Observability of evaporating lava worlds | Astronomy & Astrophysics (A&A)

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Table A.1

Sources and parameters of opacities used in this work

	Source	Line list	Cutting Length (cm⁻¹)
Al	This work^a	Kurucz¹	-
AlO	DACE^b & This work	ATP²	100
Ca	This work	Kurucz	-
CaO	DACE & This work	VBATHY³	100
Fe	This Work	Kurucz	-
K	This Work	Kurucz	-
Mg	This Work	Kurucz	-
MgO	DACE & This work	LiTY⁴	100
Na	This Work^c	VALD3⁵	Varied (300 max)
O	This Work	Kurucz	-
O₂	This Work	HITRAN⁶	100
Si	This Work	Kurucz	-
SiO	This Work	Kurucz (shortwave) & EBJT⁷	Varied (300 max)
SiO₂	DACE	OYT3⁸	100
Ti	This Work	Kurucz	-
TiO	DACE & This Work	Toto⁹	100

Al⁺	This Work	Kurucz	-
Ca⁺	This Work	Kurucz	-
Fe⁺	This Work	Kurucz	-
Mg⁺	This Work	Kurucz	-
Na⁺	This Work	Kurucz	-
O⁺	This Work	Kurucz	-
Si⁺	This Work	Kurucz	-
Ti⁺	This Work	Kurucz	-

^a Opacities are computed with HELIOS-K https://github.com/exoclime/HELIOS-K (Grimm & Heng 2015; Grimm et al. 2021) ; ^b DACE database https://dace.unige.ch/; ^c Na doublet wings computed using the unified line-shape theory of Rossi & Pascale (1985); Allard et al. (2007a,b);¹ Kurucz (Kurucz 1992);² ATP (Patrascu et al. 2015);³ VBATHY (Yurchenko et al. 2016);⁴ LiTY (Li et al. 2019);⁵ VALD3 (Ryabchikova et al. 2015);⁶ HITRAN (Gordon et al. 2017; Chubb et al. 2021);⁷ EBJT (Gordon et al. 2017; Chubb et al. 2021);⁸ OYT3 (Owens et al. 2020);⁸ Toto (McKemmish et al. 2019). We note that we only use opacities of main isotopes. In this work we make use of the DACE (Grimm & Heng 2015; Grimm et al. 2021), ExoMol (Chubb et al. 2021), HITRAN (Gordon et al. 2017), Kurucz (Kurucz 1992) and VALD3 (Ryabchikova et al. 2015) opacity databases.

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