4.6 Article

The First CHIME/FRB Fast Radio Burst Catalog

期刊

出版社

IOP Publishing Ltd
DOI: 10.3847/1538-4365/ac33ab

关键词

-

资金

  1. Canada Foundation for Innovation (CFI) 2012 Leading Edge Fund [31170]
  2. province of British Columbia
  3. province of Quebec
  4. province of Ontario
  5. CFI 2015 Innovation Fund [33213]
  6. Dunlap Institute for Astronomy and Astrophysics at the University of Toronto
  7. Canadian Institute for Advanced Research (CIFAR)
  8. McGill University
  9. McGill Space Institute via the Trottier Family Foundation
  10. University of British Columbia
  11. David Dunlap family
  12. University of Toronto
  13. Government of Canada through Industry Canada
  14. Province of Ontario through the Ministry of Research Innovation
  15. National Science Foundation [2006548]
  16. Natural Sciences and Engineering Research Council (NSERC)
  17. NSERC [RGPIN-2015-05948, RGPIN-2020-04554, RGPIN-2019-067, CRD 523638-201, RGPIN 228738-13]
  18. Canada Research Chairs (CRC) program
  19. U.S. Department of Defense (DoD) through the National Defense Science & Engineering Graduate Fellowship (NDSEG) Program
  20. John I. Watters Research Fellowship
  21. NWO Veni Fellowship
  22. CIFAR
  23. CRC Program
  24. Canadian Statistical Sciences Institute Collaborative Research Team Grant
  25. CFI John R. Evans Leaders Fund award
  26. NSF [1458952, AAG-1616042, 2008031, 1430284]
  27. Killam Fellowship
  28. FRQNT Centre de Recherche en Astrophysique du Quebec (CRAQ)
  29. FRQNT Doctoral Research award
  30. Ontario Research Fund-Research Excellence Program (ORF-RE)
  31. Simons Foundation
  32. Thoth Technology Inc.
  33. Alexander von Humboldt Foundation
  34. Gerhard Herzberg award
  35. Howard Webster Foundation Fellowship from CIFAR
  36. FRQNT CRAQ
  37. Lorne Trottier Chair in Astrophysics Cosmology
  38. Division Of Astronomical Sciences
  39. Direct For Mathematical & Physical Scien [2006548] Funding Source: National Science Foundation

向作者/读者索取更多资源

This study presents a catalog of 536 fast radio bursts detected by the CHIME/FRB Project over a one-year period, providing insights into the FRB population. The research shows consistency in sky locations and dispersion measures between repeaters and apparent nonrepeaters, while also highlighting differences in intrinsic temporal width and spectral bandwidth. Additionally, the study reveals the population properties of FRBs and conducts an absolute calibration of selection effects.
We present a catalog of 536 fast radio bursts (FRBs) detected by the Canadian Hydrogen Intensity Mapping Experiment Fast Radio Burst (CHIME/FRB) Project between 400 and 800 MHz from 2018 July 25 to 2019 July 1, including 62 bursts from 18 previously reported repeating sources. The catalog represents the first large sample, including bursts from repeaters and nonrepeaters, observed in a single survey with uniform selection effects. This facilitates comparative and absolute studies of the FRB population. We show that repeaters and apparent nonrepeaters have sky locations and dispersion measures (DMs) that are consistent with being drawn from the same distribution. However, bursts from repeating sources differ from apparent nonrepeaters in intrinsic temporal width and spectral bandwidth. Through injection of simulated events into our detection pipeline, we perform an absolute calibration of selection effects to account for systematic biases. We find evidence for a population of FRBs-composing a large fraction of the overall population-with a scattering time at 600 MHz in excess of 10 ms, of which only a small fraction are observed by CHIME/FRB. We infer a power-law index for the cumulative fluence distribution of alpha=-1.40 +/- 0.11(stat.)(-0.09)(+0.06)(sys.), consistent with the -3/2 expectation for a nonevolving population in Euclidean space. We find that alpha is steeper for high-DM events and shallower for low-DM events, which is what would be expected when DM is correlated with distance. We infer a sky rate of [820 +/- 60(stat.)(-200)(+220)(sys.)]/sky/day above a fluence of 5 Jy ms at 600 MHz, with a scattering time at 600 MHz under 10 ms and DM above 100 pc cm(-3).

作者

我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。

评论

主要评分

4.6
评分不足

次要评分

新颖性
-
重要性
-
科学严谨性
-
评价这篇论文

推荐

暂无数据
暂无数据