R. N. Caballero

European Pulsar Timing Array Limits On An Isotropic Stochastic Gravitational-Wave Background

We present new limits on an isotropic stochastic gravitational-wave background (GWB) using a six pulsar dataset spanning 18 yr of observations from the 2015 European Pulsar Timing Array data release. Performing a Bayesian analysis, we fit simultaneously for the intrinsic noise parameters for each pulsar, along with common correlated signals including clock, and Solar System ephemeris errors, obtaining a robust 95

High-precision timing of 42 millisecond pulsars with the European Pulsar Timing Array

\%

European Pulsar Timing Array Limits on Continuous Gravitational Waves from Individual Supermassive Black Hole Binaries

upper limit on the dimensionless strain amplitude

From spin noise to systematics: stochastic processes in the first International Pulsar Timing Array data release

A

Prospects for high-precision pulsar timing with the new Effelsberg PSRIX backend

of the background of

Limits on Anisotropy in the Nanohertz Stochastic Gravitational Wave Background

A<3.0\times 10^{-15}

The noise properties of 42 millisecond pulsars from the European Pulsar Timing Array and their impact on gravitational wave searches

at a reference frequency of

A glitch in the millisecond pulsar J0613-0200

1\mathrm{yr^{-1}}

21 year timing of the black-widow pulsar J2051−0827

and a spectral index of

A millisecond pulsar in an extremely wide binary system

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