Open Access
Table 9.
Best-fit double Schechter function parameters for the mass functions of grouped galaxies in filaments for different subsamples and for grouped galaxies outside of filaments, as indicated.
| Galaxy sample | log M⋆ | α1 | α2 |
|---|---|---|---|
 |
|||
| BO = 1 and Nlinks > 2 (backbone centres) | 10.84 ± 0.02 | –0.62 ± 0.08 | –0.62 ± 0.34 |
| BO > 1 and Nlinks > 2 (outskirts centres) | 10.82 ± 0.03 | –0.57 ± 0.13 | –0.57 ± 0.30 |
| BO = 1 and Nlinks = 2 (backbone intermediates) | 10.87 ± 0.02 | –0.71 ± 0.04 | –1.82 ± 0.38 |
| BO > 1 and Nlinks = 2 (outskirts intermediates) | 10.96 ± 0.03 | –0.85 ± 0.05 | –0.85 ± 0.27 |
| BO = 1 and Nlinks = 1 (backbone edges) | 10.80 ± 0.03 | –0.57 ± 0.10 | –1.36 ± 0.21 |
| BO > 1 and Nlinks = 1 (outskirts edges) | 10.79 ± 0.03 | –0.55 ± 0.09 | –1.79 ± 0.66 |
| Grouped galaxies outside of filaments (G2) | 10.70 ± 0.04 | –0.57 ± 0.25 | –1.24 ± 0.11 |
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.