activity
20152026
most citedRefined Mass and Geometric Measurements of the High-Mass PSR J0740+6620

979 citations · 5.3k across the 35 of their papers we have counts for

collaborators
Showing 2021Show all

6 papers · 1 filter

astro-ph.IM2021★ 3 cited

The Hydrogen Intensity and Real-time Analysis eXperiment: 256-Element Array Status and Overview

Devin Crichton, Moumita Aich, Adam Amara +97

The Hydrogen Intensity and Real-time Analysis eXperiment (HIRAX) is a radio interferometer array currently in development, with an initial 256-element array to be deployed at the S…

astro-ph.HE2021★ 88 cited

Sub-second periodicity in a fast radio burst

FRB Collaboration, Bridget C. Andersen, Kevin Bandura +59

Fast radio bursts (FRBs) are millisecond-duration flashes of radio waves that are visible at distances of billions of light-years. The nature of their progenitors and their emissio…

astro-ph.IM2021★ 24 cited

Localizing FRBs through VLBI with the Algonquin Radio Observatory 10-m Telescope

Tomas Cassanelli, Calvin Leung, Mubdi Rahman +38

The CHIME/FRB experiment has detected thousands of Fast Radio Bursts (FRBs) due to its sensitivity and wide field of view; however, its low angular resolution prevents it from loca…

astro-ph.HE2021★ 484 cited

The First CHIME/FRB Fast Radio Burst Catalog

FRB Collaboration, Mandana Amiri, Bridget C. Andersen +73

We present a catalog of 536 fast radio bursts (FRBs) detected by the Canadian Hydrogen Intensity Mapping Experiment Fast Radio Burst (CHIME/FRB) Project between 400 and 800 MHz fro…

astro-ph.HE2021★ 979 cited

Refined Mass and Geometric Measurements of the High-Mass PSR J0740+6620

Emmanuel Fonseca, H. Thankful Cromartie, Timothy T. Pennucci +42

We report results from continued timing observations of PSR J0740+6620, a high-mass, 2.8-ms radio pulsar in orbit with a likely ultra-cool white dwarf companion. Our data set consi…

astro-ph.HE2021★ 23 cited

High Precision Measurements of Interstellar Dispersion Measure with the upgraded GMRT

M. A. Krishnakumar, P. K. Manoharan, Bhal Chandra Joshi +19

Pulsar radio emission undergoes dispersion due to the presence of free electrons in the interstellar medium (ISM). The dispersive delay in the arrival time of pulsar signal changes…