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
 |
PG 0909+276 |
HD 76431 |
CD
 |
LSE 153 |
| (G) |
(G) |
(G) |
(G) |
(G) |
(G) |
(G) |
| 0, average |
 |
 |
 |
 |
 |
 |
| 0, smallest |
-513 |
-862 |
-792 |
-446 |
-554 |
-685 |
| 0, largest |
646 |
+831 |
+1035 |
+393 |
+540 |
+857 |
| 600, average |
 |
 |
 |
 |
 |
 |
| 600, smallest |
-62 |
-387 |
-249 |
+233 |
-699 |
-250 |
| 600, largest |
+1108 |
+1692 |
+1603 |
+964 |
+1178 |
+1346 |
| 1200, average |
 |
 |
 |
 |
 |
 |
| 1200, smallest |
+490 |
+164 |
+185 |
614 |
+507 |
+489 |
| 1200, largest |
+1740 |
+2196 |
+2016 |
+1505 |
+1786 |
1842 |
Source LaTeX |
All tables |
In the text