activity
20062021
most citedA fast radio burst associated with a Galactic magnetar

767 citations · 3.1k across the 27 of their papers we have counts for

collaborators

27 papers

astro-ph.IM2021★ 20 cited

COMAP Early Science: II. Pathfinder Instrument

James W. Lamb, Kieran A. Cleary, David P. Woody +32

Line intensity mapping (LIM) is a new technique for tracing the global properties of galaxies over cosmic time. Detection of the very faint signals from redshifted carbon monoxide…

astro-ph.CO2021★ 64 cited

COMAP Early Science: I. Overview

Kieran A. Cleary, Jowita Borowska, Patrick C. Breysse +40

The CO Mapping Array Project (COMAP) aims to use line intensity mapping of carbon monoxide (CO) to trace the distribution and global properties of galaxies over cosmic time, back t…

astro-ph.IM2020★ 7 cited

A Broadband Digital Spectrometer for the Deep Space Network

Kristen Virkler, Jonathon Kocz, Melissa Soriano +3

The Deep Space Network (DSN) enables NASA to communicate with its spacecraft in deep space. By virtue of its large antennas, the DSN can also be used as a powerful instrument for r…

astro-ph.HE2020★ 32 cited

Multiwavelength Radio Observations of Two Repeating Fast Radio Burst Sources: FRB 121102 and FRB 180916.J0158+65

Aaron B. Pearlman, Walid A. Majid, Thomas A. Prince +4

The spectra of fast radio bursts (FRBs) encode valuable information about the source's local environment, underlying emission mechanism(s), and the intervening media along the line…

astro-ph.HE2020★ 767 cited

A fast radio burst associated with a Galactic magnetar

Christopher D. Bochenek, Vikram Ravi, Konstantin V. Belov +4

Since their discovery in 2007, much effort has been devoted to uncovering the sources of the extragalactic, millisecond-duration fast radio bursts (FRBs). A class of neutron star k…

astro-ph.HE2020★ 7 cited

Bright X-ray and Radio Pulses from a Recently Reactivated Magnetar

Aaron B. Pearlman, Walid A. Majid, Thomas A. Prince +9

Magnetars are young, rotating neutron stars that possess larger magnetic fields ( - G) and longer rotational periods ( 1-12 s) than ordi…