Table 2: Numerical values of the predicted ratios between ${\rm d}F_{\rm obs}/{\rm d}\Omega$ (for the two far-infrared skeletal vibrational modes at about 85 and 150 $\mu$ m) and $\mathcal{W}_{\rm DIB}$ of the electronic transition near 9701 Å of C₃₂H₁₄⁺, as obtained through our simulation in the four different radiation fields considered. The ratios in the table are expressed in units of W cm^-2 sr^-1 mÅ^-1.
IR band ISRF ISRF Red IRAS

position 5 kpc 13 kpc Rectangle 21282+5050

$83.4~\mu{\rm m}$ $1.3\times10^{-16}$ $1.6\times10^{-17}$ $6.7\times10^{-15}$ $1.4\times10^{-11}$

$150.8~\mu{\rm m}$ $2.9\times10^{-17}$ $3.6\times10^{-18}$ $1.5\times10^{-15}$ $2.9\times10^{-12}$

**Table 2:** Numerical values of the predicted ratios between ${\rm d}F_{\rm obs}/{\rm d}\Omega$ (for the two far-infrared skeletal vibrational modes at about 85 and 150 $\mu$ m) and $\mathcal{W}_{\rm DIB}$ of the electronic transition near 9701 Å of C₃₂H₁₄⁺, as obtained through our simulation in the four different radiation fields considered. The ratios in the table are expressed in units of W cm^-2 sr^-1 mÅ^-1.
IR band	ISRF	ISRF	Red	IRAS
position	5 kpc	13 kpc	Rectangle	21282+5050
$83.4~\mu{\rm m}$	$1.3\times10^{-16}$	$1.6\times10^{-17}$	$6.7\times10^{-15}$	$1.4\times10^{-11}$
$150.8~\mu{\rm m}$	$2.9\times10^{-17}$	$3.6\times10^{-18}$	$1.5\times10^{-15}$	$2.9\times10^{-12}$

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