Online Material
Appendix A: Additional figures
![\begin{figure}
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Figure A.1: Spectropolarimetric data for SN 2006X on day -10. From top to bottom: total flux spectrum (in 10-15 erg s-1cm-2 Å-1), ISP corrected polarization degree, the Stokes parameters Q and U and polarization position angle on the plane of the sky. |
| Open with DEXTER | |
![\begin{figure}
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Figure A.2: Same as Fig. A.1 for day -8. |
| Open with DEXTER | |
![\begin{figure}
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Figure A.3: Same as Fig. A.1 for day -7. |
| Open with DEXTER | |
![\begin{figure}
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Figure A.4: Same as Fig. A.1 for day -6. |
| Open with DEXTER | |
![\begin{figure}
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Figure A.5: Same as Fig. A.1 for day -3. |
| Open with DEXTER | |
![\begin{figure}
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Figure A.6: Same as Fig. A.1 for day -2. |
| Open with DEXTER | |
![\begin{figure}
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Figure A.7: Same as Fig. A.1 for day -1. |
| Open with DEXTER | |
![\begin{figure}
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Figure A.8: Same as Fig. A.1 for day +39. |
| Open with DEXTER | |
![\begin{figure}
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Figure A.9: Spectropolarimetry of SN 2006X on day -7. Main line identifications are given in the upper panel. The red histogram traces the polarization along the dominant axys. Vertical dashed lines correspond to an expansion velocity of 19,000 km s-1, while the dotted lines correspond to 14,000 km s-1. |
| Open with DEXTER | |
![\begin{figure}
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Figure A.10: Same as Fig. A.9 for day -3. Vertical dashed lines correspond to a expansion velocity of 17,000 km s-1, while the dotted lines correspond to 12,000 km s-1. |
| Open with DEXTER | |
![\begin{figure}
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Figure A.11: Same as Fig. A.9 for day -1. Vertical dashed lines correspond to an expansion velocity of 16,000 km s-1, while the dotted lines correspond to 11,000 km s-1. |
| Open with DEXTER | |
![\begin{figure}
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Figure A.12: Same as Fig. A.9 for day +39. Vertical dotted lines correspond to a expansion velocity of 13,000 km s-1. |
| Open with DEXTER | |