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Table 2

Spectroscopic parameters of the IR H3+${\rm{H}}_3^ + $ lines reported in d203-506 and GROSBETA model predictions (see Appendix E).

Linea Banda λ Aul Eu/kBb${E_{\rm{u}}}/k_{\rm{B}}^b$ Texmodel$T_{{\rm{ex}}}^{model}$ Flinemodel,c$F_{{\rm{line}}}^{model,\,c}$ Flineobs,d$F_{{\rm{line}}}^{obs,\,d}$
P|Q|R (J″, G″)u,l ν1ν2| l|ν1ν2| l|${\nu '_1}\,{\nu '_2}^{\left| {l'} \right|} \to {\nu ''_1}\,{\nu ''_2}^{\left| {l''} \right|}$ (µm) (s−1) (K) (K) (W m-2) (W m-2)
Q(5, 0) 011 → 000 4.045 1.13E+02 5293.3 274.6 6.5E−22 1.7E−21
Q(5, 1)l 011 → 000 4.045 1.09E+02 5263.8 273.4 3.1E−22 blended
Q(5, 3)l 011 → 000 4.044 7.18E+01 5020.2 261.2 3.5E−22 blended
Q(5, 2)l 011 → 000 4.043 9.50E+01 5174.2 269.0 2.6E−22 blended
Q(1, 0) 011 → 000 3.953 1.28E+02 3672.6 257.9 4.2E−22 2.3E−21
R(1, 0) 011 → 000 3.669 9.79E+01 3954.8 272.6 4.4E−22 2.4E−22
R(7, 6)u 011 → 000 3.052 1.01E+02 6904.2 329.5 2.8E−22 3.8E−22
R(7, 0) 011 → 000 3.022 1.74E+02 8006.7 427.4 2.8E−22 7.2E−22
J′, K′ → J″, K

(5,0) → (4,3) 000 → 000 16.325 3.01E−03 1736.8 750.8 1.8E−21 <6.2 E−21 (3σ)

Notes. aFollowing Lindsay & McCall (2001). bDetermined from the lowest accessible level of H3+${\rm{H}}_3^ + $, J, K = (1, 1). cComputed using an aperture of 0.1″ (a solid angle of 2.35×10−13 sr), the same aperture used to extract the observational data. dFrom Schroetter et al. (2025b).

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