Fig. 5.
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Velocity difference, Δv, between the known MgII absorber from Anand et al. (2021) within 3 × R200 from the cluster centre and the cluster redshift, as defined in Eq. (2). The figure displays the full range of Δv within [−5000:5000] km s−1. In the subsequent analysis, we chose to focus on the range of [−2000:2000] km s−1 around the cluster as indicated by the dashed lines.
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