The HATPI ProjectLearn More
In a single 45 second exposure, the HATPI instrument
observes the full night sky, in all
directions, from the
zenith down to an elevation angle of 35 degrees, at a
spatial resolution of 20 arcseconds per pixel. The key
science aim of HATPI is to explore the
variable sky,
including studying astrophysical transient events (cosmic
explosions), transiting exoplanets, variable stars, and
moving objects (near-Earth asteroids).
HATPI is located at
Las Campanas Observatory in the Atacama Desert of
Chile | -29.010486,
-70.701080
Light CurvesVisit Page
Access the public HATPI database
PublicationsComing Soon
Team Members
Acknowledgments
Generous funding provided by the Moore, Packard, and Mt. Cuba Astronomical foundations
Site
hosting provided by Carnegie Science and Las Campanas Observatory