Table A.1
Selection of data.
| Region |
|
f ∇ | f pol | f tot |
| [1020 cm-2] | [%] | [%] | [%] | |
|
|
||||
| Taurus .................. | 6.2 | 66 | 78 | 28 |
| Ophiuchus .................. | 5.6 | 65 | 82 | 31 |
| Lupus .................. | 9.6 | 65 | 67 | 24 |
| Chamaeleon-Musca . | 6.3 | 49 | 83 | 31 |
| Corona Australia (CrA) | 5.4 | 34 | 40 | 4 |
|
|
||||
| Aquila Rift .................. | 18.4 | 48 | 96 | 32 |
| Perseus .................. | 5.3 | 60 | 59 | 16 |
|
|
||||
| IC 5146 .................. | 26.4 | 38 | 93 | 29 |
| Cepheus .................. | 7.5 | 66 | 80 | 36 |
| Orion .................. | 6.1 | 63 | 67 | 24 |
|
|
||||
| ChamEast .................. | 6.3 | 33 | 38 | 10 |
| ChamSouth .................. | 4.9 | 36 | 42 | 13 |
Notes. Mean column density of the background/foreground for each region estimated from a reference field at the same Galactic latitude; percentage f∇ of all pixels where 
; percentage fpol of all pixels where 
or 
(first polarization criterion) and where | Q | > 3σQ or | U | > 3σU (second polarization criterion); and percentage ftot of all pixels used for the HRO analysis.
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