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Sensitivity curves for searches for gravitational-wave backgrounds
Eric Thrane, Joseph D Romano
We propose a graphical representation of detector sensitivity curves for stochastic gravitational-wave backgrounds that takes into account the increase in sensitivity that comes fr…
Searching for gravitational-wave transients with a qualitative signal model: seedless clustering strategies
Eric Thrane, Michael Coughlin
Gravitational-wave bursts are observable as bright clusters of pixels in spectrograms of strain power. Clustering algorithms can be used to identify candidate gravitational-wave ev…
A Search for Nucleon Decay via and in Super-Kamiokande
Kamiokande Collaboration, K. Abe, Y. Hayato +111
We present the results of searches for nucleon decay via bound neutron to antineutrino plus pizero and proton to antineutrino plus piplus using data from a combined 172.8 kiloton-y…
Correlated magnetic noise in global networks of gravitational-wave interferometers: observations and implications
Eric Thrane, Nelson Christensen, Robert Schofield
One of the most ambitious goals of gravitational-wave astronomy is to observe the stochastic gravitational-wave background. Correlated noise in two or more detectors can introduce…
Measuring the non-Gaussian stochastic gravitational-wave background: a method for realistic interferometer data
Eric Thrane
A stochastic gravitational-wave background (SGWB) can arise from the superposition of many independent events. If the rate of events per unit time is sufficiently high, the resulti…