The O3b Data Release
- The third LIGO/Virgo observation run (O3), is divided in two parts, O3a and O3b
- O3b dates: 1st November 2019 15:00 UTC (GPS 1256655618) to 27th March 2020 17:00 UTC (GPS 1269363618)
- This documentation refers to the data available from three detectors: H1, L1, and V1.
- Data are available at the original 16 KHz and the downsampled 4KHz sample rates.
- In addition to the final version of the strain data, a few additional versions are also available.
Get O3b Data
- Strain Data: 4 kHz Data 16 kHz Data
- Segments: Timeline Data Quality
- Detections, analysis results and further information: GWTC-3
- Cluster Access: CernVM-FS
GWF Channel NamesThe final version of the strain data, available using the buttons above, is sourced from the channels:
Alternate Calibration ReleaseIn addition to the final version of the strain data, several additional versions are also available, including different calibration versions and/or cleaning methods.
- See Alternate Calibration Release for how to access these channels.
O3b Detector Performance
Astrophysical ResultsPapers including results from O3b can be found following the links below:
- GWTC-3 Catalog paper
- GWTC-3 Data Release Documentation
- The population of merging compact binaries inferred using gravitational waves through GWTC-3
- Constraints on the cosmic expansion history from the third LIGO–Virgo–KAGRA Gravitational-Wave Transient Catalog
- LIGO/Virgo Detection Papers
- LIGO/Virgo Collaboration Publications Page
Data Quality Segments
- The DATA segment list indicates times when data are publicly available.
- See the Timeline Query Page for other O3b segment lists.
- The O2/O3 LIGO detector characterization paper describes data quality categories
- Technical documents that list DQ flag names: document for LIGO and document for Virgo
- See also the technical details page
Hardware InjectionsThe O3b data set contains simulated astrophysical signals, known as hardware injections, used for testing and calibration. For an example, see the Find a Hardware Injection Tutorial (in the tutorial use the flags for the O3b run described here). For complete documentation, see:
Instrumental Spectral LinesA power spectral density of LIGO data typically shows a number of spectral lines. Many of these are associated with known instrumental resonances. The O3 instrumental spectral lines page gives an explanation, and catalog, of these instrumental lines.
- The above plots are reproduced from Figures 2 and 3 of the GWTC-3 paper
- Plots of daily sensitivity are available on the archived detector status pages
Technical DetailsGWOSC 4 kHz strain data have been repackaged and downsampled from 16384 Hz to 4096 Hz. Advanced LIGO and advanced Virgo data are not calibrated or valid below 10 Hz or above 5 kHz, and the data sampled at 4096 Hz are not valid above about 1700 Hz. In most searches for astrophysical sources, data below 20 Hz are not used because the noise is too high. More detailed information about the data set can be seen on the Technical Details page.
AcknowledgeTo acknowledge the use of O3b data, see the Acknowledgement Page.
Data Set DOI: https://doi.org/10.7935/pr1e-j706
- Nov 7, 2021: First release
- Nov 8, 2021: Updates to links in the Astrophysical Results section