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Fig. 2.


Phase-space diagram of galaxies in cluster CGr32 determined using the barycentre of the cluster members identified spectroscopically with MUSE as the cluster centre. Quiescent galaxies are indicated with red-filled dots, star-forming objects with blue-filled dots. Black open circles show blended galaxies with unavailable broad-band photometry. The galaxies ID 345 and ID 473 are indicated with “S” and “N”, respectively.

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