A wide-field survey telescope used to detect transient astronomical events.The Zwicky Transient Facility (ZTF) is a wide-field astronomical survey that scans the entire northern sky every two nights using a large-format camera mounted on the Samuel Oschin Telescope at Palomar Observatory. Its primary mission is to discover transient events—objects that appear, brighten, fade, or move—such as supernovae, tidal disruption events, and near-Earth asteroids. By providing a continuous, high-cadence survey of the sky, ZTF acts as a cosmic sentinel, alerting astronomers to fleeting phenomena that would otherwise be missed.
ZTF is the successor to the Palomar Transient Factory (PTF) and began its survey in 2018. It is named after Fritz Zwicky, a Caltech astronomer who pioneered the systematic search for supernovae and other transients in the 1930s.
ZTF uses a 47-square-degree field of view camera, one of the largest in the world, to capture wide swaths of the sky in a single exposure. The telescope rapidly slews between positions, taking hundreds of images per night. Sophisticated software then compares new images to reference images of the same sky region, automatically flagging any differences—these are the transient candidates. These candidates are immediately published as alerts, allowing other telescopes worldwide to follow up on the most interesting events.
ZTF's alerts enable rapid follow-up observations of transient events, contributing to studies of dark energy, gravitational wave counterparts, and the discovery of new astronomical objects.
ZTF generates tens of thousands of alerts per night, and its data has been used to discover over a thousand supernovae in its first few years of operation.









