activity
20022016
most citedA low-frequency radio halo associated with a cluster of galaxies

255 citations · 439 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2016★ 58 cited

Exploring the Transient Radio Sky with VLITE: Early Results

E. Polisensky, W. M. Lane, S. D. Hyman +6

We report on a search for radio transients at 340 MHz with the Jansky Very Large Array (VLA) Low band Ionospheric and Transient Experiment (VLITE). Between 2015 July 29 and 2015 Se…

physics.space-ph2012★ 18 cited

Climatology of Mid-latitude Ionospheric Disturbances from the Very Large Array Low-frequency Sky Survey

J. F. Helmboldt, W. M. Lane, W. D. Cotton

The results of a climatological study of ionospheric disturbances derived from observations of cosmic sources from the Very Large Array (VLA) Low-frequency Sky Survey (VLSS) are pr…

astro-ph.IM2012★ 60 cited

VLSS Redux: Software Improvements applied to the Very Large Array Low-frequency Sky Survey

W. M. Lane, W. D. Cotton, J. F. Helmboldt +1

We present details of improvements to data processing and analysis which were recently used for a re-reduction of the Very Large Array (VLA) Low-frequency Sky Survey (VLSS) data. A…

astro-ph2008★ 255 cited

A low-frequency radio halo associated with a cluster of galaxies

G. Brunetti, S. Giacintucci, R. Cassano +7

Clusters of galaxies are the largest gravitationally bound objects in the Universe, containing about 10^15 solar masses of hot (10^8 K) gas, galaxies and dark matter in a typical v…

astro-ph2007★ 24 cited

Radio Frequency Spectra of 388 Bright 74 MHz Sources

J. F. Helmboldt, N. E. Kassim, A. S. Cohen +2

As a service to the community, we have compiled radio frequency spectra from the literature for all sources within the VLA Low Frequency Sky Survey (VLSS) that are brighter than 15…

astro-ph2002★ 24 cited

3C 129 at 90cm: Evidence for a Radio Relic?

W. M. Lane, N. E. Kassim, T. A. Ensslin +2

We present a new wide-field map of the radio galaxy 3C 129 and its companion galaxy 3C 129.1 at lambda=90 cm. We see a distinct steep-spectrum feature near the head of 3C 129, exte…