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Table 8.

Seismic estimates of the surface gravity and stellar masses of the Li-rich giants in the CoRoT fields.

CNAME CoRoT ID log g σlog g Mass M σmassM Num. pipelines
19223053+0138518 100440565 2.35 0.05 1.25 0.14 4
19251759+0053140 100919702 0
19261134+0051569 101064590 2.34 0.07 2.75 1.37 1
19263808+0054441 101130864 2.48 0.02 0.91 0.12 2
19264134+0137595 101139596 2.39 0.07 1.55 0.19 3
19264917–0027469 101160340 1.93 0.06 1.46 0.46 1
19265013+0149070 101162874 0
19265193+0044004 101167637 2.42 0.03 1.20 0.15 4
19270600+0134446 101205220 2.48 0.05 1.74 0.56 1
19270815+0017461 101210895 2.23 0.02 1.29 0.18 1
19273856+0024149 101292381 2.10 0.04 1.54 0.27 3
19274706+0023447 101314825 0
19280508+0100139 101351658 2.30 0.08 3.03 1.60 1
19283226+0033072 101411079 0

Notes. The error in log g takes into account the error in Teff. Moreover, it includes both the standard and systematic errors for the targets for which detection was made by more than one pipeline. For the targets with only one determination, this is only the internal error of the pipeline (and thus it underestimates the uncertainty). The error in the masses also takes into account the error in vmax, which is usually large. Moreover, we remark again that masses based on scaling relations need corrections that depend on the stellar parameters, as discussed in the text, and which were not applied here.

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