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Fig. A.1

image

Fit of the [CII] fine-structure line. The blue curve is the level-2 calibrated spectrum which is best fitted by the red curve. The positive dashed black line is the best model without the OFF line corresponding to the observation that we could have done if there was no contamination from the nebula. The negative one is OFF contamination model. Both Gaussians are fitted together and the residuals of the fit are given by the green curve.

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