activity
19982007
most citedThe characteristics of millisecond pulsar emission: III.From low to high frequencies

153 citations · 571 across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph2007★ 36 cited

Arecibo HI Absorption Measurements of Pulsars and the Electron Density at Intermediate Longitudes in the First Galactic Quadrant

J. M. Weisberg, S. Stanimirovic, K. Xilouris +4

We have used the Arecibo telescope to measure the HI absorption spectra of eight pulsars. We show how kinematic distance measurements depend upon the values of the galactic constan…

astro-ph2006★ 21 cited

Abundant dust found in intergalactic space

E. Xilouris, P. Alton, J. Alikakos +3

Galactic dust constitutes approximately half of the elements more massive than helium produced in stellar nucleosynthesis. Notwithstanding the formation of dust grains in the dense…

astro-ph2005★ 97 cited

Arecibo timing and single-pulse observations of 17 pulsars

D. J. Champion, D. R. Lorimer, M. A. McLaughlin +6

We report on timing and single-pulse observations of 17 pulsars discovered at the Arecibo observatory. The highlights of our sample are the recycled pulsars J1829+2456, J1944+0907…

astro-ph2005★ 24 cited

Discovery of 10 pulsars in an Arecibo drift-scan survey

D. R. Lorimer, K. M. Xilouris, A. S. Fruchter +8

We present the results of a 430-MHz survey for pulsars conducted during the upgrade to the 305-m Arecibo radio telescope. Our survey covered a total of 1147 square degrees of sky u…

astro-ph2004★ 3 cited

New Binary and Millisecond Pulsars from Arecibo Drift-Scan Searches

M. A. McLaughlin, D. R. Lorimer, D. J. Champion +6

We discuss four recycled pulsars found in Arecibo drift-scan searches. PSR J1944+0907 has a spin period of 5.2 ms and is isolated. The 5.8-ms pulsar J1453+19 may have a low-mass co…

astro-ph2003★ 1 cited

New Pulsars Discovered in Arecibo Drift-Scan Searches

M. A. McLaughlin, D. R. Lorimer, D. J. Champion +6

We report on new pulsars discovered in Arecibo drift-scan data. Processing of 2200 square degrees of data has resulted in the detection of 41 known and 12 new pulsars. New pulsars…