Table 3: ISP-corrected polarisations for all the remaining 18 sources where both the object and surrounding interstellar polarisation can be correctly evaluated.
Source $P'_{\rm A}$ (%) $\Theta'_{\rm A} (^\circ)$ $P'_{\rm B}$ (%) $\Theta'_{\rm B} (^\circ)$
ESO H$\alpha~29$ 3.33 (0.12) 27 (1) 1.75 (0.14) 171 (2)
Sz 30 3.98 (0.14) 64 (1) 3.88 (0.14) 64 (1)
Sz2 3.90 (0.13) 22 (1) 1.48 (0.07) 11 (1)
Glass-I 4.67 (0.16) 12.7 (0.5) 12.3 (0.4) 26 (0.5)
Sz 15 2.84 (0.13) 107 (1) 0.88 (0.16) 35 (5)
Sz 62 0.12 (0.12) 23 (28) 0.17 (0.12) 43 (20)
Sz 60 2.07 (0.08) 165 (1) 0.82 (0.05) 169 (1.5)
HO Lup 0.48 (0.08) 20 (4) 0.89 (0.07) 30 (2)
Sz 116 3.5 (0.13) 75 (1) 3.73 (0.16) 75 (1)
Sz 81 0.7 (0.05) 82 (3) 0.80 (0.07) 53 (2)
Sz 65 1.56 (0.14) 65 (3) 2.37 (0.3) 39 (3)
WSB 18 1.77 (0.07) 90 (1) 1.76 (0.07) 89 (1)
WSB 26 3.52 (0.12) 76 (0.5) 3.5 (0.12) 76 (0.6)
WSB 35 2.9 (0.1) 132 (0.5) 2.6 (0.1) 134 (1)
WSB 4 1.38 (0.06) 102 (1) 1.2 (0.05) 108 (1)
WSB 28 1.28 (0.06) 159 (1) 2.7 (0.3) 164 (3)
HBC 679 1.84 (0.07) 9 (0.7) 2.3 (0.24) 10 (2)
AS 353 1.88 (0.12) 110 (2) 1.54 (0.14) 113 (2.5)


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