2020/04/29 by Weiwei Zhu, Di Li, Rui Luo +78 · 41 citations
Physics and Astronomy · #Astrophysics #Cosmology and Gravitation Theories #Detector #Energy (signal processing) #Event (particle physics) #Fast radio burst #Fluence #Flux (metallurgy) #Galaxy #Gamma-ray bursts and supernovae #Luminosity #Optics #Physics #Pulsars and Gravitational Waves Research #Pulse (music) #Radio telescope #Redshift #astro-ph.HE
paper · pdf · doi:10.3847/2041-8213/ab8e46
published in The Astrophysical Journal Letters 895(1), L6 (IOP Publishing) · 7 pages, 3 figures, accepted for publication in ApJL
arxiv created 2020/04/29 · openalex publication_date 2020/05/01 · arxiv updated 2020/05/27 · openalex created_date 2020/11/23 · openalex updated_date 2026/08/05
Abstract We report the discovery of a highly dispersed fast radio burst (FRB), FRB 181123, from an analysis of ∼1500 hr of drift scan survey data taken using the Five-hundred-meter Aperture Spherical radio Telescope (FAST). The pulse has three distinct emission components, which vary with frequency across our 1.0–1.5 GHz observing band. We measure the peak flux density to be >0.065 Jy and the corresponding fluence >0.2 Jy ms. Based on the observed dispersion measure of 1812 cm −3 pc, we infer a redshift of ∼1.9. From this, we estimate the peak luminosity and isotropic energy to be ≲2 × 10 43 erg s −1 and ≲2 × 10 40 erg, respectively. With only one FRB from the survey detected so far, our constraints on the event rate are limited. We derive a 95% confidence lower limit for the event rate of 900 FRBs per day for FRBs with fluences >0.025 Jy ms. We performed follow-up observations of the source with FAST for four hours and have not found a repeated burst. We discuss the implications of this discovery for our understanding of the physical mechanisms of FRBs.