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Planck 2013 results
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Table D.2

Cosmic IR background power spectra.

Cross-power spectra, Cℓ, and statistical uncertainty [Jy2 sr-1]
ℓ cent 3000 GHz 857 GHz 545 GHz 353 GHz 217 GHz 143 GHz
3000 GHz 187 < 5.69105 (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 ... < 2.76106 < 9.73105 < 2.91105 < 6.43104 < 1.81104
114 ... < 7.99105 < 3.23105 < 1.05105 < 2.49104 < 5.12103
187 ... (2.87 ± 0.37) × 105 (1.30 ± 0.13) × 105 (4.30 ± 0.41) × 104 (9.70 ± 1.22) × 103 (1.84 ± 0.45) × 103
320 ... (1.34 ± 0.08) × 105 (6.36 ± 0.30) × 104 (2.20 ± 0.11) × 104 (5.26 ± 0.53) × 103 (1.06 ± 0.12) × 103
502 ... (7.20 ± 0.26) × 104 (3.53 ± 0.10) × 104 (1.25 ± 0.06) × 104 (3.03 ± 0.32) × 103 (6.52 ± 0.59) × 102
684 ... (4.38 ± 0.18) × 104 (2.21 ± 0.07) × 104 (7.99 ± 0.39) × 103 (1.88 ± 0.22) × 103 (3.86 ± 0.41) × 102
890 ... (3.23 ± 0.09) × 104 (1.63 ± 0.04) × 104 (5.88 ± 0.27) × 103 (1.31 ± 0.16) × 103 (2.55 ± 0.30) × 102
1158 ... (2.40 ± 0.05) × 104 (1.22 ± 0.02) × 104 (4.25 ± 0.17) × 103 (9.18 ± 0.87) × 102 (1.76 ± 0.23) × 102
1505 ... (1.83 ± 0.03) × 104 (9.31 ± 0.11) × 103 (3.24 ± 0.10) × 103 (7.00 ± 0.23) × 102 (1.23 ± 0.16) × 102
1956 ... (1.46 ± 0.02) × 104 (7.38 ± 0.07) × 103 (2.54 ± 0.07) × 103 (5.38 ± 0.12) × 102 (1.03 ± 0.15) × 102
2649 ... (1.16 ± 0.01) × 104 (5.91 ± 0.06) × 103 ... ... ...
545 GHz 53 ... ... < 3.74105 < 1.15105 < 2.58104 < 7.04103
114 ... ... < 1.45105 < 4.84104 < 1.16104 < 2.53103
187 ... ... (6.63 ± 0.51) × 104 (2.22 ± 0.16) × 104 (4.97 ± 0.48) × 103 (1.01 ± 0.19) × 103
320 ... ... (3.34 ± 0.12) × 104 (1.19 ± 0.05) × 104 (2.79 ± 0.21) × 103 (5.98 ± 0.67) × 102
502 ... ... (1.91 ± 0.04) × 104 (6.93 ± 0.23) × 103 (1.65 ± 0.12) × 103 (3.77 ± 0.39) × 102
684 ... ... (1.25 ± 0.03) × 104 (4.61 ± 0.16) × 103 (1.06 ± 0.09) × 103 (2.29 ± 0.27) × 102
890 ... ... (9.17 ± 0.17) × 103 (3.39 ± 0.11) × 103 (7.41 ± 0.63) × 102 (1.54 ± 0.19) × 102
1158 ... ... (6.83 ± 0.10) × 103 (2.50 ± 0.07) × 103 (5.38 ± 0.35) × 102 (1.03 ± 0.14) × 102
1505 ... ... (5.34 ± 0.06) × 103 (1.93 ± 0.04) × 103 (4.30 ± 0.12) × 102 (7.09 ± 1.80) × 101
1956 ... ... (4.24 ± 0.04) × 103 (1.52 ± 0.03) × 103 (3.30 ± 0.07) × 102 (5.89 ± 1.73) × 101
2649 ... ... (3.42 ± 0.04) × 103 ... ... ...
353 GHz 53 ... ... ... < 3.68104 < 8.01103 < 2.05103
114 ... ... ... < 1.66104 < 3.82103 < 8.26102
187 ... ... ... (7.88 ± 0.53) × 103 (1.75 ± 0.15) × 103 (3.61 ± 0.62) × 102
320 ... ... ... (4.35 ± 0.18) × 103 (1.02 ± 0.06) × 103 (2.32 ± 0.24) × 102
502 ... ... ... (2.60 ± 0.10) × 103 (6.21 ± 0.38) × 102 (1.48 ± 0.14) × 102
684 ... ... ... (1.74 ± 0.07) × 103 (3.97 ± 0.27) × 102 (9.42 ± 1.06) × 101
890 ... ... ... (1.29 ± 0.05) × 103 (2.87 ± 0.20) × 102 (6.33 ± 0.83) × 101
1158 ... ... ... (9.35 ± 0.33) × 102 (1.99 ± 0.14) × 102 (4.56 ± 0.91) × 101
1505 ... ... ... (7.45 ± 0.22) × 102 (1.59 ± 0.10) × 102 (2.77 ± 1.11) × 101
1956 ... ... ... (6.08 ± 0.16) × 102 (1.35 ± 0.05) × 102 (3.53 ± 0.69) × 101
217 GHz 53 ... ... ... ... < 1.78103 < 4.74102
114 ... ... ... ... < 8.47102 < 1.89102
187 ... ... ... ... (4.17 ± 0.47) × 102 (1.04 ± 0.19) × 102
320 ... ... ... ... (2.62 ± 0.20) × 102 (7.49 ± 0.81) × 101
502 ... ... ... ... (1.75 ± 0.13) × 102 (5.87 ± 0.58) × 101
684 ... ... ... ... (1.17 ± 0.10) × 102 (3.93 ± 0.50) × 101
890 ... ... ... ... (8.82 ± 0.89) × 101 (2.64 ± 0.52) × 101
1158 ... ... ... ... (6.42 ± 1.61) × 101 (2.21 ± 1.19) × 101
1505 ... ... ... ... (3.34 ± 2.15) × 101 (1.07 ± 1.65) × 101
1956 ... ... ... ... (4.74 ± 0.65) × 101 (1.45 ± 0.54) × 101
143 GHz 53 ... ... ... ... ... < 1.55102
114 ... ... ... ... ... < 6.41101
187 ... ... ... ... ... (3.64 ± 0.73) × 101
320 ... ... ... ... ... (3.23 ± 0.35) × 101
502 ... ... ... ... ... (2.81 ± 0.30) × 101
684 ... ... ... ... ... (2.27 ± 0.29) × 101
890 ... ... ... ... ... (1.84 ± 0.35) × 101
1158 ... ... ... ... ... (1.58 ± 0.91) × 101
1505 ... ... ... ... ... (1.25 ± 1.28) × 101

Notes. These estimates are obtained from the CMB- and dust-free map power spectra (Table D.1), which have been corrected for SZ contaminations (Eqs. (5) and (9)), and for the spurious CIB contamination induced by our CMB template (Eq. (4)), computed using our best-fit model described in Sect. 5.5). The errors contain all the terms: statistical uncertainty; beam uncertainty; and errors from the SZ correction. Rows composed of entirely empty values have been omitted.

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