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Table 2.

Best-fitting parameters of the completeness and mass bias functions for the Hα tail (first row), Hα extraplanar (second row), UV tail (third row), and UV extraplanar (fourth row) mock clumps.

Filter Region k p log min, 0 a b c d e
[ ×  10−1] [ ×  10−1] [ ×  10−3] [ ×  10−1] [ ×  10−2]
(0) (1) (2) (3) (4) (5) (6) (7) (8) (9)
Hα Tail 9.91 ± 0.02 4.85 ± 0.16 4.77 ± 0.01 2.63 ± 0.15 3.8 ± 0.6 33 ± 5 2.6 ± 0.2 −0.9 ± 0.3
extra. 9.29 ± 0.08 2.95 ± 0.09 5.49 ± 0.02 2.0 ± 0.5 6.6 ± 1.5 8 ± 13 8.3 ± 0.3 −7.3 ± 0.8

UV Tail 9.87 ± 0.04 3.88 ± 0.13 5.02 ± 0.01 1.77 ± 0.20 7.6 ± 0.7 −5.2 ± 6.0 5.3 ± 0.2 −6.1 ± 0.3
extra. 7.84 ± 0.13 2.38 ± 0.08 5.80 ± 0.02 1.8 ± 0.6 6.7 ± 2.0 13 ± 15 10.6 ± 0.6 −11 ± 1

Notes. The completeness and mass bias functions are modelled as described in Sects. 3.1 and 3.2. Columns (0) and (1): Mock clump reference filter and region, respectively. Columns (2)–(4): Free parameters of the completeness (k, p, log min, 0), as described in Eq. (2) (i.e. the maximum value of the completeness, the steepness of the rise and the input mass at which the rise starts). Columns (5)–(9): Free parameters of the mass bias function, as in Eq. (5), where (a, b, c) describe the input-output mass correlation and (d, e) the intrinsic scatter of the correlation.

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