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Table A.1.

Measurements of the cosmic radio dipole in terms of the NVSS from the literature.

Survey ν Reference Estimator S N RA Dec d
(MHz) (mJy) (deg) (deg) ( × 10−2)
NVSS 1400 BW 1 ≤ l ≤ 3 S > 10 431 990 132 ± 29 65 ± 19 0.5 ± 0.2
BW 1 ≤ l ≤ 3 S > 15 311 037 148 ± 29 31 ± 31 0.8 ± 0.3
BW 1 ≤ l ≤ 3 S > 25 242 710 153 ± 27 −3 ± 29 1.1 ± 0.3
BW 1 ≤ l ≤ 3 S > 25 197 998 158 ± 30 −4 ± 34 1.1 ± 0.3
BW 1 ≤ l ≤ 3 S > 30 166 694 156 ± 32 2 ± 33 1.1 ± 0.4
BW 1 ≤ l ≤ 3 S > 35 143 524 161 ± 44 −27 ± 39 0.9 ± 0.4
BW 1 ≤ l ≤ 3 S > 40 125 603 149 ± 49 −45 ± 38 0.7 ± 0.5
S11 Source counts S ≥ 15 298 048 149 ± 9 15 ± 9 1.3 ± 0.2
S11 Source counts S ≥ 20 229 365 158 ± 10 2 ± 10 1.4 ± 0.3
S11 Source counts S ≥ 25 185 474 158 ± 11 −2 ± 10 1.4 ± 0.3
S11 Source counts S ≥ 30 154 996 156 ± 11 −2 ± 10 1.6 ± 0.3
S11 Source counts S ≥ 35 132 930 157 ± 11 −12 ± 11 1.5 ± 0.3
S11 Source counts S ≥ 40 115 837 158 ± 12 −19 ± 12 1.4 ± 0.4
S11 Source counts S ≥ 50 91 957 171 ± 13 −18 ± 14 1.7 ± 0.4
S11 Sky brightness 15 ≤ S < 1000 296 811 157 ± 9 −3 ± 8 2.0 ± 0.5
S11 Sky brightness 20 ≤ S < 1000 228 128 158 ± 10 −6 ± 9 2.1 ± 0.5
S11 Sky brightness 25 ≤ S < 1000 184 237 159 ± 10 −7 ± 9 2.2 ± 0.6
S11 Sky brightness 30 ≤ S < 1000 153 759 159 ± 11 −7 ± 10 2.2 ± 0.6
S11 Sky brightness 35 ≤ S < 1000 131 691 159 ± 11 −10 ± 10 2.2 ± 0.6
S11 Sky brightness 40 ≤ S < 1000 114 600 159 ± 12 −11 ± 11 2.2 ± 0.6
S11 Sky brightness 50 ≤ S < 1000 90 360 163 ± 12 −11 ± 11 2.3 ± 0.7
RS Linear 3D S > 15 298 289 149 ± 18 −17 ± 18 1.6 ± 0.5
RS Linear 3D S > 20 229 557 153 ± 18 2 ± 18 1.8 ± 0.6
RS Linear 3D S > 25 185 649 158 ± 19 −2 ± 19 1.8 ± 0.6
RS Linear 3D S > 30 155 120 156 ± 19 −2 ± 19 1.9 ± 0.7
RS Linear 3D S > 35 133 022 156 ± 22 −11 ± 22 1.9 ± 0.7
RS Linear 3D S > 40 115 917 158 ± 26 −18 ± 26 1.7 ± 0.8
RS Linear 3D S > 50 91 662 170 ± 23 −17 ± 23 2.0 ± 0.8
RS Linear 2DCG S > 10 447 459 133 ± 14 – 1.5 ± 0.4
RS Linear 2DCG S > 15 313 724 148 ± 14 – 1.5 ± 0.4
RS Linear 2DCG S > 20 241, 399 150 ± 14 – 1.8 ± 0.5
RS Linear 2DCG S > 25 192 245 155 ± 14 – 1.9 ± 0.5
RS Linear 2DCG S > 30 163 208 153 ± 15 – 2.0 ± 0.6
RS Linear 2DCG S > 35 139 851 152 ± 17 – 1.9 ± 0.6
RS Linear 2DCG S > 40 121 831 146 ± 20 – 1.8 ± 0.7
RS Linear 2DCG S > 50 96 337 171 ± 19 – 1.9 ± 0.7
B18 Hemispheres 20 < S < 1000 253 313 148 ± 11 −17 ± 3 2.3 ± 0.4
GH 15 211 487 117 ± 20 6 ± 14 2.7 ± 0.5
TN16 C1 15 < S < 1000 151 −6 0.9 ± 0.4
TN16 C1 20 < S < 1000 151 −14 1.2 ± 0.5
TN16 C1 30 < S < 1000 160 −16 1.3 ± 0.6
TN16 C1 40 < S < 1000 150 −35 1.4 ± 0.7
TN16 C1 50 < S < 1000 174 −36 1.7 ± 0.8

References. BW: Blake & Wall (2002); S11: Singal (2011); RS: Rubart & Schwarz (2013); B18: Bengaly et al. (2018); GH: Gibelyou & Huterer (2012); TN16: Tiwari & Nusser (2016).

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