Table 1
Standard deviation of the observed rotation measure in different regions in and around the line of sight of galaxy clusters.
| < 0.5r500 | 0.5−1r500 | < r 500 | 1−10r500 | |
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| A | 123 ± 21 | 114 ± 43 | 120 ± 21 | 57 ± 6 |
| B | 94 ± 13 | 114 ± 43 | 100 ± 15 | 57 ± 6 |
| C | 124 ± 21 | 112 ± 43 | 120 ± 21 | 52 ± 6 |
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| < 0.5 Mpc | 0.5−1 Mpc | < 1 Mpc | > 1 Mpc | |
|
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| D | 115 ± 27 | 107 ± 33 | 112 ± 21 | 68 ± 10 |
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| N e | < 6.5 × 1020 | 6.5−15.2 × 1020 | > 6.5 × 1020 | |
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| E | 58.6 ± 10.5 | 122.2 ± 35.6 | 157.0 ± 40.3 | |
Notes. Ne refers to the electron column density in the line of sight. A: RMs uncorrected for the galactic contribution; B: same as A without RMs | RM | > 500; C: with RMs corrected for Galactic contribution; D: region defined in physical radii; E: RMs as a function of electron column density given in units of cm-2. The caption for the last line gives the range of electron column densities for the bin. The bin boundaries have been chosen such that each bin has a similar number of RMs.
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