activity
20152021
most citedRates, Flux Densities, and Spectral Indices of Meteor Radio Afterglows

18 citations · 47 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.EP2021

Broadband Imaging to Study the Spectral Distribution of Meteor Radio Afterglows

S. S. Varghese, J. Dowell, K. S. Obenberger +2

We present observations of 86 meteor radio afterglows (MRAs) using the new broadband imager at the Long Wavelength Array Sevilleta (LWA-SV) station. The MRAs were detected using th…

astro-ph.HE202018 cited

Detection of a Low-frequency Cosmic Radio Transient Using Two LWA Stations

S. S. Varghese, K. S. Obenberger, J. Dowell +1

We report the detection of a potential cosmic radio transient source using the two stations of the Long Wavelength Array. The transient was detected on 18 October 2017 08:47 UTC ne…

astro-ph.EP20209 cited

Testing the Radiation Pattern of Meteor Radio Afterglow

S. S. Varghese, K. S. Obenberger, G. B. Taylor +1

Radio emission from meteors or meteor radio afterglows (MRAs) were first detected using the all-sky imaging capabilities of the first station of the Long Wavelength Array (LWA1). I…

astro-ph.IM20171 cited

Bifrost: a Python/C++ Framework for High-Throughput Stream Processing in Astronomy

Miles D. Cranmer, Benjamin R. Barsdell, Danny C. Price +11

Radio astronomy observatories with high throughput back end instruments require real-time data processing. While computing hardware continues to advance rapidly, development of rea…

astro-ph.EP201618 cited

Rates, Flux Densities, and Spectral Indices of Meteor Radio Afterglows

K. S. Obenberger, J. D. Dowell, P. J. Hancock +4

Using the narrowband all-sky imager mode of the LWA1 we have now detected 30 transients at 25.6 MHz, 1 at 34 MHz, and 93 at 38.0 MHz. While we have only optically confirmed that 37…

astro-ph.IM20151 cited

Monitoring the Sky with the Prototype All-Sky Imager on the LWA1

K. S. Obenberger, G. B. Taylor, J. M. Hartman +8

We present a description of the Prototype All-Sky Imager (PASI), a backend correlator and imager of the first station of the Long Wavelength Array (LWA1). PASI cross-correlates a l…