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Table 4:

Pipeline results for real data: rotation period, mean large separation, frequency-range of the p modes, position of maximum amplitude, and bolometric maximum amplitude per radial mode.

Star
Period (days) $\langle \Delta \nu \rangle$ ($\mu $Hz) $\epsilon$ ($\mu $Hz) $f_{\rm min}$ ($\mu $Hz) $f_{\rm max}$ ($\mu $Hz) $\nu_{\rm max}$ ($\mu $Hz) $\epsilon$ ($\mu $Hz) A $_{\rm max}$ (ppm) $\epsilon$ (ppm)
Sun 27.8 135.46 3.26 2040 4920 3074.7 1.02 2.99 0.13
HD49933 (1) 3.2 86.14 1.58 720 3060 1699.88 1.05 4.08 0.15
HD49933 (2) 3.3 86.33 1.73 720 3000 1804.34 0.28 3.90 0.08
HD181906 2.8 86.53 1.69 1200 2460 1896.9 1.2 2.85 0.13
HD181420 2.6 75.35 1.53 480 2760 1536.26 0.42 3.89 0.1


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