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Fig. 2.

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Radial spectroscopic coverage of one confirmed cluster. Each filled circle represents one red-sequence galaxy with pmem > 0.05. The x-axis is their projected distance to the X-ray centre, normalized by Rλ. Spectroscopically identified members are displayed at y = 1 and coloured in black (pi = 1), and interlopers are displayed at y = 0 and coloured in white (pi = 0). Galaxies not assigned a spectroscopic redshift are coloured according to their pmem value (pi = pmem). The dashed red line shows the completeness rate, S(< x) (Eq. (1)) within radius x. The dotted line indicates the virial radius estimated from an X-ray luminosity–mass relation.

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