activity
20012014
most citedA High-Resolution Study of Nonthermal Radio and X-Ray Emission from SNR G347.3-0.5

134 citations · 801 across the 16 of their papers we have counts for

collaborators

15 papers

astro-ph.HE2014★ 3 cited

ASTRO-H White Paper - Young Supernova Remnants

J. P. Hughes, S. Safi-Harb, A. Bamba +23

Thanks to the unprecedented spectral resolution and sensitivity of the Soft X-ray Spectrometer (SXS) to soft thermal X-ray emission, ASTRO-H will open a new discovery window for un…

astro-ph.HE2014★ 1 cited

ASTRO-H White Paper - Older Supernova Remnants and Pulsar Wind Nebulae

K. S. Long, A. Bamba, F. Aharonian +20

Most supernova remnants (SNRs) are old, in the sense that their structure has been profoundly modified by their interaction with the surrounding interstellar medium (ISM). Old SNRs…

astro-ph.HE2014★ 6 cited

A CR-hydro-NEI Model of the Structure and Broadband Emission from Tycho's SNR

P. Slane, S. -H. Lee, D. C. Ellison +5

Tycho's supernova remnant (SNR) is well-established as a source of particle acceleration to very high energies. Constraints from numerous studies indicate that the observed gamma-r…

astro-ph.IM2012★ 106 cited

The ASTRO-H X-ray Observatory

Tadayuki Takahashi, Kazuhisa Mitsuda, Richard Kelley +220

The joint JAXA/NASA ASTRO-H mission is the sixth in a series of highly successful X-ray missions initiated by the Institute of Space and Astronautical Science (ISAS). ASTRO-H will…

astro-ph.HE2011★ 44 cited

A Chandra Observation of Supernova Remnant G350.1-0.3 and Its Central Compact Object

Igor Lovchinsky, Patrick Slane, Bryan Gaensler +5

We present a new Chandra observation of supernova remnant (SNR) G350.1-0.3. The high resolution X-ray data reveal previously unresolved filamentary structures and allow us to perfo…

astro-ph.CO2010★ 130 cited

X-ray Temperature and Mass Measurements to the Virial Radius of Abell 1413 with Suzaku

A. Hoshino, J. P. Henry, K. Sato +14

We present X-ray observations of the northern outskirts of the relaxed galaxy cluster A1413 with Suzaku, whose XIS instrument has the low intrinsic background needed to make measur…