Open Access

Table A.1

Description of the opacities used to calculate temperature profiles and emission spectra.

Species Source Line list Line List Reference
Al DACEa VALD Ryabchikova et al. (2015)
AlH HELIOS-K AlHambra Yurchenko et al. (2018c)
AlO HELIOS-Kb ATP Patrascu et al. (2015)
Ca DACE VALD Ryabchikova et al. (2015)
CaH HELIOS-K MoLLIST Li et al. (2012); Bernath (2020)
CaO HELIOS-K VBATHY Yurchenko et al. (2016)
Fe DACE VALD Ryabchikova et al. (2015)
K DACE VALD Ryabchikova et al. (2015)
Mg DACE Kurucz Kurucz (1992)
MgH HELIOS-K MoLLIST GharibNezhad et al. (2013); Bernath (2020)
MgO HELIOS-K LiTY Li et al. (2019)
Na DACE VALD Ryabchikova et al. (2015)
NaH HELIOS-K Rivlin Rivlin et al. (2015)
Si DACE VALD Ryabchikova et al. (2015)
SiH HELIOS-K Sightly Yurchenko et al. (2018b)
SiO HELIOS-K SiOUVenIR Yurchenko et al. (2022)
SiO2 DACE OYT3 Owens et al. (2020)
Ti DACE VALD Ryabchikova et al. (2015)
TiH HELIOS-K MoLLIST Burrows et al. (2005); Bernath (2020)
TiO HELIOS-K Toto McKemmish et al. (2019)
Volatiles

CO DACE Li2015 Li et al. (2015)
CO2 DACE HITEMP & UCL-4000c Rothman et al. (2010); Yurchenko et al. (2020)
CH3 DACE AYYJ Adam et al. (2019)
CH4 DACE YT34to10 Yurchenko et al. (2017)
C2H2 DACE aCeTY Chubb et al. (2020)
C2H4 DACE MaYTY Mant et al. (2018)
CN HELIOS-K Trihybrid Syme & McKemmish (2021)
H2O DACE POKAZATEL Polyansky et al. (2018)
HCN HELIOS-K Harris Barber et al. (2014)
HS HELIOS-K GYT Gorman et al. (2019)
H2S DACE AYT2 Azzam et al. (2016)
NH3 DACE CoYuTe Coles et al. (2019)
OH DACE HITEMP Rothman et al. (2010)
S DACE VALD Ryabchikova et al. (2015)
CS ExoMold JnK Paulose et al. (2015)
NS ExoMol SNaSH Yurchenko et al. (2018a)
SO2 ExoMol ExoAmes Underwood et al. (2016a)
SO3 ExoMol UYT2 Underwood et al. (2016b)
PH3 DACE SAlTY Sousa-Silva et al. (2015)
PS HELIOS-K POPS Prajapat et al. (2017)
VO HELIOS-K VOMYT McKemmish et al. (2016)
Scattering and Continuum

H, H2, H2O, He, O2 Scattering
H Continuum (bf & ff) John (1988); Gray (2008)
H2–H2 HELIOS-K HITRAN Gordon et al. (2017)
H2–He, O2–O2 petitRADTRANS Mollière et al. (2019, 2020)

a DACE database https://dace.unige.ch/; b Opacities are computed with HELIOS-K https://github.com/exoclime/HELIOS-K (Grimm & Heng 2015; Grimm et al. 2021); c We use HITEMP2010 for temperature profiles and UCL-4000 for emission spectra; d For ExoMol opacities we make use of the conversion work done by Chubb et al. (2021), which are only used for generating emission spectra. In general, we make heavy use of the DACE (Grimm & Heng 2015; Grimm et al. 2021), ExoMol (Chubb et al. 2021), Kurucz (Kurucz 1992), VALD3 (Ryabchikova et al. 2015) and HITRAN (Gordon et al. 2017) databases.

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