activity
19992026
most citedThe Second Fermi Large Area Telescope Catalog of Gamma-ray Pulsars

837 citations · 5k across the 60 of their papers we have counts for

collaborators
Showing 2010Show all

6 papers · 1 filter

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★ 77 cited

The Evolution of PSR J0737-3039B and a Model for Relativistic Spin Precession

Benetge Perera, Maura McLaughlin, Michael Kramer +9

We present the evolution of the radio emission from the 2.8-s pulsar of the double pulsar system PSR J0737-3039A/B. We provide an update on the Burgay et al. (2005) analysis by des…

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★ 14 cited

Near-infrared observations of Rotating Radio Transients

N. Rea, G. Lo Curto, V. Testa +6

We report on the first near-infrared observations obtained for Rotating RAdio Transients (RRATs). Using adaptive optics devices mounted on the ESO Very Large Telescope (VLT), we ob…

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.GA2010★ 64 cited

Observations and Modelling of Relativistic Spin Precession in PSR J1141-6545

R. N. Manchester, M. Kramer, I. H. Stairs +10

Observations of the binary pulsar PSR J1141-6545 using the Parkes radio telescope over 9.3 years show clear time-variations in pulse width, shape and polarization. We interpret the…