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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, C, and uncertainty [Jy2 sr-1, νIν = cst]

cent 3000 GHz 857 GHz 545 GHz 353 GHz 217 GHz 143 GHz

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 ... ... ...

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 ... ... ...

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 ... ... ...

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

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

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 = 53 and 114) have to be considered as upper limits (see Sect. 3.2.3).

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