activity
19992023
most citedThe Angular Size and Proper Motion of the Afterglow of GRB 030329

165 citations · 966 across the 23 of their papers we have counts for

collaborators

23 papers

astro-ph.HE2023

Cannonball or Bowling Ball: A Proper Motion and Parallax for PSR J0002+6216

S. Bruzewski, F. K. Schinzel, G. B. Taylor +4

We report the results of careful astrometric measurements of the Cannonball pulsar J0002+6216 carried out over three years using the High Sensitivity Array (HSA). We significantly…

astro-ph.HE2023★ 2 cited

Compact Symmetric Objects -- III Evolution of the High-Luminosity Branch and a Possible Connection with Tidal Disruption Events

A. C. S. Readhead, V. Ravi, R. D. Blandford +18

We use a sample of 54 Compact Symmetric Objects (CSOs) to confirm that there are two unrelated CSO classes: an edge-dimmed, low-luminosity class (CSO~1), and an edge-brightened, hi…

astro-ph.HE2023★ 6 cited

Resolving the bow shock and tail of the cannonball pulsar PSR J0002+6216

P. Kumar, F. K. Schinzel, G. B. Taylor +4

We present X-ray and radio observations of the recently-discovered bow shock pulsar wind nebula associated with PSR J0002+6216, characterizing the PWN morphology, which was unresol…

astro-ph.HE2022★ 12 cited

A Combined Radio Multi-Survey Catalog of Fermi Unassociated Sources

S. Bruzewski, F. K. Schinzel, G. B. Taylor

Approximately one-third of existing -ray sources identified by the are considered to be unassociated, with no known counterpart at oth…

astro-ph.GA2022★ 8 cited

Deep VLBI Observations Challenge Previous Evidence of a Binary Supermassive Black Hole Residing in the Seyfert Galaxy NGC 7674

Peter Breiding, Sarah Burke-Spolaor, Tao An +4

Previous Ku-band (15 GHz) imaging with data obtained from the Very Long Baseline Array (VLBA) had shown two compact, sub-pc components at the location of a presumed kpc-scale radio…

astro-ph.HE2022★ 15 cited

Pulsar Observations at Low Frequencies: Applications to Pulsar Timing and Solar Wind Models

P. Kumar, S. M. White, K. Stovall +2

Efforts are underway to use high-precision timing of pulsars in order to detect low-frequency gravitational waves. A limit to this technique is the timing noise generated by disper…