Open Access
Table C.1.
Dust polarization amplitudes for six different Galactic regions at 353 GHz.
| LR24 | LR33 | LR42 | LR52 | LR62 | LR71 | |
|---|---|---|---|---|---|---|
| ℓbin |
 |
|||||
| 2–3...... | ... | ... | ... | ... | ... | 2527 ± 69 |
| 4–11...... | 43 ± 6 | 99 ± 6 | 199 ± 7 | 371 ± 9 | 697 ± 10 | 986 ± 10 |
| 12–19...... | 101 ± 5 | 91 ± 5 | 140 ± 5 | 260 ± 6 | 371 ± 6 | 739 ± 8 |
| 20–39...... | 55 ± 3 | 78 ± 3 | 133 ± 3 | 207 ± 4 | 327 ± 4 | 543 ± 5 |
| 40–59...... | 39 ± 3 | 53 ± 3 | 80 ± 3 | 143 ± 4 | 227 ± 5 | 353 ± 5 |
| 60–79...... | 34 ± 3 | 47 ± 3 | 70 ± 4 | 110 ± 4 | 181 ± 4 | 307 ± 5 |
| 80–99...... | 33 ± 4 | 42 ± 4 | 73 ± 4 | 116 ± 4 | 191 ± 4 | 310 ± 5 |
| 100–119...... | 34 ± 4 | 45 ± 4 | 73 ± 4 | 114 ± 4 | 174 ± 5 | 285 ± 5 |
| 120–139...... | 25 ± 5 | 37 ± 4 | 58 ± 4 | 91 ± 5 | 156 ± 6 | 280 ± 6 |
| 140–159...... | 32 ± 6 | 41 ± 5 | 62 ± 5 | 93 ± 5 | 145 ± 5 | 240 ± 6 |
| 160–179...... | 24 ± 6 | 35 ± 6 | 59 ± 6 | 88 ± 6 | 136 ± 6 | 218 ± 6 |
| 180–199...... | 30 ± 7 | 40 ± 6 | 51 ± 6 | 79 ± 7 | 119 ± 7 | 206 ± 7 |
| 200–219...... | 34 ± 8 | 39 ± 7 | 61 ± 6 | 89 ± 6 | 138 ± 6 | 231 ± 6 |
| 220–239...... | 28 ± 8 | 44 ± 8 | 62 ± 8 | 93 ± 8 | 130 ± 8 | 211 ± 7 |
| 240–259...... | 37 ± 9 | 39 ± 9 | 60 ± 8 | 90 ± 8 | 126 ± 8 | 201 ± 8 |
| 260–279...... | 15 ± 10 | 17 ± 9 | 40 ± 9 | 74 ± 9 | 119 ± 8 | 197 ± 9 |
| 280–299...... | 15 ± 11 | 19 ± 9 | 47 ± 9 | 71 ± 9 | 106 ± 9 | 175 ± 9 |
| 300–319...... | −6 ± 12 | 8 ± 11 | 20 ± 10 | 45 ± 11 | 86 ± 10 | 150 ± 10 |
| 320–339...... | 23 ± 13 | 36 ± 13 | 47 ± 12 | 66 ± 12 | 102 ± 11 | 166 ± 10 |
| 340–359...... | 19 ± 14 | 27 ± 13 | 38 ± 12 | 63 ± 12 | 98 ± 12 | 165 ± 11 |
| 360–379...... | 23 ± 16 | 28 ± 14 | 41 ± 13 | 52 ± 13 | 84 ± 12 | 143 ± 12 |
| 380–399...... | 8 ± 17 | 6 ± 15 | 33 ± 14 | 54 ± 13 | 85 ± 12 | 143 ± 11 |
| 400–419...... | 15 ± 17 | 33 ± 15 | 47 ± 15 | 73 ± 14 | 108 ± 14 | 157 ± 13 |
| 420–439...... | 26 ± 19 | 33 ± 18 | 56 ± 16 | 71 ± 15 | 98 ± 14 | 151 ± 14 |
| 440–459...... | 34 ± 21 | 41 ± 20 | 47 ± 19 | 66 ± 18 | 88 ± 17 | 136 ± 16 |
| 460–479...... | 7 ± 21 | 23 ± 19 | 41 ± 17 | 56 ± 16 | 82 ± 16 | 128 ± 15 |
| 480–499...... | 41 ± 24 | 64 ± 22 | 72 ± 21 | 84 ± 20 | 101 ± 19 | 142 ± 18 |
| 500–549...... | 29 ± 18 | 28 ± 16 | 43 ± 14 | 65 ± 14 | 93 ± 13 | 142 ± 12 |
| 550–599...... | 20 ± 19 | 41 ± 17 | 52 ± 16 | 67 ± 16 | 88 ± 14 | 131 ± 13 |
| ℓbin |
 |
|||||
| 2–3...... | ... | ... | ... | ... | ... | 247 ± 17 |
| 4–11...... | 36 ± 4 | 78 ± 5 | 187 ± 8 | 365 ± 8 | 357 ± 7 | 502 ± 5 |
| 12–19...... | 30 ± 3 | 44 ± 3 | 117 ± 4 | 159 ± 4 | 282 ± 5 | 422 ± 5 |
| 20–39...... | 33 ± 2 | 44 ± 2 | 91 ± 2 | 137 ± 2 | 185 ± 3 | 399 ± 3 |
| 40–59...... | 19 ± 2 | 25 ± 2 | 54 ± 2 | 86 ± 3 | 138 ± 3 | 241 ± 3 |
| 60–79...... | 15 ± 2 | 20 ± 2 | 36 ± 2 | 69 ± 2 | 108 ± 3 | 170 ± 3 |
| 80–99...... | 16 ± 2 | 20 ± 2 | 36 ± 2 | 58 ± 3 | 97 ± 3 | 173 ± 3 |
| 100–119...... | 15 ± 3 | 20 ± 3 | 33 ± 3 | 55 ± 3 | 92 ± 3 | 166 ± 3 |
| 120–139...... | 16 ± 3 | 18 ± 3 | 31 ± 3 | 54 ± 3 | 84 ± 3 | 132 ± 4 |
| 140–159...... | 12 ± 4 | 15 ± 4 | 24 ± 3 | 47 ± 4 | 76 ± 4 | 122 ± 4 |
| 160–179...... | 14 ± 5 | 18 ± 4 | 25 ± 4 | 46 ± 4 | 68 ± 4 | 111 ± 4 |
| 180–199...... | 12 ± 5 | 13 ± 5 | 23 ± 5 | 39 ± 5 | 62 ± 5 | 105 ± 5 |
| 200–219...... | 19 ± 6 | 20 ± 5 | 30 ± 5 | 44 ± 5 | 65 ± 5 | 111 ± 5 |
| 220–239...... | 28 ± 6 | 26 ± 6 | 31 ± 6 | 42 ± 5 | 64 ± 5 | 107 ± 5 |
| 240–259...... | 12 ± 8 | 12 ± 7 | 20 ± 6 | 29 ± 6 | 50 ± 6 | 88 ± 6 |
| 260–279...... | 12 ± 8 | 20 ± 7 | 29 ± 7 | 51 ± 7 | 70 ± 6 | 106 ± 6 |
| 280–299...... | 12 ± 9 | 15 ± 8 | 23 ± 8 | 30 ± 8 | 50 ± 8 | 83 ± 7 |
| 300–319...... | 21 ± 10 | 21 ± 8 | 25 ± 8 | 34 ± 8 | 55 ± 8 | 89 ± 8 |
| 320–339...... | 11 ± 11 | 15 ± 10 | 22 ± 9 | 32 ± 9 | 56 ± 8 | 88 ± 8 |
| 340–359...... | 6 ± 12 | 7 ± 11 | 17 ± 10 | 33 ± 9 | 52 ± 9 | 85 ± 8 |
| 360–379...... | 16 ± 14 | 10 ± 12 | 21 ± 12 | 38 ± 11 | 53 ± 11 | 83 ± 10 |
| 380–399...... | 4 ± 13 | 2 ± 12 | 15 ± 11 | 18 ± 11 | 35 ± 10 | 61 ± 9 |
| 400–419...... | 8 ± 15 | 8 ± 13 | 17 ± 13 | 22 ± 12 | 44 ± 11 | 73 ± 10 |
| 420–439...... | 23 ± 16 | 23 ± 15 | 31 ± 14 | 36 ± 13 | 55 ± 12 | 77 ± 12 |
| 440–459...... | −5 ± 18 | 11 ± 15 | 20 ± 15 | 45 ± 14 | 53 ± 13 | 74 ± 12 |
| 460–479...... | −22 ± 19 | −16 ± 17 | 0 ± 15 | 18 ± 15 | 30 ± 14 | 61 ± 13 |
| 480–499...... | 13 ± 21 | 7 ± 19 | 17 ± 18 | 20 ± 17 | 38 ± 17 | 71 ± 15 |
| 500–549...... | 16 ± 15 | 13 ± 13 | 12 ± 11 | 21 ± 11 | 29 ± 10 | 51 ± 9 |
| 550–599...... | 13 ± 17 | 13 ± 15 | 15 ± 14 | 21 ± 14 | 34 ± 13 | 58 ± 12 |
Notes. The CMB amplitude has been subtracted from the power spectrum level. The 1 σ error bars are derived from the E2E simulations. They do not include the 1.5% uncertainty on the 353 GHz polarization efficiency.
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