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Table 1.

Properties and lopsidedness metrics of the satellite distributions from the MATLAS survey.

Centroid Max angle Hemisphere Pairwise MRL
Host RA Dec D N rcover dnorm θmax (2 − N/Nlop)max θlop R ¯ $ \overline{R} $
name (deg) (deg) (Mpc) (kpc) (deg) (deg)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)
IC0598 153.2024 43.1455 35.3 4 320 0.07 140.6 0.667 112.6 0.16
NGC0448 18.8189 −1.6261 29.5 13 268 0.44 113.1 0.917 64.2 0.61
NGC0661 26.0610 28.7060 30.6 12 278 0.28 92.2 0.500 91.8 0.26
NGC0936 36.9061 −1.1563 22.4 18 203 0.07 75.2 0.364 93.7 0.10
NGC1121 42.6634 −1.7340 35.3 15 321 0.16 85.1 0.636 92.1 0.19
NGC1222 47.2364 −2.9552 33.3 19 303 0.37 51.6 0.643 89.3 0.25
NGC2679 132.8872 30.8654 31.1 3 283 0.26 172.9 0.500 120.0 0.30
NGC2685 133.8948 58.7344 16.7 9 123 0.44 120.6 0.714 94.8 0.23
NGC2764 137.0730 21.4434 39.6 4 360 0.40 207.8 1.000 79.7 0.58
NGC2824 139.7593 26.2700 40.7 4 370 0.16 124.2 0.667 114.8 0.11
NGC2859 141.0773 34.5134 27.0 16 246 0.28 48.9 0.545 88.9 0.29
NGC2880 142.3942 62.4906 21.3 9 194 0.20 102.0 0.500 97.8 0.08
NGC2950 145.6463 58.8512 14.5 7 132 0.34 113.8 0.600 100.6 0.17
NGC2974 145.6386 −3.6991 20.9 12 190 0.06 107.3 0.500 96.3 0.08
NGC3032 148.0341 29.2363 21.4 3 195 0.98 337.5 1.000 15.0 0.99
NGC3098 150.5695 24.7111 23.0 6 209 0.12 120.8 0.500 102.3 0.20
NGC3182 154.8876 58.2058 34.0 7 309 0.55 159.7 0.833 74.4 0.51
NGC3230 155.9331 12.5679 40.8 16 371 0.58 114.3 0.857 70.4 0.56
NGC3248 156.9393 22.8472 24.6 5 223 0.59 184.0 1.000 82.2 0.56
NGC3457 163.7026 17.6212 20.1 7 142 0.65 177.2 0.833 69.1 0.62
NGC3522 166.6685 20.0856 25.5 2 231 0.79 287.4 1.000 72.6 0.81
NGC3648 170.6312 39.8770 31.9 11 289 0.09 134.0 0.625 96.7 0.14
NGC3694 172.2256 35.4139 35.2 9 320 0.70 180.4 1.000 62.6 0.64
NGC3941 178.2307 36.9864 11.9 5 108 0.24 171.9 0.750 103.9 0.25
NGC4119 182.0402 10.3787 16.5 1 150 1.00 1.000 1.00
NGC4150 182.6402 30.4015 13.4 8 122 0.50 109.0 0.667 91.6 0.34
NGC4643 190.8339 1.9784 16.5 18 150 0.40 93.9 0.800 79.3 0.44
NGC4697 192.1496 −5.8008 11.4 12 104 0.38 124.4 0.800 81.9 0.43
NGC4753 193.0921 −1.1997 22.9 8 208 0.38 152.1 0.667 89.1 0.36
NGC5493 212.8724 −5.0437 38.8 8 352 0.29 80.0 0.400 98.7 0.16
NGC5582 215.1797 39.6936 27.7 9 204 0.62 148.1 0.875 70.0 0.58
NGC5611 216.0199 33.0475 24.5 8 223 0.38 162.0 0.857 77.7 0.51
NGC5631 216.6387 56.5827 27.0 9 216 0.38 160.9 0.875 87.6 0.38
NGC5866 226.6232 55.7633 14.9 10 136 0.17 130.4 0.571 95.1 0.23
NGC6547 271.2917 25.2326 40.8 6 371 0.39 116.8 0.800 99.0 0.23
NGC7710 353.9423 −2.8809 34.0 7 309 0.59 191.4 1.000 62.4 0.68
PGC028887 149.9313 11.6608 41.0 11 371 0.39 103.8 0.625 91.8 0.11
PGC056772 240.5483 7.0860 39.5 6 358 0.63 159.9 0.800 85.4 0.48
PGC058114 246.5178 2.9066 23.8 3 216 0.78 261.1 1.000 65.9 0.75
PGC061468 272.3607 19.1177 36.2 3 329 0.23 173.6 0.500 120.0 0.31
UGC03960 115.0949 23.2751 33.2 3 281 0.40 149.0 0.500 120.0 0.22
UGC04551 131.0246 49.7940 28.0 11 255 0.72 178.9 0.900 60.5 0.68
UGC05408 150.9661 59.4361 45.8 3 417 0.43 203.9 1.000 104.1 0.47
UGC06062 164.6567 9.0505 38.7 9 351 0.05 106.3 0.500 99.5 0.08
UGC06176 166.8528 21.6572 40.1 3 365 0.73 203.6 1.000 104.3 0.40
UGC08876 209.2419 45.9732 33.9 1 308 1.00 1.000 1.00
UGC09519 221.5880 34.3707 27.6 4 251 0.63 210.1 1.000 79.6 0.61

Notes. We present five of the six lopsidedness metrics for the 47 isolated MATLAS systems. The “wedge” metric is missing because it is a graph for each system rather than a number. Columns: (1) name of ETG, (2,3) coordinates in the J2000 frame, (4) distance to ETG, (5) number of satellites within maximum circle covered by FoV, (6) radius of maximum circle covered by FoV in kpc at the distance of the host, (7) normalized offset between ETG and centroid of 2D satellite distribution, (8) maximum opening angle without a satellite, (9) maximum contrast in satellite distribution from a 180-degree separation line where Nlop is the maximum number of satellites found on one side, (10) mean pairwise angle between the satellites, (11) MRL. Note: empty entries (-) mark systems for which a given angular metric is not applicable because they feature only a single satellite.

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