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
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gw150914.rst
###################################################
Signal Processing with GW150914
###################################################

Here are some interesting examples of how to process LIGO data using GW150914
as an example.

=====================================
Plotting the whitened strain
=====================================

.. plot:: ../examples/gw150914/gw150914_shape.py
   :include-source:

==============================================
Calculate the signal-to-noise
==============================================

.. plot:: ../examples/gw150914/gw150914_h1_snr.py
   :include-source:

==============================================
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>


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