The E-QFT framework predicts a faint but universal transverse–traceless (TT) noise signature, which so far we have only validated on simulated data. To move forward, I would need real cross-spectral datasets from co-calibrated gravitational sensors (interferometers, resonant bars, or quantum sensors).
Now the question: Are such datasets already accessible through public repositories, or would this require direct collaboration with a laboratory?
Thanks a ton for your recommendations !
In some cases, if specific data is not publicly available, it might be possible to directly contact the researchers or institutions involved in the experiments to inquire about data access for research purposes.
Thank you Mohana Sundaram P for your reply, I agree that direct collaboration with researchers or institutions would be the ideal path forward. However, based on past experience, I've found that even when laboratories do respond, they are often hesitant to share their data, especially when it involves proprietary setups or unpublished results. This makes it quite challenging to access the kind of cross-spectral datasets needed for further validation.
LIGO/Virgo/Kagra collaboration releases data after an embargo period after the end of each run. You can find released data at: https://gwosc.org/data/ as timeseries of calibrated strain for each interferometer.
Some softeare to handle public data is also available in the geosc page with tutorials.
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