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1.1k citations · 2.6k across the 34 of their papers we have counts for

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astro-ph2008★ 48 cited

High-Resolution Timing Observations of Spin-Powered Pulsars with the AGILE Gamma-Ray Telescope

A. Pellizzoni, M. Pilia, A. Possenti +67

AGILE is a small gamma-ray astronomy satellite mission of the Italian Space Agency dedicated to high-energy astrophysics launched in 2007 April. Its 1 microsecond absolute time tag…

astro-ph2008★ 43 cited

Discovery of a Young, Energetic 70.5 ms Pulsar Associated with the TeV Gamma-ray Source HESS J1837-069

E. V. Gotthelf, J. P. Halpern

We report the discovery of 70.5 ms pulsations from the X-ray source AX J1838.0-0655 using the Rossi X-ray Timing Explorer (RXTE). PSR J1838-0655 is a rotation-powered pulsar with s…

astro-ph2008★ 134 cited

The magnetar 1E 1547.0-5408: radio spectrum, polarimetry, and timing

F. Camilo, J. Reynolds, S. Johnston +2

We have investigated the radio emission from the anomalous X-ray pulsar 1E 1547.0-5408 (PSR J1550-5418) using the Parkes telescope and the Australia Telescope Compact Array. The fl…

astro-ph2007★ 18 cited

X-ray Observations and Infrared Identification of the Transient 7.8 s X-ray Binary Pulsar XTE J1829-098

J. P. Halpern, E. V. Gotthelf

XMM-Newton and Chandra observations of the transient 7.8 s pulsar XTE J1829-098 are used to characterize its pulse shape and spectrum, and to facilitate a search for an optical or…

astro-ph2007★ 32 cited

The Next Geminga: Search for Radio and X-ray Pulsations from the Neutron Star Identified with 3EG J1835+5918

J. P. Halpern, F. Camilo, E. V. Gotthelf

We report unsuccessful searches for pulsations from the neutron star RX J1836.2+5925 identified with the EGRET source 3EG J1835+5918. A 24 hr observation with the NRAO Green Bank T…

astro-ph2007★ 26 cited

GRB 050826: A Subluminous Event at z = 0.296 Finds its Place in the Luminosity Distribution of Gamma-Ray Burst Afterglows

N. Mirabal, J. P. Halpern, P. T. O'Brien

We present the optical identification and spectroscopy of the host galaxy of GRB 050826 at a redshift z = 0.296 +/- 0.001. Image subtraction among observations obtained on three co…