activity
20142021
most citedThe NANOGrav Nine-year Data Set: Mass and Geometric Measurements of Binary Millisecond Pulsars

653 citations · 2k across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.SR2021★ 29 cited

The NANOGrav 12.5-Year Data Set: Polarimetry and Faraday Rotation Measures from Observations of Millisecond Pulsars with the Green Bank Telescope

Haley M. Wahl, Maura McLaughlin, Peter A. Gentile +28

In this work, we present polarization profiles for 23 millisecond pulsars observed at 820 MHz and 1500 MHz with the Green Bank Telescope as part of the NANOGrav pulsar timing array…

astro-ph.HE2020★ 90 cited

Modeling the uncertainties of solar-system ephemerides for robust gravitational-wave searches with pulsar timing arrays

M. Vallisneri, S. R. Taylor, J. Simon +61

The regularity of pulsar emissions becomes apparent once we reference the pulses' times of arrivals to the inertial rest frame of the solar system. It follows that errors in the de…

astro-ph.HE2019★ 48 cited

The NANOGrav 11-Year Data Set: Limits on Gravitational Wave Memory

K. Aggarwal, Z. Arzoumanian, P. T. Baker +58

The mergers of supermassive black hole binaries (SMBHBs) promise to be incredible sources of gravitational waves (GWs). While the oscillatory part of the merger gravitational wavef…

astro-ph.EP2019★ 17 cited

The NANOGrav 11-year Data Set: Constraints on Planetary Masses Around 45 Millisecond Pulsars

E. A. Behrens, S. M. Ransom, D. R. Madison +27

We search for extrasolar planets around millisecond pulsars using pulsar timing data and seek to determine the minimum detectable planetary masses as a function of orbital period.…

astro-ph.HE2018★ 116 cited

Tests of Gravitational Symmetries with Pulsar Binary J1713+0747

W. W. Zhu, G. Desvignes, N. Wex +50

Symmetries play an important role in modern theories of gravity. The strong equivalence principle (SEP) constitutes a collection of gravitational symmetries which are all implement…

astro-ph.IM2017★ 30 cited

A Large-Diameter Hollow-Shaft Cryogenic Motor Based on a Superconducting Magnetic Bearing for Millimeter-Wave Polarimetry

B. R. Johnson, F. Columbro, D. Araujo +6

In this paper we present the design and measured performance of a novel cryogenic motor based on a superconducting magnetic bearing (SMB). The motor is tailored for use in millimet…

astro-ph.HE2016★ 92 cited

The NANOGrav Nine-Year Data Set: Excess Noise in Millisecond Pulsar Arrival Times

M. T. Lam, J. M. Cordes, S. Chatterjee +22

Gravitational wave astronomy using a pulsar timing array requires high-quality millisecond pulsars, correctable interstellar propagation delays, and high-precision measurements of…

astro-ph.HE2016★ 653 cited

The NANOGrav Nine-year Data Set: Mass and Geometric Measurements of Binary Millisecond Pulsars

Emmanuel Fonseca, Timothy T. Pennucci, Justin A. Ellis +17

We analyze 24 binary radio pulsars in the North American Nanohertz Observatory for Gravitational Waves (NANOGrav) nine-year data set. We make fourteen significant measurements of S…

astro-ph.IM2015★ 64 cited

The NANOGrav Nine-Year Data Set: Noise Budget for Pulsar Arrival Times on Intraday Timescales

M. T. Lam, J. M. Cordes, S. Chatterjee +21

The use of pulsars as astrophysical clocks for gravitational wave experiments demands the highest possible timing precision. Pulse times of arrival (TOAs) are limited by stochastic…

astro-ph.IM2015★ 13 cited

Single-Source Gravitational Wave Limits from the J1713+0747 24-hr Global Campaign

T. Dolch, J. A. Ellis, S. Chatterjee +34

Dense, continuous pulsar timing observations over a 24-hr period provide a method for probing intermediate gravitational wave (GW) frequencies from 10 microhertz to 20 millihertz.…

astro-ph.GA2015★ 321 cited

The NANOGrav Nine-year Data Set: Limits on the Isotropic Stochastic Gravitational Wave Background

Zaven Arzoumanian, Adam Brazier, Sarah Burke-Spolaor +45

We compute upper limits on the nanohertz-frequency isotropic stochastic gravitational wave background (GWB) using the 9-year data release from the North American Nanohertz Observat…

astro-ph.IM2015★ 219 cited

The NANOGrav Nine-year Data Set: Observations, Arrival Time Measurements, and Analysis of 37 Millisecond Pulsars

Z. Arzoumanian, A. Brazier, S. Burke-Spolaor +41

We present high-precision timing observations spanning up to nine years for 37 millisecond pulsars monitored with the Green Bank and Arecibo radio telescopes as part of the North A…

astro-ph.SR2015★ 107 cited

Testing Theories of Gravitation Using 21-Year Timing of Pulsar Binary J1713+0747

W. W. Zhu, I. H. Stairs, P. B. Demorest +17

We report 21-yr timing of one of the most precise pulsars: PSR J1713+0747. Its pulse times of arrival are well modeled by a comprehensive pulsar binary model including its three-di…

astro-ph.GA2015★ 66 cited

NANOGrav Constraints on Gravitational Wave Bursts with Memory

Z. Arzoumanian, A. Brazier, S. Burke-Spolaor +39

Among efforts to detect gravitational radiation, pulsar timing arrays are uniquely poised to detect "memory" signatures, permanent perturbations in spacetime from highly energetic…

astro-ph.HE2014★ 46 cited

A 24-Hour Global Campaign To Assess Precision Timing of the Millisecond Pulsar J1713+0747

T. Dolch, M. T. Lam, J. M. Cordes +40

The radio millisecond pulsar J1713+0747 is regarded as one of the highest-precision clocks in the sky, and is regularly timed for the purpose of detecting gravitational waves. The…

astro-ph.GA2014★ 134 cited

NANOGrav Limits on Gravitational Waves from Individual Supermassive Black Hole Binaries in Circular Orbits

Z. Arzoumanian, A. Brazier, S. Burke-Spolaor +36

The North American Nanohertz Observatory for Gravitational Waves (NANOGrav) project currently observes 43 pulsars using the Green Bank and Arecibo radio telescopes. In this work we…