Revision 87ce2d5d5d491e8629b62b99f95a9299650c2d60 authored by Arthur Tolley on 06 April 2021, 14:13:55 UTC, committed by GitHub on 06 April 2021, 14:13:55 UTC
1 parent 4022136
gw150914.rst
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Signal Processing with GW150914
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Here are some interesting examples of how to process LIGO data using GW150914
as an example.
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Plotting the whitened strain
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.. plot:: ../examples/gw150914/gw150914_shape.py
:include-source:
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Calculate the signal-to-noise
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.. plot:: ../examples/gw150914/gw150914_h1_snr.py
:include-source:
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Listen to GW150914 in Hanford
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Here we'll make a frequency shifted and slowed version of GW150914 as
it can be heard in the Hanford data.
.. literalinclude:: ../examples/gw150914/audio.py
:download:`The audio <resources/gw150914_h1_chirp.wav>`
Note, google chrome may not play wav files correctly, please download to listen.
.. raw:: html
<audio controls><source src='_downloads/gw150914_h1_chirp.wav' type='audio/wav'</audio>
![swh spinner](/static/img/swh-spinner.gif)
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