Fast Radio Bursts Trace Cosmic Star Formation with Little Delay
Yi-Ying Wang, Yin-Jie Li, Yi-Zhong Fan
astro-ph.HE, astro-ph.CO
Submitted: 2026-07-10
Comments: 15 pages, 9 figures
Project page: https://chime-frb-open-data.github.io/injections
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- A bright millisecond radio burst of extragalactic origin
- Fast Radio Bursts: An Extragalactic Enigma
- Fast Radio Bursts
- A Living Theory Catalogue for Fast Radio Bursts
- The Physics of Fast Radio Bursts
- Fast radio bursts at the dawn of the 2020s
- The Physics of Fast Radio Bursts
- A bright millisecond-duration radio burst from a Galactic magnetar
- A fast radio burst associated with a Galactic magnetar
- Detection of two bright radio bursts from magnetar SGR 1935+2154
- A nearby repeating fast radio burst in the direction of M81
- A repeating fast radio burst source in a globular cluster
- No redshift evolution of non-repeating fast radio-burst rates
- Bright Supernovae from Magnetar Birth
- Evidence for GeV emission of the superluminous supernova SN 2017egm
- Fast radio bursts: the last sign of supramassive neutron stars
- The Physical Mechanisms of Fast Radio Bursts
- Cosmological Fast Radio Bursts from Binary Neutron Star Mergers
- Fast Radio Bursts from the Inspiral of Double Neutron Stars
- An assessment of the Association Between a Fast Radio Burst and Binary Neutron Star Merger
Related papers
- Numerical Studies of Accretion Flows onto a Neutron Star Engulfed in a Massive Star
- Collisionless Accretion of Finite-Angular-Momentum Plasma onto a Spinning Black Hole
- Impact of Magnetic Field Topology on Electromagnetic and Gravitational Waves from Binary Neutron Star Merger Remnants
- XRISM Resolve Spectroscopy of GX 5-1: Constraints on Iron Spectral Features in a Luminous Neutron-Star Binary
- SN 1006: A Cosmic Laboratory for Investigating Shock Acceleration Physics
- Neutrino Spectral Pinching in 3D Core-Collapse Supernovae: Late-Time Convergence, Failed-Explosion Signatures, and Viewing-Angle Dispersion