diff --git a/docs/0.11.0/_sources/citing.rst.txt b/docs/0.11.0/_sources/citing.rst.txt index 83c4ff851..eb6709134 100644 --- a/docs/0.11.0/_sources/citing.rst.txt +++ b/docs/0.11.0/_sources/citing.rst.txt @@ -81,4 +81,4 @@ For older versions, please `click here `_ -(the joint LSC-Virgo publication announcing this detection). \ No newline at end of file +(the joint LSC-Virgo publication announcing this detection). diff --git a/docs/0.11.0/_sources/examples/spectrogram/spectrogram2.rst.txt b/docs/0.11.0/_sources/examples/spectrogram/spectrogram2.rst.txt index 592088cc6..5e1e570b0 100644 --- a/docs/0.11.0/_sources/examples/spectrogram/spectrogram2.rst.txt +++ b/docs/0.11.0/_sources/examples/spectrogram/spectrogram2.rst.txt @@ -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) `_ -(the joint LSC-Virgo publication announcing this detection). \ No newline at end of file +(the joint LSC-Virgo publication announcing this detection). diff --git a/docs/0.11.0/_sources/examples/timeseries/qscan.rst.txt b/docs/0.11.0/_sources/examples/timeseries/qscan.rst.txt index 67c1be414..70d3a3ae7 100644 --- a/docs/0.11.0/_sources/examples/timeseries/qscan.rst.txt +++ b/docs/0.11.0/_sources/examples/timeseries/qscan.rst.txt @@ -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/. \ No newline at end of file +http://www.ligo.org/science/Publication-GW150914/. diff --git a/docs/0.11.0/_sources/table/io.rst.txt b/docs/0.11.0/_sources/table/io.rst.txt index 822a1da4a..8813a3ca0 100644 --- a/docs/0.11.0/_sources/table/io.rst.txt +++ b/docs/0.11.0/_sources/table/io.rst.txt @@ -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 `_ 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 `_ 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 diff --git a/docs/0.11.0/_sources/timeseries/remote-access.rst.txt b/docs/0.11.0/_sources/timeseries/remote-access.rst.txt index 06fde94f7..dc354208f 100644 --- a/docs/0.11.0/_sources/timeseries/remote-access.rst.txt +++ b/docs/0.11.0/_sources/timeseries/remote-access.rst.txt @@ -26,7 +26,7 @@ Open data releases The `LIGO Open Science Center `_ 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 `_, 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 `_, 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 diff --git a/docs/0.11.0/citing.html b/docs/0.11.0/citing.html index a2664ddcf..bdf33d7fb 100644 --- a/docs/0.11.0/citing.html +++ b/docs/0.11.0/citing.html @@ -243,4 +243,4 @@

0.6.1 - \ No newline at end of file + diff --git a/docs/0.11.0/examples/signal/gw150914.html b/docs/0.11.0/examples/signal/gw150914.html index 51feeaab4..b246b2bc9 100644 --- a/docs/0.11.0/examples/signal/gw150914.html +++ b/docs/0.11.0/examples/signal/gw150914.html @@ -299,4 +299,4 @@ - \ No newline at end of file + diff --git a/docs/0.11.0/examples/spectrogram/spectrogram2.html b/docs/0.11.0/examples/spectrogram/spectrogram2.html index 5308f02f1..9d81ac03a 100644 --- a/docs/0.11.0/examples/spectrogram/spectrogram2.html +++ b/docs/0.11.0/examples/spectrogram/spectrogram2.html @@ -223,4 +223,4 @@ - \ No newline at end of file + diff --git a/docs/0.11.0/examples/timeseries/qscan.html b/docs/0.11.0/examples/timeseries/qscan.html index b3c8ba8c9..2463091c7 100644 --- a/docs/0.11.0/examples/timeseries/qscan.html +++ b/docs/0.11.0/examples/timeseries/qscan.html @@ -232,4 +232,4 @@ - \ No newline at end of file + diff --git a/docs/0.11.0/table/io.html b/docs/0.11.0/table/io.html index c8ed7b64e..6e6b27c9c 100644 --- a/docs/0.11.0/table/io.html +++ b/docs/0.11.0/table/io.html @@ -326,7 +326,7 @@

Writing

Coherence WaveBurst ASCII (aka EVENTS.txt)

-

The Coherent WaveBurst 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 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

@@ -869,4 +869,4 @@

Available file formats - \ No newline at end of file + diff --git a/docs/0.11.0/timeseries/remote-access.html b/docs/0.11.0/timeseries/remote-access.html index 0d23a4cca..a86653640 100644 --- a/docs/0.11.0/timeseries/remote-access.html +++ b/docs/0.11.0/timeseries/remote-access.html @@ -197,7 +197,7 @@

Open data releases

The LIGO Open Science Center 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, 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, 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:

>>> from gwpy.timeseries import TimeSeries
 >>> data = TimeSeries.fetch_open_data('L1', 1126259446, 1126259478)
@@ -272,4 +272,4 @@
- \ No newline at end of file + diff --git a/docs/0.12.0/_sources/citing.rst.txt b/docs/0.12.0/_sources/citing.rst.txt index 1c7373931..639b3aff5 100644 --- a/docs/0.12.0/_sources/citing.rst.txt +++ b/docs/0.12.0/_sources/citing.rst.txt @@ -81,4 +81,4 @@ For older versions, please `click here `_ -(the joint LSC-Virgo publication announcing this detection). \ No newline at end of file +(the joint LSC-Virgo publication announcing this detection). diff --git a/docs/0.12.0/_sources/examples/spectrogram/spectrogram2.rst.txt b/docs/0.12.0/_sources/examples/spectrogram/spectrogram2.rst.txt index d4320a1aa..1ba3d450c 100644 --- a/docs/0.12.0/_sources/examples/spectrogram/spectrogram2.rst.txt +++ b/docs/0.12.0/_sources/examples/spectrogram/spectrogram2.rst.txt @@ -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) `_ -(the joint LSC-Virgo publication announcing this detection). \ No newline at end of file +(the joint LSC-Virgo publication announcing this detection). diff --git a/docs/0.12.0/_sources/examples/timeseries/qscan.rst.txt b/docs/0.12.0/_sources/examples/timeseries/qscan.rst.txt index a58d915f0..ceba40976 100644 --- a/docs/0.12.0/_sources/examples/timeseries/qscan.rst.txt +++ b/docs/0.12.0/_sources/examples/timeseries/qscan.rst.txt @@ -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/. \ No newline at end of file +http://www.ligo.org/science/Publication-GW150914/. diff --git a/docs/0.12.0/_sources/examples/timeseries/statevector.rst.txt b/docs/0.12.0/_sources/examples/timeseries/statevector.rst.txt index 88bceea38..4aabcb68c 100644 --- a/docs/0.12.0/_sources/examples/timeseries/statevector.rst.txt +++ b/docs/0.12.0/_sources/examples/timeseries/statevector.rst.txt @@ -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 `__. \ No newline at end of file +`Abbott et al. 2017 `__. diff --git a/docs/0.12.0/_sources/table/io.rst.txt b/docs/0.12.0/_sources/table/io.rst.txt index 822a1da4a..8813a3ca0 100644 --- a/docs/0.12.0/_sources/table/io.rst.txt +++ b/docs/0.12.0/_sources/table/io.rst.txt @@ -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 `_ 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 `_ 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 diff --git a/docs/0.12.0/_sources/timeseries/remote-access.rst.txt b/docs/0.12.0/_sources/timeseries/remote-access.rst.txt index 06fde94f7..dc354208f 100644 --- a/docs/0.12.0/_sources/timeseries/remote-access.rst.txt +++ b/docs/0.12.0/_sources/timeseries/remote-access.rst.txt @@ -26,7 +26,7 @@ Open data releases The `LIGO Open Science Center `_ 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 `_, 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 `_, 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 diff --git a/docs/0.12.0/citing.html b/docs/0.12.0/citing.html index 01f9164d3..dddbd3dba 100644 --- a/docs/0.12.0/citing.html +++ b/docs/0.12.0/citing.html @@ -234,4 +234,4 @@

0.7.0

- \ No newline at end of file + diff --git a/docs/0.12.0/examples/signal/gw150914.html b/docs/0.12.0/examples/signal/gw150914.html index fe8c0aa2e..9e83e2875 100644 --- a/docs/0.12.0/examples/signal/gw150914.html +++ b/docs/0.12.0/examples/signal/gw150914.html @@ -300,4 +300,4 @@

- \ No newline at end of file + diff --git a/docs/0.12.0/examples/spectrogram/spectrogram2.html b/docs/0.12.0/examples/spectrogram/spectrogram2.html index 2b0ede619..21c52e506 100644 --- a/docs/0.12.0/examples/spectrogram/spectrogram2.html +++ b/docs/0.12.0/examples/spectrogram/spectrogram2.html @@ -224,4 +224,4 @@ - \ No newline at end of file + diff --git a/docs/0.12.0/examples/timeseries/qscan.html b/docs/0.12.0/examples/timeseries/qscan.html index d7cf33b43..391b8b593 100644 --- a/docs/0.12.0/examples/timeseries/qscan.html +++ b/docs/0.12.0/examples/timeseries/qscan.html @@ -214,4 +214,4 @@ - \ No newline at end of file + diff --git a/docs/0.12.0/examples/timeseries/statevector.html b/docs/0.12.0/examples/timeseries/statevector.html index 715aad2f5..2370fdd35 100644 --- a/docs/0.12.0/examples/timeseries/statevector.html +++ b/docs/0.12.0/examples/timeseries/statevector.html @@ -208,4 +208,4 @@ - \ No newline at end of file + diff --git a/docs/0.12.0/table/io.html b/docs/0.12.0/table/io.html index 8310e6074..f62496944 100644 --- a/docs/0.12.0/table/io.html +++ b/docs/0.12.0/table/io.html @@ -317,7 +317,7 @@

Writing

Coherence WaveBurst ASCII (aka EVENTS.txt)

-

The Coherent WaveBurst 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 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

@@ -860,4 +860,4 @@

Available file formats - \ No newline at end of file + diff --git a/docs/0.12.0/timeseries/remote-access.html b/docs/0.12.0/timeseries/remote-access.html index e6f7c6afb..1427bca10 100644 --- a/docs/0.12.0/timeseries/remote-access.html +++ b/docs/0.12.0/timeseries/remote-access.html @@ -188,7 +188,7 @@

Open data releases

The LIGO Open Science Center 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, 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, 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:

>>> from gwpy.timeseries import TimeSeries
 >>> data = TimeSeries.fetch_open_data('L1', 1126259446, 1126259478)
@@ -263,4 +263,4 @@
- \ No newline at end of file + diff --git a/docs/0.6.1/_sources/examples/signal/gw150914.rst.txt b/docs/0.6.1/_sources/examples/signal/gw150914.rst.txt index 690908291..d945940d5 100644 --- a/docs/0.6.1/_sources/examples/signal/gw150914.rst.txt +++ b/docs/0.6.1/_sources/examples/signal/gw150914.rst.txt @@ -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) `_ -(the joint LSC-Virgo publication announcing this detection). \ No newline at end of file +(the joint LSC-Virgo publication announcing this detection). diff --git a/docs/0.6.1/_sources/examples/spectrogram/spectrogram2.rst.txt b/docs/0.6.1/_sources/examples/spectrogram/spectrogram2.rst.txt index 592088cc6..5e1e570b0 100644 --- a/docs/0.6.1/_sources/examples/spectrogram/spectrogram2.rst.txt +++ b/docs/0.6.1/_sources/examples/spectrogram/spectrogram2.rst.txt @@ -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) `_ -(the joint LSC-Virgo publication announcing this detection). \ No newline at end of file +(the joint LSC-Virgo publication announcing this detection). diff --git a/docs/0.6.1/_sources/examples/timeseries/qscan.rst.txt b/docs/0.6.1/_sources/examples/timeseries/qscan.rst.txt index 67c1be414..70d3a3ae7 100644 --- a/docs/0.6.1/_sources/examples/timeseries/qscan.rst.txt +++ b/docs/0.6.1/_sources/examples/timeseries/qscan.rst.txt @@ -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/. \ No newline at end of file +http://www.ligo.org/science/Publication-GW150914/. diff --git a/docs/0.6.1/_sources/table/io.rst.txt b/docs/0.6.1/_sources/table/io.rst.txt index 5ed483d6e..cfd725eb1 100644 --- a/docs/0.6.1/_sources/table/io.rst.txt +++ b/docs/0.6.1/_sources/table/io.rst.txt @@ -187,7 +187,7 @@ Table name Format name Coherence WaveBurst ASCII (aka `EVENTS.txt`) ============================================ -The `Coherent WaveBurst `_ 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 `_ 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 diff --git a/docs/0.6.1/_sources/timeseries/remote-access.rst.txt b/docs/0.6.1/_sources/timeseries/remote-access.rst.txt index f0961fa64..4b0c55700 100644 --- a/docs/0.6.1/_sources/timeseries/remote-access.rst.txt +++ b/docs/0.6.1/_sources/timeseries/remote-access.rst.txt @@ -29,7 +29,7 @@ Open data releases The `LIGO Open Science Center `_ 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 `_, 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 `_, 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 diff --git a/docs/0.6.1/examples/signal/gw150914.html b/docs/0.6.1/examples/signal/gw150914.html index 3bc7dde98..64909e6df 100644 --- a/docs/0.6.1/examples/signal/gw150914.html +++ b/docs/0.6.1/examples/signal/gw150914.html @@ -269,4 +269,4 @@
- \ No newline at end of file + diff --git a/docs/0.6.1/examples/spectrogram/spectrogram2.html b/docs/0.6.1/examples/spectrogram/spectrogram2.html index 99d16323c..df5936c3b 100644 --- a/docs/0.6.1/examples/spectrogram/spectrogram2.html +++ b/docs/0.6.1/examples/spectrogram/spectrogram2.html @@ -234,4 +234,4 @@

- \ No newline at end of file + diff --git a/docs/0.6.1/examples/timeseries/qscan.html b/docs/0.6.1/examples/timeseries/qscan.html index e388e3efe..261b83fec 100644 --- a/docs/0.6.1/examples/timeseries/qscan.html +++ b/docs/0.6.1/examples/timeseries/qscan.html @@ -233,4 +233,4 @@ - \ No newline at end of file + diff --git a/docs/0.6.1/table/io.html b/docs/0.6.1/table/io.html index 781dcce7c..fceb2f667 100644 --- a/docs/0.6.1/table/io.html +++ b/docs/0.6.1/table/io.html @@ -439,7 +439,7 @@

Supported LIGO_LW tables

Coherence WaveBurst ASCII (aka EVENTS.txt)

-

The Coherent WaveBurst 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 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

@@ -1205,4 +1205,4 @@

Available file formats - \ No newline at end of file + diff --git a/docs/0.6.1/timeseries/remote-access.html b/docs/0.6.1/timeseries/remote-access.html index 371b0d54b..0a3a54cfa 100644 --- a/docs/0.6.1/timeseries/remote-access.html +++ b/docs/0.6.1/timeseries/remote-access.html @@ -199,7 +199,7 @@

Open data releases

Additional dependencies: h5py

The LIGO Open Science Center 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, 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, 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:

>>> from gwpy.timeseries import TimeSeries
 >>> data = TimeSeries.fetch_open_data('L1', 1126259446, 1126259478)
@@ -266,4 +266,4 @@
- \ No newline at end of file + diff --git a/docs/0.6.2/_sources/examples/signal/gw150914.rst.txt b/docs/0.6.2/_sources/examples/signal/gw150914.rst.txt index 2d8e5aa8c..0d143c334 100644 --- a/docs/0.6.2/_sources/examples/signal/gw150914.rst.txt +++ b/docs/0.6.2/_sources/examples/signal/gw150914.rst.txt @@ -128,4 +128,4 @@ 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) `_ -(the joint LSC-Virgo publication announcing this detection). \ No newline at end of file +(the joint LSC-Virgo publication announcing this detection). diff --git a/docs/0.6.2/_sources/examples/spectrogram/spectrogram2.rst.txt b/docs/0.6.2/_sources/examples/spectrogram/spectrogram2.rst.txt index 592088cc6..5e1e570b0 100644 --- a/docs/0.6.2/_sources/examples/spectrogram/spectrogram2.rst.txt +++ b/docs/0.6.2/_sources/examples/spectrogram/spectrogram2.rst.txt @@ -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) `_ -(the joint LSC-Virgo publication announcing this detection). \ No newline at end of file +(the joint LSC-Virgo publication announcing this detection). diff --git a/docs/0.6.2/_sources/examples/timeseries/qscan.rst.txt b/docs/0.6.2/_sources/examples/timeseries/qscan.rst.txt index 67c1be414..70d3a3ae7 100644 --- a/docs/0.6.2/_sources/examples/timeseries/qscan.rst.txt +++ b/docs/0.6.2/_sources/examples/timeseries/qscan.rst.txt @@ -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/. \ No newline at end of file +http://www.ligo.org/science/Publication-GW150914/. diff --git a/docs/0.6.2/_sources/table/io.rst.txt b/docs/0.6.2/_sources/table/io.rst.txt index 5ed483d6e..cfd725eb1 100644 --- a/docs/0.6.2/_sources/table/io.rst.txt +++ b/docs/0.6.2/_sources/table/io.rst.txt @@ -187,7 +187,7 @@ Table name Format name Coherence WaveBurst ASCII (aka `EVENTS.txt`) ============================================ -The `Coherent WaveBurst `_ 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 `_ 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 diff --git a/docs/0.6.2/_sources/timeseries/remote-access.rst.txt b/docs/0.6.2/_sources/timeseries/remote-access.rst.txt index f0961fa64..4b0c55700 100644 --- a/docs/0.6.2/_sources/timeseries/remote-access.rst.txt +++ b/docs/0.6.2/_sources/timeseries/remote-access.rst.txt @@ -29,7 +29,7 @@ Open data releases The `LIGO Open Science Center `_ 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 `_, 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 `_, 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 diff --git a/docs/0.6.2/examples/signal/gw150914.html b/docs/0.6.2/examples/signal/gw150914.html index 10f152b9c..b88b5bdc2 100644 --- a/docs/0.6.2/examples/signal/gw150914.html +++ b/docs/0.6.2/examples/signal/gw150914.html @@ -270,4 +270,4 @@

- \ No newline at end of file + diff --git a/docs/0.6.2/examples/spectrogram/spectrogram2.html b/docs/0.6.2/examples/spectrogram/spectrogram2.html index 78ad5da42..0eb2a4462 100644 --- a/docs/0.6.2/examples/spectrogram/spectrogram2.html +++ b/docs/0.6.2/examples/spectrogram/spectrogram2.html @@ -234,4 +234,4 @@ - \ No newline at end of file + diff --git a/docs/0.6.2/examples/timeseries/qscan.html b/docs/0.6.2/examples/timeseries/qscan.html index d4396f476..3b818a9be 100644 --- a/docs/0.6.2/examples/timeseries/qscan.html +++ b/docs/0.6.2/examples/timeseries/qscan.html @@ -233,4 +233,4 @@ - \ No newline at end of file + diff --git a/docs/0.6.2/table/io.html b/docs/0.6.2/table/io.html index fca6919c8..354d5c785 100644 --- a/docs/0.6.2/table/io.html +++ b/docs/0.6.2/table/io.html @@ -439,7 +439,7 @@

Supported LIGO_LW tables

Coherence WaveBurst ASCII (aka EVENTS.txt)

-

The Coherent WaveBurst 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 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

@@ -1205,4 +1205,4 @@

Available file formats - \ No newline at end of file + diff --git a/docs/0.6.2/timeseries/remote-access.html b/docs/0.6.2/timeseries/remote-access.html index 03fcc4051..216071c4a 100644 --- a/docs/0.6.2/timeseries/remote-access.html +++ b/docs/0.6.2/timeseries/remote-access.html @@ -199,7 +199,7 @@

Open data releases

Additional dependencies: h5py

The LIGO Open Science Center 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, 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, 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:

>>> from gwpy.timeseries import TimeSeries
 >>> data = TimeSeries.fetch_open_data('L1', 1126259446, 1126259478)
@@ -266,4 +266,4 @@
- \ No newline at end of file + diff --git a/docs/0.7.0/_sources/examples/signal/gw150914.rst.txt b/docs/0.7.0/_sources/examples/signal/gw150914.rst.txt index 2d8e5aa8c..0d143c334 100644 --- a/docs/0.7.0/_sources/examples/signal/gw150914.rst.txt +++ b/docs/0.7.0/_sources/examples/signal/gw150914.rst.txt @@ -128,4 +128,4 @@ 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) `_ -(the joint LSC-Virgo publication announcing this detection). \ No newline at end of file +(the joint LSC-Virgo publication announcing this detection). diff --git a/docs/0.7.0/_sources/examples/spectrogram/spectrogram2.rst.txt b/docs/0.7.0/_sources/examples/spectrogram/spectrogram2.rst.txt index 592088cc6..5e1e570b0 100644 --- a/docs/0.7.0/_sources/examples/spectrogram/spectrogram2.rst.txt +++ b/docs/0.7.0/_sources/examples/spectrogram/spectrogram2.rst.txt @@ -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) `_ -(the joint LSC-Virgo publication announcing this detection). \ No newline at end of file +(the joint LSC-Virgo publication announcing this detection). diff --git a/docs/0.7.0/_sources/examples/timeseries/qscan.rst.txt b/docs/0.7.0/_sources/examples/timeseries/qscan.rst.txt index 67c1be414..70d3a3ae7 100644 --- a/docs/0.7.0/_sources/examples/timeseries/qscan.rst.txt +++ b/docs/0.7.0/_sources/examples/timeseries/qscan.rst.txt @@ -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/. \ No newline at end of file +http://www.ligo.org/science/Publication-GW150914/. diff --git a/docs/0.7.0/_sources/table/io.rst.txt b/docs/0.7.0/_sources/table/io.rst.txt index 334666422..399caca6c 100644 --- a/docs/0.7.0/_sources/table/io.rst.txt +++ b/docs/0.7.0/_sources/table/io.rst.txt @@ -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 `_ 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 `_ 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 diff --git a/docs/0.7.0/_sources/timeseries/remote-access.rst.txt b/docs/0.7.0/_sources/timeseries/remote-access.rst.txt index 7353e3eed..b8dbb7e91 100644 --- a/docs/0.7.0/_sources/timeseries/remote-access.rst.txt +++ b/docs/0.7.0/_sources/timeseries/remote-access.rst.txt @@ -28,7 +28,7 @@ Open data releases The `LIGO Open Science Center `_ 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 `_, 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 `_, 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 diff --git a/docs/0.7.0/examples/signal/gw150914.html b/docs/0.7.0/examples/signal/gw150914.html index 030389cef..5dd4c06d2 100644 --- a/docs/0.7.0/examples/signal/gw150914.html +++ b/docs/0.7.0/examples/signal/gw150914.html @@ -265,4 +265,4 @@

- \ No newline at end of file + diff --git a/docs/0.7.0/examples/spectrogram/spectrogram2.html b/docs/0.7.0/examples/spectrogram/spectrogram2.html index cab1b8843..5329a20a9 100644 --- a/docs/0.7.0/examples/spectrogram/spectrogram2.html +++ b/docs/0.7.0/examples/spectrogram/spectrogram2.html @@ -229,4 +229,4 @@ - \ No newline at end of file + diff --git a/docs/0.7.0/examples/timeseries/qscan.html b/docs/0.7.0/examples/timeseries/qscan.html index 862de0d19..303fe9771 100644 --- a/docs/0.7.0/examples/timeseries/qscan.html +++ b/docs/0.7.0/examples/timeseries/qscan.html @@ -228,4 +228,4 @@ - \ No newline at end of file + diff --git a/docs/0.7.0/table/io.html b/docs/0.7.0/table/io.html index 906c44081..57fb12455 100644 --- a/docs/0.7.0/table/io.html +++ b/docs/0.7.0/table/io.html @@ -322,7 +322,7 @@

Writing

Coherence WaveBurst ASCII (aka EVENTS.txt)

-

The Coherent WaveBurst 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 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

@@ -1083,4 +1083,4 @@

Available file formats - \ No newline at end of file + diff --git a/docs/0.7.0/timeseries/remote-access.html b/docs/0.7.0/timeseries/remote-access.html index f86e3ad63..0c28145c1 100644 --- a/docs/0.7.0/timeseries/remote-access.html +++ b/docs/0.7.0/timeseries/remote-access.html @@ -194,7 +194,7 @@

Open data releases

Additional dependencies: h5py

The LIGO Open Science Center 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, 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, 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:

>>> from gwpy.timeseries import TimeSeries
 >>> data = TimeSeries.fetch_open_data('L1', 1126259446, 1126259478)
@@ -261,4 +261,4 @@
- \ No newline at end of file + diff --git a/docs/0.7.5/_sources/examples/signal/gw150914.rst.txt b/docs/0.7.5/_sources/examples/signal/gw150914.rst.txt index 2d8e5aa8c..0d143c334 100644 --- a/docs/0.7.5/_sources/examples/signal/gw150914.rst.txt +++ b/docs/0.7.5/_sources/examples/signal/gw150914.rst.txt @@ -128,4 +128,4 @@ 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) `_ -(the joint LSC-Virgo publication announcing this detection). \ No newline at end of file +(the joint LSC-Virgo publication announcing this detection). diff --git a/docs/0.7.5/_sources/examples/spectrogram/spectrogram2.rst.txt b/docs/0.7.5/_sources/examples/spectrogram/spectrogram2.rst.txt index 592088cc6..5e1e570b0 100644 --- a/docs/0.7.5/_sources/examples/spectrogram/spectrogram2.rst.txt +++ b/docs/0.7.5/_sources/examples/spectrogram/spectrogram2.rst.txt @@ -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) `_ -(the joint LSC-Virgo publication announcing this detection). \ No newline at end of file +(the joint LSC-Virgo publication announcing this detection). diff --git a/docs/0.7.5/_sources/examples/timeseries/qscan.rst.txt b/docs/0.7.5/_sources/examples/timeseries/qscan.rst.txt index 67c1be414..70d3a3ae7 100644 --- a/docs/0.7.5/_sources/examples/timeseries/qscan.rst.txt +++ b/docs/0.7.5/_sources/examples/timeseries/qscan.rst.txt @@ -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/. \ No newline at end of file +http://www.ligo.org/science/Publication-GW150914/. diff --git a/docs/0.7.5/_sources/table/io.rst.txt b/docs/0.7.5/_sources/table/io.rst.txt index 334666422..399caca6c 100644 --- a/docs/0.7.5/_sources/table/io.rst.txt +++ b/docs/0.7.5/_sources/table/io.rst.txt @@ -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 `_ 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 `_ 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 diff --git a/docs/0.7.5/_sources/timeseries/remote-access.rst.txt b/docs/0.7.5/_sources/timeseries/remote-access.rst.txt index 7353e3eed..b8dbb7e91 100644 --- a/docs/0.7.5/_sources/timeseries/remote-access.rst.txt +++ b/docs/0.7.5/_sources/timeseries/remote-access.rst.txt @@ -28,7 +28,7 @@ Open data releases The `LIGO Open Science Center `_ 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 `_, 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 `_, 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 diff --git a/docs/0.7.5/examples/signal/gw150914.html b/docs/0.7.5/examples/signal/gw150914.html index 75b58ee73..2bca3b6d1 100644 --- a/docs/0.7.5/examples/signal/gw150914.html +++ b/docs/0.7.5/examples/signal/gw150914.html @@ -268,4 +268,4 @@

- \ No newline at end of file + diff --git a/docs/0.7.5/examples/spectrogram/spectrogram2.html b/docs/0.7.5/examples/spectrogram/spectrogram2.html index 525c270c3..5a9a8441e 100644 --- a/docs/0.7.5/examples/spectrogram/spectrogram2.html +++ b/docs/0.7.5/examples/spectrogram/spectrogram2.html @@ -232,4 +232,4 @@ - \ No newline at end of file + diff --git a/docs/0.7.5/examples/timeseries/qscan.html b/docs/0.7.5/examples/timeseries/qscan.html index adb78b98c..7d412f667 100644 --- a/docs/0.7.5/examples/timeseries/qscan.html +++ b/docs/0.7.5/examples/timeseries/qscan.html @@ -231,4 +231,4 @@ - \ No newline at end of file + diff --git a/docs/0.7.5/table/io.html b/docs/0.7.5/table/io.html index d470caad7..76d71fa38 100644 --- a/docs/0.7.5/table/io.html +++ b/docs/0.7.5/table/io.html @@ -325,7 +325,7 @@

Writing

Coherence WaveBurst ASCII (aka EVENTS.txt)

-

The Coherent WaveBurst 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 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

@@ -1086,4 +1086,4 @@

Available file formats - \ No newline at end of file + diff --git a/docs/0.7.5/timeseries/remote-access.html b/docs/0.7.5/timeseries/remote-access.html index db63a7037..38cfa4d3c 100644 --- a/docs/0.7.5/timeseries/remote-access.html +++ b/docs/0.7.5/timeseries/remote-access.html @@ -197,7 +197,7 @@

Open data releases

Additional dependencies: h5py

The LIGO Open Science Center 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, 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, 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:

>>> from gwpy.timeseries import TimeSeries
 >>> data = TimeSeries.fetch_open_data('L1', 1126259446, 1126259478)
@@ -264,4 +264,4 @@
- \ No newline at end of file + diff --git a/docs/0.8.0/_sources/examples/signal/gw150914.rst.txt b/docs/0.8.0/_sources/examples/signal/gw150914.rst.txt index 2d8e5aa8c..0d143c334 100644 --- a/docs/0.8.0/_sources/examples/signal/gw150914.rst.txt +++ b/docs/0.8.0/_sources/examples/signal/gw150914.rst.txt @@ -128,4 +128,4 @@ 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) `_ -(the joint LSC-Virgo publication announcing this detection). \ No newline at end of file +(the joint LSC-Virgo publication announcing this detection). diff --git a/docs/0.8.0/_sources/examples/spectrogram/spectrogram2.rst.txt b/docs/0.8.0/_sources/examples/spectrogram/spectrogram2.rst.txt index 592088cc6..5e1e570b0 100644 --- a/docs/0.8.0/_sources/examples/spectrogram/spectrogram2.rst.txt +++ b/docs/0.8.0/_sources/examples/spectrogram/spectrogram2.rst.txt @@ -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) `_ -(the joint LSC-Virgo publication announcing this detection). \ No newline at end of file +(the joint LSC-Virgo publication announcing this detection). diff --git a/docs/0.8.0/_sources/examples/timeseries/qscan.rst.txt b/docs/0.8.0/_sources/examples/timeseries/qscan.rst.txt index 67c1be414..70d3a3ae7 100644 --- a/docs/0.8.0/_sources/examples/timeseries/qscan.rst.txt +++ b/docs/0.8.0/_sources/examples/timeseries/qscan.rst.txt @@ -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/. \ No newline at end of file +http://www.ligo.org/science/Publication-GW150914/. diff --git a/docs/0.8.0/_sources/table/io.rst.txt b/docs/0.8.0/_sources/table/io.rst.txt index 334666422..399caca6c 100644 --- a/docs/0.8.0/_sources/table/io.rst.txt +++ b/docs/0.8.0/_sources/table/io.rst.txt @@ -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 `_ 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 `_ 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 diff --git a/docs/0.8.0/_sources/timeseries/remote-access.rst.txt b/docs/0.8.0/_sources/timeseries/remote-access.rst.txt index 7353e3eed..b8dbb7e91 100644 --- a/docs/0.8.0/_sources/timeseries/remote-access.rst.txt +++ b/docs/0.8.0/_sources/timeseries/remote-access.rst.txt @@ -28,7 +28,7 @@ Open data releases The `LIGO Open Science Center `_ 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 `_, 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 `_, 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 diff --git a/docs/0.8.0/examples/signal/gw150914.html b/docs/0.8.0/examples/signal/gw150914.html index 8829692b1..ebb4c1758 100644 --- a/docs/0.8.0/examples/signal/gw150914.html +++ b/docs/0.8.0/examples/signal/gw150914.html @@ -268,4 +268,4 @@

- \ No newline at end of file + diff --git a/docs/0.8.0/examples/spectrogram/spectrogram2.html b/docs/0.8.0/examples/spectrogram/spectrogram2.html index 3ac48084b..7277d3f92 100644 --- a/docs/0.8.0/examples/spectrogram/spectrogram2.html +++ b/docs/0.8.0/examples/spectrogram/spectrogram2.html @@ -232,4 +232,4 @@ - \ No newline at end of file + diff --git a/docs/0.8.0/examples/timeseries/qscan.html b/docs/0.8.0/examples/timeseries/qscan.html index fe24b58e1..30a6b166f 100644 --- a/docs/0.8.0/examples/timeseries/qscan.html +++ b/docs/0.8.0/examples/timeseries/qscan.html @@ -231,4 +231,4 @@ - \ No newline at end of file + diff --git a/docs/0.8.0/table/io.html b/docs/0.8.0/table/io.html index ba2fa65e1..73c8271f2 100644 --- a/docs/0.8.0/table/io.html +++ b/docs/0.8.0/table/io.html @@ -325,7 +325,7 @@

Writing

Coherence WaveBurst ASCII (aka EVENTS.txt)

-

The Coherent WaveBurst 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 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

@@ -1086,4 +1086,4 @@

Available file formats - \ No newline at end of file + diff --git a/docs/0.8.0/timeseries/remote-access.html b/docs/0.8.0/timeseries/remote-access.html index 47c680c9f..b18ae4043 100644 --- a/docs/0.8.0/timeseries/remote-access.html +++ b/docs/0.8.0/timeseries/remote-access.html @@ -197,7 +197,7 @@

Open data releases

Additional dependencies: h5py

The LIGO Open Science Center 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, 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, 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:

>>> from gwpy.timeseries import TimeSeries
 >>> data = TimeSeries.fetch_open_data('L1', 1126259446, 1126259478)
@@ -264,4 +264,4 @@
- \ No newline at end of file + diff --git a/docs/0.8.1/_sources/examples/signal/gw150914.rst.txt b/docs/0.8.1/_sources/examples/signal/gw150914.rst.txt index 2d8e5aa8c..0d143c334 100644 --- a/docs/0.8.1/_sources/examples/signal/gw150914.rst.txt +++ b/docs/0.8.1/_sources/examples/signal/gw150914.rst.txt @@ -128,4 +128,4 @@ 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) `_ -(the joint LSC-Virgo publication announcing this detection). \ No newline at end of file +(the joint LSC-Virgo publication announcing this detection). diff --git a/docs/0.8.1/_sources/examples/spectrogram/spectrogram2.rst.txt b/docs/0.8.1/_sources/examples/spectrogram/spectrogram2.rst.txt index 592088cc6..5e1e570b0 100644 --- a/docs/0.8.1/_sources/examples/spectrogram/spectrogram2.rst.txt +++ b/docs/0.8.1/_sources/examples/spectrogram/spectrogram2.rst.txt @@ -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) `_ -(the joint LSC-Virgo publication announcing this detection). \ No newline at end of file +(the joint LSC-Virgo publication announcing this detection). diff --git a/docs/0.8.1/_sources/examples/timeseries/qscan.rst.txt b/docs/0.8.1/_sources/examples/timeseries/qscan.rst.txt index 67c1be414..70d3a3ae7 100644 --- a/docs/0.8.1/_sources/examples/timeseries/qscan.rst.txt +++ b/docs/0.8.1/_sources/examples/timeseries/qscan.rst.txt @@ -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/. \ No newline at end of file +http://www.ligo.org/science/Publication-GW150914/. diff --git a/docs/0.8.1/_sources/table/io.rst.txt b/docs/0.8.1/_sources/table/io.rst.txt index 334666422..399caca6c 100644 --- a/docs/0.8.1/_sources/table/io.rst.txt +++ b/docs/0.8.1/_sources/table/io.rst.txt @@ -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 `_ 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 `_ 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 diff --git a/docs/0.8.1/_sources/timeseries/remote-access.rst.txt b/docs/0.8.1/_sources/timeseries/remote-access.rst.txt index 7353e3eed..b8dbb7e91 100644 --- a/docs/0.8.1/_sources/timeseries/remote-access.rst.txt +++ b/docs/0.8.1/_sources/timeseries/remote-access.rst.txt @@ -28,7 +28,7 @@ Open data releases The `LIGO Open Science Center `_ 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 `_, 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 `_, 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 diff --git a/docs/0.8.1/citing.html b/docs/0.8.1/citing.html index fab63b013..d326d49c4 100644 --- a/docs/0.8.1/citing.html +++ b/docs/0.8.1/citing.html @@ -243,4 +243,4 @@

0.5.2

- \ No newline at end of file + diff --git a/docs/0.8.1/examples/signal/gw150914.html b/docs/0.8.1/examples/signal/gw150914.html index a6bae3db9..5aaf15ae7 100644 --- a/docs/0.8.1/examples/signal/gw150914.html +++ b/docs/0.8.1/examples/signal/gw150914.html @@ -269,4 +269,4 @@ - \ No newline at end of file + diff --git a/docs/0.8.1/examples/spectrogram/spectrogram2.html b/docs/0.8.1/examples/spectrogram/spectrogram2.html index effdcccfb..a35ad146d 100644 --- a/docs/0.8.1/examples/spectrogram/spectrogram2.html +++ b/docs/0.8.1/examples/spectrogram/spectrogram2.html @@ -233,4 +233,4 @@ - \ No newline at end of file + diff --git a/docs/0.8.1/examples/timeseries/qscan.html b/docs/0.8.1/examples/timeseries/qscan.html index 1851d1e06..8f6055cc2 100644 --- a/docs/0.8.1/examples/timeseries/qscan.html +++ b/docs/0.8.1/examples/timeseries/qscan.html @@ -232,4 +232,4 @@ - \ No newline at end of file + diff --git a/docs/0.8.1/table/io.html b/docs/0.8.1/table/io.html index 9bd75993b..3e5b61cc1 100644 --- a/docs/0.8.1/table/io.html +++ b/docs/0.8.1/table/io.html @@ -326,7 +326,7 @@

Writing

Coherence WaveBurst ASCII (aka EVENTS.txt)

-

The Coherent WaveBurst 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 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

@@ -1087,4 +1087,4 @@

Available file formats - \ No newline at end of file + diff --git a/docs/0.8.1/timeseries/remote-access.html b/docs/0.8.1/timeseries/remote-access.html index 30f42bedf..cfabff74e 100644 --- a/docs/0.8.1/timeseries/remote-access.html +++ b/docs/0.8.1/timeseries/remote-access.html @@ -198,7 +198,7 @@

Open data releases

Additional dependencies: h5py

The LIGO Open Science Center 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, 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, 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:

>>> from gwpy.timeseries import TimeSeries
 >>> data = TimeSeries.fetch_open_data('L1', 1126259446, 1126259478)
@@ -265,4 +265,4 @@
- \ No newline at end of file + diff --git a/docs/0.9.0/_sources/examples/signal/gw150914.rst.txt b/docs/0.9.0/_sources/examples/signal/gw150914.rst.txt index 53318bc8d..f73deb634 100644 --- a/docs/0.9.0/_sources/examples/signal/gw150914.rst.txt +++ b/docs/0.9.0/_sources/examples/signal/gw150914.rst.txt @@ -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) `_ -(the joint LSC-Virgo publication announcing this detection). \ No newline at end of file +(the joint LSC-Virgo publication announcing this detection). diff --git a/docs/0.9.0/_sources/examples/spectrogram/spectrogram2.rst.txt b/docs/0.9.0/_sources/examples/spectrogram/spectrogram2.rst.txt index 592088cc6..5e1e570b0 100644 --- a/docs/0.9.0/_sources/examples/spectrogram/spectrogram2.rst.txt +++ b/docs/0.9.0/_sources/examples/spectrogram/spectrogram2.rst.txt @@ -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) `_ -(the joint LSC-Virgo publication announcing this detection). \ No newline at end of file +(the joint LSC-Virgo publication announcing this detection). diff --git a/docs/0.9.0/_sources/examples/timeseries/qscan.rst.txt b/docs/0.9.0/_sources/examples/timeseries/qscan.rst.txt index 67c1be414..70d3a3ae7 100644 --- a/docs/0.9.0/_sources/examples/timeseries/qscan.rst.txt +++ b/docs/0.9.0/_sources/examples/timeseries/qscan.rst.txt @@ -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/. \ No newline at end of file +http://www.ligo.org/science/Publication-GW150914/. diff --git a/docs/0.9.0/_sources/table/io.rst.txt b/docs/0.9.0/_sources/table/io.rst.txt index 334666422..399caca6c 100644 --- a/docs/0.9.0/_sources/table/io.rst.txt +++ b/docs/0.9.0/_sources/table/io.rst.txt @@ -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 `_ 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 `_ 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 diff --git a/docs/0.9.0/_sources/timeseries/remote-access.rst.txt b/docs/0.9.0/_sources/timeseries/remote-access.rst.txt index 6dcbdced6..0bb2e3d02 100644 --- a/docs/0.9.0/_sources/timeseries/remote-access.rst.txt +++ b/docs/0.9.0/_sources/timeseries/remote-access.rst.txt @@ -28,7 +28,7 @@ Open data releases The `LIGO Open Science Center `_ 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 `_, 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 `_, 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 diff --git a/docs/0.9.0/citing.html b/docs/0.9.0/citing.html index d2d59dfe1..07b8a42a7 100644 --- a/docs/0.9.0/citing.html +++ b/docs/0.9.0/citing.html @@ -243,4 +243,4 @@

0.5.2

- \ No newline at end of file + diff --git a/docs/0.9.0/examples/signal/gw150914.html b/docs/0.9.0/examples/signal/gw150914.html index 2fd3cebb8..5bcabb953 100644 --- a/docs/0.9.0/examples/signal/gw150914.html +++ b/docs/0.9.0/examples/signal/gw150914.html @@ -309,4 +309,4 @@ - \ No newline at end of file + diff --git a/docs/0.9.0/examples/spectrogram/spectrogram2.html b/docs/0.9.0/examples/spectrogram/spectrogram2.html index 89ca38c92..d635e6ceb 100644 --- a/docs/0.9.0/examples/spectrogram/spectrogram2.html +++ b/docs/0.9.0/examples/spectrogram/spectrogram2.html @@ -233,4 +233,4 @@ - \ No newline at end of file + diff --git a/docs/0.9.0/examples/timeseries/qscan.html b/docs/0.9.0/examples/timeseries/qscan.html index 91e52770a..e073ff730 100644 --- a/docs/0.9.0/examples/timeseries/qscan.html +++ b/docs/0.9.0/examples/timeseries/qscan.html @@ -232,4 +232,4 @@ - \ No newline at end of file + diff --git a/docs/0.9.0/table/io.html b/docs/0.9.0/table/io.html index 69d883525..e7d10fed8 100644 --- a/docs/0.9.0/table/io.html +++ b/docs/0.9.0/table/io.html @@ -326,7 +326,7 @@

Writing

Coherence WaveBurst ASCII (aka EVENTS.txt)

-

The Coherent WaveBurst 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 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

@@ -1087,4 +1087,4 @@

Available file formats - \ No newline at end of file + diff --git a/docs/0.9.0/timeseries/remote-access.html b/docs/0.9.0/timeseries/remote-access.html index 9dbf3c36f..730a16e53 100644 --- a/docs/0.9.0/timeseries/remote-access.html +++ b/docs/0.9.0/timeseries/remote-access.html @@ -198,7 +198,7 @@

Open data releases

Additional dependencies: h5py

The LIGO Open Science Center 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, 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, 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:

>>> from gwpy.timeseries import TimeSeries
 >>> data = TimeSeries.fetch_open_data('L1', 1126259446, 1126259478)
@@ -273,4 +273,4 @@
- \ No newline at end of file + diff --git a/docs/latest/_sources/citing.rst.txt b/docs/latest/_sources/citing.rst.txt index ef055116e..b310b7684 100644 --- a/docs/latest/_sources/citing.rst.txt +++ b/docs/latest/_sources/citing.rst.txt @@ -81,4 +81,4 @@ For older versions, please `click here `_ -(the joint LSC-Virgo publication announcing this detection). \ No newline at end of file +(the joint LSC-Virgo publication announcing this detection). diff --git a/docs/latest/_sources/examples/spectrogram/spectrogram2.rst.txt b/docs/latest/_sources/examples/spectrogram/spectrogram2.rst.txt index d4320a1aa..1ba3d450c 100644 --- a/docs/latest/_sources/examples/spectrogram/spectrogram2.rst.txt +++ b/docs/latest/_sources/examples/spectrogram/spectrogram2.rst.txt @@ -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) `_ -(the joint LSC-Virgo publication announcing this detection). \ No newline at end of file +(the joint LSC-Virgo publication announcing this detection). diff --git a/docs/latest/_sources/examples/timeseries/qscan.rst.txt b/docs/latest/_sources/examples/timeseries/qscan.rst.txt index a58d915f0..ceba40976 100644 --- a/docs/latest/_sources/examples/timeseries/qscan.rst.txt +++ b/docs/latest/_sources/examples/timeseries/qscan.rst.txt @@ -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/. \ No newline at end of file +http://www.ligo.org/science/Publication-GW150914/. diff --git a/docs/latest/_sources/examples/timeseries/statevector.rst.txt b/docs/latest/_sources/examples/timeseries/statevector.rst.txt index 51aae408b..af16b0686 100644 --- a/docs/latest/_sources/examples/timeseries/statevector.rst.txt +++ b/docs/latest/_sources/examples/timeseries/statevector.rst.txt @@ -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 `__. \ No newline at end of file +`Abbott et al. 2017 `__. diff --git a/docs/latest/_sources/table/io.rst.txt b/docs/latest/_sources/table/io.rst.txt index 822a1da4a..8813a3ca0 100644 --- a/docs/latest/_sources/table/io.rst.txt +++ b/docs/latest/_sources/table/io.rst.txt @@ -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 `_ 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 `_ 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 diff --git a/docs/latest/_sources/timeseries/index.txt b/docs/latest/_sources/timeseries/index.txt index 543252434..ba7d3bc34 100644 --- a/docs/latest/_sources/timeseries/index.txt +++ b/docs/latest/_sources/timeseries/index.txt @@ -28,7 +28,7 @@ Method Restricted? Description Public ------ -For example, to fetch 32 seconds of strain data around event `GW150914 `_:: +For example, to fetch 32 seconds of strain data around event `GW150914 `_:: from gwpy.timeseries import TimeSeries data = TimeSeries.fetch_open_data('L1', 1126259446, 1126259478) diff --git a/docs/latest/_sources/timeseries/remote-access.rst.txt b/docs/latest/_sources/timeseries/remote-access.rst.txt index 06fde94f7..dc354208f 100644 --- a/docs/latest/_sources/timeseries/remote-access.rst.txt +++ b/docs/latest/_sources/timeseries/remote-access.rst.txt @@ -26,7 +26,7 @@ Open data releases The `LIGO Open Science Center `_ 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 `_, 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 `_, 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 diff --git a/docs/latest/citing.html b/docs/latest/citing.html index b7ddcf5d4..5f6b337fd 100644 --- a/docs/latest/citing.html +++ b/docs/latest/citing.html @@ -234,4 +234,4 @@

0.7.1

- \ No newline at end of file + diff --git a/docs/latest/examples/signal/gw150914.html b/docs/latest/examples/signal/gw150914.html index 8b39c54d3..1988b2f42 100644 --- a/docs/latest/examples/signal/gw150914.html +++ b/docs/latest/examples/signal/gw150914.html @@ -300,4 +300,4 @@ - \ No newline at end of file + diff --git a/docs/latest/examples/spectrogram/spectrogram2.html b/docs/latest/examples/spectrogram/spectrogram2.html index 37040e59c..87078e32e 100644 --- a/docs/latest/examples/spectrogram/spectrogram2.html +++ b/docs/latest/examples/spectrogram/spectrogram2.html @@ -224,4 +224,4 @@ - \ No newline at end of file + diff --git a/docs/latest/examples/timeseries/qscan.html b/docs/latest/examples/timeseries/qscan.html index dd40e9794..05a0c7b89 100644 --- a/docs/latest/examples/timeseries/qscan.html +++ b/docs/latest/examples/timeseries/qscan.html @@ -214,4 +214,4 @@ - \ No newline at end of file + diff --git a/docs/latest/examples/timeseries/statevector.html b/docs/latest/examples/timeseries/statevector.html index f27d120a1..989b436b3 100644 --- a/docs/latest/examples/timeseries/statevector.html +++ b/docs/latest/examples/timeseries/statevector.html @@ -208,4 +208,4 @@ - \ No newline at end of file + diff --git a/docs/latest/table/io.html b/docs/latest/table/io.html index 3f15ad4d0..e3bb859e6 100644 --- a/docs/latest/table/io.html +++ b/docs/latest/table/io.html @@ -317,7 +317,7 @@

Writing

Coherence WaveBurst ASCII (aka EVENTS.txt)

-

The Coherent WaveBurst 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 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

@@ -860,4 +860,4 @@

Available file formats - \ No newline at end of file + diff --git a/docs/latest/timeseries/remote-access.html b/docs/latest/timeseries/remote-access.html index 160a32c22..69dae3106 100644 --- a/docs/latest/timeseries/remote-access.html +++ b/docs/latest/timeseries/remote-access.html @@ -188,7 +188,7 @@

Open data releases

The LIGO Open Science Center 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, 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, 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:

>>> from gwpy.timeseries import TimeSeries
 >>> data = TimeSeries.fetch_open_data('L1', 1126259446, 1126259478)
@@ -263,4 +263,4 @@
- \ No newline at end of file + diff --git a/docs/v0.1/_sources/timeseries/index.txt b/docs/v0.1/_sources/timeseries/index.txt index 543252434..ba7d3bc34 100644 --- a/docs/v0.1/_sources/timeseries/index.txt +++ b/docs/v0.1/_sources/timeseries/index.txt @@ -28,7 +28,7 @@ Method Restricted? Description Public ------ -For example, to fetch 32 seconds of strain data around event `GW150914 `_:: +For example, to fetch 32 seconds of strain data around event `GW150914 `_:: from gwpy.timeseries import TimeSeries data = TimeSeries.fetch_open_data('L1', 1126259446, 1126259478) diff --git a/docs/v0.1/timeseries/index.html b/docs/v0.1/timeseries/index.html index 86d133336..e74d04557 100644 --- a/docs/v0.1/timeseries/index.html +++ b/docs/v0.1/timeseries/index.html @@ -201,7 +201,7 @@

Remote data access

Public

-

For example, to fetch 32 seconds of strain data around event GW150914:

+

For example, to fetch 32 seconds of strain data around event GW150914:

from gwpy.timeseries import TimeSeries
 data = TimeSeries.fetch_open_data('L1', 1126259446, 1126259478)
@@ -5783,4 +5783,4 @@

Reference/API

Coherence WaveBurst ASCII (aka EVENTS.txt)

-

The Coherent WaveBurst 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 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

@@ -1024,4 +1024,4 @@

Available file formats - \ No newline at end of file + diff --git a/docs/v0.3/timeseries/remote-access.html b/docs/v0.3/timeseries/remote-access.html index c1592054b..641764c0c 100644 --- a/docs/v0.3/timeseries/remote-access.html +++ b/docs/v0.3/timeseries/remote-access.html @@ -199,7 +199,7 @@

Open data releases

Additional dependencies: h5py

The LIGO Open Science Center 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, 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, 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:

>>> from gwpy.timeseries import TimeSeries
 >>> data = TimeSeries.fetch_open_data('L1', 1126259446, 1126259478)
@@ -266,4 +266,4 @@
- \ No newline at end of file + diff --git a/docs/v0.4/_sources/examples/signal/gw150914.rst.txt b/docs/v0.4/_sources/examples/signal/gw150914.rst.txt index 690908291..d945940d5 100644 --- a/docs/v0.4/_sources/examples/signal/gw150914.rst.txt +++ b/docs/v0.4/_sources/examples/signal/gw150914.rst.txt @@ -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) `_ -(the joint LSC-Virgo publication announcing this detection). \ No newline at end of file +(the joint LSC-Virgo publication announcing this detection). diff --git a/docs/v0.4/_sources/examples/spectrogram/spectrogram2.rst.txt b/docs/v0.4/_sources/examples/spectrogram/spectrogram2.rst.txt index 592088cc6..5e1e570b0 100644 --- a/docs/v0.4/_sources/examples/spectrogram/spectrogram2.rst.txt +++ b/docs/v0.4/_sources/examples/spectrogram/spectrogram2.rst.txt @@ -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) `_ -(the joint LSC-Virgo publication announcing this detection). \ No newline at end of file +(the joint LSC-Virgo publication announcing this detection). diff --git a/docs/v0.4/_sources/examples/timeseries/qscan.rst.txt b/docs/v0.4/_sources/examples/timeseries/qscan.rst.txt index 67c1be414..70d3a3ae7 100644 --- a/docs/v0.4/_sources/examples/timeseries/qscan.rst.txt +++ b/docs/v0.4/_sources/examples/timeseries/qscan.rst.txt @@ -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/. \ No newline at end of file +http://www.ligo.org/science/Publication-GW150914/. diff --git a/docs/v0.4/_sources/table/io.rst.txt b/docs/v0.4/_sources/table/io.rst.txt index 1085728af..cf0867331 100644 --- a/docs/v0.4/_sources/table/io.rst.txt +++ b/docs/v0.4/_sources/table/io.rst.txt @@ -178,7 +178,7 @@ Table name Format name Coherence WaveBurst ASCII (aka `EVENTS.txt`) ============================================ -The `Coherent WaveBurst `_ 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 `_ 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 diff --git a/docs/v0.4/_sources/timeseries/remote-access.rst.txt b/docs/v0.4/_sources/timeseries/remote-access.rst.txt index f0961fa64..4b0c55700 100644 --- a/docs/v0.4/_sources/timeseries/remote-access.rst.txt +++ b/docs/v0.4/_sources/timeseries/remote-access.rst.txt @@ -29,7 +29,7 @@ Open data releases The `LIGO Open Science Center `_ 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 `_, 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 `_, 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 diff --git a/docs/v0.4/examples/signal/gw150914.html b/docs/v0.4/examples/signal/gw150914.html index d716f1e8d..7302b1cfd 100644 --- a/docs/v0.4/examples/signal/gw150914.html +++ b/docs/v0.4/examples/signal/gw150914.html @@ -269,4 +269,4 @@

- \ No newline at end of file + diff --git a/docs/v0.4/examples/spectrogram/spectrogram2.html b/docs/v0.4/examples/spectrogram/spectrogram2.html index 874cca48c..f5c4cafd4 100644 --- a/docs/v0.4/examples/spectrogram/spectrogram2.html +++ b/docs/v0.4/examples/spectrogram/spectrogram2.html @@ -234,4 +234,4 @@

- \ No newline at end of file + diff --git a/docs/v0.4/examples/timeseries/qscan.html b/docs/v0.4/examples/timeseries/qscan.html index dda93f0c8..de76cc60a 100644 --- a/docs/v0.4/examples/timeseries/qscan.html +++ b/docs/v0.4/examples/timeseries/qscan.html @@ -233,4 +233,4 @@

- \ No newline at end of file + diff --git a/docs/v0.4/table/io.html b/docs/v0.4/table/io.html index 37e259a4e..4be5ef260 100644 --- a/docs/v0.4/table/io.html +++ b/docs/v0.4/table/io.html @@ -431,7 +431,7 @@

Supported LIGO_LW tables

Coherence WaveBurst ASCII (aka EVENTS.txt)

-

The Coherent WaveBurst 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 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

@@ -1071,4 +1071,4 @@

Available file formats - \ No newline at end of file + diff --git a/docs/v0.4/timeseries/remote-access.html b/docs/v0.4/timeseries/remote-access.html index fd3cca69f..7a35932ad 100644 --- a/docs/v0.4/timeseries/remote-access.html +++ b/docs/v0.4/timeseries/remote-access.html @@ -199,7 +199,7 @@

Open data releases

Additional dependencies: h5py

The LIGO Open Science Center 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, 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, 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:

>>> from gwpy.timeseries import TimeSeries
 >>> data = TimeSeries.fetch_open_data('L1', 1126259446, 1126259478)
@@ -266,4 +266,4 @@
- \ No newline at end of file + diff --git a/docs/v0.5/_sources/examples/signal/gw150914.rst.txt b/docs/v0.5/_sources/examples/signal/gw150914.rst.txt index 690908291..d945940d5 100644 --- a/docs/v0.5/_sources/examples/signal/gw150914.rst.txt +++ b/docs/v0.5/_sources/examples/signal/gw150914.rst.txt @@ -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) `_ -(the joint LSC-Virgo publication announcing this detection). \ No newline at end of file +(the joint LSC-Virgo publication announcing this detection). diff --git a/docs/v0.5/_sources/examples/spectrogram/spectrogram2.rst.txt b/docs/v0.5/_sources/examples/spectrogram/spectrogram2.rst.txt index 592088cc6..5e1e570b0 100644 --- a/docs/v0.5/_sources/examples/spectrogram/spectrogram2.rst.txt +++ b/docs/v0.5/_sources/examples/spectrogram/spectrogram2.rst.txt @@ -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) `_ -(the joint LSC-Virgo publication announcing this detection). \ No newline at end of file +(the joint LSC-Virgo publication announcing this detection). diff --git a/docs/v0.5/_sources/examples/timeseries/qscan.rst.txt b/docs/v0.5/_sources/examples/timeseries/qscan.rst.txt index 67c1be414..70d3a3ae7 100644 --- a/docs/v0.5/_sources/examples/timeseries/qscan.rst.txt +++ b/docs/v0.5/_sources/examples/timeseries/qscan.rst.txt @@ -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/. \ No newline at end of file +http://www.ligo.org/science/Publication-GW150914/. diff --git a/docs/v0.5/_sources/table/io.rst.txt b/docs/v0.5/_sources/table/io.rst.txt index b474eb327..43a81369b 100644 --- a/docs/v0.5/_sources/table/io.rst.txt +++ b/docs/v0.5/_sources/table/io.rst.txt @@ -187,7 +187,7 @@ Table name Format name Coherence WaveBurst ASCII (aka `EVENTS.txt`) ============================================ -The `Coherent WaveBurst `_ 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 `_ 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 diff --git a/docs/v0.5/_sources/timeseries/index.txt b/docs/v0.5/_sources/timeseries/index.txt index 543252434..ba7d3bc34 100644 --- a/docs/v0.5/_sources/timeseries/index.txt +++ b/docs/v0.5/_sources/timeseries/index.txt @@ -28,7 +28,7 @@ Method Restricted? Description Public ------ -For example, to fetch 32 seconds of strain data around event `GW150914 `_:: +For example, to fetch 32 seconds of strain data around event `GW150914 `_:: from gwpy.timeseries import TimeSeries data = TimeSeries.fetch_open_data('L1', 1126259446, 1126259478) diff --git a/docs/v0.5/_sources/timeseries/remote-access.rst.txt b/docs/v0.5/_sources/timeseries/remote-access.rst.txt index f0961fa64..4b0c55700 100644 --- a/docs/v0.5/_sources/timeseries/remote-access.rst.txt +++ b/docs/v0.5/_sources/timeseries/remote-access.rst.txt @@ -29,7 +29,7 @@ Open data releases The `LIGO Open Science Center `_ 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 `_, 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 `_, 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 diff --git a/docs/v0.5/examples/signal/gw150914.html b/docs/v0.5/examples/signal/gw150914.html index 19d3929a1..b08b48792 100644 --- a/docs/v0.5/examples/signal/gw150914.html +++ b/docs/v0.5/examples/signal/gw150914.html @@ -269,4 +269,4 @@

- \ No newline at end of file + diff --git a/docs/v0.5/examples/spectrogram/spectrogram2.html b/docs/v0.5/examples/spectrogram/spectrogram2.html index f6597b8cc..ec99f627f 100644 --- a/docs/v0.5/examples/spectrogram/spectrogram2.html +++ b/docs/v0.5/examples/spectrogram/spectrogram2.html @@ -234,4 +234,4 @@

- \ No newline at end of file + diff --git a/docs/v0.5/examples/timeseries/qscan.html b/docs/v0.5/examples/timeseries/qscan.html index 67b3e0370..711339acc 100644 --- a/docs/v0.5/examples/timeseries/qscan.html +++ b/docs/v0.5/examples/timeseries/qscan.html @@ -233,4 +233,4 @@ - \ No newline at end of file + diff --git a/docs/v0.5/table/io.html b/docs/v0.5/table/io.html index 2723990c8..bc24d3942 100644 --- a/docs/v0.5/table/io.html +++ b/docs/v0.5/table/io.html @@ -439,7 +439,7 @@

Supported LIGO_LW tables

Coherence WaveBurst ASCII (aka EVENTS.txt)

-

The Coherent WaveBurst 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 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

@@ -1197,4 +1197,4 @@

Available file formats - \ No newline at end of file + diff --git a/docs/v0.5/timeseries/remote-access.html b/docs/v0.5/timeseries/remote-access.html index 8998a8f00..58cd9c6d6 100644 --- a/docs/v0.5/timeseries/remote-access.html +++ b/docs/v0.5/timeseries/remote-access.html @@ -199,7 +199,7 @@

Open data releases

Additional dependencies: h5py

The LIGO Open Science Center 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, 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, 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:

>>> from gwpy.timeseries import TimeSeries
 >>> data = TimeSeries.fetch_open_data('L1', 1126259446, 1126259478)
@@ -266,4 +266,4 @@
- \ No newline at end of file +