Open Access
Table 10.
of the extragalactic foreground components for space-based and balloon-borne experiments: radio galaxies, dusty galaxies (IR), and CIB one-halo (completely negligible for ν ≤ 90 GHz and thus not computed).
| Experiment | ν | δν | C |
 Radio |
 IR |
 CIB (ℓ = 80) |
 CIB (ℓ = 1000) |
 CIB (ℓ = 4000) |
|---|---|---|---|---|---|---|---|---|
| GHz | % | Jy2 sr−1 | Jy2 sr−1 | Jy2 sr−1 | Jy2 sr−1 | Jy2 sr−1 | ||
| Planck | 30 | 30 | 26.81 | 8.918 10−3 | 6.542 10−6 | – | – | – |
| 44 | 30 | 56.17 | 9.882 10−3 | 6.766 10−6 | – | – | – | |
| 70 | 30 | 131.85 | 3.537 10−3 | 5.973 10−6 | – | – | – | |
| 100 | 30 | 237.01 | 2.515 10−3 | 1.840 10−5 | 4.517 10−6 | 4.367 10−6 | 4.032 10−6 | |
| 143 | 30 | 377.14 | 1.583 10−3 | 1.267 10−4 | 4.387 10−5 | 4.212 10−5 | 3.835 10−5 | |
| 217 | 30 | 480.18 | 7.009 10−4 | 1.465 10−3 | 4.986 10−4 | 4.724 10−4 | 4.189 10−4 | |
| 353 | 30 | 294.65 | 9.675 10−4 | 2.052 10−2 | 6.724 10−3 | 6.164 10−3 | 5.125 10−3 | |
| IDS | 150 | 30 | 395.55 | 1.581 10−3 | 1.684 10−4 | 5.998 10−5 | 5.751 10−5 | 5.223 10−5 |
| 180 | 30 | 454.58 | 1.027 10−3 | 4.920 10−4 | 1.671 10−4 | 1.595 10−4 | 1.435 10−4 | |
| 220 | 30 | 480.08 | 4.473 10−4 | 1.569 10−3 | 5.321 10−4 | 5.040 10−4 | 4.466 10−4 | |
| 250 | 30 | 463.95 | 2.754 10−4 | 3.209 10−3 | 1.106 10−3 | 1.041 10−3 | 9.097 10−4 | |
| 280 | 30 | 426.14 | 5.747 10−4 | 6.116 10−3 | 2.008 10−3 | 1.877 10−3 | 1.620 10−3 | |
| 320 | 30 | 356.86 | 4.049 10−4 | 1.223 10−2 | 4.052 10−3 | 3.750 10−3 | 3.174 10−3 | |
| 360 | 30 | 281.64 | 3.683 10−4 | 2.186 10−2 | 7.369 10−3 | 6.745 10−3 | 5.589 10−3 | |
| PIPER | 200 | 30 | 474.77 | 1.412 10−2 | 1.060 10−3 | 3.087 10−4 | 2.935 10−4 | 2.622 10−4 |
| 270 | 30 | 440.61 | 6.468 10−3 | 5.397 10−3 | 1.677 10−3 | 1.570 10−3 | 1.361 10−3 | |
| 350 | 16 | 301.91 | 4.355 10−3 | 2.058 10−2 | 6.448 10−3 | 5.916 10−3 | 4.925 10−3 | |
| 600 | 10 | 31.88 | 5.911 10−3 | 2.083 10−1 | 7.684 10−2 | 6.487 10−2 | 4.589 10−2 | |
| SPIDER | 94 | 24 | 216.11 | 3.652 10−2 | 3.789 10−5 | 1.595 10−6 | 1.554 10−6 | 1.457 10−6 |
| 150 | 24 | 396.64 | 2.542 10−2 | 2.359 10−4 | 5.998 10−5 | 5.751 10−5 | 5.223 10−5 | |
| LiteBIRD | 40 | 30 | 46.82 | 3.891 10−2 | 1.667 10−5 | – | – | – |
| 50 | 30 | 71.49 | 3.855 10−2 | 1.731 10−5 | – | – | – | |
| 60 | 23 | 100.42 | 3.617 10−2 | 1.796 10−5 | – | – | – | |
| 68 | 23 | 125.69 | 3.094 10−2 | 1.765 10−5 | – | – | – | |
| 78 | 23 | 159.42 | 2.798 10−2 | 1.993 10−5 | – | – | – | |
| 89 | 23 | 198.26 | 2.494 10−2 | 2.476 10−5 | – | – | – | |
| 100 | 23 | 237.76 | 2.263 10−2 | 3.390 10−5 | 4.517 10−6 | 4.367 10−6 | 4.032 10−6 | |
| 119 | 30 | 303.30 | 1.929 10−2 | 6.655 10−5 | 1.377 10−5 | 1.327 10−5 | 1.219 10−5 | |
| 140 | 30 | 368.76 | 1.724 10−2 | 1.465 10−4 | 3.696 10−5 | 3.553 10−5 | 3.240 10−5 | |
| 166 | 30 | 431.24 | 1.964 10−2 | 3.864 10−4 | 1.082 10−4 | 1.035 10−4 | 9.349 10−5 | |
| 195 | 30 | 471.16 | 1.656 10−2 | 9.365 10−4 | 2.733 10−4 | 2.600 10−4 | 2.325 10−4 | |
| 235 | 30 | 475.27 | 1.322 10−2 | 2.629 10−3 | 7.830 10−4 | 7.390 10−4 | 6.504 10−4 | |
| 280 | 30 | 426.14 | 5.453 10−3 | 6.534 10−3 | 2.008 10−3 | 1.877 10−3 | 1.620 10−3 | |
| 337 | 30 | 324.81 | 3.446 10−3 | 1.687 10−2 | 5.305 10−3 | 4.886 10−3 | 4.098 10−3 | |
| 402 | 23 | 209.33 | 2.715 10−3 | 3.910 10−2 | 1.269 10−2 | 1.147 10−2 | 9.275 10−3 | |
| PICO | 21 | 25 | 13.33 | 9.236 10−3 | 7.227 10−6 | – | – | – |
| 25 | 25 | 18.80 | 7.127 10−3 | 6.041 10−6 | – | – | – | |
| 30 | 25 | 26.88 | 6.550 10−3 | 5.586 10−6 | – | – | – | |
| 36 | 25 | 38.31 | 5.421 10−3 | 4.964 10−6 | – | – | – | |
| 43 | 25 | 53.89 | 5.817 10−3 | 5.160 10−6 | – | – | – | |
| 52 | 25 | 77.10 | 4.826 10−3 | 4.953 10−6 | – | – | – | |
| 62 | 25 | 106.48 | 2.782 10−3 | 4.479 10−6 | – | – | – | |
| 75 | 25 | 148.98 | 2.354 10−3 | 6.148 10−6 | – | – | – | |
| 90 | 25 | 201.67 | 2.136 10−3 | 1.114 10−5 | – | – | – | |
| 108 | 25 | 266.03 | 1.599 10−3 | 2.575 10−5 | 8.413 10−6 | 8.117 10−6 | 7.465 10−6 | |
| 129 | 25 | 336.61 | 1.558 10−3 | 6.925 10−5 | 2.447 10−5 | 2.354 10−5 | 2.152 10−5 | |
| 155 | 25 | 408.65 | 1.080 10−3 | 2.015 10−4 | 7.149 10−5 | 6.851 10−5 | 6.214 10−5 | |
| 186 | 25 | 463.34 | 4.249 10−4 | 5.855 10−4 | 2.096 10−4 | 1.997 10−4 | 1.791 10−4 | |
| 223 | 25 | 480.81 | 2.666 10−4 | 1.673 10−3 | 5.823 10−4 | 5.510 10−4 | 4.874 10−4 | |
| 268 | 25 | 444.34 | 4.014 10−4 | 4.758 10−3 | 1.611 10−3 | 1.509 10−3 | 1.309 10−3 | |
| 321 | 25 | 355.82 | 2.258 10−4 | 1.218 10−2 | 4.126 10−3 | 3.817 10−3 | 3.229 10−3 | |
| 385 | 25 | 237.49 | 3.078 10−4 | 2.977 10−2 | 1.031 10−2 | 9.368 10−3 | 7.650 10−3 | |
| 462 | 25 | 126.74 | 3.463 10−4 | 6.681 10−2 | 2.442 10−2 | 2.166 10−2 | 1.688 10−2 | |
| 555 | 25 | 51.31 | 3.142 10−4 | 1.358 10−1 | 5.530 10−2 | 4.746 10−2 | 3.470 10−2 | |
| 666 | 25 | 15.07 | 3.317 10−4 | 2.478 10−1 | 1.177 10−1 | 9.688 10−2 | 6.511 10−2 | |
| 799 | 25 | 3.00 | 3.298 10−4 | 4.063 10−1 | 2.357 10−1 | 1.839 10−1 | 1.109 10−1 | |
Notes. They are given in Jy2 sr−1. The unit conversion factor is also given (C = MJy sr−1[νIν= constant] 
). The power spectra in Jy2 sr−1 have to be divided by C2 to obtain power spectra in μ
.
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