Abstract
What we look for affects how we look for it. I summarize current and predicted sources of gravitational waves, how the physics affects the signals, and how the signal morphologies affect analysis techniques. Expecting long and short signals, well modeled signals and unknown signals, means that gravitational waves use a variety of techniques familiar from acoustics, from matched filtering to wavelets and cross-correlation of data streams. These tell us today about black holes, and one day will tell us about neutron stars, cosmic explosions, and perhaps even stranger things.
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