Abstract / Description of output
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$\%$ upper limit on the dimensionless strain amplitude $A$ of the background of $A $G\muc^2$\Omega^\mathrm{relic}_\mathrm{gw}(f)h^2
Original language | English |
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Pages (from-to) | 2567-2598 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 453 |
Issue number | 3 |
DOIs | |
Publication status | Published - 1 Nov 2015 |
Keywords / Materials (for Non-textual outputs)
- astro-ph.CO
- astro-ph.IM