Advancing the accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary

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Volume 699 (July 2025)

A&A, 699 (2025) A152

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Table G.2.

Asteroseismic and dynamical measurements of the RG in KIC 10001167.

Quantity^a	Value
Mass_dyn (M_⊙)	0.9337(77)
Mass_{sis,CLÉS,l = 0 (PBJam)} (M_⊙)	0.947(15)
Mass_{sis,CLÉS,l = 0 (FAMED)} (M_⊙)	0.954(42)
Mass_{sis, MESA, l = 0(PBJam)} (M_⊙)	0.948(15)
Mass_{sis, MESA, l = 0, 2(PBJam)} (M_⊙)	0.947(13)
Mass_{sis, MESA, l = 0, 2(PBJam),Y = free} (M_⊙)	0.956(29)
Mass_{sis, scaling} (M_⊙)^b	1.149(46)
Mass_{sis, scaling, corr} (M_⊙)^b	0.970(39)

Radius_dyn (R_⊙)	13.03(12)
Radius_{sis,CLÉS,l = 0 (PBJam)} (R_⊙)	12.748(68)
Radius_{sis,CLÉS,l = 0 (FAMED)} (R_⊙)	12.77(21)
Radius_{sis, MESA, l = 0(PBJam)} (R_⊙)	12.793(75)
Radius_{sis, MESA, l = 0, 2(PBJam)} (R_⊙)	12.803(66)
Radius_{sis, MESA, l = 0, 2(PBJam),Y = free} (R_⊙)	12.85(15)
Radius_{sis, scaling} (R_⊙)^b	14.16(23)
Radius_{sis, scaling, corr} (R_⊙)^b	13.01(21)

ρ_dyn (10⁻³ρ_⊙)	0.422(11)
ρ_{sis,CLÉS,l = 0(PBJam)} (10⁻³ρ_⊙)	0.45733(92)
ρ_{sis,CLÉS,l = 0(FAMED)} (10⁻³ρ_⊙)	0.4569(29)
ρ_{sis, MESA, l = 0(PBJam)} (10⁻³ρ_⊙)	0.4521(46)
ρ_{sis, MESA, l = 0, 2(PBJam)} (10⁻³ρ_⊙)	0.4508(36)
ρ_{sis, MESA, l = 0, 2(PBJam),Y = free} (10⁻³ρ_⊙)	0.4507(42)
ρ_{sis, scaling} (10⁻³ρ_⊙)^b	0.4048(51)
ρ_{sis, scaling, corr} (10⁻³ρ_⊙)^b	0.4405(55)

log g_dyn (dex)	2.1786(78)
log g_{sis,CLÉS,l = 0(PBJam)} (dex)	2.2037(22)
log g_{sis,CLÉS,l = 0(FAMED)} (dex)	2.2040(52)
log g_{sis,MESA,l = 0 (PBJam)} (dex)	2.2005(40)
log g_{sis,MESA,l = 0,2 (PBJam)} (dex)	2.1996(32)
log g_{sis,MESA,l = 0,2 (PBJam), Y=free} (dex)	2.2008(41)
log g_sis,scaling (dex) ^b	2.1963(45)
log g_{sis,scaling,corr} (dex) ^b	2.1963(45)

age_{dyn, MESA, FIES} (Gyr)	9.95 (70)
age_{dyn, CLÉS, FIES} (Gyr)	10.33 (48)
age_{dyn, CLÉS, DR17} (Gyr)	10.16 (47)
age_{sis, CLÉS, l = 0 (PBJam)} (Gyr)	9.68 (64)
age_{sis, CLÉS, l = 0 (FAMED)} (Gyr)	9.5 (16)
age_{sis, MESA, l = 0,2 (PBJam)} (Gyr)	10.23 (87)
age_{sis, MESA, l = 0,2 (FAMED), Y=free} (Gyr)	10.56 (88)
age_{sis, MESA, l = 0 (PBJam)} (Gyr)	10.21 (90)

^(a)

Notes. All measurements are obtained using the same photospheric constraints (APOGEE DR17) unless otherwise stated.

^(b)

For asteroseismic scaling relations, the following stellar and solar values are used (where applicable): ν_max = 19.784 ± 0.158μHz, Δν = 2.714 ± 0.017μHz, T_eff = 4625 ± 60K, f_Δν = 0.95863, ν_max, ⊙ = 3090μHz, Δν_⊙ = 134.9μHz, T_eff, ⊙ = 5772K.

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