Table 1.
MSCC supercluster properties.
| Name | MSCC-ID | RA, Dec | ⟨z⟩ | Nmem | NCl | Vbox | Vfil/Vbox |
|---|---|---|---|---|---|---|---|
| [deg, deg] | [ Mpc3] |
[%] | |||||
| Corona Borealis | 463 | 232.18, 30.42 | 0.073 | 226 | 14 | 959.2 | 1.1 |
| Leo | 278 | 169.37, 28.34 | 0.033 | 115 | 6 | 459.3 | 1.6 |
| Hercules | 474 | 241.56, 16.22 | 0.036 | 90 | 5 | 343.8 | 0.9 |
Notes. MSCC superclusters properties. We list the superclusters selected for this study (1) names, (2) their MSCC-ID (Chow-Martínez et al. 2014), (3) their coordinates (J2000), (4) the mean redshift, (5) the total number of members, (6) the number of Abell/ACO clusters, (7) the volume of the box containing the SDSS galaxies, and (8) the filling factor of filaments as found in Santiago-Bautista et al. (2020).
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