Self-consistent atmosphere modeling with cloud formation for low-mass stars and exoplanets

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Table 2

Molecular line transitions and their sources.

Molecule	Transitions	Reference

Hydrides
LiH	vib-rot	Coppola et al. (2011)
MgH	vib-rot	Yadin et al. (2012)
	A-X, B’-X	GharibNezhad et al. (2013)
SiH	A-X	Kurucz (2011)
CaH	vib-rot	Yadin et al. (2012)
	A-X, B-X, C-X, D-X, E-X	Weck et al. (2003)
TiH	A-X, B-X	Burrows et al. (2005)
CrH	A-X	Burrows et al. (2002)
FeH	F-X	Wende et al. (2010)
CH	vib-rot, A-X, B-X, C-X	Masseron et al. (2014)
NH	vib-rot	Brooke et al. (2014a)
	A-X, A-C	Kurucz (2011)
OH	vib-rot, A-X	Kurucz (2011)

Oxides
SiO	vib-rot	Barton et al. (2013)
	A-X, E-X	Kurucz (2011)
TiO	A-X, B-X, C-X, E-X	Schwenke (1998)
	c-a, b-a, b-d, f-a
VO	A-X, B-X, C-X	Kurucz (2011)
ZrO	B-A, B-X, C-X, E-A	Plez et al. (2003)
	b-a, d-a, e-a, f-a
CO	vib-rot, A-X	Kurucz (2011)
NO	vib-rot	Rothman et al. (2010)
H₂O	vib-rot	Jørgensen et al. (2001)

Other
H₂, HD	vib-rot, quad, B-X, C-X	Kurucz (2011)
C₂	A-X, b-a, E-A	Kurucz (2011)
	d-a	Brooke et al. (2013)
CN	vib-rot, A-X, B-X	Brooke et al. (2014b)
CO₂	vib-rot	Rothman et al. (2010)
HCN	vib-rot	Harris et al. (2006)
		Harris et al. (2008)
H₂-H₂	CIA	Borysow et al. (2001)
H₂-He	CIA	Jørgensen et al. (2000)

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