Non-radial oscillations in the red giant HR 7349 measured by CoRoT

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Table 1:

Frequency and amplitude of identified modes.
Degree	Frequency	Mode height	S/N	Amplitude
$\ell$	$\mu$ Hz	ppm² * 1000/ $\mu$ Hz		ppm
0	20.94 (7)	7.8	10.8	79 $\pm$ 15
0	24.20 (7)	10.0	17.6	89 $\pm$ 15
0	27.65 (6)	11.3	24.8	94 $\pm$ 16
0	31.08 (6)	9.0	23.7	84 $\pm$ 14
0	34.59 (7)	4.6	14.0	60 $\pm$ 11
0	38.17 (9)	1.6	5.6	35 $\pm$ 8
1	19.16 (7)	5.3	6.2	65 $\pm$ 14
1	22.59 (7)	5.5	8.6	66 $\pm$ 13
1	25.94 (5)	16.8	33.1	115 $\pm$ 19
1	29.45 (5)	16.0	38.8	112 $\pm$ 18
1	32.88 (5)	9.1	26.0	85 $\pm$ 14
1	36.41 (6)	4.4	14.6	59 $\pm$ 11
1	39.93 (6)	2.3	8.8	43 $\pm$ 9
2	20.19 (8)	6.5	8.4	71 $\pm$ 14
2	23.58 (7)	6.5	10.9	71 $\pm$ 13
2	26.88 (7)	6.5	13.7	72 $\pm$ 13
2	30.48 (6)	9.5	24.1	86 $\pm$ 15
2	33.91 (8)	2.3	7.0	43 $\pm$ 9
2	37.68 (8)	2.1	7.3	41 $\pm$ 8

Notes. The uncertainties in the last given digit of the frequencies are noted in parentheses. For the S/N estimates (see Barban et al. 2007), the signal is taken to be the height of the fitted Lorentzian profile and the noise is determined according to the procedure described in Sect. 4.1.

Source LaTeX | All tables | In the text

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