期刊
ASTROPHYSICAL JOURNAL LETTERS
卷 910, 期 2, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.3847/2041-8213/abeaa6
关键词
Radio transient sources; Radio bursts; Transient sources; Radio pulsars
资金
- Canada Foundation for Innovation 2015 Innovation Fund [33213]
- Province of British Columbia
- Province of Quebec
- Dunlap Institute for Astronomy and Astrophysics at the University of Toronto
- Canadian Institute for Advanced Research (CIFAR) Gravity & Extreme Universe Program, McGill University
- McGill Space Institute
- University of British Columbia
- Space Telescope Science Institute under U.S. Government [NAG W-2166]
- National Geographic Society
- National Science Foundation
- Sloan Foundation
- Samuel Oschin Foundation
- Eastman Kodak Corporation
- UK Particle Physics and Astronomy Research Council
- European Southern Observatory
- FRQNT Doctoral Research Award
- David Dunlap family
- University of Toronto
- Natural Sciences and Engineering Research Council of Canada (NSERC) [RGPIN-2015-05948]
- Canada Research Chairs program
- Lorne Trottier Chair in Astrophysics Cosmology
- Distinguished James McGill Professorship
- NSERC Discovery Grant [RGPIN 228738-13]
- Gerhard Herzberg Award
- R. Howard Webster Foundation Fellowship from CIFAR
- U.S. Department of Defense (DoD) through the National Defense Science & Engineering Graduate Fellowship (NDSEG) Program
- Killam fellowship
- NSERC Discovery Grant
- CIFAR
- FRQNT Centre de Recherche en Astrophysique du Quebec
- NSF Graduate Research Fellowship Program
- CFI JELF award
- FRQNT CRAQ
We report the discovery of FRB 20200120E, a repeating fast radio burst with a low dispersion measure, detected by the Canadian Hydrogen Intensity Mapping Experiment FRB project. The FRB is located near the spiral galaxy M81 at a distance of 3.6 Mpc. Several cataloged M81 sources and a radio point source have been found within the localization region of the FRB.
We report on the discovery of FRB 20200120E, a repeating fast radio burst (FRB) with a low dispersion measure (DM) detected by the Canadian Hydrogen Intensity Mapping Experiment FRB project. The source DM of 87.82 pc cm(-3) is the lowest recorded from an FRB to date, yet it is significantly higher than the maximum expected from the Milky Way interstellar medium in this direction (similar to 50 pc cm(-3)). We have detected three bursts and one candidate burst from the source over the period 2020 January-November. The baseband voltage data for the event on 2020 January 20 enabled a sky localization of the source to within 14 arcmin(2) (90% confidence). The FRB localization is close to M81, a spiral galaxy at a distance of 3.6 Mpc. The FRB appears on the outskirts of M81 (projected offset similar to 20 kpc) but well inside its extended H i and thick disks. We empirically estimate the probability of a chance coincidence with M81 to be <10(-2). However, we cannot reject a Milky Way halo origin for the FRB. Within the FRB localization region, we find several interesting cataloged M81 sources and a radio point source detected in the Very Large Array Sky Survey. We search for prompt X-ray counterparts in Swift Burst Alert Telescope and Fermi/GBM data, and, for two of the FRB 20200120E bursts, we rule out coincident SGR 1806-20-like X-ray bursts. Due to the proximity of FRB 20200120E, future follow-up for prompt multiwavelength counterparts and subarcsecond localization could be constraining of proposed FRB models.
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