The Disc Miner - I. A statistical framework to detect and quantify kinematical perturbations driven by young planets in discs

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Fig. 4

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Best-fit attributes obtained by the DISCMINER for the 0.3 M_Jup snapshot. Left panel: freeze-out and gas phase regions for ¹²CO. The coloured circles indicate the height of the model emitting surfaces. Right panels: model peak brightness temperature and line width as a function of radius on both emitting surfaces.

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