William G. Lamb 🏴󠁧󠁢󠁷󠁬󠁳󠁿
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astrolamb.bsky.social
William G. Lamb 🏴󠁧󠁢󠁷󠁬󠁳󠁿
@astrolamb.bsky.social
📡 NANOGrav Gravitational Wave Researcher
🔭 Astrophysics PhD Candidate, Vanderbilt University, Nashville TN
🏴󠁧󠁢󠁷󠁬󠁳󠁿 Siaradwr Cymraeg o Eryri
✍️ Writer - Astrobites.org
👽 US “Resident Alien”
🎓 Uni of York Alumnus
🐱 Dad of WiggleWorm
🏊🚲🏃Triathlete
💃 Swing Dancer
Agreed
January 16, 2026 at 4:01 PM
If stop talking about Wallen is just "a small change." What are the bigger changes you want to see?
January 16, 2026 at 3:29 PM
“In the beginning the Universe was created.

“This had made many people very angry and has been widely regarded as a bad move.”
- Douglas Adams
December 18, 2025 at 8:32 PM
Absolutely, it's his favourite way to relax in the evening ❤️
December 9, 2025 at 5:31 PM
(Also, apologies for being so quiet recently. I am a non-citizen in a country that is monitoring my social media 🙃)
November 14, 2025 at 5:13 AM
...which we didn't expect! We plan further work to understand it better.

What does this all mean? We should model Fourier coefficients of the GWB, not PSDs! By modelling PSDs, we assume Gaussianity, which we have shown to mismodel the statistics of the astrophysical GWB.

Happy reading! 📖 (4/4)
November 14, 2025 at 5:13 AM
...under-estimate the tails of the distribution.

Additionally, we found that finite observation introduces a covariance term in our statistics. While small, it may be significant enough at the lowest frequencies for high amplitude sources. This is also a source of non-Gaussianity... (3/4)
November 14, 2025 at 5:13 AM
At low frequencies, the Gaussian approximation is fine. But at frequencies with few sources, we really need to stop assuming Gaussianity!

We find that Poisson variance (aka "shot noise") drives non-Gaussianity when there are very few sources. Modelling this region as Gaussian can... (2/4)
November 14, 2025 at 5:13 AM
Welp, don’t you dare shill on astrobites…
July 10, 2025 at 7:41 PM