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Table 2.

References for the atomic and molecular opacities available for use in petitRADTRANS.

Opacity source Spectral range (μm) Line list Partition function Pressure broadening Line Cutoff
CH4 0.83 <  λ YT14 F03 Eq. (15), SB07 HB02
C2H2 1 <  λ <  16.5 HITRAN F03 γair HB02
CO 1.18 <  λ HITEMP F03 γair HB02
CO 0.112 <  λ <  0.43 K93 F03 Eq. (15), SB07 HB02
CO2 1 <  λ <  38.76 HITEMP F03 γair BG69
H2S 0.88 <  λ HITRAN F03 γair HB02
H2 0.28 <  λ HITRAN F03 γair HB02
H2 0.08 <  λ <  0.18 K93 F03 Eq. (15), SB07 HB02
HCN 2.92 <  λ HT06, BS14 F03 Eq. (15), SB07 HB02
H2O 0.33 <  λ HITEMP F03 γair HB02
K 0.05 <  λ PK95 ST84 N. Allard (a), SH96 HB02
Na 0.1 <  λ PK95 ST84 N. Allard (a), SH96 HB02
NH3 0.8 <  λ YB11 SH14 Eq. (15), SB07 HB02
O3 1.43 <  λ HITRAN F03 γair HB02
OH 0.52 <  λ HITEMP F03 γair HB02
PH3 1 <  λ SA15 F03 Eq. (15), SB07 HB02
TiO 0.32 <  λ B. Plez (a) U. Jørgensen (b) Eq. (15), SB07 HB02
VO 0.36 <  λ <  2.6 B. Plez (a) B. Plez (a) Eq. (15), SB07 HB02
SiO 1.6 <  λ BY13 BY13 Eq. (15), SB07 HB02
FeH 0.67 <  λ WR10 WR10 Eq. (15), SB07 HB02

Notes.

(a)

priv. comm.

(b)

partition function retrievable from http://www.astro.ku.dk/~uffegj/scan/scan_tio.pdf. For all molecules, except for CO and TiO, only the main isotopologue opacities are used in the low resolution mode. At high resolution also secondary isotopologues are available for some species, see the documentation at https://petitradtrans.readthedocs.io for an up-to-date list. The documentation website also contains a short tutorial of the ExoCross code (Yurchenko et al. 2018), and how to convert its resulting Exomol opacity calculations for use in petitRADTRANS. This allows the petitRADTRANS user to calculate line opacities of additional species, for the low and high resolution modes.

References. HITEMP: Rothman et al. (2010), HITRAN Rothman et al. (2013), SB07: Sharp & Burrows (2007), F03: Fischer et al. (2003), ST84: Sauval & Tatum (1984), K93: Kurucz (1993), YT14: Yurchenko & Tennyson (2014), YB11: Yurchenko et al. (2011), SH96: Schweitzer et al. (1996), SH14: Sousa-Silva et al. (2014), SA15: Sousa-Silva et al. (2015), HT06: Harris et al. (2006), BS14: Barber et al. (2014), PK95: Piskunov et al. (1995), HB02: Hartmann et al. (2002), BG69: Burch et al. (1969), BY13: Barton et al. (2013), WR10: Wende et al. (2010).

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