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Zwicky Transient Facility - Observatory
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Zwicky Transient Facility

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description Zwicky Transient Facility Overview

The Zwicky Transient Facility (ZTF) is a wide-field astronomical survey instrument operating at Palomar Observatory in southern California. It uses the 48-inch Samuel Oschin Telescope, equipped with a large-format CCD camera, to repeatedly image the northern sky. Operational since 2018, ZTF scans the visible sky every two to three nights to detect transient astronomical phenomena including supernovae, near-Earth asteroids, and variable stars. The project is named for astronomer Fritz Zwicky, who was based at Caltech and helped establish Palomar Observatory.

insights Ranking position

Zwicky Transient Facility ranks #33 of 270 in the Observatory ranking, behind IRAM NOEMA, ahead of Planck.

help Zwicky Transient Facility FAQ

What kinds of events does the Zwicky Transient Facility detect?

ZTF searches for objects that brighten, fade, or move, including supernovae, variable stars, asteroids, and the optical counterparts of gravitational-wave events. It has operated at Palomar Observatory since 2018.

Which telescope does the Zwicky Transient Facility use?

ZTF is installed on the 48-inch Samuel Oschin Telescope at Palomar Observatory in California. Its large camera gives the telescope an unusually wide field of view, allowing it to survey broad areas rather than study one small target at a time.

How often does ZTF photograph the night sky?

Its survey strategy can revisit the visible northern sky every few nights, with selected fields observed much more frequently. Repeated images are compared so that changing or newly appearing sources can generate alerts.

How is ZTF related to the Vera C. Rubin Observatory?

Both are time-domain surveys designed to find changes in the sky, but ZTF uses the existing Oschin Telescope at Palomar while Rubin uses the newer 8.4-meter Simonyi Survey Telescope in Chile. ZTF has also served as a practical precursor for handling large transient-alert streams.

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