The Zwicky Transient Facility: Observing System

By R. Dekany, Roger M. Smith, R. Riddle, M. Feeney, Michael E. Porter, D. Hale, J. Zolkower, J. Belicki, S. Kaye, J. Henning and 16 more. Astronomical Telescopes and Instrumentation, 2014

269 citations recorded by the source corpus.

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.

Subfields: Atomic and Molecular Physics, and Optics, Electrical and Electronic Engineering, Instrumentation

View Paper: https://www.semanticscholar.org/paper/c199836ae0ced5498d354575320ff777f52271d2

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In Atomic and Molecular Physics, and Optics

  1. S. Burke-Spolaor
  2. J. Sollerman
  3. J. Neill
  4. M. Birkinshaw
  5. Shrinivas R. Kulkarni
  6. Heinz Andernach
  7. W. N. Brandt
  8. Bryan Butler

In Electrical and Electronic Engineering

  1. A. Gal-yam
  2. C. O’Dea
  3. Željko Ivezic´
  4. J. Sollerman
  5. R. Weeren
  6. A. Filippenko
  7. W. N. Brandt
  8. Gordon Richards

In Instrumentation

  1. Gordon Richards
  2. W. N. Brandt
  3. A. Filippenko
  4. Željko Ivezic´
  5. T. Brink
  6. A. Gal-yam
  7. E. Berger
  8. Mansi M. Kasliwal

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