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most citedLimits on the Stochastic Gravitational Wave Background from the North American Nanohertz Observatory for Gravitational Waves

361 citations · 547 across the 5 of their papers we have counts for

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5 papers

gr-qc2026

Narrowband searches for continuous gravitational waves from known pulsars in the first two parts of the fourth LIGO--Virgo--KAGRA observing run

The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1853

Rotating non-axisymmetric neutron stars (NSs) are promising sources for continuous gravitational waves (CWs). Such CWs can, if detected, inform us about the internal structure and…

astro-ph.HE2025★ 17 cited

Search for continuous gravitational waves from known pulsars in the first part of the fourth LIGO-Virgo-KAGRA observing run

The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1816

Continuous gravitational waves (CWs) emission from neutron stars carries information about their internal structure and equation of state, and it can provide tests of General Relat…

astro-ph.IM2016★ 123 cited

From Spin Noise to Systematics: Stochastic Processes in the First International Pulsar Timing Array Data Release

L. Lentati, R. M. Shannon, W. A. Coles +80

We analyse the stochastic properties of the 49 pulsars that comprise the first International Pulsar Timing Array (IPTA) data release. We use Bayesian methodology, performing model…

astro-ph.CO2012★ 361 cited

Limits on the Stochastic Gravitational Wave Background from the North American Nanohertz Observatory for Gravitational Waves

P. B. Demorest, R. D. Ferdman, M. E. Gonzalez +24

We present an analysis of high-precision pulsar timing data taken as part of the North American Nanohertz Observatory for Gravitational waves (NANOGrav) project. We have observed 1…

astro-ph2001★ 46 cited

PSR J1740+1000: A Young Pulsar Well Out Of The Galactic Plane

M. A. McLaughlin, Z. Arzoumanian, J. M. Cordes +4

We discuss PSR J1740+1000, one of five pulsars recently discovered in a search of 470 square degrees at 430 MHz during the upgrade of the 305-m Arecibo telescope. The period of 154…