Table A.1
Model parameters affecting directly the stellar background, mode linewidth, and mode height.
| Fitter | Mode | Background | Linewidth | Mode | |
| ratio | configuration | configuration | |||
|
|
|||||
| Appourchaux, IAS | 1.0/1.5/0.5/0.0 | One Harvey+white noise | Single per Δν | A | |
| Howe, BIR | 1.0/1.5/0.5/0.2 | Two Harvey+white noise | Single per true order | a | |
| Davies, BIR | Free | One Harvey+white noise | Single per Δν | A | |
| Antia, TAT | Free | One Harvey+white noise | Single per Δν | A | |
| Régulo, IAC | Free | One Harvey + power law+white noise | Single per Δν | A | |
| Campante, BIR | 1.0/1.49/0.5/0.0 | One Harvey+white noise | Single per Δν | B | |
| Benomar, SYD | Free | One Harvey+white noise | Single per Δν | A, B | |
| Handberg, AAU | 1.0/Free/0.5/0.0 | One Harvey+white noise | Single per Δν | A | |
Notes. The first column provides the fitter name. The second column provides the mode height ratio between the l = 0,1,2,3 mode, respectively. The third column provides the model of the stellar background with the mention of the number of components of the modified Harvey model. The fourth column provides how the linewidth is assigned to the modes per order. The last column provides the location of the l = 1 mode with respect to the l = 0 mode: configuration A: l = 0 mode at the left hand side of the l = 1 mode; configuration B: l = 0 mode at the right hand side of the l = 1 mode. Configuration a follows the formal order definition.
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