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Table D.1.

Relevant data on testing for the effect of the Andromeda gravitational field on Andromeda dSphs.

Galaxy D host kpc $ \frac {D_{\textrm {host}}}{{\mathrm {kpc}}} $ log 10 ( g host m s 2 ) $ \log _{10}(\frac {g_{\textrm {host}}}{{\mathrm {m\,s}}^{-2}}) $ log 10 ( g N m s 2 ) $ \log _{10}(\frac {g_{\textrm {N}}}{{\mathrm {m\,s}}^{-2}}) $ p
NGC 147 118 −10.70 −10.67±0.12 1.9±2.3
NGC 185 181 −11.07 −10.52±0.12 7±64
NGC 205 46 −9.88 −9.88±0.19 3±31
And I 68 −10.22 −12.06±0.15 1.3±1.8
A. II 195 −11.13 −12.27±0.16 1.9±0.7
A. III 86 −10.42 −12.23±0.18 1.4±1.8
A. V 113 −10.66 −12.43±0.19 2.2±3.0
A. VI 268 −11.41 −11.88±0.16 3.2±2.8
A. VII 217 −11.23 −11.85±0.17 2.4±1.0
A. IX 182 −11.07 −13.42±0.45 2.5±2.8
A. X 92 −10.48 −12.72±0.43 1.4±1.4
A. XI 102 −10.57 −12.80±0.49 2±11
A. XII 181 −11.07 −13.58±0.51 1.8±3.8
A. XIII 115 −10.68 −13.12±0.50 1.8±3.7
A. XIV 161 −10.97 −12.76±0.48 1.8±1.8
A. XV 174 −11.04 −12.11±0.17 1.8±1.7
A. XVI 319 −11.56 −11.76±0.17 2.8±2.8
A. XVII 67 −10.21 −12.47±0.21 1.3±5.0
A. XIX 116 −10.68 −13.84±0.26 1.38±0.76
A. XX 128 −10.77 −12.67±0.45 3±20
A. XXI 135 −10.82 −13.01±0.28 1.50±0.76
A. XXII 275 −11.43 −12.89±0.41 2.0±2.5
A. XXIII 127 −10.76 −12.88±0.24 1.60±0.68
A. XXIV 169 −11.01 −13.14±0.24 1.9±6.3
A. XXV 90 −10.46 −12.85±0.24 1.27±0.87
A. XXVI 103 −10.58 −12.90±0.25 2.0±7.8
A. XXVII 482 −11.92 −13.07±0.40 4.4±8.9
A. XXVIII 384 −11.72 −12.37±0.20 2.5±2.1
A. XXIX 198 −11.15 −12.68±0.18 2.1±1.4
A. XXX 145 −10.88 −12.63±0.17 3±31
A. XXXI 262 −11.39 −12.43±0.32 2.24±0.72
A. XXXII 140 −10.85 −12.31±0.37 1.66±0.73
Cetus 688 −12.23 −12.22±0.16 2.74±0.84
Perseus I 351 −11.65 −12.00±0.45 2.1±4.2
Pisces I 268 −11.41 −12.37±0.14 2.4±5.2

Notes. Columns, from left to right: name of galaxy, distance, Dhost, between Andromeda and galaxy, Andromeda gravitational field, ghost, exerted on galaxy, Newtonian field, gN, of galaxy, p parameter from p-Laplacian inferred from ghost+gN. Dhost and gN taken from Lelli et al. (2017). ghost inferred from Eq. (55). p calculated from Eq. (53).

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