Elemental abundance pattern and temperature inversion on the dayside of HAT-P-70b observed with CARMENES and PEPSI

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Table A.1

Opacity databases employed for CCF calculation and atmospheric retrieval.

Chemical species	Opacity	References
Al i, Ba i, Ba ii, C i, Ca i, Ca ii, Cr i, Cr ii, Fe i Fe II, Li i Mg i Mg ii Na i, Ni i Si i Ti i Ti ii Y i	Kurucz	Kurucz (2018)
Co i Co ii Mn i Sc i Sc ii V i V ii	VALD	Pakhomov et al. (2019); Ryabchikova et al. (2015)
CaH, CrH, FeH, MgH, OH	MOLLIST	Bernath (2020); Li et al. (2012); GharibNezhad et al. (2013); Burrows et al. (2002); Yousefi et al. (2018); Brooke et al. (2016)
K I	Allard	Mollière et al. (2019)
AlH	AlHambra	Yurchenko et al. (2018)
AlO	ExoMol	Patrascu et al. (2015)
NaH	Rivlin	Rivlin et al. (2015)
TiO	Toto	McKemmish et al. (2019)
VO	VOMYT	McKemmish et al. (2016)

Notes. Opacity data for AlH, Ba I, Ba II, Co I, Co II, Cr I, CrH, Mn I, NaH, Ni I, Sc I, Sc II, V I, and V II were downloaded from the DACE, while the remaining species were obtained via petitRADTRANS opacity database.

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