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This presentation from the March 2007 LIGO/Virgo Meeting discusses the significance of spectral line cataloging in gravitational wave (GW) searches. It highlights how broad peaks influence bandwidth in pulsar observations and how narrow and broad coherences impact signal analysis. The non-stationarity of line sources can lead to transients that complicate detection efforts. By understanding these spectral characteristics, researchers can enhance the accuracy and effectiveness of gravitational wave searches.
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