Table 4: For Bz=0, 600, and 1200 G we produced 1000 simulated polarisation spectra with the same noise level as the programme stars and used the same spectral lines as in the fits of Table 3. We list the weighted means and standard deviations (from all spectral lines) of the fits at each input Bz and additionally the smallest and largest value from all fits.
input Bz UVO 0512-08 CPD  $-64^\circ 481$ PG 0909+276 HD 76431 CD  $-31^\circ 4800$ LSE 153
(G) (G) (G) (G) (G) (G) (G)
0, average $-5\pm188$ $3\pm300$ $18\pm266$ $4\pm 128$ $0\pm 163$ $-1\pm 239$
0, smallest -513 -862 -792 -446 -554 -685
0, largest 646 +831 +1035 +393 +540 +857
600, average $550\pm184$ $582\pm294$ $555\pm269$ $578\pm 125$ $539\pm 170$ $603\pm243$
600, smallest -62 -387 -249 +233 -699 -250
600, largest +1108 +1692 +1603 +964 +1178 +1346
1200, average $1106\pm186$ $1170\pm291$ $1119\pm266$ $1131\pm 130$ $1090\pm 170$ $1194\pm243$
1200, smallest +490 +164 +185 614 +507 +489
1200, largest +1740 +2196 +2016 +1505 +1786 1842


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