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Fig. 3.

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ACA Detection of [C I]1 → 0 at z = 2.39 toward the lensed galaxy SGASJ0033-A. Upper panel: continuum subtracted spectrum at 145 GHz extracted from the A.1+A.2 aperture (dashed gray line in lower panel) with 2 channel binning (gray line). The overlaid purple curve is the result of the convolution between the observed spectrum and a Gaussian kernel with FWHM equal to the best fit value of the 12CO(4 → 3) line. The velocity axis is centered at the redshift of 12CO(4 → 3). Lower panel: integrated [C I] emission contours (black solid/dahsed curves) at the ±2, 3σ levels on top of the 12CO(4 → 3) moment map. The crossed ellipse at the lower left corner indicates the size and orientation of the [C I] beam.

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