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19972026
most citedThe NANOGrav 11-year Data Set: High-precision timing of 45 Millisecond Pulsars

611 citations · 2.8k across the 58 of their papers we have counts for

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17 papers · 1 filter

astro-ph.HE2024

Pulse Profile Variability of PSR J1022+1001 in NANOGrav Data

William Fiore, Maura A. McLaughlin, Gabriella Agazie +46

Pulse profile stability is a central assumption of standard pulsar timing methods. Thus, it is important for pulsar timing array experiments such as the North American Nanohertz Ob…

astro-ph.HE2024

The NANOGrav 15 yr Data Set: Harmonic Analysis of the Pulsar Angular Correlations

Gabriella Agazie, Jeremy G. Baier, Paul T. Baker +86

Pulsar timing array observations have found evidence for an isotropic gravitational wave background with the Hellings-Downs angular correlations, expected from general relativity.…

astro-ph.HE2024★ 4 cited

Inference on inner galaxy structure via gravitational waves from supermassive binaries

Yifan Chen, Matthias Daniel, Daniel J. D'Orazio +107

The detection of a stochastic gravitational wave background by pulsar-timing arrays indicates the presence of a population of supermassive black hole binaries. Although the observe…

astro-ph.HE2024

Sharp Periodic Flares and Long-Term Variability in the High-Mass X-ray Binary XTE J1829-098 from RXTE PCA, Swift BAT and MAXI Observations

Robin H. D. Corbet, Ralf Ballhausen, Peter A. Becker +20

XTE J1829-098 is a transient X-ray pulsar with a period of ~7.8 s. It is a candidate Be star system, although the evidence for this is not yet definitive. We investigated the twent…

astro-ph.HE2024★ 4 cited

A growing braking index and spin-down swings for the pulsar PSR B0540-69

Cristóbal M. Espinoza, Lucien Kuiper, Wynn C. G. Ho +5

The way pulsars spin down is not understood in detail, but a number of possible physical mechanisms produce a spin-down rate that scales as a power of the rotation rate ($\dotν\pro…

astro-ph.HE2024★ 86 cited

A NICER View of PSR J12311411: A Complex Case

Tuomo Salmi, Julia S. Deneva, Paul S. Ray +16

Recent constraints on neutron star mass and radius have advanced our understanding of the equation of state (EOS) of cold dense matter. Some of them have been obtained by modeling…