The kinematic contribution to the cosmic number count dipole

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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	ℳ	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

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

			β	𝒟_resid
			(×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 CatWISE^a	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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