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20032009
most citedAn Eccentric Binary Millisecond Pulsar in the Galactic Plane

193 citations · 236 across the 5 of their papers we have counts for

collaborators

8 papers

astro-ph.HE20094 cited

Constraining the Bulk Properties of Dense Matter by Measuring Millisecond Pulsar Masses - A White Paper for the Astronomy and Astrophysics Decadal Survey, CFP Panel

Paulo C. Freire, David Nice, James Lattimer +4

More than four decades after the discovery of pulsars, the composition of matter at their cores is still a mystery. This white paper summarizes how recent high-precision measuremen…

astro-ph200837 cited

PSR J1856+0245: Arecibo Discovery of a Young, Energetic Pulsar Coincident with the TeV Gamma-ray Source HESS J1857+026

J. W. T. Hessels, D. J. Nice, B. M. Gaensler +21

We present the discovery of the Vela-like radio pulsar J1856+0245 in the Arecibo PALFA survey. PSR J1856+0245 has a spin period of 81ms, a characteristic age of 21kyr, and a spin-d…

astro-ph2008193 cited

An Eccentric Binary Millisecond Pulsar in the Galactic Plane

D. J. Champion, S. M. Ransom, P. Lazarus +28

Binary pulsar systems are superb probes of stellar and binary evolution and the physics of extreme environments. In a survey with the Arecibo telescope, we have found PSR J1903+032…

astro-ph20072 cited

Pulsar surveys present and future: The Arecibo pulsar-ALFA survey and projected SKA survey

J. S. Deneva

The Arecibo Pulsar-ALFA (PALFA) survey of the Galactic plane began in 2004 when the new ALFA (Arecibo L-band Feed Array) receiver was commissioned. It is slated to continue for the…

astro-ph2006

Arecibo and the ALFA Pulsar Survey

J. van Leeuwen, J. M. Cordes, D. R. Lorimer +34

The recently started Arecibo L-band Feed Array (ALFA) pulsar survey aims to find ~1000 new pulsars. Due to its high time and frequency resolution the survey is especially sensitive…

astro-ph2005

The young, highly relativistic binary pulsar J1906+0746

D. R. Lorimer, I. H. Stairs, P. C. C. Freire +33

We report the discovery of PSR J1906+0746, a young 144-ms pulsar in a highly relativistic 3.98-hr orbit with an eccentricity of 0.085 and expected gravitational wave coalescence ti…