Placing limits on the stochastic gravitational-wave background using European Pulsar Timing Array data

R. van Haasteren, Y. Levin, G. H. Janssen +16

Direct detection of low-frequency gravitational waves ($10^{-9}-10^{-8}$ Hz) is the main goal of pulsar timing array (PTA) projects. One of the main targets for the PTAs is to me…