Open Access

Table C.1.

Best-fitting parameters of the radius-mass relation, modelled as described in Sect. C.

Hα UV

Parameter Tail Extra. Tail Extra.

m/10−1 0.3 ± 0.6 2.0 ± 0.7 1.7 ± 0.3 2.2 ± 0.3
q −1.2 ± 0.3 −2.2 ± 0.4 −1.9 ± 0.1 −2.3 ± 0.2
σr/10−2 3.4 ± 1.8 8.1 ± 1.7 7.5 ± 0.9 11 ± 1

Notes. From left to right: List of free parameters (slope m, intercept q and radius intrinsic scatter σr), the results for Hα tail clumps, Hα extraplanar clumps, UV tail clumps, and UV extraplanar clumps.

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