Dynamics of DiskMass Survey galaxies in refracted gravity

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Volume 637 (May 2020)

A&A, 637 (2020) A70

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Table 5.

Correlations of the RAR residuals of RG models, QUMOND models, and DMS data with the galaxy properties.

Galaxy	RG				QUMOND				DMS

property	τ	−log₁₀p_τ	ρ	−log₁₀p_ρ	τ	−log₁₀p_τ	ρ	−log₁₀p_ρ	τ	−log₁₀p_τ	ρ	−log₁₀p_ρ
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)	(11)	(12)	(13)
h_R [kpc]	−0.030	2.62	−0.038	1.96	−0.065	9.85	−0.094	9.72	−0.042	0.68	−0.060	0.66
	+0.0083	0.39	+0.0052	0.14	+0.049	5.92	+0.073	6.10	−0.099	2.55	−0.15	2.64
M_bar [M_⊙]	−0.16	56.6	−0.23	54.4	−0.053	6.77	−0.074	6.26	−0.27	15.7	−0.38	15.2
R_e [kpc]	+0.046	5.14	+0.061	4.18	−0.094	19.0	−0.14	20.3	+0.0020	0.022	−0.012	0.086
	−0.10	22.6	−0.15	23.6	−0.00023	0.0088	+0.011	0.31	−0.15	5.21	−0.23	5.41
F_gas	+0.33	237	+0.48	256	−0.11	29.0	−0.17	31.6	+0.21	9.82	+0.31	10.1
R [kpc]	−0.41	377	−0.59	419	+0.15	53.9	+0.27	76.1	−0.16	6.10	−0.21	4.89
	+0.41	368	+0.57	395	−0.17	62.6	−0.28	84.5	+0.033	0.49	+0.041	0.40
f_gas(R)	+0.073	12.9	+0.12	16.6	+0.14	42.0	+0.20	43.2	+0.16	6.10	+0.24	6.12

Notes. Column 1: name of the galaxy property; Cols. 2–5: correlations of the RAR residuals of RG models with the galaxy properties; Cols. 6–9: correlations of the RAR residuals of QUMOND models with the galaxy properties; Cols. 10–13: correlations of the RAR residuals of DMS data with the galaxy properties. τ and ρ are the Kendall and Spearman correlation coefficients, respectively; p_τ and p_ρ the corresponding significance levels of the lack of correlation.

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