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Table 2

Definitions of the galaxy shape and lensing catalogues.

Cluster field n KSB n gal d ani m bright m faint n lc S max
[px] [px] [px] [mag] [mag]  [arcmin-2  [arcmin-2 [mag] [mag]  [arcmin-2
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13)

CL 0030+2618 2.55 2.80 2.95 16.75 22.5 44.79 22.64 5 20.0 22.5 21.28 5.84
CL 0159+0030 2.65 2.95 3.10 17.5 22.5 37.27 18.91 3 20.0 24.6 11.58 4.12
CL 0230+1836 2.05 2.33 2.45 16.75 22.5 29.28 13.22 4 21.5 23.0 11.04 3.64
CL 0809+2811 2.35 2.66 2.80 17.0 22.5 33.39 16.56 2 22.5 24.8 10.31 5.39
CL 1357+6232 2.85 3.18 3.35 17.5 22.25 29.52 14.24 5 18.5 14.23 4.47
CL 1416+4446 2.55 2.80 2.95 16.75 22.5 42.50 21.51 5 18.5 21.50 4.25
CL 1641+4001 2.90 3.135 3.30 16.75 22.5 39.95 19.58 3 22.7 17.65 4.12
CL 1701+6414 2.60 2.95 3.10 16.75 22.5 40.71 20.72 4 21.9 19.47 3.75

Notes. The parameters , , , and delineate the stellar locus. The galaxy shape catalogue considers sources for and for (Cols. (1) to (5)). The number densities nKSB and ngal of sources in the KSB and galaxy shape catalogues are shown in Cols. (6) and (7); followed by the degree dani of the polynomial for PSF anisotropy correction. Columns (9) to (13) present the photometric cuts mbright and mfaint, defining the lensing catalogue with a source density nlc. Using a filter scale of θout in Eq. (1), we find a maximum shear peak significance Smax. CL 0030+2618 (Paper I) is included for completeness.

(†)

No significant decrease of S(θout) at the shear peak was found out to the largest probed value θout = 16′. See Sect. 4 for more details on the CL 1701+6414 and CL 1641+4001 cases.

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