Observations and modeling of the dust emission from the H2-bright galaxy-wide shock in Stephan's Quintet

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Table 4:

Fluxes of the PAH bands measured with the PAHFit IDL tool on the *Spitzer IRS* spectrum of the center of the SQ ridge and the *ISO-CVF* spectrum of the Galactic light.
	Integrated fluxes (see notes for units)
PAH band	$6.2~\mu$ m	$7.7~\mu$ m³	$11.3~\mu$ m³	$12.6~\mu$ m³	$17~\mu$ m³
SQ ridge (IRS)¹	< 0.75	$3.8 \pm 0.1$	$2.8 \pm 0.1$	$1.2 \pm 0.2$	$0.93 \pm 0.04$
Galactic (CVF)²	$5.19 \pm 0.09$	$19.05 \pm 0.03$	$6.49 \pm 0.17$	$2.90 \pm 0.05$	No data

Notes. ⁽¹⁾ Fluxes are in units of $\times 10^{-9}$ [W m^-2 sr^-1].
⁽²⁾ Fluxes are in units of $\times 10^{-7}$ [W m^-2 sr^-1].
⁽³⁾ In the case of PAH blended complexes, we sum the fluxes of the different Lorentzian components that contribute to the feature.

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