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Table B.1

Structural parameters (median values of the marginalized posterior distributions) obtained with the MCMC Hammer for mock galaxies with number of analysed stars N = 200, 1000 and 5000 (top, middle and bottom sequences of rows respectively).

e i Side σ c,i r e θ e σ c
(re) (#/arcmin2) () (°) (#/arcmin2)

0.1 2 0.100 29.1 63 0.45 0.209
0.1 5 0.016 8.7 48 0.11 0.022
0.1 10 0.004 9.8 65 0.10 0.007
0.3 2 0.100 18.7 53 0.39 0.258
0.3 5 0.016 7.5 35 0.26 0.035
0.3 10 0.004 10.6 51 0.21 0.003

0.1 2 0.50 8.9 73 0.16 0.74
0.1 5 0.08 10.0 40 0.14 0.09
0.1 10 0.02 9.4 43 0.08 0.02
0.3 2 0.50 9.4 47 0.17 0.58
0.3 5 0.08 10.2 46 0.38 0.07
0.3 10 0.02 10.9 51 0.36 0.02

0.1 2 2.50 11.3 52 0.10 1.41
0.1 5 0.40 10.3 47 0.04 0.32
0.1 10 0.10 10.0 54 0.09 0.10
0.3 2 2.50 10.6 48 0.30 2.52
0.3 5 0.40 10.3 47 0.29 0.40
0.3 10 0.10 10.1 49 0.31 0.10

Notes. From left to right: input ellipticity (ei = 1−b/a), coverage (in re units), input contamination density (σc,i) and fitted parameters: exponential radius (re), position angle (θ), ellipticity (e) and contamination density (σc).

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