activity
20092026
most citedThe Millisecond Radio Sky: Transients from a Blind Single Pulse Search

123 citations · 444 across the 10 of their papers we have counts for

collaborators

13 papers

astro-ph.HE2026

Constraints on Supermassive Black Hole Binaries from the Lack of Resolvable Sources in the NANOGrav 15-yr Dataset

Emiko C. Gardiner, Kayhan Gültekin, Philippe Turgeon +116

Pulsar timing arrays (PTAs) have found evidence of a gravitational wave background (GWB) consistent with a population of supermassive black hole binaries (SMBHBs), but have not yet…

astro-ph.IM2026

Pulsar Timing Array Sensitivity to Anisotropy: Empirical Sensitivity Curves, Scaling Relations, and the Multi-Resolution Pixel Basis

Taha T. Moursy, Nihan S. Pol, Gabriella Agazie +115

We quantify pulsar timing array (PTA) sensitivity to anisotropy in the gravitational wave background using the cross-correlation based Fisher information matrix in the pixel and sp…

astro-ph.CO2026

The NANOGrav 15 yr Data Set: Impacts of Customized Chromatic Noise Models on Gravitational Wave Analyses

Nikita Agarwal, Gabriella Agazie, Alessandra Amosso +120

We report updated nHz gravitational wave (GW) significance, characterization, and interpretations using the customized chromatic-noise models (CNMs) developed in Larsen, Baier et a…

astro-ph.HE2026

Gravitational Wave Measurement of the - Intrinsic Scatter at High Redshift

Cayenne Matt, Kayhan Gültekin, Gabriella Agazie +109

The observed GWB spectrum is higher in amplitude than model predictions by a factor of 2-3. Using a semi-analytic model, we evaluate the effect of a high-scatter supermassive black…

astro-ph.GA2026

Chandra X-ray Observations of Quasars with Velocity-Offset Broad Lines: Assessing the Binary Supermassive Black Hole Hypothesis

Peter Breiding, Michael Eracleous, Tamara Bogdanović +2

During the final stages of a galaxy merger, dynamical friction acting on the supermassive black holes (SMBHs) in the post-merger remnant can lead to the formation of a gravitationa…

astro-ph.HE2018

Multiple messengers of fast radio bursts

Sarah Burke-Spolaor

We review the potential information that can be gleaned from multi-wavelength and multi-messenger detections of Fast Radio Bursts (FRBs). The primary function of such detections, f…

astro-ph.GA2017★ 14 cited

A Radio Relic and a Search for the Central Black Hole in the Abell 2261 Brightest Cluster Galaxy

Sarah Burke-Spolaor, Kayhan Gultekin, Marc Postman +4

We present VLA images and HST/STIS spectra of sources within the center of the brightest cluster galaxy (BCG) in Abell 2261. These observations were obtained to test the hypothesis…

astro-ph.SR2012★ 8 cited

Rotating Radio Transients and Their Place Among Pulsars

S. Burke-Spolaor

Six years ago, the discovery of Rotating Radio Transients (RRATs) marked what appeared to be a new type of sparsely-emitting pulsar. Since 2006, more than 70 of these objects have…

astro-ph.SR2011★ 27 cited

Rotation measure variations for 20 millisecond pulsars

Wenming Yan, R. N. Manchester, Willem van Straten +14

We report on variations in the mean position angle of the 20 millisecond pulsars being observed as part of the Parkes Pulsar Timing Array (PPTA) project. It is found that the obser…

astro-ph.SR2011★ 95 cited

The High Time Resolution Universe Survey - III. Single-pulse searches and preliminary analysis

S. Burke-Spolaor, M. Bailes, S. Johnston +12

We present the search methods and initial results for transient radio signals in the High Time Resolution Universe (HTRU) Survey. The HTRU survey's single-pulse search, the softwar…

astro-ph.SR2011★ 51 cited

The High Time Resolution Universe Survey II: Discovery of 5 Millisecond Pulsars

S. D. Bates, M. Bailes, N. D. R. Bhat +13

We present the discovery of 5 millisecond pulsars found in the mid-Galactic latitude portion of the High Time Resolution Universe (HTRU) Survey. The pulsars have rotational periods…

astro-ph.EP2010★ 112 cited

Measuring the mass of solar system planets using pulsar timing

D. J. Champion, G. B. Hobbs, R. N. Manchester +19

High-precision pulsar timing relies on a solar-system ephemeris in order to convert times of arrival (TOAs) of pulses measured at an observatory to the solar system barycenter. Any…

astro-ph.SR2009★ 123 cited

The Millisecond Radio Sky: Transients from a Blind Single Pulse Search

S. Burke-Spolaor, M. Bailes

We present the results of a search for transient radio bursts of between 0.125 and 32 millisecond duration in two archival pulsar surveys of intermediate galactic latitudes with th…