Buoyancy glitches in pulsating stars revisited | Astronomy & Astrophysics (A&A)

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Table B.1.

Lower and upper limits of the uniform prior distributions applied in the fit of equation (10) to model data, for the cases of a step-like glitch (equation (16)) and Gaussian-like glitch (equation (22)).

Parameter	Step-like	Gaussian-like
P_s, min (s)	49000	14900
P_s, min (s)	56000	15000

ΔP_as (s)	7000	65
ΔP_as (s)	10000	69

A_st or A_G (10⁻⁶ rad/s)	1	300
A_st or A_G (10⁻⁶ rad/s)	15	800

$ω_{g}^{⋆}$ $\omega_{\rm g}^\star$ (10⁻⁶ rad/s)	300	1500
$ω_{g}^{⋆}$ $\omega_{\rm g}^\star$ (10⁻⁶ rad/s)	400	2000

Δ_g (10⁻⁶ rad/s)	–	100
Δ_g (10⁻⁶ rad/s)	–	200

δ	-π/2	-π/2
δ	π/2	π/2

jiter ≡ σ (s)	0	0
jiter ≡ σ (s)	inf	inf

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