Table 2
Main results of the weak lensing analysis.
| Galaxy system | α | δ | z | ⟨β⟩ | SIS | NFW | |||
|---|---|---|---|---|---|---|---|---|---|
| ID | (J2000) | (J2000) | σV | M200 | c200 | R200 | M200 | ||
| km s−1 |  |
 Mpc |
 |
||||||
| A1204 I | 11h 13m 20.5s | +17°35′41.0″ | 0.1703 | 0.689 | 750 ± 80 | 3.7 ± 1.2 | 3.52 | 1.41 ± 0.22 | 3.8 ± 1.8 |
| A1204 II | 11h 14m 07.2s | +17°27′41.0″ | 0.1705 | 0.689 | 640 ± 100 | 2.3 ± 1.1 | 3.52 | 1.11 ± 0.23 | 1.9 ± 1.2 |
| A2029 | 15h 10m 56.1s | +05°44′41.7″ | 0.0775 | 0.778 | 840 ± 110 | 5.3 ± 2.0 | 3.40 | 1.95 ± 0.40 | 9.1 ± 5.6 |
| A2033 | 15h 11m 26.5s | +06°20′56.9″ | 0.0822 | 0.766 | 780 ± 120 | 4.3 ± 2.1 | 3.49 | 1.75 ± 0.36 | 6.5 ± 4.0 |
Notes. Column (1): the cluster identification; Cols. (2), (3) and (4): the coordinates of the center and the redshift adopted for the lensing analysis; Cols. (4) and (5): the mP and mmax magnitudes considered for the galaxy background selection (see Sect. 3.1); Col. (6): the geometrical factor; Cols. (7) and (8): the results from the SIS profile fit, the velocity dispersion and M200 (see Eqs. (4) and (6)); Cols. (9), (10) and (11): the results from the NFW profile fit, the adopted c200 , R200 obtained from fitting the shear profile and its correspondence M200.
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