiian island of Maui in mid-2015, and began operations with their second telescope early 2017 at the Maunaloa Observatory on the big island of Hawai`i. Each ATLAS telescope takes four 30s exposures per night of 200-250 target fields covering half of the accessible night sky. ATLAS uses two customized, wide filters designed to optimize detections of faint objects: the cyan filter (c) covering 420-650nm and the orange filter (o) covering 560-820nm.

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