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20112026
most citedThe NANOGrav 11-year Data Set: High-precision timing of 45 Millisecond Pulsars

611 citations · 2.4k across the 27 of their papers we have counts for

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14 papers · 1 filter

astro-ph.HE2026

Generalized Non-linear Bayesian Pulsar Timing with Enterprise

Andrew R. Kaiser, Jeffrey S. Hazboun, Maura A. McLaughlin +56

In this study, we use the Bayesian methods in the Enterprise package to examine the fully general parameterization of pulsar timing models in tandem with noise. We investigate four…

astro-ph.HE2024★ 6 cited

The NANOGrav 12.5-Year Data Set: Probing Interstellar Turbulence and Precision Pulsar Timing with PSR J1903+0327

Abra Geiger, James M. Cordes, Michael T. Lam +33

Free electrons in the interstellar medium refract and diffract radio waves along multiple paths, resulting in angular and temporal broadening of radio pulses that limits pulsar tim…

astro-ph.HE2024★ 5 cited

Exploring pulsar timing precision: A comparative study of polarization calibration methods for NANOGrav data from the Green Bank Telescope

Lankeswar Dey, Maura A. McLaughlin, Haley M. Wahl +32

Pulsar timing array experiments have recently uncovered evidence for a nanohertz gravitational wave background by precisely timing an ensemble of millisecond pulsars. The next sign…

astro-ph.HE2023★ 17 cited

The NANOGrav 12.5-year data set: A computationally efficient eccentric binary search pipeline and constraints on an eccentric supermassive binary candidate in 3C 66B

Gabriella Agazie, Zaven Arzoumanian, Paul T. Baker +85

The radio galaxy 3C 66B has been hypothesized to host a supermassive black hole binary (SMBHB) at its center based on electromagnetic observations. Its apparent 1.05-year period an…

astro-ph.HE2023★ 41 cited

The NANOGrav 15-year Gravitational-Wave Background Methods

Aaron D. Johnson, Patrick M. Meyers, Paul T. Baker +93

Pulsar timing arrays (PTAs) use an array of millisecond pulsars to search for gravitational waves in the nanohertz regime in pulse time of arrival data. This paper presents rigorou…

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.HE2019★ 43 cited

The NANOGrav 11-Year Data Set: Evolution of Gravitational Wave Background Statistics

J. S. Hazboun, J. Simon, S. R. Taylor +60

An ensemble of inspiraling supermassive black hole binaries should produce a stochastic background of very low frequency gravitational waves. This stochastic background is predicte…

astro-ph.HE2018★ 45 cited

The NANOGrav 12.5-Year Data Set: The Frequency Dependence of Pulse Jitter in Precision Millisecond Pulsars

M. T. Lam, M. A. McLaughlin, Z. Arzoumanian +25

Low-frequency gravitational-wave experiments require the highest timing precision from an array of the most stable millisecond pulsars. Several known sources of noise on short time…

astro-ph.HE2018★ 52 cited

PSR J2234+0611: A new laboratory for stellar evolution

K. Stovall, P. C. C. Freire, J. Antoniadis +30

We report timing results for PSR J2234+0611, a 3.6-ms pulsar in a 32-day, eccentric (e = 0.13) orbit with a helium white dwarf companion discovered as part of the Arecibo Observato…

astro-ph.HE2018★ 611 cited

The NANOGrav 11-year Data Set: High-precision timing of 45 Millisecond Pulsars

Zaven Arzoumanian, Adam Brazier, Sarah Burke-Spolaor +53

We present high-precision timing data over time spans of up to 11 years for 45 millisecond pulsars observed as part of the North American Nanohertz Observatory for Gravitational Wa…

astro-ph.HE2017★ 71 cited

A Second Chromatic Timing Event of Interstellar Origin toward PSR J1713+0747

M. T. Lam, J. A. Ellis, G. Grillo +34

The frequency dependence of radio pulse arrival times provides a probe of structures in the intervening media. Demorest et al. 2013 was the first to show a short-term (~100-200 day…

astro-ph.HE2016★ 116 cited

The NANOGrav Nine-Year Data Set: Measurement and Interpretation of Variations in Dispersion Measures

M. L. Jones, M. A. McLaughlin, M. T. Lam +21

We analyze dispersion measure (DM) variations of 37 millisecond pulsars in the 9-year NANOGrav data release and constrain the sources of these variations. Variations are significan…

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…