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Red-giant seismic properties analyzed with CoRoT

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Figure

Fig. 1. Fourier spectrum of a target with a very low mean value of the large separation ( Δν = 0.74 μHz, centered at ν max = 3.45 μHz)
Fig. 3. ν max − Δν relation for red-giant stars in LRa01 and LRc01, with all data satisfying a rejection of the null hypothesis at the 1% level.
Fig. 5. Histogram of Δν , with the red clump signature around 4 μHz.
Table 2. Number of detected peaks.
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