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Fig. 1.

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Color (F606W − F814W) vs. magnitude (F814W) diagram of all sources present in the RELICS catalogue (Black points). Possible cluster members selected using both the red sequence colors (0.6134 < F606W − F814W < 1.2478 mag; orange horizontal lines) and the magnitude limits (25.62 < mF814W < 18.35 mag; orange vertical lines) are shown in red. The subsample of 22 spectroscopically confirmed cluster members by Mahler et al. (2023) are shown in blue. The subsample of 61 spectroscopically confirmed cluster members by Noirot et al. (2023) are shown in orange. The brightest cluster galaxy (BCG) of the cluster is represented with a grey star.

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