Table B.1
Galaxy groups identified in the 2M++ catalogue (Lavaux & Hudson 2011).
Id | Ng | RA | Dec | vcm | σv | Rvir | ℳvir |
[deg] | [deg] | [km s-1] | [km s-1] | [Mpc h-1] | [1014 ℳ⊙ ⟨ − ∞] | ||
|
|||||||
1 | 4 | 324.127 | –83.894 | 18002.965 | 224.195 | 1.250 | 0.4383 |
2 | 4 | 5.229 | –81.026 | 16871.429 | 213.153 | 1.464 | 0.4640 |
3 | 4 | 337.707 | –80.216 | 11734.202 | 187.328 | 1.208 | 0.2956 |
4 | 6 | 336.104 | –80.243 | 11217.477 | 223.655 | 0.515 | 0.1796 |
5 | 5 | 253.364 | –79.943 | 12761.345 | 271.959 | 1.104 | 0.5697 |
6 | 10 | 278.508 | –77.019 | 5597.198 | 84.888 | 0.922 | 0.0463 |
7 | 4 | 74.464 | –74.851 | 5806.220 | 193.855 | 0.598 | 0.1568 |
8 | 5 | 101.298 | –74.279 | 6377.974 | 200.810 | 0.383 | 0.1076 |
9 | 4 | 94.245 | –74.193 | 11696.234 | 76.082 | 0.751 | 0.0303 |
10 | 7 | 101.903 | –71.665 | 4281.469 | 80.630 | 0.730 | 0.0331 |
11 | 9 | 304.395 | –70.813 | 3710.980 | 223.876 | 0.115 | 0.0403 |
12 | 4 | 285.085 | –69.761 | 14098.694 | 193.275 | 1.368 | 0.3565 |
13 | 4 | 93.125 | –67.870 | 10871.720 | 89.479 | 0.890 | 0.0497 |
14 | 4 | 339.991 | –66.724 | 12378.471 | 283.765 | 0.441 | 0.2479 |
15 | 7 | 92.323 | –65.670 | 10952.375 | 254.096 | 0.893 | 0.4020 |
16 | 4 | 103.901 | –65.527 | 8988.492 | 135.257 | 0.495 | 0.0631 |
17 | 5 | 94.878 | –65.094 | 8748.338 | 119.096 | 1.161 | 0.1149 |
18 | 4 | 341.554 | –65.201 | 3389.487 | 139.634 | 0.429 | 0.0584 |
19 | 24 | 95.603 | –64.903 | 7729.567 | 439.018 | 0.688 | 0.9251 |
20 | 5 | 101.649 | –64.124 | 3485.746 | 66.548 | 0.554 | 0.0171 |
Notes. Group ID, Number of galaxies linked by the FoF algorithm, RA: group centre right ascension (J2000), Dec: group centre declination (J2000), vcm: mean group radial velocity, σv: radial velocity dispersion, Rvir: 3D virial radius, ℳvir: group virial mass. Groups in this table were identified using a FoF algorithm with a contour overdensity contrast of 433, and having four or more members, mean group radial velocities greater than 3000 km s-1, and virial masses greater than 1012ℳ⊙h-1. The complete table can be found at the CDS.
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