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The LIGO Open Science Center

· 2014 · gr-qc · arXiv 1410.4839

2 Pith papers cite this work. Polarity classification is still indexing.

2 Pith papers citing it
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abstract

The LIGO Open Science Center (LOSC) fulfills LIGO's commitment to release, archive, and serve LIGO data in a broadly accessible way to the scientific community and to the public, and to provide the information and tools necessary to understand and use the data. In August 2014, the LOSC published the full dataset from Initial LIGO's "S5" run at design sensitivity, the first such large-scale release and a valuable testbed to explore the use of LIGO data by non-LIGO researchers and by the public, and to help teach gravitational-wave data analysis to students across the world. In addition to serving the S5 data, the LOSC web portal (losc.ligo.org) now offers documentation, data-location and data-quality queries, tutorials and example code, and more. We review the mission and plans of the LOSC, focusing on the S5 data release.

citation-role summary

dataset 1

citation-polarity summary

use dataset 1

fields

gr-qc 2

years

2019 2

verdicts

ACCEPT 1 UNVERDICTED 1

roles

dataset 1

polarities

use dataset 1

representative citing papers

Testing the no-hair theorem with GW150914

gr-qc · 2019-05-02 · unverdicted · novelty 6.0

Ringdown analysis of GW150914 with overtones measures remnant mass and spin consistent with a Kerr black hole, supporting the no-hair theorem at the 10% level.

citing papers explorer

Showing 2 of 2 citing papers.

  • Open data from the first and second observing runs of Advanced LIGO and Advanced Virgo gr-qc · 2019-12-25 · accept · none · ref 21 · internal anchor

    The LIGO and Virgo collaborations have released the gravitational-wave strain time series data from O1 and O2 observing runs, sampled at 16384 Hz, together with data-quality information through the Gravitational Wave Open Science Center.

  • Testing the no-hair theorem with GW150914 gr-qc · 2019-05-02 · unverdicted · none · ref 56 · internal anchor

    Ringdown analysis of GW150914 with overtones measures remnant mass and spin consistent with a Kerr black hole, supporting the no-hair theorem at the 10% level.