Abstract
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 |
|---|---|
| Pages (from-to) | 2576-2598 |
| Journal | Royal Astronomical Society. Monthly Notices |
| Volume | 453 |
| Issue number | 3 |
| Early online date | 31 Aug 2015 |
| DOIs | |
| Publication status | Published - 1 Nov 2015 |
Bibliographical note
24 pages, 5 tables, 17 figuresKeywords
- astro-ph.CO
- astro-ph.IM
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