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Table A.1.

Best-fit dipole estimates for different data combinations and cuts. When catalogues are combined, only hypothesis (i) is tested, with results shown in Fig. A.1.

Catalogue(s) S0 N 𝒟 RA Dec.
(mJy) counts/pixel (×10−2) (deg) (deg)
NVSS 20 272,977 7.87 ± 0.02 1.60 ± 0.34 150 ± 13 −25 ± 14
RACS-low 20 346,092 11.14 ± 0.02 1.68 ± 0.27 191 ± 10 9 ± 13
CatWISE 0.09 1,216,501 52.49 ± 0.05 1.56 ± 0.19 141 ± 6 −6 ± 7

NVSSa 15 349,439 10.02 ± 0.02 1.17 ± 0.30 149 ± 14 −9 ± 17
RACS-lowa 15 438,085 14.07 ± 0.02 1.25 ± 0.24 194 ± 12 5 ± 15

β 𝒟resid
(×10−3) (×10−2)

NVSS CatWISE 15 0.078 1,884,811 < 1.85 0.98 ± 0.50 144 ± 6 −11 ± 6
RACS-low CatWISE 15 0.078 1,973,705 1 . 23 1.03 + 0.87 $ 1.23^{+0.87}_{-1.03} $ 0 . 62 0.44 + 0.57 $ 0.62^{+0.57}_{-0.44} $ 152 ± 6 −10 ± 6
NVSS RACS-low CatWISE 20 20 0.09 1,579,687 < 0.90 1 . 47 0.44 + 0.20 $ 1.47_{-0.44}^{+0.20} $ 144 ± 5 −8 ± 6
NVSS RACS-low CatWISEa 15 15 0.078 2,032,858 1.06 ± 0.93 0.84 ± 0.50 145 ± 5 −9 ± 6

Notes. a Excluded sources matched to the 2MRS catalogue at z < 0.1.

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