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From the 1 of 35 linked papers with an AI index.

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20242026
most citedInference on inner galaxy structure via gravitational waves from supermassive binaries

3 citations · 5 across the 11 of their papers we have counts for

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14 papers · 1 filter

astro-ph.HE2025

Inferring Mbh-Mbulge Evolution from the Gravitational Wave Background

Cayenne Matt, Kayhan Gultekin, Luke Kelley +104

We test the impact of an evolving supermassive black hole (SMBH) mass scaling relation (Mbh-Mbulge) on the predictions for the gravitational wave background (GWB). The observed GWB…

astro-ph.HE2025

The NANOGrav 15-year Data Set: Search for Gravitational Scattering of Pulsars by Free-Floating Objects in Interstellar Space

Lankeswar Dey, Ross J. Jennings, Jackson D. Taylor +48

Free-floating objects (FFOs) in interstellar spacerogue planets, brown dwarfs, and large asteroids that are not gravitationally bound to any starare expected to be ubiquitous…

astro-ph.HE2025

Nonlinear Orbital Variations in Binary Radio Pulsars from Lense-Thirring Precession

Emmanuel Fonseca

A future measurement of Lense-Thirring (LT) precession using a binary radio pulsar is expected to yield the pulsar's moment of inertia (). However, most of the known pul…

astro-ph.IM2025

The NANOGrav 12.5-year Data Set: Chromatic Noise Characterization & Mitigation with Time-Domain Kernels

Jeffrey S. Hazboun, Joseph Simon, Jeremy Baier +64

Pulsar timing arrays (PTAs) have recently entered the detection era, quickly moving beyond the goal of simply improving sensitivity at the lowest frequencies for the sake of observ…

astro-ph.HE2025

The NANOGrav 15-Year Data Set: Improved Timing Precision With VLBI Astrometric Priors

Sofia V. Sosa Fiscella, Michael T. Lam, Gabriella Agazie +47

Accurate pulsar astrometric estimates play an essential role in almost all high-precision pulsar timing experiments. Traditional pulsar timing techniques refine these estimates by…

astro-ph.HE2025

Testing Gravitation from Light-second to Cosmological Scales with Radio Pulsars

Emmanuel Fonseca

Pulsars are spinning neutron stars typically observed as pulses emitted at radio wavelengths. These pulsations exhibit a rotational stability that rival the best atomic clocks, mak…