Table A.1
Input parameters
| # | Name 1 | Name 2 | B-V | TS | THEIA | Dist. | Mass | Luminosity | Teff |  |
 |
PHZmid |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Mlim | ||||||||||||
| (MEarth) | (pc) | (solar) | (solar) | (K) | (days) | |||||||
| 1 | α Cen. A | Gl559A | 0.71 | G2V | 0.23 | 1.35(***) | 1.12 | 1.52 | 5585(22) | -5.059(8) | -4.970(4) | 671.1 |
| 2 | α Cen. B | Gl559B | 0.90 | K1V | 0.30 | 1.35(***) | 0.84 | 0.51 | 5248(18) | -4.920(4) | -4.940(4) | 355.2 |
| 3 | ϵ Eridani | Gl144 | 0.88 | K2V | 1.08 | 3.22(*) | 0.76 | 0.35 | 4999(8) | -4.598(8) | -4.331(2) | 290.2 |
| 4 | 61 Cygni A | Gl820A | 1.18 | K5V | 1.11 | 3.50(**) | 0.59 | 0.13 | 4379(24) | -4.910(2) | -4.668(2) | 172.4 |
| 5 | 61 Cygni B | Gl820B | 1.37 | K7V | 1.25 | 3.49(**) | 0.52 | 0.08 | 4040(24) | -4.999(12) | -4.900(5) | 130.6 |
| 6 | Procyon A | Gl280A | 0.42 | F5IV-V | 0.46 | 3.51(*) | 1.65 | 6.76 | 6592(22) | -4.820(2) | -4.614(2) | 1483.3 |
| 7 | ϵ Indi | Gl845 | 1.06 | K5V | 1.32 | 3.64(**) | 0.65 | 0.19 | 4571(22) | -4.851(6) | -4.809(13) | 210.4 |
| 8 | τ Ceti | Gl71 | 0.72 | G8V | 1.09 | 3.65(*) | 0.81 | 0.44 | 5338(8) | -5.065(8) | -4.895(2) | 322.2 |
| 9 | Groombridge 1618 | Gl380 | 1.33 | K6V | 2.19 | 4.87(**) | 0.53 | 0.09 | 4002(24) | -4.682(12) | -4.615(2) | 137.1 |
| 10 | 70 Ophiuchi A | Gl702A | 0.86 | K0V | 1.16 | 5.08(*) | 0.84 | 0.52 | 5023(22) | -4.663(2) | -4.367(2) | 370.3 |
| 11 | 70 Ophiuchi B | Gl702B | 1.19 | K4V | 1.60 | 5.12(**) | 0.59 | 0.13 | 4475(24) | -4.759(3) | -4.557(1) | 169.1 |
| 12 | σ Draconis | Gl764 | 0.78 | K0V | 1.80 | 5.75(*) | 0.78 | 0.40 | 5272(22) | -4.921(12) | -4.666(2) | 304.7 |
| 13 | 33G Librae A | Gl570A | 1.11 | K4V | 1.85 | 5.88(**) | 0.66 | 0.21 | 4519(22) | -4.875(16) | -4.480(4) | 221.7 |
| 14 | η Cassio. A | Gl34A | 0.58 | F9V+M0V | 1.19 | 5.95(*) | 1.05 | 1.22 | 5902(22) | -4.985(2) | -4.930(7) | 563.7 |
| 15 | η Cassio. B | Gl34B | 1.39 | K7V | 2.39 | 5.93(**) | 0.48 | 0.06 | 4011(23) | -4.936(2) | -4.806(12) | 112.2 |
| 16 | 36 Ophiuchi A | Gl663A | 0.85 | K2V | 1.43 | 5.96(**) | 0.70 | 0.26 | 5370(18) | -4.684(2) | -4.406(2) | 233.0 |
| 17 | 36 Ophiuchi B | Gl663B | 0.85 | K1V | 1.44 | 5.96(**) | 0.70 | 0.26 | 5370(18) | -4.664(2) | -4.415(2) | 228.9 |
| 18 | 279G Sagit. A | Gl783 | 0.87 | K2.5V | 2.08 | 6.02(**) | 0.69 | 0.24 | 4857(8) | -5.079(8) | -4.940(9) | 232.9 |
| 19 | 82G Eridani | Gl139 | 0.71 | G6V | 1.76 | 6.04(*) | 0.91 | 0.69 | 5478(8) | -5.025(13) | -4.949(15) | 418.7 |
| 20 | δ Pavonis | Gl780 | 0.76 | G8IV | 1.43 | 6.11(*) | 1.03 | 1.13 | 5512(8) | -5.030(4) | -4.980(4) | 564.5 |
| 21 | ξ Bootis A | Gl566A | 0.73 | G7Ve | 1.59 | 6.73(**) | 0.85 | 0.54 | 5570(21) | -4.442(2) | -4.146(2) | 353.2 |
| 22 | ξ Bootis B | Gl566B | 1.17 | K5Ve | 2.37 | 6.75(**) | 0.54 | 0.10 | 4418(24) | -4.418(1) | -4.356(12) | 140.8 |
| 23 | β Hydri | Gl19 | 0.62 | G0V | 1.31 | 7.46(*) | 1.30 | 2.68 | 5784(8) | -5.050(4) | -4.960(4) | 928.7 |
| 24 | μ Cassio. A | Gl53A | 0.69 | G5V | 2.16 | 7.55(*) | 0.79 | 0.42 | 5395(22) | -4.992(2) | -4.933(2) | 309.1 |
| 25 | π 3O Orionis | Gl178 | 0.44 | F6V | 1.58 | 8.07(*) | 1.25 | 2.37 | 6412(22) | -4.650(7) | -4.626(2) | 793.7 |
| 26 | pEridani A | Gl66A | 0.86 | K2V | 1.93 | 8.19(**) | 0.67 | 0.22 | 5023(22) | -4.899(8) | -4.740(4) | 214.3 |
| 27 | pEridani B | Gl66B | 0.90 | K2V | 2.00 | 8.19(**) | 0.64 | 0.19 | 5093(22) | -4.830(6) | -4.830(6) | 194.9 |
| 28 | μ Herculis A | Gl695A | 0.75 | G5IV | 1.30 | 8.31(*) | 1.33 | 2.96 | 5562(25) | -5.193(2) | -5.043(12) | 1017.4 |
| 29 | γ Pavonis | Gl827 | 0.48 | F9V | 2.12 | 9.26(*) | 1.06 | 1.24 | 6205(8) | -4.811(15) | -4.491(6) | 545.6 |
| 30 | ζ Tucanae | Gl17 | 0.57 | F9.5V | 1.91 | 8.59(*) | 0.97 | 0.89 | 5991(8) | -4.954(13) | -4.810(4) | 457.0 |
| 31 | ξ Ursae Major A | Gl423A | 0.55 | F8.5V | 1.79 | 8.73(***) | 1.15 | 1.69 | 5875(22) | -4.218(2) | -4.218(2) | 690.6 |
| 32 | ξ Ursae Major B | Gl423B | 0.65 | G2V | 1.95 | 8.73(**) | 1.05 | 1.19 | 5650(19) | -4.289(2) | -4.289(2) | 571.1 |
| 33 | γ Leporis A | Gl216A | 0.47 | F6V | 1.36 | 8.93(*) | 1.18 | 1.89 | 6372(8) | -4.966(12) | -4.770(4) | 694.4 |
| 34 | γ Leporis B | Gl216B | 0.94 | K3 | 2.21 | 8.90(**) | 0.69 | 0.24 | 4875(22) | -4.657(6) | -4.100(4) | 234.8 |
| 35 | δ Eridani | Gl150 | 0.92 | K0+IV | 1.81 | 9.04(*) | 1.42 | 3.80 | 4866(8) | -5.232(2) | -5.039(2) | 1288.8 |
| 36 | β Com. Ber. | Gl502 | 0.59 | F9.5V | 2.08 | 9.13(*) | 1.04 | 1.15 | 5970(22) | -4.832(2) | -4.619(12) | 536.8 |
| 37 | β Canum Ven. | Gl475 | 0.61 | G0V | 2.13 | 8.44(*) | 1.06 | 1.25 | 5888(18) | -4.990(10) | -4.879(2) | 572.5 |
| 38 | 66G Cen. A | Gl442A | 0.67 | G2V | 2.06 | 9.29(**) | 1.00 | 1.01 | 5688(8) | -5.031(11) | -4.874(14) | 514.9 |
| 39 | ζ Herculis A | Gl635A | 0.64 | G0IV | 1.29 | 10.10(***) | 1.61 | 6.05 | 6026(18) | -5.193(2) | -5.090(14) | 1491.2 |
| 40 | ζ Herculis B | Gl635B | 0.80 | K0V | 2.19 | 10.10(***) | 0.89 | 0.64 | 5300(20) | -4.830(17) | -4.830(17) | 407.8 |
| 41 | β Virginis | Gl449 | 0.55 | F9V | 2.00 | 10.93(*) | 1.34 | 3.04 | 6109(22) | -4.966(12) | -4.813(12) | 963.7 |
| 42 | η Bootis | Gl534 | 0.57 | G0IV | 1.58 | 11.40(*) | 1.63 | 6.46 | 6012(22) | -5.250(10) | -5.250(10) | 1555.8 |
| 43 | γ Virginis A | Gl482A | 0.36 | F1-F2V | 1.48 | 11.62(**) | 1.37 | 3.27 | 6808(22) | -5.039(14) | -4.479(16) | 920.2 |
| 44 | β Tri. Aus. A | Gl601A | 0.29 | F1V | 1.43 | 12.38(*) | 1.75 | 8.30 | 7109(8) | - | - | 1573.5 |
| 45 | γ Virginis B | Gl482B | 0.36 | F0mF2V | 1.44 | 12.74(**) | 1.41 | 3.65 | 6694(23) | -4.298(16) | -4.298(16) | 999.6 |
| 46 | γ Cephei | Gl903 | 1.04 | K1III-IV | 2.08 | 13.54(**) | 1.99 | 13.77 | 4786(18) | -5.315(2) | -5.256(12) | 2882.8 |
| 47 | β Aquilae A | Gl771A | 0.85 | G8IV | 1.73 | 13.70(*) | 1.59 | 5.87 | 5057(8) | -5.238(6) | -5.034(1) | 1649.0 |
| 48 | α Fornacis A | Gl127A | 0.53 | F6V | 1.99 | 13.95(**) | 1.44 | 4.03 | 6258(8) | -4.990(10) | -4.901(6) | 1126.1 |
| 49 | θ Bootis A | Gl549A | 0.51 | F7V | 1.92 | 14.53(*) | 1.33 | 2.92 | 6152(22) | -4.601(14) | -4.410(14) | 935.7 |
| 50 | η Cephei | Gl807 | 0.91 | K0IV | 2.08 | 14.27(*) | 1.71 | 7.71 | 4898(22) | - | - | 1988.6 |
| 51 | τ Bootis A | Gl527A | 0.49 | F7IV-V | 2.17 | 15.62(*) | 1.25 | 2.32 | 6310(22) | -4.964(2) | -4.964(2) | 793.9 |
| 52 | 10 Ursae Major A | Gl332 | 0.43 | F3V+G5V | 2.16 | 16.07(*) | 1.44 | 3.99 | 6516(22) | -4.639(14) | -4.547(14) | 1081.7 |
| 53 | Ψ Velorum A | Gl351A | 0.34 | F3V | 2.15 | 18.31(**) | 1.46 | 4.21 | 6837(8) | -4.669(14) | -4.362(11) | 1071.4 |
| 54 | Ψ Velorum B | Gl351B | 0.53 | F | 2.33 | 18.41(**) | 1.34 | 3.05 | 6148(27) | - | - | 960.2 |
| 55 | δ Gemini A | Gl271A | 0.34 | F2V | 2.22 | 18.54(*) | 1.71 | 7.64 | 6902(22) | - | - | 1536.5 |
Notes. B, V, and spectral types from CDS except the spectral type for ζ Herculis A (Morel et al. 2001)and Ψ Velorum B (F star deduced from its B-V value). The THEIA detection limits are from Theia Collaboration (2017), as are the masses and luminosities. The distances are derived from parallaxes from Hipparcos (van Leeuwen 2007), indicated with a (*), from GAIA DR2 (Gaia Collaboration 2018), indicated with (**), and from other references for a few stars indicated as (***): α Cen A and B (Pourbaix & Boffin 2016); ξ Ursae Major A (Gaia value for the B component);ζ Herculis A and B (Theia Collaboration 2017). References for 
and 
are the following: (1) Noyes et al. (1984); (2) Duncan et al. (1991); (3) Baliunas et al. (1995); (4) Henry et al. (1996); (5) Radick et al. (1998); (6) Gray et al. (2003); (7) Wright et al. (2004); (8) Gray et al. (2006); (9)
Jenkins et al. (2006) ; (10) Hall et al. (2007); (11) Schröder et al. (2009); (12) Isaacson & Fischer (2010); (13) Lovis et al. (2011); (14) Pace (2013); (15) Meunier et al. (2017); (16) Boro Saikia et al. (2018) ; (17) Deduced from the age (Morel et al. 2001) and relationship from Mamajek & Hillenbrand (2008). Reference for Teff are the following: (18) Allende Prieto & Lambert (1999); (19) Cayrel de Strobel et al. (2001); (20) Morel et al. (2001); (21) Valenti & Fischer (2005); (8) Gray et al. (2006); (22) Holmberg et al. (2009); (23) Aleo et al. (2017); (24) Houdebine et al. (2019); (25) Marfil et al. (2019); (26) White et al. (2020) ; (27) Derived from a law between B-V and Teff established from data in Gray et al. (2003).
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