Deep SVDD anomaly detection on synthetic normal flares finds 30-36% of Kepler events and 15-32% of STIX events as anomalous, more often in higher-energy channels.
R., Ireland, J., & Dominique, M
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
years
2026 2verdicts
UNVERDICTED 2representative citing papers
A hybrid MCMC-CWT approach infers time-dependent power-law plus white-noise backgrounds to evaluate local significance of oscillations in non-stationary astrophysical signals.
citing papers explorer
-
Time-domain anomalies in solar and stellar flares
Deep SVDD anomaly detection on synthetic normal flares finds 30-36% of Kepler events and 15-32% of STIX events as anomalous, more often in higher-energy channels.
-
A Markov-Chain-Monte-Carlo-based Hybrid Noise Inference for Continuous Wavelet Power Spectra: with Applications to Solar and Stellar Oscillatory Signals
A hybrid MCMC-CWT approach infers time-dependent power-law plus white-noise backgrounds to evaluate local significance of oscillations in non-stationary astrophysical signals.