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2 changes: 1 addition & 1 deletion docs/0.11.0/_sources/citing.rst.txt
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Expand Up @@ -81,4 +81,4 @@ For older versions, please `click here <https://zenodo.org//search?page=2&size=1
-----

.. image:: https://zenodo.org/badge/doi/10.5281/zenodo.853178.svg
:target: https://doi.org/10.5281/zenodo.853178
:target: https://doi.org/10.5281/zenodo.853178
2 changes: 1 addition & 1 deletion docs/0.11.0/_sources/examples/signal/gw150914.rst.txt
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Expand Up @@ -188,4 +188,4 @@ and finally make a new plot with both detectors:
The above filtering is (almost) the same as what was applied to LIGO data
to produce Figure 1 in
`Abbott et al. (2016) <https://doi.org/10.1103/PhysRevLett.116.061102>`_
(the joint LSC-Virgo publication announcing this detection).
(the joint LSC-Virgo publication announcing this detection).
2 changes: 1 addition & 1 deletion docs/0.11.0/_sources/examples/spectrogram/spectrogram2.rst.txt
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Expand Up @@ -78,4 +78,4 @@ Here we can see the trace of a high-mass binary black hole system,
referred to as GW150914.
For more details on this signal, please see
`Abbott et al. (2016) <https://doi.org/10.1103/PhysRevLett.116.061102>`_
(the joint LSC-Virgo publication announcing this detection).
(the joint LSC-Virgo publication announcing this detection).
2 changes: 1 addition & 1 deletion docs/0.11.0/_sources/examples/timeseries/qscan.rst.txt
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Expand Up @@ -71,4 +71,4 @@ specific window around the interesting time
Here we can clearly see the trace of a compact binary coalescence,
specifically a binary black hole coalescence!
For more details on this result, please see
http://www.ligo.org/science/Publication-GW150914/.
http://www.ligo.org/science/Publication-GW150914/.
2 changes: 1 addition & 1 deletion docs/0.11.0/_sources/table/io.rst.txt
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Expand Up @@ -158,7 +158,7 @@ To replace an existing table of the given type in an existing file, while preser
Coherence WaveBurst ASCII (aka `EVENTS.txt`)
============================================

The `Coherent WaveBurst <http://dx.doi.org/10.1088/0264-9381/25/11/114029>`_ analysis pipeline is used to detect generic gravitational-wave bursts, without using a signal model to restrict the analysis, and runs in both low-latency (online) and offline modes over current GWO data.
The `Coherent WaveBurst <https://doi.org/10.1088/0264-9381/25/11/114029>`_ analysis pipeline is used to detect generic gravitational-wave bursts, without using a signal model to restrict the analysis, and runs in both low-latency (online) and offline modes over current GWO data.
The analysis uses the ROOT framework for most data products, but also produces ASCII data in a custom format commonly written in a file called ``EVENTS.txt``.

Reading
Expand Down
2 changes: 1 addition & 1 deletion docs/0.11.0/_sources/timeseries/remote-access.rst.txt
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Expand Up @@ -26,7 +26,7 @@ Open data releases

The `LIGO Open Science Center <https://losc.ligo.org/>`_ hosts a large quantity of open (meaning publicly-available) data from LIGO science runs, including the full strain record for the sixth LIGO science run (S6, 2009-2010) and short extracts of the strain record surrounding published GW observations from Advanced LIGO.

To fetch 32 seconds of strain data around event `GW150914 <http://dx.doi.org/10.1103/PhysRevLett.116.061102>`_, you need to give the prefix of the relevant observatory (``'H1'`` for the LIGO Hanford Observatory, ``'L1'`` for LIGO Livingston), and the start and end times of your query:
To fetch 32 seconds of strain data around event `GW150914 <https://doi.org/10.1103/PhysRevLett.116.061102>`_, you need to give the prefix of the relevant observatory (``'H1'`` for the LIGO Hanford Observatory, ``'L1'`` for LIGO Livingston), and the start and end times of your query:

.. plot::
:context: reset
Expand Down
2 changes: 1 addition & 1 deletion docs/0.11.0/citing.html
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Expand Up @@ -243,4 +243,4 @@ <h2>0.6.1<a class="headerlink" href="#id10" title="Permalink to this headline">
</div>
</footer>
</body>
</html>
</html>
2 changes: 1 addition & 1 deletion docs/0.11.0/examples/signal/gw150914.html
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</div>
</footer>
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2 changes: 1 addition & 1 deletion docs/0.11.0/examples/spectrogram/spectrogram2.html
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</div>
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2 changes: 1 addition & 1 deletion docs/0.11.0/examples/timeseries/qscan.html
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</div>
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4 changes: 2 additions & 2 deletions docs/0.11.0/table/io.html
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Expand Up @@ -326,7 +326,7 @@ <h3>Writing<a class="headerlink" href="#writing" title="Permalink to this headli
</div>
<div class="section" id="coherence-waveburst-ascii-aka-events-txt">
<span id="gwpy-table-io-ascii-cwb"></span><h2>Coherence WaveBurst ASCII (aka <code class="xref py py-obj docutils literal"><span class="pre">EVENTS.txt</span></code>)<a class="headerlink" href="#coherence-waveburst-ascii-aka-events-txt" title="Permalink to this headline">¶</a></h2>
<p>The <a class="reference external" href="http://dx.doi.org/10.1088/0264-9381/25/11/114029">Coherent WaveBurst</a> analysis pipeline is used to detect generic gravitational-wave bursts, without using a signal model to restrict the analysis, and runs in both low-latency (online) and offline modes over current GWO data.
<p>The <a class="reference external" href="https://doi.org/10.1088/0264-9381/25/11/114029">Coherent WaveBurst</a> analysis pipeline is used to detect generic gravitational-wave bursts, without using a signal model to restrict the analysis, and runs in both low-latency (online) and offline modes over current GWO data.
The analysis uses the ROOT framework for most data products, but also produces ASCII data in a custom format commonly written in a file called <code class="docutils literal"><span class="pre">EVENTS.txt</span></code>.</p>
<div class="section" id="id1">
<h3>Reading<a class="headerlink" href="#id1" title="Permalink to this headline">¶</a></h3>
Expand Down Expand Up @@ -869,4 +869,4 @@ <h2>Available file formats<a class="headerlink" href="#available-file-formats" t
</div>
</footer>
</body>
</html>
</html>
4 changes: 2 additions & 2 deletions docs/0.11.0/timeseries/remote-access.html
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Expand Up @@ -197,7 +197,7 @@
<div class="section" id="open-data-releases">
<span id="gwpy-timeseries-remote-public"></span><h2>Open data releases<a class="headerlink" href="#open-data-releases" title="Permalink to this headline">¶</a></h2>
<p>The <a class="reference external" href="https://losc.ligo.org/">LIGO Open Science Center</a> hosts a large quantity of open (meaning publicly-available) data from LIGO science runs, including the full strain record for the sixth LIGO science run (S6, 2009-2010) and short extracts of the strain record surrounding published GW observations from Advanced LIGO.</p>
<p>To fetch 32 seconds of strain data around event <a class="reference external" href="http://dx.doi.org/10.1103/PhysRevLett.116.061102">GW150914</a>, you need to give the prefix of the relevant observatory (<code class="docutils literal"><span class="pre">'H1'</span></code> for the LIGO Hanford Observatory, <code class="docutils literal"><span class="pre">'L1'</span></code> for LIGO Livingston), and the start and end times of your query:</p>
<p>To fetch 32 seconds of strain data around event <a class="reference external" href="https://doi.org/10.1103/PhysRevLett.116.061102">GW150914</a>, you need to give the prefix of the relevant observatory (<code class="docutils literal"><span class="pre">'H1'</span></code> for the LIGO Hanford Observatory, <code class="docutils literal"><span class="pre">'L1'</span></code> for LIGO Livingston), and the start and end times of your query:</p>
<div class="highlight-default"><div class="highlight"><pre><span></span><span class="gp">&gt;&gt;&gt; </span><span class="kn">from</span> <span class="nn">gwpy.timeseries</span> <span class="k">import</span> <span class="n">TimeSeries</span>
<span class="gp">&gt;&gt;&gt; </span><span class="n">data</span> <span class="o">=</span> <span class="n">TimeSeries</span><span class="o">.</span><span class="n">fetch_open_data</span><span class="p">(</span><span class="s1">&#39;L1&#39;</span><span class="p">,</span> <span class="mi">1126259446</span><span class="p">,</span> <span class="mi">1126259478</span><span class="p">)</span>
</pre></div>
Expand Down Expand Up @@ -272,4 +272,4 @@
</div>
</footer>
</body>
</html>
</html>
2 changes: 1 addition & 1 deletion docs/0.12.0/_sources/citing.rst.txt
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Expand Up @@ -81,4 +81,4 @@ For older versions, please `click here <https://zenodo.org//search?page=2&size=1
-----

.. image:: https://zenodo.org/badge/doi/10.5281/zenodo.1155470.svg
:target: https://doi.org/10.5281/zenodo.1155470
:target: https://doi.org/10.5281/zenodo.1155470
2 changes: 1 addition & 1 deletion docs/0.12.0/_sources/examples/signal/gw150914.rst.txt
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Expand Up @@ -188,4 +188,4 @@ and finally make a new plot with both detectors:
The above filtering is (almost) the same as what was applied to LIGO data
to produce Figure 1 in
`Abbott et al. (2016) <https://doi.org/10.1103/PhysRevLett.116.061102>`_
(the joint LSC-Virgo publication announcing this detection).
(the joint LSC-Virgo publication announcing this detection).
2 changes: 1 addition & 1 deletion docs/0.12.0/_sources/examples/spectrogram/spectrogram2.rst.txt
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Expand Up @@ -78,4 +78,4 @@ Here we can see the trace of a high-mass binary black hole system,
referred to as GW150914.
For more details on this signal, please see
`Abbott et al. (2016) <https://doi.org/10.1103/PhysRevLett.116.061102>`_
(the joint LSC-Virgo publication announcing this detection).
(the joint LSC-Virgo publication announcing this detection).
2 changes: 1 addition & 1 deletion docs/0.12.0/_sources/examples/timeseries/qscan.rst.txt
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Expand Up @@ -62,4 +62,4 @@ specific window around the interesting time
Here we can clearly see the trace of a compact binary coalescence,
specifically a binary black hole merger!
For more details on this result, please see
http://www.ligo.org/science/Publication-GW150914/.
http://www.ligo.org/science/Publication-GW150914/.
2 changes: 1 addition & 1 deletion docs/0.12.0/_sources/examples/timeseries/statevector.rst.txt
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Expand Up @@ -52,4 +52,4 @@ This plot shows that for a short time exactly overlapping with GW170817
there was a data quality issue recorded that would negatively impact a
search for generic gravitational-wave transients (bursts).
For more details on this _glitch_, and on how it was excised, please see
`Abbott et al. 2017 <https://doi.org/10.1103/PhysRevLett.119.161101>`__.
`Abbott et al. 2017 <https://doi.org/10.1103/PhysRevLett.119.161101>`__.
2 changes: 1 addition & 1 deletion docs/0.12.0/_sources/table/io.rst.txt
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Expand Up @@ -158,7 +158,7 @@ To replace an existing table of the given type in an existing file, while preser
Coherence WaveBurst ASCII (aka `EVENTS.txt`)
============================================

The `Coherent WaveBurst <http://dx.doi.org/10.1088/0264-9381/25/11/114029>`_ analysis pipeline is used to detect generic gravitational-wave bursts, without using a signal model to restrict the analysis, and runs in both low-latency (online) and offline modes over current GWO data.
The `Coherent WaveBurst <https://doi.org/10.1088/0264-9381/25/11/114029>`_ analysis pipeline is used to detect generic gravitational-wave bursts, without using a signal model to restrict the analysis, and runs in both low-latency (online) and offline modes over current GWO data.
The analysis uses the ROOT framework for most data products, but also produces ASCII data in a custom format commonly written in a file called ``EVENTS.txt``.

Reading
Expand Down
2 changes: 1 addition & 1 deletion docs/0.12.0/_sources/timeseries/remote-access.rst.txt
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Expand Up @@ -26,7 +26,7 @@ Open data releases

The `LIGO Open Science Center <https://losc.ligo.org/>`_ hosts a large quantity of open (meaning publicly-available) data from LIGO science runs, including the full strain record for the sixth LIGO science run (S6, 2009-2010) and short extracts of the strain record surrounding published GW observations from Advanced LIGO.

To fetch 32 seconds of strain data around event `GW150914 <http://dx.doi.org/10.1103/PhysRevLett.116.061102>`_, you need to give the prefix of the relevant observatory (``'H1'`` for the LIGO Hanford Observatory, ``'L1'`` for LIGO Livingston), and the start and end times of your query:
To fetch 32 seconds of strain data around event `GW150914 <https://doi.org/10.1103/PhysRevLett.116.061102>`_, you need to give the prefix of the relevant observatory (``'H1'`` for the LIGO Hanford Observatory, ``'L1'`` for LIGO Livingston), and the start and end times of your query:

.. plot::
:context: reset
Expand Down
2 changes: 1 addition & 1 deletion docs/0.12.0/citing.html
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Expand Up @@ -234,4 +234,4 @@ <h2>0.7.0<a class="headerlink" href="#id10" title="Permalink to this headline">
</div>
</footer>
</body>
</html>
</html>
2 changes: 1 addition & 1 deletion docs/0.12.0/examples/signal/gw150914.html
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</div>
</footer>
</body>
</html>
</html>
2 changes: 1 addition & 1 deletion docs/0.12.0/examples/spectrogram/spectrogram2.html
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</div>
</footer>
</body>
</html>
</html>
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</div>
</footer>
</body>
</html>
</html>
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</div>
</footer>
</body>
</html>
</html>
4 changes: 2 additions & 2 deletions docs/0.12.0/table/io.html
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Expand Up @@ -317,7 +317,7 @@ <h3>Writing<a class="headerlink" href="#writing" title="Permalink to this headli
</div>
<div class="section" id="coherence-waveburst-ascii-aka-events-txt">
<span id="gwpy-table-io-ascii-cwb"></span><h2>Coherence WaveBurst ASCII (aka <code class="xref py py-obj docutils literal notranslate"><span class="pre">EVENTS.txt</span></code>)<a class="headerlink" href="#coherence-waveburst-ascii-aka-events-txt" title="Permalink to this headline">¶</a></h2>
<p>The <a class="reference external" href="http://dx.doi.org/10.1088/0264-9381/25/11/114029">Coherent WaveBurst</a> analysis pipeline is used to detect generic gravitational-wave bursts, without using a signal model to restrict the analysis, and runs in both low-latency (online) and offline modes over current GWO data.
<p>The <a class="reference external" href="https://doi.org/10.1088/0264-9381/25/11/114029">Coherent WaveBurst</a> analysis pipeline is used to detect generic gravitational-wave bursts, without using a signal model to restrict the analysis, and runs in both low-latency (online) and offline modes over current GWO data.
The analysis uses the ROOT framework for most data products, but also produces ASCII data in a custom format commonly written in a file called <code class="docutils literal notranslate"><span class="pre">EVENTS.txt</span></code>.</p>
<div class="section" id="id1">
<h3>Reading<a class="headerlink" href="#id1" title="Permalink to this headline">¶</a></h3>
Expand Down Expand Up @@ -860,4 +860,4 @@ <h2>Available file formats<a class="headerlink" href="#available-file-formats" t
</div>
</footer>
</body>
</html>
</html>
4 changes: 2 additions & 2 deletions docs/0.12.0/timeseries/remote-access.html
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Expand Up @@ -188,7 +188,7 @@
<div class="section" id="open-data-releases">
<span id="gwpy-timeseries-remote-public"></span><h2>Open data releases<a class="headerlink" href="#open-data-releases" title="Permalink to this headline">¶</a></h2>
<p>The <a class="reference external" href="https://losc.ligo.org/">LIGO Open Science Center</a> hosts a large quantity of open (meaning publicly-available) data from LIGO science runs, including the full strain record for the sixth LIGO science run (S6, 2009-2010) and short extracts of the strain record surrounding published GW observations from Advanced LIGO.</p>
<p>To fetch 32 seconds of strain data around event <a class="reference external" href="http://dx.doi.org/10.1103/PhysRevLett.116.061102">GW150914</a>, you need to give the prefix of the relevant observatory (<code class="docutils literal notranslate"><span class="pre">'H1'</span></code> for the LIGO Hanford Observatory, <code class="docutils literal notranslate"><span class="pre">'L1'</span></code> for LIGO Livingston), and the start and end times of your query:</p>
<p>To fetch 32 seconds of strain data around event <a class="reference external" href="https://doi.org/10.1103/PhysRevLett.116.061102">GW150914</a>, you need to give the prefix of the relevant observatory (<code class="docutils literal notranslate"><span class="pre">'H1'</span></code> for the LIGO Hanford Observatory, <code class="docutils literal notranslate"><span class="pre">'L1'</span></code> for LIGO Livingston), and the start and end times of your query:</p>
<div class="highlight-default notranslate"><div class="highlight"><pre><span></span><span class="gp">&gt;&gt;&gt; </span><span class="kn">from</span> <span class="nn">gwpy.timeseries</span> <span class="k">import</span> <span class="n">TimeSeries</span>
<span class="gp">&gt;&gt;&gt; </span><span class="n">data</span> <span class="o">=</span> <span class="n">TimeSeries</span><span class="o">.</span><span class="n">fetch_open_data</span><span class="p">(</span><span class="s1">&#39;L1&#39;</span><span class="p">,</span> <span class="mi">1126259446</span><span class="p">,</span> <span class="mi">1126259478</span><span class="p">)</span>
</pre></div>
Expand Down Expand Up @@ -263,4 +263,4 @@
</div>
</footer>
</body>
</html>
</html>
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Expand Up @@ -127,4 +127,4 @@ first ever directly-detected gravitational wave signal, GW150914!
The above filtering is (almost) the same as what was applied to LIGO data
to produce Figure 1 in
`Abbott et al. (2016) <https://doi.org/10.1103/PhysRevLett.116.061102>`_
(the joint LSC-Virgo publication announcing this detection).
(the joint LSC-Virgo publication announcing this detection).
2 changes: 1 addition & 1 deletion docs/0.6.1/_sources/examples/spectrogram/spectrogram2.rst.txt
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Expand Up @@ -78,4 +78,4 @@ Here we can see the trace of a high-mass binary black hole system,
referred to as GW150914.
For more details on this signal, please see
`Abbott et al. (2016) <https://doi.org/10.1103/PhysRevLett.116.061102>`_
(the joint LSC-Virgo publication announcing this detection).
(the joint LSC-Virgo publication announcing this detection).
2 changes: 1 addition & 1 deletion docs/0.6.1/_sources/examples/timeseries/qscan.rst.txt
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Expand Up @@ -71,4 +71,4 @@ specific window around the interesting time
Here we can clearly see the trace of a compact binary coalescence,
specifically a binary black hole coalescence!
For more details on this result, please see
http://www.ligo.org/science/Publication-GW150914/.
http://www.ligo.org/science/Publication-GW150914/.
2 changes: 1 addition & 1 deletion docs/0.6.1/_sources/table/io.rst.txt
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Expand Up @@ -187,7 +187,7 @@ Table name Format name
Coherence WaveBurst ASCII (aka `EVENTS.txt`)
============================================

The `Coherent WaveBurst <http://dx.doi.org/10.1088/0264-9381/25/11/114029>`_ analysis pipeline is used to detect generic gravitational-wave bursts, without using a signal model to restrict the analysis, and runs in both low-latency (online) and offline modes over current GWO data.
The `Coherent WaveBurst <https://doi.org/10.1088/0264-9381/25/11/114029>`_ analysis pipeline is used to detect generic gravitational-wave bursts, without using a signal model to restrict the analysis, and runs in both low-latency (online) and offline modes over current GWO data.
The analysis uses the ROOT framework for most data products, but also produces ASCII data in a custom format commonly written in a file called ``EVENTS.txt``.

Reading
Expand Down
2 changes: 1 addition & 1 deletion docs/0.6.1/_sources/timeseries/remote-access.rst.txt
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Expand Up @@ -29,7 +29,7 @@ Open data releases

The `LIGO Open Science Center <https://losc.ligo.org/>`_ hosts a large quantity of open (meaning publicly-available) data from LIGO science runs, including the full strain record for the sixth LIGO science run (S6, 2009-2010) and short extracts of the strain record surrounding published GW observations from Advanced LIGO.

To fetch 32 seconds of strain data around event `GW150914 <http://dx.doi.org/10.1103/PhysRevLett.116.061102>`_, you need to give the prefix of the relevant observatory (``'H1'`` for the LIGO Hanford Observatory, ``'L1'`` for LIGO Livingston), and the start and end times of your query:
To fetch 32 seconds of strain data around event `GW150914 <https://doi.org/10.1103/PhysRevLett.116.061102>`_, you need to give the prefix of the relevant observatory (``'H1'`` for the LIGO Hanford Observatory, ``'L1'`` for LIGO Livingston), and the start and end times of your query:

.. plot::
:context: reset
Expand Down
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