activity
19962017
most citedCosmic Ray Acceleration at the Forward Shock in Tycho's Supernova Remnant: Evidence from Chandra X-ray Observations

313 citations · 1.1k across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.HE2017★ 19 cited

The fading of Cassiopeia A, and improved models for the absolute spectrum of primary radio calibration sources

A. S. Trotter, D. E. Reichart, R. E. Egger +20

Based on five years of observations with the 40-foot telescope at Green Bank Observatory (GBO), Reichart & Stephens (2000) found that the radio source Cassiopeia A had either faded…

astro-ph.GA2013★ 118 cited

On the Radio Polarization Signature of Efficient and Inefficient Particle Acceleration in Supernova Remnant SN 1006

Estela M. Reynoso, John P. Hughes, David A. Moffett

We present a radio polarization study of SN 1006, based on combined VLA and ATCA observations at 20 cm that resulted in sensitive images with an angular resolution of 10 arcsec. Th…

astro-ph.HE2012★ 46 cited

A Broadband Study of the Emission from the Composite Supernova Remnant MSH 11-62

Patrick Slane, John P. Hughes, Tea Temim +10

MSH 11-62 (G291.1-0.9) is a composite supernova remnant for which radio and X-ray observations have identified the remnant shell as well as its central pulsar wind nebula. The obse…

astro-ph.HE2011★ 103 cited

Evidence For Particle Acceleration to the Knee of the Cosmic Ray Spectrum in Tycho's Supernova Remnant

Kristoffer A. Eriksen, John P. Hughes, Carles Badenes +7

Supernova remnants (SNRs) have long been assumed to be the source of cosmic rays (CRs) up to the "knee" of the CR spectrum at 10^15 eV, accelerating particles to relativistic energ…

astro-ph2008★ 116 cited

Morphological evidence for azimuthal variations of the cosmic ray ion acceleration at the blast wave of SN 1006

Gamil Cassam-Chenai, John P. Hughes, Estela M. Reynoso +2

Using radio, X-ray and optical observations, we present evidence for morphological changes due to efficient cosmic ray ion acceleration in the structure of the southeastern region…

astro-ph2006★ 13 cited

Correlation between X-ray Lightcurve Shape and Radio Arrival Time in the Vela Pulsar

A. Lommen, J. Donovan, C. Gwinn +6

We report the results of simultaneous observations of the Vela pulsar in X-rays and radio from the RXTE satellite and the Mount Pleasant Radio Observatory in Tasmania. We sought co…