Table 2. Open in new tab Virial mass,...

Table 2.

Virial mass, associated uncertainty, and radius of the spectroscopic groups in the field of HE 0435−1223 identified in Sluse et al. (2017). The last column shows our weak-lensing detection limit in terms of virial mass for haloes at each of the group redshifts. The limit is obtained according to equation (19).

\|$\bar{z}_{\mathrm{ group}}$\|	log(M_vir/M_⊙)	R_vir (Mpc)	log(M_vir/M_⊙)_limit
0.0503	13.32 ± 0.61	0.635	15.52
0.1744	13.81 ± 0.40	1.071	14.57
0.1841	13.65 ± 0.46	0.954	14.57
0.3202	13.83 ± 0.36	1.259	14.37
0.4185	13.18 ± 0.48	0.873	14.37
0.4547	13.72 ± 0.36	1.385	14.42
0.5059	13.72 ± 0.36	1.373	14.42
0.5650	13.33 ± 0.43	0.971	14.52
0.7019	12.49 ± 0.63	0.654	14.72

\|$\bar{z}_{\mathrm{ group}}$\|	log(M_vir/M_⊙)	R_vir (Mpc)	log(M_vir/M_⊙)_limit
0.0503	13.32 ± 0.61	0.635	15.52
0.1744	13.81 ± 0.40	1.071	14.57
0.1841	13.65 ± 0.46	0.954	14.57
0.3202	13.83 ± 0.36	1.259	14.37
0.4185	13.18 ± 0.48	0.873	14.37
0.4547	13.72 ± 0.36	1.385	14.42
0.5059	13.72 ± 0.36	1.373	14.42
0.5650	13.33 ± 0.43	0.971	14.52
0.7019	12.49 ± 0.63	0.654	14.72

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