Connection between planetary He I λ10 830 Å absorption and extreme-ultraviolet emission of planet-host stars

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Table A.1

Comparison of modeled EUV broadband luminosities^a .

Reference	AU Mic	TRAPPIST-1	Barnard’s Star Ba	rnard’s Star	HD 209458
			(quiescence)	(flare)
DUV21, LOU17	28.93	27.33	25.71	26.61	28.20
This work	29.39	26.29	26.13		28.45

Notes. ^(a) log L_EUV,H (erg s⁻¹) in the 100–912 Å range as reported by DUV21 and LOU17, and compared with our model.

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