Table A.1.
All relevant quantities for the dSphs and galaxy clusters.
| Galaxy |  |
 |
 |
 |
p |  |
|---|---|---|---|---|---|---|
| Carina | 5.57(20) | 273(45) | -12.15(27) | -10.81(18) | 3.51(59) | 7.6±5.5 |
| Draco | 5.45(8) | 244(9) | -12.18(14) | -10.48(12) | 5.04(90) | 8.1±2.7 |
| Fornax | 7.31(12) | 792(58) | -11.35(17) | -10.77(8) | 2.68(26) | 17.2±7.4 |
| Leo I | 6.74(12) | 298(29) | -11.06(18) | -10.56(6) | 2.78(33) | 87±41 |
| Leo II | 5.87(12) | 219(52) | -11.67(26) | -10.71(14) | 3.22(51) | 30±24 |
| Sculptor | 6.36(20) | 311(46) | -11.48(26) | -10.58(13) | 3.37(61) | 32±22 |
| Sextans | 5.64(20) | 748(66) | -12.96(24) | -11.09(15) | 3.59(39) | 0.44±0.26 |
| Bootes I | 4.29(8) | 283(7) | -13.47(14) | -11.14(15)⋆ | 3.91(38) | 0.36±0.12 |
| Canes V. I | 5.08(8) | 647(27) | -13.40(14) | -11.06(5) | 4.05(18) | 0.186±0.062 |
| Canes V. II | 4.10(8) | 101(5) | -12.76(14) | -10.69(19) | 4.69(93) | 5.1±1.8 |
| Coma B. | 3.46(24) | 79(6) | -13.19(27) | -10.59(16) | 5.9(12) | 2.5±1.6 |
| Hydra II | 3.87(12) | 88(17) | -12.88(28)⋆ | -10.65(87)⋆ | 5.1(49) | 4.6±3.1 |
| Leo IV | 3.91(8) | 149(47) | -13.30(30) | -11.15(47) | 3.8(11) | 1.0±1.0) |
| Leo T | 5.57(7) | 160(10) | -11.70(14) | -10.47(19) | 4.2(12) | 38±13 |
| Segue II | 2.94(12) | 43(6) | -13.17(20) | -10.81(87) | 4.7(36) | 4.6±2.6 |
| NGC 147 | 7.84(4) | 672(23) | -10.67(12) | -10.43(6) | 2.47(29) | 96±27 |
| NGC 185 | 7.84(4) | 565(7) | -10.52(12) | -10.00(4) | 8.6(42) | 161±43 |
| NGC 205 | 8.52(4) | 594(107) | -9.88(19) | -9.70(15) | 1.18(87) | 660±400 |
| And II | 6.85(8) | 1355(142) | -12.27(16) | -11.21(11) | 2.82(20) | 1.19±0.53 |
| And V | 5.55(8) | 365(57) | -12.43(19) | -10.53(11) | 5.12(81) | 3.1±1.7 |
| And VI | 6.44(8) | 537(54) | -11.88(16) | -10.55(11) ⋆ | 4.11(60) | 7.5±3.2 |
| And VII | 6.98(12) | 965(52) | -11.85(17) | -10.77(7) | 3.27(27) | 4.5±1.8 |
| And IX | 4.97(44) | 582(23) | -13.42(45) | -10.70(17)⋆ | 5.5(11) | 0.20±0.21 |
| And X | 5.13(40) | 312(41) | -12.72(43) | -11.32(27) | 3.00(49) | 1.9±1.9 |
| And XIV | 5.37(20) | 434(212) | -12.76(48) | -11.20(29)⋆ | 3.22(63) | 1.2±1.9 |
| And XV | 5.69(12) | 294(12) | -12.11(17) | -11.28(31) | 2.61(39) | 8.1±3.2 |
| And XVI | 5.53(12) | 164(9) | -11.76(17) | -10.70(17)⋆ | 3.36(56) | 32±13 |
| And XVII | 5.34(16) | 299(31) | -12.47(21) | -10.86(44)⋆ | 3.7(13) | 3.4±1.9 |
| And XXIII | 6.00(20) | 1034(97) | -12.88(24) | -11.32(13) | 3.11(26) | 0.38±23 |
| And XXIV | 5.32(20) | 633(52) | -13.14(24) | -11.09(87)⋆ | 3.8(21) | 0.35±0.20 |
| And XXVIII | 5.39(16) | 285(12) | -12.37(20) | -11.09(29) | 3.09(55) | 4.4±2.1 |
| And XXIX | 5.33(12) | 377(30) | -12.68(18) | -11.08(19) | 3.38(42) | 1.67±0.74 |
| And XXXI | 6.61(28) | 1231(132) | -12.43(32)⋆ | -11.08(9) | 3.16(32) | 0.91±0.70 |
| Cetus | 6.44(8) | 791(75) | -12.22(16) | -11.07(11) | 3.00(24) | 2.33±0.98 |
| Perseus I | 6.04(28) | 391(143) | -12.00(45)⋆ | -11.36(88)⋆ | 2.44(94) | 8±10 |
Notes. Above the horizontal line are Milky Way satellites; below it are Andromeda satellites. The columns are, from left to right: the name of the galaxy, the V-band-luminosity, LV, the half-light-radius, r1/2, the Newtonian acceleration, gN, observationally deduced acceleration, a, the p parameter from p-Laplacian p (Eq. (1)), and the mean density, 
. The first four quantities were adopted from Lelli et al. (2017) and p and 
were calculated from them.
The uncertainty deviates from the data by Lelli et al. (2017), because it has been symmetrized.
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