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Fig. 4.

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Maps of the CO fraction defined as the ratio of the CO(2−1) line emission to the observed 1.15 mm emission in NGC 2146 (left) and NGC 2976 (right) at 18″ angular resolution. Only pixels above the 3σrms level of the observed NIKA2 map are shown. Contours show the intensity of CO emission in each galaxy, starting from 1σrms and increasing by factors of 3. The circles in the bottom left corners indicate the beam area.

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