Quasar light curves constrain short-term volatility η better than timescale τ in DRW models; hierarchical Bayesian fit on 570 curves shows volatility decreases with bolometric luminosity and rest wavelength.
Radio Frequency Interference (RFI , year = 2017, month = jan, eid =
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The SKA is described as a key future tool for technosignature searches due to its sensitivity, field of view, and resolution, requiring high temporal and spectral resolution data products.
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The Information Content of Quasar Variability Light Curves: How Well Can we Infer Stochastic Model Parameters?
Quasar light curves constrain short-term volatility η better than timescale τ in DRW models; hierarchical Bayesian fit on 570 curves shows volatility decreases with bolometric luminosity and rest wavelength.
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Searching for Extraterrestrial Intelligence with the SKA
The SKA is described as a key future tool for technosignature searches due to its sensitivity, field of view, and resolution, requiring high temporal and spectral resolution data products.