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Table 1

Polarimetric observations of SN 2008D/XT 080109 and SN 2007uy.

Datea Telescope Exposure  Seeing SN 2008D/XT 080109 SN 2007uyb
2008, UT (+Instrument) time (s) (′′) P ± σP (%) θ ± σθ (deg) V ± σVc P ± σP (%) θ ± σθ (deg) V ± σVc

Jan. 13.1644 NOT(+ALFOSC) 12  ×  600 0.7 0.95 ± 0.20 114.9 ± 5.9 18.44 ± 0.05
Jan. 13.2642 VLT(+FORS1) 2330d 1.0 0.68 ± 0.22 119.2 ± 9.5 18.39 ± 0.05 1.45 ± 0.25 178.6 ± 4.6 15.78 ± 0.05
(0.65 ± 0.33)e (124.5 ± 13.3) (1.59 ± 0.04) (177.4 ± 0.7)
Jan. 15.0780 NOT(+ALFOSC) 12  ×  600 0.9 0.85 ± 0.28 106.1 ± 9.4 18.28 ± 0.05
Jan. 17.2518 VLT(+FORS1) 8  ×  285 1.0 0.84 ± 0.45 138.3 ± 8.1 17.90 ± 0.05 1.43 ± 0.14 182.5 ± 5.1 15.69 ± 0.05
(1.14 ± 0.51) (141.0 ± 7.2) (1.59 ± 0.04) (177.4 ± 0.7)
Jan. 30.1858 VLT(+FORS1) 4  ×  285 0.8 1.05 ± 0.06 135.3 ± 1.7 17.31 ± 0.05 1.64 ± 0.06 178.5 ± 1.1 16.39 ± 0.05
(1.11 ± 0.08) (134.0 ± 2.0) (1.59 ± 0.04) (177.4 ± 0.7)
Jan. 30.2022 VLT(+FORS1) 4  ×  285 0.8 1.28 ± 0.06 132.5 ± 1.4 17.27 ± 0.05 1.56 ± 0.06 176.1 ± 1.1 16.36 ± 0.05
(1.21 ± 0.08) (133.3 ± 1.9) (1.59 ± 0.04) (177.4 ± 0.7)
Feb. 11.9326 CAHA(+CAFOS) 13  ×  400 2.0 1.58 ± 0.97 126.6 ± 16.4 17.82 ± 0.09 0.92 ± 0.88 179.8 ± 26.0 17.09 ± 0.11
(1.19 ± 1.51) (131.6 ± 20.5) (1.59 ± 0.04) (177.4 ± 0.7)
Feb. 26.1107 CAHA(+CAFOS) 16  ×  600 1.9  < 2.76f 18.52 ± 0.09 1.81 ± 0.63 173.5 ± 14.4 17.56 ± 0.08
(< 2.94f ) (1.59 ± 0.04) (177.4 ± 0.7)
Feb. 26.9444 NOT(+ALFOSC) 16  ×  400 1.3 0.98 ± 0.80 124.6 ± 23.2 18.79 ± 0.08
Mar. 2.1102 VLT(+FORS1) 4  ×  525 1.1 1.42 ± 0.46 139.0 ± 9.1 18.80 ± 0.05 1.83 ± 0.19 174.6 ± 3.2 17.55 ± 0.05
(1.17 ± 0.51) (134.7 ± 11.4) (1.59 ± 0.04) (177.4 ± 0.7)
Mar. 28.0207 VLT(+FORS1) 4  ×  525 1.1 0.75 ± 0.57 111.2 ± 21.9 19.42 ± 0.05 1.58 ± 0.42 179.6 ± 7.6 17.98 ± 0.05
(0.73 ± 0.78) (112.7 ± 21.0) (1.59 ± 0.04) (177.4 ± 0.7)

Notes.

(a)

Mean observing epoch.

(b)

For the NOT epochs SN 2007uy was out of the FoV, so the degree of linear polarization (P), the position angle (θ), and the magnitude (V) could not be determined.

(c)

Calibration based on Malesani et al. (2009). The photometric errors include the zero point uncertainty.

(d)

The polarimetric cycle was interrupted and restarted several times. The SN 2007uy observing epoch and the exposure time are slightly different from the SN 2008D/XT 080109 ones, corresponding to Jan. 13.2708 UT and 990 seconds, respectively.

(e)

The SN 2008D/XT 080109P and θ values given for VLT and CAHA in between parentheses assume a constant SN 2007uy polarization given by   〈P〉 = 1.59 ± 0.04% and  〈θ〉 = 177.4 ± 0.7°.

(f)

1σ upper limit.

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