4.7 Article

The CHIME Fast Radio Burst Project: System Overview

期刊

ASTROPHYSICAL JOURNAL
卷 863, 期 1, 页码 -

出版社

IOP Publishing Ltd
DOI: 10.3847/1538-4357/aad188

关键词

instrumentation: interferometers; methods: observational; radio continuum: general; techniques: interferometric; telescopes

资金

  1. Canada Foundation for Innovation 2015 Innovation Fund [33213]
  2. Province of British Columbia
  3. Province of Quebec
  4. Canadian Institute for Advanced Research (CIFAR) Gravity & Extreme Universe Program, McGill University
  5. McGill Space Institute, University of British Columbia
  6. University of Toronto Dunlap Institute
  7. David Dunlap family
  8. University of Toronto
  9. Government of Canada through Industry Canada
  10. Province of Ontario through the Ministry of Research Innovation
  11. Natural Sciences and Engineering Research Council of Canada (NSERC)
  12. Mitacs Globalink Graduate Fellowship
  13. NSERC
  14. CIFAR
  15. Fonds de Recherche du Quebec-Nature et technologies Centre de Recherche en Astrophysique du Quebec (FRQNT/CRAQ)
  16. Canada Research Chairs program
  17. Lorne Trottier Chair in Astrophysics Cosmology
  18. Canada Research Chair, CIFAR
  19. Herzberg Award
  20. FRQNT/CRAQ
  21. Canadian Institute for Theoretical Astrophysics National Fellows program
  22. NSF Physics Frontiers Center [1430284]
  23. DRAO Covington Fellowship from the National Research Council Canada

向作者/读者索取更多资源

The Canadian Hydrogen Intensity Mapping Experiment (CHIME) is a novel transit radio telescope operating across the 400-800 MHz band. CHIME is composed of four 20 m x 100 m semicylindrical paraboloid reflectors, each of which has 256 dual-polarization feeds suspended along its axis, giving it a greater than or similar to 200 deg(2) field of view. This, combined with wide bandwidth, high sensitivity, and a powerful correlator, makes CHIME an excellent instrument for the detection of fast radio bursts (FRBs). The CHIME Fast Radio Burst Project (CHIME/FRB) will search beam-formed, high time and frequency resolution data in real time for FRBs in the CHIME field of view. Here we describe the CHIME/FRB back end, including the real-time FRB search and detection software pipeline, as well as the planned offline analyses. We estimate a CHIME/FRB detection rate of 2-42 FRBs sky(-1) day(-1) normalizing to the rate estimated at 1.4 GHz by Vander Wiel et al. Likely science outcomes of CHIME/FRB are also discussed. CHIME/FRB is currently operational in a commissioning phase, with science operations expected to commence in the latter half of 2018.

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