Relative orientation of L-shaped interferometers drastically impacts detectability of isotropic and anisotropic gravitational-wave backgrounds in cross-correlation searches.
Targeted search for the stochastic gravitational-wave background from the galac- tic millisecond pulsar population,
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Orientation matters: Consequences for gravitational-wave background detectability
Relative orientation of L-shaped interferometers drastically impacts detectability of isotropic and anisotropic gravitational-wave backgrounds in cross-correlation searches.