activity
19962026
most citedShapiro delay measurement of a two solar mass neutron star

3.9k citations · 48.4k across the 396 of their papers we have counts for

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Showing 2008Show all

9 papers · 1 filter

astro-ph2008★ 4 cited

The Full Spectrum Galactic Terrarium: MHz to TeV Observations of Various Critters

Mallory S. E. Roberts, C. Brogan, S. Ransom +13

Multi-wavelength studies at radio, infrared, optical, X-ray, and TeV wavelengths have discovered probable counterparts to many Galactic sources of GeV emission detected by EGRET. T…

astro-ph2008★ 134 cited

Arecibo Pulsar Survey Using ALFA: Probing Radio Pulsar Intermittency and Transients

J. S. Deneva, J. M. Cordes, M. A. McLaughlin +23

We present radio transient search algorithms, results, and statistics from the ongoing Arecibo Pulsar ALFA (PALFA) Survey of the Galactic plane. We have discovered seven objects by…

astro-ph2008★ 97 cited

Pulsar Timing for the Fermi Gamma-ray Space Telescope

D. A. Smith, L. Guillemot, F. Camilo +25

We describe a comprehensive pulsar monitoring campaign for the Large Area Telescope (LAT) on the {\em Fermi Gamma-ray Space Telescope} (formerly GLAST). The detection and study of…

astro-ph2008★ 47 cited

Discovery of High-Energy Gamma-Ray Pulsations from PSR J2021+3651 with AGILE

J. P. Halpern, F. Camilo, A. Giuliani +7

Discovered after the end of the Compton Gamma-Ray Observatory mission, the radio pulsar PSR J2021+3651 was long considered a likely counterpart of the high-energy gamma-ray source…

astro-ph2008

Relativistic Spin Precession in the Double Pulsar

Rene P. Breton, Victoria M. Kaspi, Michael Kramer +7

The double pulsar PSR J0737-3039A/B consists of two neutron stars in a highly relativistic orbit that displays a roughly 30-second eclipse when pulsar A passes behind pulsar B. Des…

astro-ph2008★ 33 cited

Chandra X-Ray Observatory Observations of the Globular Cluster M71

R. F. Elsner, C. O. Heinke, H. N. Cohn +12

We observed the nearby, low-density globular cluster M71 (NGC 6838) with the Chandra X-ray Observatory to study its faint X-ray populations. Five X-ray sources were found inside th…