On the detection of Lorentzian profiles in a power spectrum: a Bayesian approach using ignorance priors

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Table 1:

Input parameters for the simulated solar-type pulsator.
	f₁	f₂
frequency	132.3	136.6
rms amplitude	1	1
estimated mode height	0.033	0.033
mode lifetime	0.5 d	0.5 d

White noise model with SNR of 0.1 in the time domain.

Source LaTeX | All tables | In the text

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