CHIME/FRB Discovery and Localization of the Swift-observed FRB 20241228A
Abstract
Abstract On 2024 December 28, the Canadian Hydrogen Intensity Mapping Experiment (CHIME) FRB project detected the thus-far nonrepeating FRB 20241228A with a real-time signal-to-noise ratio of >50. Approximately 112 s later, the X-ray Telescope on board the Neil Gehrels Swift Observatory was on-source, the fastest follow-up to date of a nonrepeating fast radio burst (FRB). Using CHIME/FRB and two of the three CHIME/FRB Outriggers, we obtained a very-long-baseline interferometry (VLBI) localization for FRB 20241228A with a 1 σ confidence ellipse of 11″ by 0 . ″ 2. This represents the first published localization using both the CHIME k’niʔatn k’l⌣stk’masqt and CHIME Green Bank Observatory Outriggers. We associate FRB 20241228A with a star-forming galaxy at a redshift of z = 0.1614 ± 0.0002. The persistent X-ray luminosity limit at this source’s location and distance is
Fields of Study & Subjects
Gamma-ray bursts and supernovae
Pulsars and Gravitational Waves Research
Astrophysical Phenomena and Observations
Publication details
- Journal / source
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Volume
- 998
- Issue
- 1
- Pages
- 97–97
- Publication date
- 4 February 2026
- Language
- EN