Abstract We present a Monte Carlo–based population synthesis study of fast radio burst (FRB) dispersion and scattering focusing on the first catalog of sources detected with the Canadian Hydrogen Intensity Mapping Experiment Fast Radio Burst (CHIME/FRB) project. We simulate intrinsic properties and propagation effects for a variety of FRB population models and compare the simulated distributions of dispersion measures and scattering timescales with the corresponding distributions from the CHIME/FRB catalog. Our simulations confirm the results of previous population studies, which suggested that the interstellar medium of the host galaxy alone (simulated based on the NE2001 model) cannot explain the observed scattering timesc...
© 2020. The American Astronomical Society. All rights reserved.. We report on the discovery and anal...
We examine how the various observable statistical properties of the fast radio burst (FRB) populatio...
The dispersion measure(DM) of fast radio burst encodes important information such as its distance, p...
Fast radio bursts (FRBs) are brief, energetic, typically extragalactic flashes of radio emission who...
Fast radio bursts (FRBs) are bright millisecond duration transients that are primarily detected from...
We present constraints on the origins of fast radio bursts (FRBs) using large cosmological simulatio...
High time resolution radio surveys over the last few years have discovered a population of milliseco...
Fast Radio Bursts (FRBs) are cosmological transients of unknown origin. While first discovered just ...
Abstract We present a synthesis of fast radio burst (FRB) morphology (the change in ...
Fast radio bursts (FRBs) have excessive dispersion measures (DMs) and an all-sky distribution, which...
© 2019, Springer Nature Limited. Fast radio bursts (FRBs) are highly dispersed millisecond-duration ...
The time-variable long-wavelength sky harbours a number of known but unsolved astrophysical problems...
Fast radio bursts are extragalactic, sub-millisecond radio impulses of unknown origin. Their dispers...
Fast radio bursts (FRBs) are highly dispersed, sporadic radio pulses that are likely extragalactic i...
Fast radio bursts (FRBs) are energetic, short, bright transients that occur frequently over the enti...
© 2020. The American Astronomical Society. All rights reserved.. We report on the discovery and anal...
We examine how the various observable statistical properties of the fast radio burst (FRB) populatio...
The dispersion measure(DM) of fast radio burst encodes important information such as its distance, p...
Fast radio bursts (FRBs) are brief, energetic, typically extragalactic flashes of radio emission who...
Fast radio bursts (FRBs) are bright millisecond duration transients that are primarily detected from...
We present constraints on the origins of fast radio bursts (FRBs) using large cosmological simulatio...
High time resolution radio surveys over the last few years have discovered a population of milliseco...
Fast Radio Bursts (FRBs) are cosmological transients of unknown origin. While first discovered just ...
Abstract We present a synthesis of fast radio burst (FRB) morphology (the change in ...
Fast radio bursts (FRBs) have excessive dispersion measures (DMs) and an all-sky distribution, which...
© 2019, Springer Nature Limited. Fast radio bursts (FRBs) are highly dispersed millisecond-duration ...
The time-variable long-wavelength sky harbours a number of known but unsolved astrophysical problems...
Fast radio bursts are extragalactic, sub-millisecond radio impulses of unknown origin. Their dispers...
Fast radio bursts (FRBs) are highly dispersed, sporadic radio pulses that are likely extragalactic i...
Fast radio bursts (FRBs) are energetic, short, bright transients that occur frequently over the enti...
© 2020. The American Astronomical Society. All rights reserved.. We report on the discovery and anal...
We examine how the various observable statistical properties of the fast radio burst (FRB) populatio...
The dispersion measure(DM) of fast radio burst encodes important information such as its distance, p...