Dataset Open Access

GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run — O1+O2+O3 Search Sensitivity Estimates

LIGO Scientific Collaboration and Virgo Collaboration and KAGRA Collaboration

This material is part of several data products associated with GWTC-3, the third Gravitational-Wave Transient Catalog from the LIGO Scientific Collaboration, the Virgo Collaboration, and the KAGRA Collaboration. For more information, see the papers (dcc.ligo.org/LIGO-P2000318/public and dcc.ligo.org/LIGO-P2100239/public), the related material linked from this page, and the GWTC-3 data release documentation (www.gw-openscience.org/GWTC-3/).

O1 + O2 + O3 Search Sensitivity Estimates

This document contains HDF injection summary files for search sensitivity estimates spanning the LIGO–Virgo–KAGRA (LVK) Collaborations' first (O1), second (O2), and third (O3) observing runs.

Details of individual files can be found in

  •   o1+o2+o3-sensitivity-estimates.md

including descriptions of the HDF file format adopted.

Separate files are provided for individual subpopulations that span the Binary Neutron Star (bns), Neutron Star–Black Hole (nsbh), Binary Black Hole (bbh), and Intermediate Mass Black Hole (imbh) mass ranges. Additionally, a single file spanning the union of those mass ranges (mixture) is provided.

Sensitivity estimates for O1 and O2 are available via semi-analytic methods (estimates of the optimal network signal-to-noise ratio). Sensitivity estimates for O3 are available from real search results. Analysts should specify detection thresholds separately for each type of sensitivity estimate (e.g., a signal-to-noise cut for O1+O2 and a false alarm rate cut for O3).

How to download all files from this page

If you would like to download all files on this page, we recommend zenodo_get:

pip install zenodo_get
zenodo-get RECORD_ID_OR_DOI

where the record ID for the most recent version of this page is 5636815 and IDs for other versions can be found in the Versions section at the side of this page.

 

For more general background on gravitational-wave search analyses, try the materials from a GW Open Data Workshop or the guide to LIGO–Virgo data analysis.

LIGO Laboratory and Advanced LIGO are funded by the United States National Science Foundation (NSF) as well as the Science and Technology Facilities Council (STFC) of the United Kingdom, the Max-Planck-Society (MPS), and the State of Niedersachsen/Germany for support of the construction of Advanced LIGO and construction and operation of the GEO600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. Virgo is funded, through the European Gravitational Observatory (EGO), by the French Centre National de Recherche Scientifique (CNRS), the Italian Istituto Nazionale di Fisica Nucleare (INFN) and the Dutch Nikhef, with contributions by institutions from Belgium, Germany, Greece, Hungary, Ireland, Japan, Monaco, Poland, Portugal, Spain. The construction and operation of KAGRA are funded by Ministry of Education, Culture, Sports, Science and Technology (MEXT), and Japan Society for the Promotion of Science (JSPS), National Research Foundation (NRF) and Ministry of Science and ICT (MSIT) in Korea, Academia Sinica (AS) and the Ministry of Science and Technology (MoST) in Taiwan.
Files (649.8 MB)
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o1+o2+o3-sensitivity-estimates.md
md5:9deff09c2a798752b74656dd0d6b2bf0
8.2 kB Download
o1+o2+o3_bbhpop_real+semianalytic-LIGO-T2100377-v2.hdf5
md5:c21337a25b7318fdfd471cce549a547e
63.1 MB Download
o1+o2+o3_bnspop_real+semianalytic-LIGO-T2100377-v2.hdf5
md5:e8771ffe77576f5092fb3d35e70c6749
74.5 MB Download
o1+o2+o3_imbhpop_real+semianalytic-LIGO-T2100377-v2.hdf5
md5:c3017cd8cf1afa8bcd34c6447e9fc9da
85.0 MB Download
o1+o2+o3_mixture_real+semianalytic-LIGO-T2100377-v2.hdf5
md5:d9c14e817dac05c83c66e83fa8a211a0
361.7 MB Download
o1+o2+o3_nsbhpop_real+semianalytic-LIGO-T2100377-v2.hdf5
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65.4 MB Download
  • LIGO Scientific Collaboration and Virgo Collaboration and KAGRA Collaboration, GWTC-3, https://doi.org/10.7935/b024-1886

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