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DeepStreaks: Identifying fast-moving objects in the Zwicky Transient Facility data with deep learning

  • Dmitry A. Duev
  • , Ashish Mahabal
  • , Quanzhi Ye
  • , Kushal Tirumala
  • , Justin Belicki
  • , Richard Dekany
  • , Sara Frederick
  • , Matthew J. Graham
  • , Russ R. Laher
  • , Frank J. Masci
  • , Thomas A. Prince
  • , Reed Riddle
  • , Philippe Rosnet
  • , Maayane T. Soumagnac
  • California Institute of Technology
  • University of Maryland, College Park
  • Université Clermont Auvergne
  • Weizmann Institute of Science

Research output: Contribution to journalArticlepeer-review

41 Scopus citations

Abstract

We present DeepStreaks, a convolutional-neural-network, deep-learning system designed to efficiently identify streaking fast-moving near-Earth objects that are detected in the data of the Zwicky Transient Facility (ZTF), a wide-field, time-domain survey using a dedicated 47 deg2 camera attached to the Samuel Oschin 48-inch Telescope at the Palomar Observatory in California, United States. The system demonstrates a 96-98 per cent true positive rate, depending on the night, while keeping the false positive rate below 1 per cent. The sensitivity of DeepStreaks is quantified by the performance on the test data sets as well as using known near-Earth objects observed by ZTF. The system is deployed and adapted for usage within the ZTF Solar system framework and has significantly reduced human involvement in the streak identification process, from several hours to typically under 10 min per day.

Original languageEnglish
Pages (from-to)4158-4165
Number of pages8
JournalMonthly Notices of the Royal Astronomical Society
Volume486
Issue number3
DOIs
StatePublished - 1 Jul 2019
Externally publishedYes

Bibliographical note

Publisher Copyright:
© 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society.

Funding

DAD acknowledges support from the Heising-Simons Foundation under Grant No. 12540303. QY is supported by the GROWTH project funded by the U.S. National Science Foundation under Grant No. 1545949. Based on observations obtained with the Samuel Oschin Telescope 48-inch Telescope at the Palomar Observatory as part of the Zwicky Transient Facility project. Major funding has been provided by the U.S. National Science Foundation under Grant No. AST-1440341 and by the ZTF partner institutions: the Caltech, the Oskar Klein Centre, the Weizmann Institute of Science, the University of Maryland, the University of Washington, Deutsches Elektronen-Synchrotron, the University of Wisconsin-Milwaukee, and the TANGO Program of the University System of Taiwan. AM acknowledges support from the U.S. National Science Foundation (NSF) (1640818 and AST-1815034).

FundersFunder number
U.S. National Science FoundationAST-1440341
National Science Foundation1440341, 1545949
American Committee for the Weizmann Institute of Science
University of Wisconsin-Milwaukee1640818, AST-1815034
University of Washington
University of Maryland
Heising-Simons Foundation12540303

    Keywords

    • asteroids: general
    • methods: data analysis
    • minor planets
    • surveys

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