activity
20202026
most citedEnergy functions of fast radio bursts derived from the first CHIME/FRB catalogue

67 citations · 619 across the 60 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

18 papers · 1 filter

astro-ph.HE2026

Discovery of Two Consecutive Profile Change Events in the Millisecond Pulsar PSR J0437-4715

Rami F. Mandow, Andrew Zic, J. R. Dawson +19

The closest and brightest millisecond pulsar (MSP), PSR J0437-4715, is a high-priority pulsar for precision timing experiments, including the Parkes Pulsar Timing Array (PPTA) proj…

astro-ph.HE2026

A search for Fast Radio Bursts from globular clusters in M49 with FAST

Simon C. -C. Ho, Chris Flynn, Matthew Bailes +7

The origins of fast radio bursts (FRBs) remain uncertain, although magnetars are a leading progenitor candidate. Because magnetars are thought to form primarily through core-collap…

astro-ph.HE2026★ 1 cited

A fast radio burst cyclone in technicolour: evidence of plasma lensing

Pavan A. Uttarkar, Ryan M. Shannon, Kelly Gourdji +9

Fast radio bursts (FRBs) are bright, energetic, radio pulses of extragalactic origin. A dichotomy has emerged in the population: some produce repeat bursts, while the majority do n…

astro-ph.HE2026

Single-Pulse Correlations in PSR B0329+54: Implications for Radio Emission Zones

Shyam S. Sharma, Tetsuya Hashimoto, Tomotsugu Goto +3

Individual radio pulses from a pulsar are directly linked to the underlying emission processes and the associated magnetic field geometry within its magnetosphere. Thus, single-pul…

astro-ph.HE2025

Machine learning classification of baseband data of CHIME FRBs

Mohanraj Madheshwaran, Tetsuya Hashimoto, Tomotsugu Goto +5

Fast Radio Bursts (FRBs) are bright millisecond radio pulses. Their origin is still unknown in the field of astronomy. A notable distinction among FRBs is that some sources repeat,…

astro-ph.HE2025

Detection of over 37,000 giant pulses per hour from PSR J18233021A with UHF baseband observations from MeerKAT

Simon C. -C. Ho, Matthew Bailes, Chris Flynn +1

Giant pulses (GPs) occur in high magnetic-field millisecond pulsars (MSPs) and young Crab-like pulsars. Motivated by the fast radio bursts (FRBs) discovered in a globular cluster (…