Hi everyone,
I’m currently working on a gravitational-wave theory project focused on bimetric ECO ringdowns, discrete-scale-invariant spectra, and post-ringdown mode phenomenology. My current analysis pipeline is already fully operational on public O4a data (GWpy / PyCBC / Bilby / HPC workflow), and I’m now trying to understand the realistic and legitimate path toward working with O4b-era data.
The reason I’m interested in O4b specifically is that my current work depends strongly on:
higher-SNR ringdown events,
improved statistics for post-merger spectral structure,
better constraints on subdominant mode content,
and potentially larger event populations for consistency tests.
I’m NOT asking for confidential data or for anyone to violate LVK/IGWN policies.
What I’m looking for is mainly:
expected public release timeline for O4b,
official academic/collaboration access routes,
public low-latency or derived products,
mock data / injections / metadata useful for ringdown studies,
or contacts/groups already working on related ECO or beyond-GR analyses.
The project is theory-heavy but intended to become observationally testable against real GW catalog data, so I’m mainly trying to understand what resources are realistically accessible now and what the recommended path is for researchers preparing O4b-scale analyses.
If there’s a better forum, mailing list, workshop, collaboration channel, or documentation page for this kind of question, I’d really appreciate being pointed in the right direction.
Thanks a lot.