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The document outlines a process for analyzing gravitational wave data from the merger event GW170817 using Python libraries such as PyCBC. It includes steps for reading strain data, applying a high-pass filter, estimating the power spectral density (PSD), and performing matched filtering to identify the optimal component masses of the merging objects. The analysis aims to determine the best mass parameters based on the signal-to-noise ratio (SNR) derived from the filtered data.

Author

singhaayatri

Language

EN