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Table 1.
Galaxies that contribute data within the white ellipse of Fig. 1.
| Name | Data points | Percentage |
|---|---|---|
| NGC 4631 | 343 | 17.8% |
| NGC 3079 | 200 | 10.4% |
| NGC 3628 | 199 | 10.3% |
| NGC 3556 | 177 | 9.2% |
| NGC 4666 | 173 | 9.0% |
| NGC 5775 | 150 | 7.8% |
| NGC 4565 | 107 | 5.5% |
| NGC 4192 | 96 | 5.0% |
| NGC 891 | 95 | 4.9% |
| NGC 4217 | 78 | 4.0% |
| NGC 3735 | 74 | 3.8% |
| NGC 4157 | 71 | 3.7% |
| NGC 4845 | 45 | 2.3% |
| NGC 3044 | 42 | 2.2% |
| NGC 5907 | 21 | 1.1% |
| NGC 2683 | 20 | 1.0% |
| NGC 4388 | 13 | 0.7% |
| NGC 3448 | 7 | 0.4% |
| NGC 4302 | 7 | 0.4% |
| NGC 4013 | 4 | 0.2% |
| NGC 3432 | 3 | 0.2% |
| NGC 4096 | 3 | 0.2% |
| NGC 5792 | 2 | 0.1% |
| NGC 5297 | 1 | 0.1% |
| Total | 1931 | 100% |
Notes. The second and third columns list the number of RM measurements within the ellipse and the corresponding fractions, respectively. The RM maps are shown in Appendix A.
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