Revision 15fd8a754be04123dc305169fc87f7b95d6cb811 authored by Tito Dal Canton on 17 April 2018, 13:00:16 UTC, committed by Alex Nitz on 17 April 2018, 13:00:16 UTC
* Update citation guide with Nitz+ 2017 * Use code-block
1 parent e439768
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:
==============================================
Calculate the signal-to-noise
==============================================
.. plot:: ../examples/gw150914/gw150914_h1_snr.py
:include-source:
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Listen to GW150914 in Hanford
==============================================
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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