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Fig. A.1


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70 μm flux from Spezzi et al. (2013). Circles indicate detected sources, and the triangles are the upper limits for the non-detections. Red circles indicate sources observed with our ALMA program, and blue squares show the sources that were not detected by our millimeter observations. Finally, the orange squares display the sources that were confirmed as Cha II cluster member by the analysis of Galli et al. (2021).

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