Open Access

Table A.1.

15 structures from Sarron et al. (2018) with PFG ≥ 50%.

CFHTLS field RA RA uncertainty Dec Dec uncertainty S/N Redshift M200 R200 dnode dfil PFG
(deg) (deg) (deg) (deg) M Mpc Mpc Mpc %
W1 34.72 0.05 −9.27 0.05 6 0.22 4.20E13 0.78 1.77 0.51 50
W1 36.76 0.03 −9.27 0.03 4 0.32 1.20E14 1.15 3.42 0.64 51
W1 35.89 0.05 −8.69 0.05 6 0.26 1.39E13 0.56 2.59 0.17 52
W1 32.20 0.05 −6.60 0.05 3 0.20 3.97E13 0.77 2.10 0.50 65
W1 30.80 0.01 −9.80 0.01 4 0.66 1.30E14 1.35 0.83 0.19 65
W1 36.82 0.02 −4.55 0.02 10 0.28 2.38E14 1.47 0.81 0.21 69
W1 38.18 0.03 −9.77 0.03 3 0.36 6.92E13 1.00 2.07 0.32 71
W1 38.69 0.03 −5.64 0.03 6 0.30 1.13E14 1.15 1.69 0.26 78
W1 37.14 0.03 −5.84 0.04 4 0.30 1.15E13 0.55 0.51 0.57 91

W2 136.19 0.02 −4.65 0.02 6 0.68 8.06E13 1.17 0.39 0.10 53
W2 135.46 0.04 −4.33 0.04 4 0.22 1.97E13 0.61 2.41 0.19 60

W3 213.46 0.01 54.78 0.01 6 0.56 4.75E13 0.94 1.92 0.80 50
W3 212.57 0.06 57.69 0.03 6 0.36 3.63E13 0.77 3.15 2.31 56
W3 219.40 0.07 56.55 0.04 5 0.26 4.18E13 0.79 35.54 35.64 66

W4 334.64 0.02 −0.76 0.02 7 0.36 5.48E13 0.93 0.16 0.09 59

Notes. The table lists: (1) the corresponding CFHTLS field, (2–3): RA and uncertainty, (4–5): Dec and uncertainty, (6) detection signal-to-noise ratio (S/N) within the CFHTLS structure sample, (7) redshift, (8) M200, (9) R200, (10) distance to the nearest node, (11) distance to the nearest filament, (12) probability of being a FG. The structure at coordinates (219.40, 56.55) is probably in a region where filament detection has been inoperative.

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