Table 4.
Polarization of our CLAGNs.
| AGN | Pd (%) | θ (°) | ISP? |
|---|---|---|---|
| IRAS 23226-3843 | 0.32 ± 0.1 | 138.7 ± 0.9 | X |
| NGC 1346 | 0.27 ± 0.1 | 29.1 ± 1.3 | ✓ |
| NGC 2617 | 0.11 ± 0.1 | 142.6 ± 2.7 | ✓ |
| NGC 7582 (V) | 0.46 ± 0.1 | 0.3 ± 0.8 | X |
| NGC 7582 (R) | 0.22 ± 0.1 | 1.9 ± 1.3 | X |
| NGC 7603 | 0.45 ± 0.1 | 150.5 ± 0.9 | X |
Notes. Debiased polarization integrated over the whole waveband, uncorrected for ISP and host galaxy dilution. In all but one case (NGC 2617), the polarization is substantially higher than the instrumental polarization. The last column indicates if the signal appears ISP-dominated. The V and R indicators for NGC 7582 refer to the two synthetic Kron-Cousins broad band filters used to highlight the wavelength-dependence of Pd in this AGN.
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