Bayesian peak bagging analysis of 19 low-mass low-luminosity red giants observed with Kepler

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Volume 579 (July 2015)

A&A, 579 (2015) A83

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This article has an erratum: [https://doi.org/10.1051/0004-6361/201525895e]

Table 1

Literature values for Δν, mass, ΔΠ₁, and q used for the mode identification of the stars.


KIC ID	Δν	Mass	ΔΠ₁	q
	(μHz)	(M_⊙)	(s)


03744043	9.90	1.3	75.98	0.16
06117517	10.16	1.3	76.91	0.14
06144777^a	11.01	1.1	69.91	0.22
07060732^a	10.94	1.3	72.78	0.18
07619745	13.13	1.5	79.17	0.15
08366239^a	13.70	1.9	86.77	0.17
08475025^a^,^b	9.66	1.4	74.80	0.13
08718745	11.40	1.1	79.45	0.11
09145955	11.00	1.4	77.01	0.16
09267654^a^,^b	10.34	1.3	78.41	0.13
09475697	9.88	1.5	75.70	0.12
09882316	13.68	1.6	80.59	0.15
10123207	13.67	1.0	83.88	0.17
10200377	12.47	1.1	81.58	0.16
10257278	12.20	1.4	79.81	0.18
11353313^a^,^b	10.76	1.5	76.00	0.14
11913545	10.18	1.3	77.84	0.12
11968334	11.41	1.4	78.10	0.13
12008916^a	12.90	1.3	80.47	0.14

Notes. All the values are available from Mosser et al. (2012c).

^(a)

Stars for which an auxiliary fit for (ΔΠ₁, q) was required.

^(b)

Stars with a large rotational splitting, of the same magnitude of the frequency spacing between adjacent mixed modes. A careful mode identification of the split components was required for this case.

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