Bolometric corrections of stellar oscillation mode amplitudes as observed by the PLATO mission - I. Planck-spectrum estimates

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Table A.1.

Parameters of the bolometric correction relations.

Model	T_o	α	a₀	a₁	a₂	σ_rms
	(K)		(K)	(K⁻¹)	(K⁻²)
P_{1, N − CAM}	5446	0.81	⋯	⋯	⋯	1.73 × 10⁻³
P_{2, N − CAM}	5446	⋯	1	1.512 × 10⁻⁴	−4.229 × 10⁻⁹	1.54 × 10⁻⁴
P_1,FCB	6137	0.90	⋯	⋯	⋯	2.10 × 10⁻³
P_2,FCB	6137	⋯	1	1.451 × 10⁻⁴	−3.530 × 10⁻⁹	1.90 × 10⁻⁴
P_1,FCR	4728	0.84	⋯	⋯	⋯	4.19 × 10⁻³
P_2,FCR	4728	⋯	1	1.874 × 10⁻⁴	−6.856 × 10⁻⁹	1.35 × 10⁻⁴

Notes. The table provide the parameters for the power-law (Eq. A.1; subscript ‘1’) and polynomial (Eq. A.2; subscript ‘2’) model fits between T_eff and c_{BP − bol} (see Lund 2019). The quality of the fits is quantified by the root-mean-square-error σ_rms.

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