Table C.2.
Model fit parameters for stacked [O III] profiles in the low redshift sample
| Luminosity | Groups | N | Anarrow | FWHMnarrow | vnarrow | Abroad | FWHMbroad | vbroad | FWHMavg |
|---|---|---|---|---|---|---|---|---|---|
| [×10−17] | [×10−17] | ||||||||
| Controlling L1.4GHz | |||||||||
| 1023 − 1024 W Hz−1 | PS | 77 | 5.9±0.1 | 551±11 | 0±4 | - | - | - | 551±11 |
| NPS | 36 | 11.1±0.1 | 517±7 | 0±2 | - | - | - | 517±7 | |
| 1024 − 1025 W Hz−1 | PS | 107 | 3.0±0.1 | 469±8 | 17±2 | 0.9±0.1 | 1338±51 | 0±12 | 667±34 |
| NPS | 91 | 5.3±0.1 | 441±4 | 0±1 | 0.7±0.1 | 1179±58 | 0±12 | 448±38 | |
| 1025 − 1026 W Hz−1 | PS | 14 | 3.0±0.1 | 509±18 | 0±5 | 0.8±0.1 | 1639±132 | 0±36 | 805±88 |
| NPS | 61 | 6.9±0.1 | 384±4 | 1±1 | 1.7±0.1 | 1091±36 | 0±8 | 503±25 | |
| Controlling L[O III] | |||||||||
| 1039 − 1040 erg s−1 | PS | 22 | 7.4±0.2 | 433±13 | 5±5 | - | - | - | 433±13 |
| NPS | 9 | 5.4±0.2 | 459±16 | 0±6 | - | - | - | 459±16 | |
| 1040 − 1041 erg s−1 | PS | 143 | 2.2±0.1 | 488±16 | 0±4 | 0.5±0.01 | 1353±126 | 0±33 | 603±81 |
| NPS | 112 | 2.1±0.1 | 401±11 | 0±2 | 0.7±0.1 | 981±61 | 22±12 | 493±40 | |
| 1041 − 1042 erg s−1 | PS | 47 | 5.1±0.1 | 479±8 | 16±2 | 1.5±0.1 | 1434±46 | 0±13 | 718±29 |
| NPS | 73 | 10.5±0.1 | 417±3 | 0±0 | 1.8±0.1 | 1202±35 | 0±9 | 486±23 | |
| Spectral shape | |||||||||
| 1024 − 1026 W Hz−1 | HFPS | 54 | 2.3±0.1 | 470±11 | 17±3 | 0.7±0.1 | 1642±69 | 0±22 | 876±45 |
| LFPS | 67 | 3.6±0.1 | 483±9 | 11±2 | 0.9±0.1 | 1333±58 | 0±15 | 615±36 | |
| NPS | 152 | 6.0±0.1 | 414±3 | 0±0 | 1.1±0.1 | 1145±34 | 0±8 | 473±23 |
Note. Best-fit model parameters for the stacked [O III] profiles discussed in Sect. 4.4 and 4.5. The ‘Luminosity’ column lists the luminosity range of the stacked bins, and the spectral shape is listed under ‘Groups’. Column ’N’ lists the number of sources in each group. The ‘Anarrow’ and ‘Abroad’ columns list the amplitudes in erg s−1 cm−2 Å−1, ‘FWHMnarrow’ and ‘FWHMbroad’ columns list the full width at half maximums in km s−1 and, ‘vnarrow’ and ‘vbroad’ list the velocity offsets in km s−1 of the Gaussian components in the best-fit model. ‘FWHMavg’ lists the flux-weighted average FWHM of the stacked profile in km s−1.
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