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Table 3.

Parameters for the single-star case scenario (cf. Sect. 5.1) of the sample targets with error bars indicated in parentheses in terms of the last digit.

RM solution IM solution CBM solution IM-CBM solution

Object/ M fov Age Mcc
M fov Age Mcc
M fov Age Mcc
M fov Age Mcc
parameter (M) (Hp) (Myr) (M) (%) (M) (Hp) (Myr) (M) (%) (M) (Hp) (Myr) (M) (%) (M) (Hp) (Myr) (M) (%)
V578 Mon 14.55(9) (A) 0.005 3.80(50) 4.90(13) 33.7(1.0) 14.77(59) (A) 0.005 3.74(55) 5.13(40) 34.7(4.3) 14.55(9) (A) 0.020(20) 4.13(77) 5.12(40) 35.2(3.0)
10.30(6) (A) 5.0(1.0) 3.04(7) 29.5(8) 10.55(34) (A) 5.0(1.0) 3.12(22) 29.6(3.1) 10.30(6) (A) 0.040(−40) 5.8(1.5) 3.21(35) 31.2(3.6)
V453 Cyg 14.10(40) (B) 0.005 10.9(3) 3.22(8) 22.8(1.3) 16.80(70) (A) 0.005 8.65(35) 4.43(30) 26.4(3.0) 14.00(20) (B) 0.040(−5) 12.38(40) 4.26(25) 30.4(2.3) 14.95(35) (A) 0.040 11.00(40) 4.82(20) 32.2(2.2)
11.15(15) (B) 10.8(4) 2.78(6) 24.9(9) 12.38(50) (A) 9.00(75) 3.33(23) 26.9(3.1) 11.11(15) (B) 0.040(−15) 12.32(55) 3.32(34) 29.9(3.5) 11.91(57) (A) 11.00(98) 3.66(30) 30.7(4.2)
V478 Cyg 15.60(20) (B) 0.005 7.40(20) 4.54(7) 29.1(8) 17.60(60) (A) 0.005 6.32(45) 5.49(40) 31.2(3.5) 15.58(22) (B) 0.040(−10) 8.21(25) 5.49(40) 35.2(3.4) 16.74(73) (A) 0.040 7.47(52) 6.05(50) 36.1(4.8)
15.10(10) (B) 7.83(25) 4.27(9) 28.3(8) 17.20(60) (A) 6.65(45) 5.36(37) 31.2(3.3) 15.22(22) (B) 0.040(−10) 8.69(25) 5.25(37) 34.5(3.0) 16.39(71) (A) 7.87(55) 5.97(50) 36.4(4.9)
AH Cep 16.28(15) (B) 0.005 4.90(20) 5.51(9) 33.8(9) 17.30(40) (A) 0.005 4.46(29) 6.09(20) 35.2(2.0) 16.26(18) (A) 0.040(−20) 5.41(30) 6.19(55) 38.1(3.8)
13.80(10) (B) 7.00(17) 4.10(5) 29.7(6) 15.20(30) (A) 5.90(50) 4.81(13) 31.6(1.6) 13.79(14) (B) 0.040(−15) 7.80(30) 4.72(35) 34.2(2.9) 14.86(70) (A) 0.040 6.98(58) 5.22(45) 35.1(4.9)
V346 Cen 12.19(15) (B) 0.005 13.66(30) 2.54(10) 20.8(1.1) 14.90(20) (A) 0.005 10.50(15) 3.42(2) 23.0(4) 12.02(14) (B) 0.040(−2) 15.96(18) 3.33(6) 27.7(8) 13.76(40) (A) 0.040 13.11(55) 4.14(20) 30.1(2.4)
8.41(9) (A) 13.2(1.0) 2.05(8) 24.4(1.2) 8.42(22) (A) 13.2(1.1) 2.05(11) 24.3(2.0) 8.40(10) (A) 0.005(+35) 13.5(1.6) 2.04(30) 24.3(4.1)
V573 Car 15.95(40) (B) 0.005 2.77(32) 5.72(35) 35.9(3.1) 16.88(39) (A) 0.005 2.50(20) 6.41(25) 38.0(2.4) 15.80(30) (B) 0.040(−20) 3.06(28) 6.11(40) 38.7(3.3) 16.62(45) (A) 0.040 2.89(23) 6.58(30) 40.0(2.5)
12.55(17) (B) 1.67(29) 4.29(10) 34.2(1.3) 12.89(30) (A) 1.50(15) 4.49(15) 34.8(2.1) 12.49(17) (A) 0.040(−40) 1.90(35) 4.37(25) 35.0(2.5)
V1034 Sco 17.13(10) (B) 0.005 6.37(18) 5.33(12) 31.1(9) 19.90(1.0) (A) 0.005 5.00(50) 7.00(60) 35.2(5.0) 17.15(13) (B) 0.040(−6) 7.00(15) 6.42(27) 37.4(1.9) 18.97(77) (A) 0.040 6.06(37) 7.44(50) 39.2(4.4)
9.66(7) (B) 6.42(60) 2.73(5) 28.3(6) 10.64(24) (A) 5.42(49) 3.12(16) 29.3(2.2) 9.65(7) (B) 0.040(−6) 7.76(65) 2.88(5) 29.8(8) 10.47(24) (A) 0.040 6.51(58) 3.29(15) 31.4(2.2)
V380 Cyg 11.43(19) (B),(1) 0.005 17.3(1.0) 0.38(38) 3.3(3.3) 15.00(−5) (B) 0.005 12.40(1.0) 2.41(1) 16.1(1) 11.43(19) (B),(1) 0.005(5) 17.3(1.0) 0.38(38) 3.3(3.3) 15.00(50) (A),(2) 0.040 14.1(1) 3.86(5) 25.7(5)
7.07(14) (B) 19.6(1.3) 1.61(5) 22.8(1.2) 8.55(75) (A) 12.50(2.50) 2.12(30) 24.8(5.2) 7.06(13) (B) 0.040(30) 22.6(2.7) 1.81(30) 25.6(4.8) 8.32(75) (A) 0.040 15.7(3.3) 2.26(30) 27.2(6.6)
CW Cep 13.01(6) (A) 0.005 6.70(56) 3.84(8) 29.5(8) 13.49(48) (A) 0.005 6.50(56) 4.09(25) 30.3(3.1) 13.01(7) (A) 0.038(−38) 7.09(65) 4.38(60) 33.7(4.8)
11.99(6) (B) 5.66(57) 3.65(6) 30.4(7) 12.38(16) (A) 6.39(55) 3.69(14) 29.8(1.5) 11.95(9) (A) 0.040(−30) 7.62(65) 3.86(45) 32.3(4.0)
U Oph 5.10(2) (A) 0.005 51.7(5.8) 0.93(5) 18.2(1.1) 5.04(20) (A) 0.005 51.3(5.8) 0.93(5) 18.5(1.7) 5.10(5) (A) 0.013(13) 52.9(3.0) 1.01(10) 19.8(2.2)
4.60(2) (A) 57.5(7.5) 0.87(5) 18.9(1.2) 4.63(18) (A) 57.6(10.0) 0.87(5) 18.8(1.9) 4.60(5) (A) 0.017(12) 57.4(3.3) 0.93(7) 20.2(1.8)
V621 Per 9.44(46) (B),(1) 0.005 21.8(1) 1.55(75) 16.4(9.2) 12.5(1) (B) 0.005 14.9(4) 2.13(5) 17.0(6) 9.44(46) (B),(1) 0.030(5) 24.1(1) 2.08(15) 22.0(2.8) 11.81(30) (A) 0.030 17.5(7) 2.80(12) 23.7(1.7)

Notes. The convective core mass is provided both in absolute (solar mass units) and relative (to the stellar mass) values. For each object, the first/second line corresponds to the primary/secondary component. Stars that do not have parameters for the IM-CBM solution could already be fitted in the CBM solution and did not require variable initial mass on top of the core-boundary mixing parameter. Detailed description of the individual solutions is provided in Sect. 4.3. (A/B)Within/outside error box. (1)Dynamical mass was enforced. (2)Maximum amount of the core-boundary mixing is assumed (see Sect. 6).

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