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Table 1.

Properties of the cluster CGr32.

Variable Value Ref. Comment
RA (J2000) 149°55′19.0″ TW MUSE barycentre
Dec (J2000) 2°31′15.5″ TW MUSE barycentre
RA (J2000) 149°55′14.8″ 1 From X-rays data
Dec (J2000) 2°31′18.0″ 1 From X-rays data
z 0.7303 1
σ 931 km s−1 TW Full sample
σQ 697 km s−1 TW Quiescent galaxies
σSF 1085 km s−1 TW Star-forming galaxies
R200 1.53 Mpc TW From MUSE data
M200 8.14 × 1014M TW From MUSE data (a)
R200 0.983 Mpc 1 From X-rays data
M200 2.33 × 1014M 1 From X-rays data



This mass reduces to M200 = 3.41 × 1014M if derived using the velocity dispersion of the quiescent population only, rather than the full sample.

References. TW: this work, (1) Gozaliasl et al. (2019).

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