activity
19982026
most citedFast Radio Bursts

590 citations · 5.7k across the 92 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

6 papers · 1 filter

astro-ph.GA2011★ 31 cited

Arecibo PALFA Survey and Einstein@Home: Binary Pulsar Discovery by Volunteer Computing

B. Knispel, P. Lazarus, B. Allen +35

We report the discovery of the 20.7 ms binary pulsar J1952+2630, made using the distributed computing project Einstein@Home in Pulsar ALFA survey observations with the Arecibo tele…

astro-ph.GA2010★ 314 cited

On the nature and evolution of the unique binary pulsar J1903+0327

P. C. C. Freire, C. G. Bassa, N. Wex +16

(abridged) PSR J1903+0327, a millisecond pulsar in an eccentric (e = 0.44) 95-day orbit with a (~ 1Msun) companion poses a challenge to our understanding of stellar evolution in bi…

astro-ph.GA2010

Probing fundamental physics with pulsars

D. R. Lorimer, M. A. McLaughlin

Pulsars provide a wealth of information about General Relativity, the equation of state of superdense matter, relativistic particle acceleration in high magnetic fields, the Galaxy…

astro-ph.GA2010★ 30 cited

Lutz-Kelker bias in pulsar parallax measurements

J. P. W. Verbiest, D. R. Lorimer, M. A. McLaughlin

Lutz & Kelker showed that parallax measurements are systematically overestimated because they do not properly account for the larger volume of space that is sampled at smaller para…

astro-ph.GA2009★ 87 cited

New Limits on Radio Emission from X-ray Dim Isolated Neutron Stars

V. I. Kondratiev, M. A. McLaughlin, D. R. Lorimer +5

We have carried out a search for radio emission at 820 MHz from six X-ray dim isolated neutron stars with the Robert C. Byrd Green Bank Radio Telescope. No transient or pulsed emis…

astro-ph.GA2009★ 37 cited

Discovery of the energetic pulsar J1747-2809 in the supernova remnant G0.9+0.1

F. Camilo, S. M. Ransom, B. M. Gaensler +1

The supernova remnant G0.9+0.1 has long been inferred to contain a central energetic pulsar. In observations with the NRAO Green Bank Telescope at 2 GHz, we have detected radio pul…