activity
20002013
most citedProbing eV-scale axions with CAST

221 citations · 255 across the 3 of their papers we have counts for

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astro-ph20065 cited

PSR J1119-6127 and the X-ray Emission from High Magnetic Field Radio Pulsars

M. E. Gonzalez, V. M. Kaspi, F. Camilo +2

The existence of radio pulsars having inferred magnetic fields in the magnetar regime suggests that possible transition objects could be found in the radio pulsar population. The d…

astro-ph2005

Time Variability in the X-ray Nebula Powered by Pulsar B1509-58

T. DeLaney, B. M. Gaensler, J. Arons +1

We use new and archival Chandra and ROSAT data to study the time variability of the X-ray emission from the pulsar wind nebula (PWN) powered by PSR B1509-58 on timescales of one we…

astro-ph2005

Unusual Pulsed X-ray Emission from the Young, High Magnetic Field Pulsar PSR J1119-6127

M. E. Gonzalez, V. M. Kaspi, F. Camilo +2

We present XMM-Newton observations of the radio pulsar PSR J1119-6127, which has an inferred age of 1,700 yr and surface dipole magnetic field strength of 4.1x10^13 G. We report th…

astro-ph2002

XMM-Newton observations of PSR B1823-13: An asymmetric synchrotron nebula around a Vela-like pulsar

Bryan Gaensler, Norbert Schulz, Vicky Kaspi +2

We present a deep observation with the X-ray Multi-Mirror Mission of PSR B1823-13, a young pulsar with similar properties to the Vela pulsar. We detect two components to the X-ray…

astro-ph2001

Chandra observations of PSR B1509-58 and Supernova Remnant G320.4-1.2

B. M. Gaensler, J. Arons, M. J. Pivovaroff +1

The young and energetic pulsar B1509-58 powers a bright X-ray synchrotron nebula, embedded in the unusual supernova remnant G320.4-1.2. We present observations of this system with…

astro-ph2001

A Sensitive Targeted Search Campaign at Parkes to Find Young Radio Pulsars at 20 cm

F. Crawford, M. J. Pivovaroff, V. M. Kaspi +1

We describe a sensitive targeted search campaign at Parkes to find faint young radio pulsars using the center beam of the 20-cm multibeam receiver. The high frequency of the receiv…