This material is part of several data products associated with GWTC-2.1, the deep extended catalog of compact binary coalescences observed by the LIGO Scientific Collaboration and the Virgo Collaboration during the first half of the third observing run. For further information, see the paper (dcc.ligo.org/LIGO-P2100063/public), the related material linked from this page, and the GWTC-2.1 data release documentation (www.gw-openscience.org/GWTC-2.1/). Glitch model for GWTC-2.1 events Glitch model for events in the GWTC_2.1 catalog that used BayesWave glitch subtraction. This includes LIGO Livingston Observatory (L1) data for the following events: GW190413_134308 GW190425_081805 GW190503_185404 GW190513_205428 GW190514_065416 GW190701_203306 GW190924_021846 Each data file contains three channels: the calibrated strain data, including any glitches that are present, a model of the glitches, produced using the BayesWave algorithm, the calibrated data with the glitch model subtracted, used for parameter estimation For the L1 data for all events, these channels have the following names and sample rates (in Hz): L1:DCS-CALIB_STRAIN_CLEAN_SUB60HZ_C01 16384 L1:DCS-CALIB_STRAIN_CLEAN_SUB60HZ_C01_glitch 16384 L1:DCS-CALIB_STRAIN_CLEAN_SUB60HZ_C01_T1700406_v4 16384 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 6477075 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 data quality, 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.

{"references": ["10.7935/nfnt-hm34"]}