TESS data show stochastic low-frequency variability dominates in most extreme helium stars, with characteristic timescales of 0.5-10 days correlating to stellar parameters and matching subsurface convection predictions.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
years
2026 2verdicts
UNVERDICTED 2representative citing papers
A PCA-based generalization of template matching corrects jitter noise in pulsar TOA measurements by modeling pulse shape variations.
citing papers explorer
-
TESS Observations of Stochastic Low-frequency Variability in Extreme Helium Stars
TESS data show stochastic low-frequency variability dominates in most extreme helium stars, with characteristic timescales of 0.5-10 days correlating to stellar parameters and matching subsurface convection predictions.
-
A Generalized Template Matching Algorithm for Correcting Jitter Noise in Pulsar Timing
A PCA-based generalization of template matching corrects jitter noise in pulsar TOA measurements by modeling pulse shape variations.