Table 1.
Data points from the H I spectral stacking analysis used in this work.
| log10(M⋆/M⊙) bin | Median log10(M⋆/M⊙) | Ngal | ⟨log10(MHI/M⊙)⟩ |
|---|---|---|---|
| Combined | |||
| 8.0 < log10(M⋆/M⊙) < 9.5 | 9.10 | 3507 | 9.51 ± 0.05 |
| 9.5 < log10(M⋆/M⊙) < 9.8 | 9.65 | 909 | 9.68 ± 0.06 |
| 9.8 < log10(M⋆/M⊙) < 10.5 | 10.17 | 1564 | 9.94 ± 0.02 |
| log10(M⋆/M⊙) > 10.5 | 10.85 | 636 | 10.07 ± 0.04 |
| MIGHTEE | |||
| 8.0 < log10(M⋆/M⊙) < 9.5 | 9.10 | 2286 | 9.60 ± 0.04 |
| 9.5 < log10(M⋆/M⊙) < 10.5 | 10.06 | 1796 | 9.94 ± 0.02 |
| log10(M⋆/M⊙) > 10.5 | 10.85 | 494 | 10.12 ± 0.03 |
| CHILES | |||
| 8.0 < log10(M⋆/M⊙) < 9.5 | 9.10 | 1221 | 9.55 ± 0.07 |
| 9.5 < log10(M⋆/M⊙) < 10.5 | 10.03 | 767 | 9.82 ± 0.06 |
| log10(M⋆/M⊙) > 10.5 | 10.83 | 142 | 10.13 ± 0.08 |
Notes. Data from the H I spectral stacking analysis from Bianchetti et al. (2025). The first column reports the M⋆ interval underlying each of the measured data point, the second column the corresponding median M⋆, the third column the number of stacked galaxies, and the fourth column the average MHI measured from stacking.
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