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Paper detail

The Zwicky Transient Facility: Observing System

The Zwicky Transient Facility (ZTF) Observing System (OS) is the data collector for the ZTF project to study astrophysical phenomena in the time domain. ZTF OS is based upon the 48-inch aperture Schmidt-type design Samuel Oschin Telescope at the Palomar Observatory in Southern California. It incorporates new telescope aspheric corrector optics, dome and telescope drives, a large-format exposure shutter, a flat-field illumination system, a robotic bandpass filter exchanger, and the key element: a new 47-square-degree, 600 megapixel cryogenic CCD mosaic science camera, along with supporting equipment. The OS collects and delivers digitized survey data to the ZTF Data System (DS). Here, we describe the ZTF OS design, optical implementation, delivered image quality, detector performance, and robotic survey efficiency.

preprint2020arXivOpen access
Richard DekanyRoger M. SmithReed RiddleMichael FeeneyMichael PorterDavid HaleJeffry ZolkowerJustin BelickiStephen KayeJohn HenningRichard WaltersJohn CromerAlex DelacroixHector RodriguezDaniel J. ReileyPeter MaoDavid HoverPatrick MurphyRick BurrussJohn BakerMarek KowalskiKlaus ReifPhillip MuellerEric BellmMatthew GrahamShrinivas R. Kulkarni
physics.ins-detastro-ph.IMphysics.optics
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Richard DekanyRoger M. SmithReed RiddleMichael FeeneyMichael PorterDavid HaleJeffry ZolkowerJustin BelickiStephen KayeJohn HenningRichard WaltersJohn CromerAlex DelacroixHector RodriguezDaniel J. ReileyPeter MaoDavid HoverPatrick MurphyRick BurrussJohn BakerMarek KowalskiKlaus ReifPhillip MuellerEric BellmMatthew GrahamShrinivas R. Kulkarni

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