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Home All issues Volume 506 / No 1 (October IV 2009) A&A, 506 1 (2009) 15-32 Full HTML
   

Table 2:

Priors used for the analysis of the simulated spectra for the inclination angle i, the rotational splitting $\nu _{\rm s}$, the large separation $\Delta \nu $ (Eq. (2)) and the small separation $\langle \delta\nu_{02}\rangle_{\rm th}$ (Eq. (15)).
  i $\nu _{\rm s}$ $\Delta \nu $ $\langle \delta\nu_{02}\rangle_{\rm th}$
1 [0-90] $2 \pm 0.2$ $90.2 \pm 0.5$ $8 \pm 4$
2 [0-90] $2 \pm 0.2$ $89.9 \pm 0.6$ $8 \pm 4$
3 [0-90] $3.5 \pm 0.35$ $90.2 \pm 0.6$ $8 \pm 4$
4 [0-90] $3.5 \pm 0.35$ $90.0 \pm 0.3$ $5 \pm 2.5$
5 [0-90] $3.5 \pm 0.35$ $90.0 \pm 0.4$ $6 \pm 3$
6 [0-90] $3.5 \pm 0.35$ $90.1 \pm 0.5$ $6 \pm 3$
The prior on i is uniform and Gaussian for the other parameters (with the indicated $\sigma $ width).
Priors on mode frequencies are also Gaussian with a 6 $\mu$Hz width.

Source LaTeX | All tables | In the text

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