Table B.1.
1D marginalised constraints (to 1σ) upon the 1-parameter NLA amplitude AIA for each sample under consideration – each of the points shown in Fig. 6 corresponds to a row here.
| Sample | fred | ⟨z⟩ | ⟨L/Lpiv⟩ | bg | AIA |
|---|---|---|---|---|---|
| G+S: full | 0.54 | – | – | – |  |
| G: full | 0.43 | 0.23 | 0.51 |  |
 |
| S: full | 0.60 | 0.11 | 0.22 |  |
 |
| All blue | 0 | – | – | – |  |
| G: high-M*, blue | 0 | 0.36 | 2.69 |  |
 |
| †G: z > 0.26, blue | 0 | 0.33 | 1.06 |  |
 |
| †G: z < 0.26, blue | 0 | 0.15 | 0.21 |  |
 |
| †S: blue | 0 | 0.09 | 0.14 |  |
 |
| All red | 1 | – | – | – |  |
| G: high-M*, red | 1 | 0.31 | 2.03 |  |
 |
| †G: z > 0.26, red | 1 | 0.33 | 1.47 |  |
 |
| †G: z < 0.26, red | 1 | 0.17 | 0.50 |  |
 |
| †S: red | 1 | 0.12 | 0.29 |  |
 |
Notes. “G” and “S” denote GAMA and SDSS samples, respectively. The independent galaxy samples whose signals constrain the “All blue” or “All red” amplitudes are denoted with †. Samples denoted “high-M*” are selected from GAMA to have stellar masses >1011 M⊙. Also shown are red galaxy fractions fred, mean redshifts and mean luminosities (relative to the pivot Lpiv = 4.6 × 1010 L⊙) per shapes sample, and marginalised galaxy bias fits to corresponding density samples. Rows without these numbers correspond to amplitudes which were fit to multiple wg+ signals from samples with different properties.
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