Open Access
Table B.1.
Output of our f(J) model for the 25 early-type galaxies analysed in this work.
Name | log M⋆/M⊙ | log Mh/M⊙ | c |
---|---|---|---|
NGC 720 | 11.27 ± 0.13 | 12.85 ± 0.32 | 7.1 ± 2.0 |
NGC 821 | 11.00 ± 0.13 | 13.00 ± 0.43 | 6.5 ± 1.8 |
NGC 1023 | 10.99 ± 0.12 | 12.98 ± 0.65 | 5.9 ± 1.8 |
NGC 1400 | 11.08 ± 0.13 | 12.71 ± 0.35 | 4.6 ± 1.3 |
NGC 1407 | 11.60 ± 0.13 | 13.70 ± 0.31 | 3.9 ± 1.0 |
NGC 2768 | 11.21 ± 0.13 | 12.60 ± 0.39 | 8.2 ± 2.5 |
NGC 2974 | 10.93 ± 0.12 | 12.71 ± 0.30 | 4.7 ± 1.1 |
NGC 3115 | 10.93 ± 0.14 | 13.01 ± 0.62 | 6.5 ± 2.1 |
NGC 3377 | 10.50 ± 0.13 | 12.22 ± 0.34 | 7.3 ± 1.9 |
NGC 3607 | 11.39 ± 0.12 | 13.08 ± 0.37 | 4.1 ± 1.1 |
NGC 3608 | 11.03 ± 0.12 | 13.15 ± 0.55 | 5.8 ± 1.6 |
NGC 4278 | 10.95 ± 0.13 | 13.40 ± 0.50 | 6.0 ± 1.7 |
NGC 4365 | 11.51 ± 0.13 | 13.84 ± 0.43 | 4.6 ± 1.2 |
NGC 4374 | 11.51 ± 0.14 | 13.69 ± 0.57 | 9.0 ± 2.8 |
NGC 4459 | 10.98 ± 0.11 | 12.82 ± 0.42 | 5.2 ± 1.4 |
NGC 4473 | 10.96 ± 0.12 | 12.88 ± 0.51 | 5.5 ± 1.7 |
NGC 4486 | 11.62 ± 0.14 | 13.75 ± 0.24 | 9.7 ± 1.8 |
NGC 4494 | 11.02 ± 0.12 | 12.35 ± 0.46 | 4.4 ± 1.3 |
NGC 4526 | 11.26 ± 0.13 | 13.16 ± 0.48 | 4.9 ± 1.2 |
NGC 4564 | 10.58 ± 0.12 | 12.88 ± 0.78 | 5.3 ± 2.0 |
NGC 4649 | 11.60 ± 0.13 | 13.76 ± 0.43 | 5.3 ± 1.4 |
NGC 4697 | 11.15 ± 0.12 | 13.17 ± 0.54 | 5.4 ± 1.6 |
NGC 5846 | 11.46 ± 0.13 | 13.85 ± 0.45 | 4.6 ± 1.1 |
NGC 5866 | 10.83 ± 0.13 | 12.06 ± 0.66 | 11.2 ± 5.5 |
NGC 7457 | 10.13 ± 0.24 | 12.02 ± 0.47 | 7.1 ± 2.3 |
Notes. The table provides estimates of the stellar mass (M⋆), the halo mass (Mh), and the halo concentration (c) together with their 1-σ uncertainties.
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.