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ZENODO
Dataset . 2025
License: CC BY
Data sources: ZENODO
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
ZENODO
Dataset . 2025
License: CC BY
Data sources: ZENODO
ZENODO
Dataset . 2025
License: CC BY
Data sources: Datacite
ZENODO
Dataset . 2025
License: CC BY
Data sources: Datacite
ZENODO
Dataset . 2025
License: CC BY
Data sources: Datacite
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GW230814: investigation of a loud gravitational-wave signal observed with a single detector

Authors: LIGO Scientific Collaboration; Virgo Collaboration; KAGRA Collaboration;

GW230814: investigation of a loud gravitational-wave signal observed with a single detector

Abstract

This data release contains the analysis results and data behind the figures of the GW230814 discovery paper. Strain data for this event (the L1:GDS-CALIB_STRAIN_CLEAN_AR channel) can be downloaded from GWOSC. The content of this repository is: the C00-Combined-XO4a.h5 file contains the combined posterior samples for the 4 different models described in the paper. In addition to containing the posterior samples, the .h5 file also contain metadata about the analyses including the configuration files (which specify details such as the detector data analysed), noise power spectral densities and calibration uncertainty envelopes. The inference of the source parameters were performed with Bilby and we assume the calibration envelopes for LIGO Livingston maps calibrated data to theoretical strain. The .h5 files are formatted using PESummary. the figures_data.tar.gz file contains minimal, post-processed data to reproduce all figures of the paper. the scripts.tar.gz file contains a number of notebook to reproduce the content of the paper. In detail: `posteriors_minimal.ipynb` reads the posterior samples and produces Figures 2,3,4,5; `tgr_minimal.ipynb` reads from the figure data and produces Figures 7,8,9,10,11,14,16 and 17; `TauFisher.ipynb` produces Figure 12; `plot_mismatches_minimal.ipynb` produces Figure 15; `waveform-with-data_minimal.ipynb` produces Figures 1 and 12; the 230814.yaml file contains the dependencies to set-up a conda environment to run all the scripts above. For more information, see this page. the configs.tar.gz file contains configuration files and/or instructions to reproduce the analyses performed with the pSEOBNR, QNMRF and pyRing pipelines.

Keywords

Gravitational waves

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average
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