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Table D.1
Cross-power spectra and error bars for all pairs of frequencies, measured on Galactic dust- and CMB-free residual maps.
| Cross-power spectra, Cℓ, and uncertainty [Jy2 sr-1, νIν = cst] | |||||||
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| ℓ cent | 3000 GHz | 857 GHz | 545 GHz | 353 GHz | 217 GHz | 143 GHz | |
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| 3000 GHz | 187 | (4.35 ± 1.34) × 105 | (1.12 ± 0.85) × 105 | (3.94 ± 3.88) × 104 | (8.92 ± 12.4) × 103 | (5.59 ± 26.7) × 102 | ... |
| 320 | (7.89 ± 3.14) × 104 | (7.49 ± 2.09) × 104 | (3.04 ± 0.85) × 104 | (1.13 ± 0.27) × 104 | (2.34 ± 0.71) × 103 | ... | |
| 502 | (3.46 ± 1.15) × 104 | (3.10 ± 0.79) × 104 | (1.23 ± 0.33) × 104 | (4.49 ± 1.15) × 103 | (1.18 ± 0.34) × 103 | ... | |
| 684 | (2.90 ± 0.70) × 104 | (2.24 ± 0.47) × 104 | (9.35 ± 2.10) × 103 | (2.87 ± 0.73) × 103 | (6.88 ± 2.61) × 102 | ... | |
| 890 | (1.87 ± 0.47) × 104 | (1.62 ± 0.30) × 104 | (6.61 ± 1.34) × 103 | (1.99 ± 0.45) × 103 | (2.34 ± 1.66) × 102 | ... | |
| 1158 | (1.43 ± 0.40) × 104 | (1.17 ± 0.22) × 104 | (4.71 ± 0.93) × 103 | (1.25 ± 0.31) × 103 | (3.55 ± 1.43) × 102 | ... | |
| 1505 | (1.09 ± 0.41) × 104 | (8.30 ± 1.85) × 103 | (3.12 ± 0.76) × 103 | (1.14 ± 0.30) × 103 | (2.41 ± 1.07) × 102 | ... | |
| 1956 | (1.05 ± 0.58) × 104 | (8.04 ± 2.39) × 103 | (3.16 ± 1.00) × 103 | (9.67 ± 3.44) × 102 | (2.58 ± 1.14) × 102 | ... | |
| 2649 | (1.06 ± 1.04) × 104 | (6.47 ± 3.27) × 103 | (2.61 ± 1.38) × 103 | ... | ... | ... | |
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| 857 GHz | 53 | ... | (1.49 ± 1.27) × 106 | (5.59 ± 4.14) × 105 | (1.70 ± 1.17) × 105 | (3.61 ± 2.53) × 104 | (5.15 ± 11.6) × 103 |
| 114 | ... | (6.37 ± 1.62) × 105 | (2.67 ± 0.57) × 105 | (8.63 ± 1.68) × 104 | (1.91 ± 0.38) × 104 | (2.53 ± 1.56) × 103 | |
| 187 | ... | (2.87 ± 0.37) × 105 | (1.30 ± 0.13) × 105 | (4.18 ± 0.39) × 104 | (8.61 ± 0.89) × 103 | (1.16 ± 0.45) × 103 | |
| 320 | ... | (1.34 ± 0.08) × 105 | (6.36 ± 0.30) × 104 | (2.12 ± 0.09) × 104 | (4.61 ± 0.22) × 103 | (6.43 ± 1.20) × 102 | |
| 502 | ... | (7.20 ± 0.26) × 104 | (3.53 ± 0.10) × 104 | (1.20 ± 0.03) × 104 | (2.65 ± 0.09) × 103 | (4.26 ± 0.59) × 102 | |
| 684 | ... | (4.38 ± 0.18) × 104 | (2.21 ± 0.07) × 104 | (7.68 ± 0.22) × 103 | (1.62 ± 0.06) × 103 | (2.39 ± 0.41) × 102 | |
| 890 | ... | (3.23 ± 0.09) × 104 | (1.63 ± 0.04) × 104 | (5.66 ± 0.12) × 103 | (1.14 ± 0.04) × 103 | (1.55 ± 0.30) × 102 | |
| 1158 | ... | (2.40 ± 0.05) × 104 | (1.22 ± 0.02) × 104 | (4.12 ± 0.07) × 103 | (8.29 ± 0.25) × 102 | (1.29 ± 0.23) × 102 | |
| 1505 | ... | (1.83 ± 0.03) × 104 | (9.31 ± 0.11) × 103 | (3.19 ± 0.04) × 103 | (6.82 ± 0.16) × 102 | (1.13 ± 0.16) × 102 | |
| 1956 | ... | (1.46 ± 0.02) × 104 | (7.38 ± 0.07) × 103 | (2.50 ± 0.03) × 103 | (5.36 ± 0.11) × 102 | (1.03 ± 0.15) × 102 | |
| 2649 | ... | (1.16 ± 0.01) × 104 | (5.91 ± 0.06) × 103 | ... | ... | ... | |
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| 545 GHz | 53 | ... | ... | (2.36 ± 1.37) × 105 | (7.46 ± 3.90) × 104 | (1.61 ± 0.85) × 104 | (2.46 ± 3.80) × 103 |
| 114 | ... | ... | (1.24 ± 0.21) × 105 | (4.12 ± 0.63) × 104 | (9.32 ± 1.44) × 103 | (1.35 ± 0.57) × 103 | |
| 187 | ... | ... | (6.63 ± 0.51) × 104 | (2.16 ± 0.15) × 104 | (4.48 ± 0.35) × 103 | (6.11 ± 1.78) × 102 | |
| 320 | ... | ... | (3.34 ± 0.12) × 104 | (1.15 ± 0.04) × 104 | (2.49 ± 0.09) × 103 | (3.51 ± 0.52) × 102 | |
| 502 | ... | ... | (1.91 ± 0.04) × 104 | (6.73 ± 0.15) × 103 | (1.48 ± 0.04) × 103 | (2.38 ± 0.28) × 102 | |
| 684 | ... | ... | (1.25 ± 0.03) × 104 | (4.48 ± 0.09) × 103 | (9.39 ± 0.29) × 102 | (1.37 ± 0.21) × 102 | |
| 890 | ... | ... | (9.17 ± 0.17) × 103 | (3.29 ± 0.05) × 103 | (6.59 ± 0.19) × 102 | (9.04 ± 1.60) × 101 | |
| 1158 | ... | ... | (6.83 ± 0.10) × 103 | (2.45 ± 0.03) × 103 | (4.97 ± 0.14) × 102 | (7.53 ± 1.33) × 101 | |
| 1505 | ... | ... | (5.34 ± 0.06) × 103 | (1.91 ± 0.02) × 103 | (4.21 ± 0.10) × 102 | (7.10 ± 1.01) × 101 | |
| 1956 | ... | ... | (4.24 ± 0.04) × 103 | (1.51 ± 0.02) × 103 | (3.29 ± 0.07) × 102 | (6.47 ± 1.01) × 101 | |
| 2649 | ... | ... | (3.42 ± 0.04) × 103 | ... | ... | ... | |
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| 353 GHz | 53 | ... | ... | ... | (2.53 ± 1.12) × 104 | (5.52 ± 2.45) × 103 | (7.70 ± 10.8) × 102 |
| 114 | ... | ... | ... | (1.43 ± 0.19) × 104 | (3.23 ± 0.45) × 103 | (4.65 ± 1.72) × 102 | |
| 187 | ... | ... | ... | (7.69 ± 0.48) × 103 | (1.66 ± 0.11) × 103 | (2.34 ± 0.56) × 102 | |
| 320 | ... | ... | ... | (4.23 ± 0.12) × 103 | (9.59 ± 0.32) × 102 | (1.51 ± 0.18) × 102 | |
| 502 | ... | ... | ... | (2.54 ± 0.05) × 103 | (5.91 ± 0.16) × 102 | (1.01 ± 0.11) × 102 | |
| 684 | ... | ... | ... | (1.70 ± 0.03) × 103 | (3.76 ± 0.11) × 102 | (6.22 ± 0.82) × 101 | |
| 890 | ... | ... | ... | (1.25 ± 0.02) × 103 | (2.72 ± 0.08) × 102 | (3.96 ± 0.69) × 101 | |
| 1158 | ... | ... | ... | (9.15 ± 0.14) × 102 | (1.87 ± 0.09) × 102 | (2.99 ± 0.90) × 101 | |
| 1505 | ... | ... | ... | (7.37 ± 0.11) × 102 | (1.54 ± 0.09) × 102 | (2.19 ± 1.09) × 101 | |
| 1956 | ... | ... | ... | (6.05 ± 0.09) × 102 | (1.34 ± 0.04) × 102 | (3.41 ± 0.64) × 101 | |
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| 217 GHz | 53 | ... | ... | ... | ... | (1.37 ± 0.55) × 103 | (2.16 ± 2.41) × 102 |
| 114 | ... | ... | ... | ... | (7.59 ± 1.08) × 102 | (1.10 ± 0.42) × 102 | |
| 187 | ... | ... | ... | ... | (4.27 ± 0.38) × 102 | (7.80 ± 1.60) × 101 | |
| 320 | ... | ... | ... | ... | (2.65 ± 0.13) × 102 | (5.68 ± 0.60) × 101 | |
| 502 | ... | ... | ... | ... | (1.78 ± 0.08) × 102 | (4.77 ± 0.47) × 101 | |
| 684 | ... | ... | ... | ... | (1.18 ± 0.07) × 102 | (3.05 ± 0.43) × 101 | |
| 890 | ... | ... | ... | ... | (8.78 ± 0.71) × 101 | (1.87 ± 0.48) × 101 | |
| 1158 | ... | ... | ... | ... | (5.97 ± 1.57) × 101 | (1.46 ± 1.19) × 101 | |
| 1505 | ... | ... | ... | ... | (3.08 ± 2.15) × 101 | (8.40 ± 16.4) × 100 | |
| 1956 | ... | ... | ... | ... | (4.73 ± 0.65) × 101 | (1.49 ± 0.53) × 101 | |
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| 143 GHz | 53 | ... | ... | ... | ... | ... | (7.23 ± 6.67) × 101 |
| 114 | ... | ... | ... | ... | ... | (3.05 ± 1.43) × 101 | |
| 187 | ... | ... | ... | ... | ... | (2.20 ± 0.67) × 101 | |
| 320 | ... | ... | ... | ... | ... | (2.14 ± 0.31) × 101 | |
| 502 | ... | ... | ... | ... | ... | (1.99 ± 0.28) × 101 | |
| 684 | ... | ... | ... | ... | ... | (1.55 ± 0.29) × 101 | |
| 890 | ... | ... | ... | ... | ... | (1.16 ± 0.35) × 101 | |
| 1158 | ... | ... | ... | ... | ... | (1.02 ± 0.91) × 101 | |
| 1505 | ... | ... | ... | ... | ... | (1.26 ± 1.27) × 101 | |
Notes. Error bars here include uncertainties on foreground and CMB residuals, beam and projection. To obtain the CIB power spectra (given in Table D.2), the power spectra have to be further corrected for 
(Eq. (4)), 
(Eq. (5)), and 
(Eq. (9)). Moreover, the first two points (at ℓ = 53 and 114) have to be considered as upper limits (see Sect. 3.2.3).
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