activity
20102024
most citedA repeating fast radio burst source localised to a nearby spiral galaxy

436 citations · 2.3k across the 31 of their papers we have counts for

collaborators
Showing 2020Show all

6 papers · 1 filter

astro-ph.IM2020★ 25 cited

Your: Your Unified Reader

Kshitij Aggarwal, Devansh Agarwal, Joseph W Kania +9

The advancement in signal processing and GPU based systems has enabled new transient detectors at various telescopes to perform much more sensitive searches than their predecessors…

astro-ph.HE2020★ 96 cited

A Distant Fast Radio Burst Associated to its Host Galaxy with the Very Large Array

C. J. Law, B. J. Butler, J. X. Prochaska +17

We present the discovery and subarcsecond localization of a new Fast Radio Burst with the Karl G. Jansky Very Large Array and realfast search system. The FRB was discovered on 2019…

astro-ph.HE2020★ 29 cited

VLA/Realfast Detection of a Burst from FRB180916.J0158+65 and Tests for Periodic Activity

Kshitij Aggarwal, Casey J. Law, Sarah Burke-Spolaor +5

We report on the detection of a burst from FRB180916 by realfast/VLA and present software for interpreting fast radio bursts (FRB) periodicity. We demonstrate a range of periodicit…

astro-ph.HE2020

A Demonstration of Extremely Low Latency -ray, X-Ray & UV Follow-Up of a Millisecond Radio Transient

Aaron Tohuvavohu, Casey J. Law, Jamie A. Kennea +18

We report results of a novel high-energy follow-up observation of a potential Fast Radio Burst. The radio burst was detected by VLA/realfast and followed-up by the Neil Gehrels Swi…

astro-ph.HE2020★ 436 cited

A repeating fast radio burst source localised to a nearby spiral galaxy

B. Marcote, K. Nimmo, J. W. T. Hessels +51

Fast radio bursts (FRBs) are brief, bright, extragalactic radio flashes. Their physical origin remains unknown, but dozens of possible models have been postulated. Some FRB sources…

astro-ph.HE2020★ 90 cited

Modeling the uncertainties of solar-system ephemerides for robust gravitational-wave searches with pulsar timing arrays

M. Vallisneri, S. R. Taylor, J. Simon +61

The regularity of pulsar emissions becomes apparent once we reference the pulses' times of arrivals to the inertial rest frame of the solar system. It follows that errors in the de…