Table G.1.
Asteroseismic frequencies and average measures for the RG in KIC 10001167.
| Quantitya | Value | ||||
|---|---|---|---|---|---|
| Δνps (μHz) | 2.731(13) | ||||
| Δν0 (μHz) | 2.714(17) | ||||
| fΔν b | 0.95863 | ||||
| νmax (μHz) | i. 20.103(366) | ii. 19.784(158) | iii. 19.65(10) | iv. > 19.68(33) | |
| v. 19.93(44) | vi. 19.90(7) | vii. 20.038(127) | viii. 19.70(35) | ||
| ix. 19.68(18) | x. 19.92(45) | ||||
| (n, l)c | A+FAMED | B+FAMED | C+(Arentoft et al. 2017) | A+PBJam | D |
| (3, 2) | 13.1840(274) SN 1.3 | 13.197(61) | |||
| (4, 0) | 13.5806(256) SN 2.7 | 13.627(64) | |||
| (4, 1) | 15.1617(247) SN 6.5 | ||||
| (4, 2) | 15.8455(449) | 15.8256(181) | 15.8403(246) SN 7.5 | 15.834(17) | 15.840(25) |
| (5, 0) | 16.2474(222) | 16.2496(227) | 16.2251(246) SN 7.1 | 16.249(12) | 16.198(28) |
| (5, 1) | 17.6567(603) | 17.6706(451) | 17.6670(242) SN 19.5 | ||
| (5, 2) | 18.4370(491) | 18.4317(509) | 18.4139(243) SN 14.5 | 18.440(16) | 18.444(17) |
| (6, 0) | 18.9109(263) | 18.9087(288) | 18.9093(257) SN 42.1 | 18.912(5) | 18.909(5) |
| (6, 1) | 20.4459(465) | 20.4267(419) | 20.4361(242) SN 25.6 | ||
| (6, 2) | 21.2769(482) | 21.2808(316) | 21.2741(242) SN 25.2 | 21.261(18) | 21.262(15) |
| (7, 0) | 21.6452(285) | 21.6417(267) | 21.6452(241) SN 38.5 | 21.647(10) | 21.647(10) |
| (7, 1) | 23.0965(216) | 23.1025(225) | 23.0943(242) SN 20.9 | ||
| (7, 2) | 24.0602(228) | 24.0665(218) | 24.0683(242) SN 19.7 | 24.058(16) | 24.044(22) |
| (8, 0) | 24.4011(195) | 24.4768(202) | 24.4396(243) SN 17.6 | 24.458(25) | 24.456(32) |
| (8, 1) | 26.0151(228) | 26.0034(183) | |||
| (8, 2) | 26.9052(806) | 27.0274(710) | 26.970(65) | 26.941(85) | |
| (9, 0) | 27.2022(84) | 27.339(51) | 27.342(135) | ||
Notes. Asteroseismic global parameters of the RG in KIC 10001167. The νmax measurements are from the following sources (see Sect. 2.6.1 for descriptions of the first three): i. KEPSEISMIC+FAMED. ii. KASOC+FAMED. iii. KASOC+(Arentoft et al. 2017) method. iv. (Montalbán et al. 2021). v. (Yu et al. 2018). vi. (Gaulme et al. 2016). vii. (Kallinger et al. 2010). viii. (Mosser & Appourchaux 2009). ix. (Hekker et al. 2010). x. (Huber et al. 2009).
Theoretical correction factor to Δν scaling relation according to (Rodrigues et al. 2017, Figure 3) assuming RGB star with [M/H] = -0.38 and M = 0.93M⨀. Interpolated linearly based on nearest grid points on the plot.
Observed asteroseismic frequencies of the RG. See text for details on the different methods. Only showing frequencies detected by at least two pipelines.
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