Processing Images from the Zwicky Transient Facility

  • Russ Laher IPAC, Caltech
  • Frank Masci IPAC, Caltech
  • Steve Groom IPAC, Caltech
  • Benjamin Rusholme IPAC, Caltech
  • David Shupe IPAC, Caltech
  • Ed Jackson IPAC, Caltech
  • David Flynn IPAC, Caltech
  • Walter Landry IPAC, Caltech
  • Scott Terek IPAC, Caltech
  • George Helou IPAC, Caltech
  • Jason Surace IPAC, Caltech
  • Ron Beck IPAC, Caltech
  • Eugean Hacopians Anre Technologies Inc.
  • Umaa Rebbapragada JPL, Caltech
  • Brian Bue JPL, Caltech
  • Richard M. Smith Caltech Optical Observatories
  • Adam Miller Northwestern University
  • Brad Cenko NASA Goddard Space Flight Centre
  • Thomas Kupfer Caltech
  • Lin Yan Caltech
  • Tom Barlow Caltech
  • Eric Bellm University of Washington
  • Martin J. Graham Caltech
  • Mansi Kasliwal Caltech
  • Tom Prince Caltech
  • Shrinivas Kulkarni Caltech
Keywords: asteroids --- stars: variables, binaries, supernovae, cataclysmic variables --- galactic: active nuclei --- techniques: image processing, photometric --- methods: observational, data analysis

Abstract

The Zwicky Transient Facility is a new robotic-observing program, in which a newly engineered 600-MP digital camera with a pioneeringly large field of view, 47~square degrees, will be installed into the 48-inch Samuel Oschin Telescope at the Palomar Observatory. The camera will generate ~petabyte of raw imagery over three years of operations.  In parallel related work, new hardware and software systems are being developed to process these data in real time and build a long-term archive for the processed products.  The first public release of archived products is planned for 2018, which will include processed images and astronomical-source catalogs of the northern sky in the $g$ and $r$ bands. Source catalogs based on two different methods will be  generated for the archive: aperture photometry and point-spread-function fitting.

Published
2018-10-18