Diffuse and specular brightness models applied to LEO satellites - Case study: The ONEWEB constellation

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Table A.2

DEMC-fitted parameters and errors of the DS, DSS, and RR brightness models, for the V filter samples.

			V filter	V filter On Station	V filter Off Station
	p		0.402 ± 0.041	0.445 ± 0.047	0.364 ± 0.083
DS Model	ζ	(m²)	0.127 ± 0.005	0.125 ± 0.006	0.142 ± 0.013
	σ_demc,ds	(mag)	0.679 ± 0.020	0.632 ± 0.022	0.775 ± 0.044
	β		0.215 ± 0.006	0.203 ± 0.006	0.249 ± 0.014
DSS Model	ζ	(m²)	0.430 ± 0.040	0.465 ± 0.046	0.395 ± 0.083
	σ_demc,dss	(mag)	0.663 ± 0.020	0.614 ± 0.021	0.762 ± 0.043
	k		0.489 ± 0.075	0.514 ± 0.082	0.243 ± 0.141
RR Model	$H_{(70, 0)}^{1200}$ $Mathematical equation: $H_{(70,0)}^{1200}$$	(mag)	7.691 ± 0.040	7.760 ± 0.042	7.416 ± 0.091
	σ_demc,rr	(mag)	0.704 ± 0.021	0.669 ± 0.023	0.768 ± 0.043

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