activity
19942025
most citedA Radio Counterpart to a Neutron Star Merger

543 citations · 6.2k across the 97 of their papers we have counts for

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Showing 2005Show all

9 papers · 1 filter

astro-ph2005★ 25 cited

A New Radio Detection of the Bursting Source GCRT J1745-3009

Scott D. Hyman, T. Joseph W. Lazio, Subhashis Roy +2

GCRT J1745-3009 is a transient bursting radio source located in the direction of the Galactic center, discovered in 330 MHz VLA observations from 2002 September 30--October 1 by Hy…

astro-ph2005★ 122 cited

Evidence for a Weak Galactic Center Magnetic Field from Diffuse Low Frequency Nonthermal Radio Emission

T. N. LaRosa, C. L. Brogan, S. N. Shore +3

New low-frequency 74 and 330 MHz observations of the Galactic center (GC) region reveal the presence of a large-scale ($6\arcdeg\times 2\arcdeg$) diffuse source of nonthermal synch…

astro-ph2005★ 65 cited

Discovery of a Radio Supernova Remnant and Non-thermal X-rays Coincident with the TeV Source HESS J1813-178

C. L. Brogan, B. M. Gaensler, J. D. Gelfand +4

We present the discovery of non-thermal radio and X-ray emission positionally coincident with the TeV -ray source HESS J1813--178. We demonstrate that the non-thermal radio emis…

astro-ph2005★ 51 cited

Low Frequency Radio Observations of X-ray Ghost Bubbles in Abell 2597: A History of Radio Activity in the Core

T. E. Clarke, C. L. Sarazin, E. L. Blanton +2

A previous analysis of the Chandra X-ray image of the center of the cooling core cluster Abell 2597 showed two ``ghost holes'' in the X-ray emission to the west and northeast of th…

astro-ph2005★ 21 cited

Spatially Resolved Low Frequency VLA observations of the Supernova Remnant 3C 391

C. L. Brogan, T. J. Lazio, N. E. Kassim +1

We present VLA images of the supernova remnant (SNR) 3C~391 at 74, 330, and 1465 MHz. This remnant has been known for some time to exhibit a turnover in its integrated radio contin…

astro-ph2005★ 183 cited

A powerful bursting radio source towards the Galactic Centre

S. D. Hyman, T. J. W. Lazio, N. E. Kassim +3

Transient astronomical sources are typically powered by compact objects and usually signify highly explosive or dynamic events. While radio astronomy has an impressive record of ob…