activity
20042026
most citedLOFAR: The LOw-Frequency ARray

2.7k citations · 9.3k across the 122 of their papers we have counts for

collaborators
Showing 2019Show all

8 papers · 1 filter

astro-ph.HE2019★ 18 cited

A LOFAR radio search for single and periodic pulses from M31

Joeri van Leeuwen, Klim Mikhailov, Evan Keane +5

Bright, short radio bursts are emitted by sources at a large range of distances: from the nearby Crab pulsar to remote Fast Radio Bursts (FRBs). FRBs are likely to originate from d…

astro-ph.HE2019★ 31 cited

Synthesizing the intrinsic FRB population using frbpoppy

D. W. Gardenier, J. van Leeuwen, L. Connor +1

Fast Radio Bursts (FRBs) are radio transients of an unknown origin. Naturally, we are curious as to their nature. Enough FRBs have been detected for a statistical approach to parts…

astro-ph.HE2019★ 85 cited

Radio emission from a pulsar's magnetic pole revealed by general relativity

Gregory Desvignes, Michael Kramer, Kejia Lee +7

Binary pulsars are affected by general relativity (GR), causing the spin axes of each pulsar to precess. We present polarimetric radio observations of PSR J1906+0746 that demonstra…

astro-ph.HE2019★ 31 cited

A LOFAR census of non-recycled pulsars: extending below 80 MHz

A. V. Bilous, L. Bondonneau, V. I. Kondratiev +9

We present the results from the low-frequency (40--78 MHz) extension of the first LOFAR pulsar census of non-recycled pulsars. We have used the Low-Band Antennas of the LOFAR core…

astro-ph.HE2019★ 41 cited

The Green Bank North Celestial Cap Pulsar Survey. V. Pulsar Census and Survey Sensitivity

Alexander McEwen, Renee Spiewak, Joseph Swiggum +23

The Green Bank North Celestial Cap (GBNCC) pulsar survey will cover the entire northern sky () at 350 MHz, and is one of the most uniform and sensitive all-sky pulsar…

astro-ph.HE2019★ 32 cited

Eight Millisecond Pulsars Discovered in the Arecibo PALFA Survey

E. Parent, V. M. Kaspi, S. M. Ransom +18

We report on eight millisecond pulsars (MSPs) in binary systems discovered with the Arecibo PALFA survey. Phase-coherent timing solutions derived from 2.5 to 5 years of observation…