Table 2: Magnetic fields derived from the four strongest lines in our sample of central stars of planetary nebulae. The error margins correspond to a $1\sigma$ (68.3% confidence) and $6.6\sigma$ (99% confidence) level.
Target Date B/G B/G

H $\delta +$ He II H $\gamma +$ He II He II 4686 H $\beta +$ He II total

NGC 1360 03/11/03 $-493\pm 835$ $2483\pm688$ $-1114\pm427$ $-1355\pm413$ $-1343\pm259$

$(\pm 2153)$ $(\pm 1772)$ $(\pm 1101)$ $(\pm 1066)$ $(\pm 668)$

NGC 1360 14/12/03 $342\pm 624$ $3553\pm528$ $1726\pm426$ $768\pm543$ $1708\pm257$

$(\pm 1607)$ $(\pm 1361)$ $(\pm 1099)$ $(\pm 1399)$ $(\pm 664)$

NGC 1360 15/12/03 $3146\pm 735$ $2082\pm695$ $3714\pm389$ $1324\pm557$ $2832\pm269$

$(\pm 1895)$ $(\pm 1790)$ $(\pm 1002)$ $(\pm 1437)$ $(\pm 695)$

NGC 1360 16/12/03 $2548\pm 1024$ $1303\pm505$ $-1176\pm591$ $316\pm438$ $194\pm277$

$(\pm 2638)$ $(\pm 1302)$ $(\pm 1522)$ $(\pm 1128)$ $(\pm 2548)$

EGB 5 14/12/03 $577\pm 1171$ $2875\pm1022$ $484\pm4707$ $2171\pm837$ $1992\pm562$

$(\pm 3016)$ $(\pm 2633)$ $(\pm 12121)$ $(\pm 2156)$ $(\pm 1449)$

LSS 1362 15/12/03 $-299\pm 1295$ $2089\pm729$ $3608\pm894$ $1550\pm531$ $1891\pm371$

$(\pm 3335)$ $(\pm 1878)$ $(\pm 1848)$ $(\pm 1368)$ $(\pm 912)$

Abell 36 26/01/04 $1863\pm 1144$ $-448\pm949$ $1842\pm1134$ $1553\pm719$ $1169\pm466$

$(\pm 2946)$ $(\pm 2444)$ $(\pm 2920)$ $(\pm 1852)$ $(\pm 1202)$

**Table 2:** Magnetic fields derived from the four strongest lines in our sample of central stars of planetary nebulae. The error margins correspond to a $1\sigma$ (68.3% confidence) and $6.6\sigma$ (99% confidence) level.
Target	Date	B/G	B/G
		H $\delta +$ He II	H $\gamma +$ He II	He II 4686	H $\beta +$ He II	total
NGC 1360	03/11/03	$-493\pm 835$	$2483\pm688$	$-1114\pm427$	$-1355\pm413$	$-1343\pm259$
		$(\pm 2153)$	$(\pm 1772)$	$(\pm 1101)$	$(\pm 1066)$	$(\pm 668)$
NGC 1360	14/12/03	$342\pm 624$	$3553\pm528$	$1726\pm426$	$768\pm543$	$1708\pm257$
		$(\pm 1607)$	$(\pm 1361)$	$(\pm 1099)$	$(\pm 1399)$	$(\pm 664)$
NGC 1360	15/12/03	$3146\pm 735$	$2082\pm695$	$3714\pm389$	$1324\pm557$	$2832\pm269$
		$(\pm 1895)$	$(\pm 1790)$	$(\pm 1002)$	$(\pm 1437)$	$(\pm 695)$
NGC 1360	16/12/03	$2548\pm 1024$	$1303\pm505$	$-1176\pm591$	$316\pm438$	$194\pm277$
		$(\pm 2638)$	$(\pm 1302)$	$(\pm 1522)$	$(\pm 1128)$	$(\pm 2548)$
EGB 5	14/12/03	$577\pm 1171$	$2875\pm1022$	$484\pm4707$	$2171\pm837$	$1992\pm562$
		$(\pm 3016)$	$(\pm 2633)$	$(\pm 12121)$	$(\pm 2156)$	$(\pm 1449)$
LSS 1362	15/12/03	$-299\pm 1295$	$2089\pm729$	$3608\pm894$	$1550\pm531$	$1891\pm371$
		$(\pm 3335)$	$(\pm 1878)$	$(\pm 1848)$	$(\pm 1368)$	$(\pm 912)$
Abell 36	26/01/04	$1863\pm 1144$	$-448\pm949$	$1842\pm1134$	$1553\pm719$	$1169\pm466$
		$(\pm 2946)$	$(\pm 2444)$	$(\pm 2920)$	$(\pm 1852)$	$(\pm 1202)$

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations and data reduction
	3 Determination of the magnetic field strenghs
	4 Parameters of the target stars and nebulae
	5 Discussion and conclusions
	References