🔭 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
“This had made many people very angry and has been widely regarded as a bad move.”
- Douglas Adams
“This had made many people very angry and has been widely regarded as a bad move.”
- Douglas Adams
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)
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)
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)
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)
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)
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)