Table 5:

Polarisation parameters of CSSs from mas-resolution observations.

Name	Alt. Name	z	Id.	m	DP		Notes	Ref.
				(%)		(rad m-2)
3C 43	B0127+233	1.459	Q	0.4		14 236	E, 1600 pc from core	1
3C 119a	B0429+415	1.023	Q?	14.4	0.08 5.0/8.4	10 200	C, 325 pc from core	2
3C 138	B0518+165	0.759	Q	3.6		-5287	B1, 40 pc from core	3
3C 147	B0538+498	0.545	Q	6.6		-4872	BN, 37 pc from core A0	4
4C 16.14b	B0548+165	0.474	Q	6.2	0.26 4.6/8.4	-4275	5C, 540 pc from core	5
3C 216	B0906+430	0.670	Q	30.0	0.97 4.8/8.4	2200	Arc, 1050 pc from core	6
3C 286c	B1328+307	0.849	Q	11.0			Core unclear	7,12
3C 287d	B1328+254	1.055	Q	4.6		0	Based on only 8.15 and 8.54 GHz	8
OQ 172e	B1442+101	3.529	Q	2.7		40 000	Within 20 pc from core	9,11
3C 309.1	B1458+718	0.905	Q	1.5	0.108.4/15	-1633	Core RM between 8.4 and 15 GHz	10
3C 318	B1517+204	1.574	NG	3.5		3030	K2, Core unclear	2
OR-140f	B1524-136	1.687	Q	30.2	1 4.6-5.1/8.4	-10 000	C, 810 pc from core F	5
3C 343g	B1634+628	0.988	Q	4.8	0.91 4.6-5.1/8.4	>6000	core unclear	2
3C 454	B2249+185	1.757	Q	10.9		5334	B, 300 pc from possible core	1

Notes. Table 5 is organised as follows: Col. 1, source name; 2, alternative name; 3, redshift; 4, optical identification; 5, polarisation percentage of the emission; 6, highest value of depolarisation; 7, highest measured rest frame RM; 8, notes: letters refer to components designetion as in references quoted in Col. 9; 9, references: 1) Cotton et al. (2003); 2) present work; 3) Cotton et al. (2003b); 4) Rossetti et al. (2009); 5) Mantovani et al. (2002); 6) Venturi & Taylor (1999); 7) Jiang et al. (1996); 8) Dallacasa et al. (1998); 9) Udomprasert et al. (1997); 10) Aaron et al. (1997); 11) Mantovani, private communication; 12) Cotton et al. (1997).
^am and DP values are for component C, where the peak of polarised intensity is surrounded by a region with RM in the range of 9000-10 200 rad m^-2; ^bm and DP values are for the entire component 5; ^cfractional polarisations are 8.9 and 11.0% at 5 GHz for the western and eastern knots respectively (Cotton et al. 1997); polarisation is 11.3% for the dominant component with the VLA-A array at 4.885 GHz (Perley 1982); RM expected to be low but not determined with mas resolution; ^dpolarisation is 4.6% with the VLA-A array at 4.885 GHz (Perley 1982); ^epolarisation is 2.0% with the VLA-A array at 4.885 GHz (Perley 1982); ^fDP estimated using 8.4 GHz and the mean of four measurements between 4.6 to 5.1 GHz; ^gDP estimated using 8.4 GHz and the mean of four measurements between 4.6 to 5.1 GHz for component A; there appears to be different regions of high RM.