Table A.1.
Source properties and ISM properties (from Planck’s GNILC 353GHz thermal dust map) with corrected Stokes parameters.
| Source | Gal. long. | Gal. lat. | Qobs | Uobs | QGNILC | UGNILC | AV | Qconv | Uconv | Qcorr | Ucorr |
|---|---|---|---|---|---|---|---|---|---|---|---|
| [deg.] | [deg.] | [%] | [%] | [%] | [%] | [mag] | [%] | [%] | [%] | [%] | |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) |
| Mrk 1044 | 179.694 | -60.477 | 0.039 | -0.148 | 3.307 | -0.252 | 0.095 | -0.075 | 0.006 | 0.114 | -0.153 |
| SDSSJ080101 | 203.015 | +23.510 | -0.305 | -0.422 | 2.761 | -0.142 | 0.086 | -0.057 | 0.003 | -0.249 | -0.423 |
| IRAS04416 | 185.854 | -21.088 | -0.125 | 0.149 | 2.623 | 0.098 | 1.187 | -0.741 | -0.028 | 0.616 | 0.176 |
| Fairall 9 | 295.073 | -57.827 | -1 | -2.5 | -0.697 | -3.412 | 0.071 | 0.012 | 0.058 | -1.012 | -2.558 |
Notes. The columns show the (1) name of the source, (2-3) sky coordinates in a galactic coordinate system, (4-5) observed values of Q (Qobs) and U (Uobs) from our measurements, (6-7) QGNILC and UGNILC obtained from Planck’s GNILC dust maps, (8) optical extinction coefficient AV, (9-10) converted Q (Qconv) and U (Uconv) from sub-mm to optical V-band, and (11-12) corrected values of Qcorr and Ucorr.
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