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

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Table 3:

Optical *HST* V-band and near-infrared *WIRC* surface brightnesses¹ in the J, H, and $K_{\rm s}$ bands for the SQ ridge.
Band		V	J	H	$K_{\rm s}$	J:H: $K_{\rm s}$
	Flux	$7.2\pm 1.6$	$8.45 \pm 0.64$	$8.54 \pm 0.65$	$8.07 \pm 0.61$	1.048:1.058:1
	Dered	$12.2 \pm 2.9$	$9.93 \pm 0.77$	$9.44 \pm 0.77$	$8.60 \pm 0.75$	1.154:1.096:1

Notes. ⁽¹⁾ The fluxes are given in units of 10^-7 W m^-2 sr^-1. ``Dered'' indicates the extinction-corrected brightness, and the `` $J{:}H{:}K_{\rm s}$ '' column shows flux ratios between the bands.

Source LaTeX | All tables | In the text

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