HATNet telescopes at Fred Lawrence Whipple Observatory, Mount Hopkins, Arizona. Exoplanet Survey is a geographically distributed network of 7 small telescopes optimized for detecting transiting exoplanets. Since first light in 2003, we have discovered 61 exoplanets. 2018, The Trustees of Princeton University. HATNet is supported by NASA grants NNG04GN74G and NNX13AJ15G.

HATPI will enable the detection of a diverse array of objects. Ranging from near-earth asteroids and exoplanets around bright stars to novae and bright gamma-ray bursts. The large field of view of this instrument, coupled with the dense time-sampling, will vastly improve our understanding of transient astronomical events over a large range in time scales. On-sky testing of the HATPI instrument began in February 2018. At the Instituto de Astrofísica.

HATSouth telescopes at Las Campanas Observatory, Chile with the Small Magellanic Cloud overhead. This website describes the project, and presents all data used to detect and characterize the transiting exoplanets discovered by the HATSouth survey. Use the links on the sidebar to learn more. 2018, The Trustees of Princeton University. The HATSouth mounts are built by.

Princeton Astrophysical Sciences Daily Astro-Coffee.

Kepler K2 Light Curves reduced by the HAT team. This page lists all base light curve data for the Kepler K2 mission. Using tools developed for the HATNet and HATSouth exoplanet surveys. If you use these data, please cite the papers listed in the table below for each data release.