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An interactive demonstration of matched filtering with some examples using real gravitational-wave data and your computer's audio.

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The signal-to-noise ratio variables currently in the notebook are actually time-domain quantities based on the amplitude of the data. Because they need to be audible WAV files, the data can't...

enhancement

The normalization of the data as stored in the WAV files has nothing to do with the amplitude we'd actually expect in LIGO, and that might be informative. Maybe we...

enhancement