Observing in visible and infrared wavelengths, the Zwicky Transient Facility is designed to detect
transient objects that rapidly change in brightness, for example
supernovae,
gamma ray bursts, and collision between two
neutron stars, and moving objects like
comets and
asteroids. The new camera is made of 16
CCDs of 6144×6160 pixels each, enabling each exposure to cover an area of 47 square degrees. The Zwicky Transient Facility is designed to image the entire northern sky in three nights and scan the plane of the
Milky Way twice each night to a limiting
magnitude of 20.5 (r band, 5σ). The amount of data produced by ZTF is expected to be ten times larger than its predecessor, the Intermediate Palomar Transient Factory. ZTF's large data allows it to act as a prototype for the
Vera C. Rubin Observatory (formerly Large Synoptic Survey Telescope) that is expected to be in full operation in late 2025 and will accumulate ten times more data than ZTF. The first confirmed findings from the ZTF project were reported on 7 February 2018, with the discovery of
2018 CL, a small
near-Earth asteroid. == Discoveries==