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Table 1

Physical properties of ALMA-EMISSA main-sequence stars.

ID HD/GJ ID SIMBAD ID Sp.type RA Dec Distance Mass Radius Teff log g [Fe/H]
deg deg pc M R K cm s−2
A HD 48915A Alf CMa A1V 101.287[3] −16.716 [3] 2.64 ± 0.01 [14] 2.15 [4] 1.71 ± 0.01 [43] 9880 ± 200 4.31 0.29 ± 0.5 [3]
B HD 216956 Alf PsA A4V [33] 344.413[3] −29.622 [3] 7.70 ± 0.03 [14] 1.97 [4] 1.84 ± 0.02 [36] 8900 ± 300 4.20 0.45 ± 0.2 [3]
C HD 110379 Gam Vir A F0V [29] 190.4151 [3] −1.44939 [3] 11.62 ± 0.09 [14] 1.57 [60] 1.39 ± 0.19 [*] 7100 ± 100 4.35 −0.07 ± 0.08 [3]
D HD 110380 Gam Vir B F0V [29] 190.4148 [3] −1.44940 [3] 11.62 ± 0.09 [14] 1.43 [60] 1.49 ± 0.2 [*] 6960 ± 146 4.25 −0.09 ± 0.06 [62]
E HD 109085 Eta Crv F2V 188.018 [3] −16.196 [3] 18.28 ± 0.06 [14] 1.48 [12] 1.52 ± 0.06 [12] 6871 ± 48 4.25 0.00 ± 0.06 [51]
F HD 38393 Gam Lep F6V 86.116 [13] −22.448 [13] 8.88 ± 0.02 [14] 1.22 [12] 1.30 ± 0.06 [12] 6599 ± 556 4.30 −0.02 ± 0.1 [49]
G HD 128620 Alf Cen A G2V 219.902 [1] −60.834 [1] 1.325 ± 0.007 [38] 1.11 [16] 1.25 ± 0.03 [17] 5745 ± 80 4.29 0.2 ± 0.02 [50]
H HD 115617 61 Vir G6.5V 199.601 [3] −18.311 [3] 8.53 ± 0.02 [14] 0.92 [25] 0.98 ± 0.04 [10] 5618 ± 70 4.42 0.02 ± 0.46 [49]
I HD128621 Alf Cen B K1V 219.896[13] −60.838 [13] 1.325 ± 0.007 [38] 0.90 [25] 0.86 ± 0.02 [17] 5145 ± 80 4.53 0.23 ± 0.03 [50]
J HD 22049 Eps Eri K2V 53.233 [2] −9.458 [2] 3.202 ± 0.005 [38] 0.86 [21] 0.77 ± 0.02 [21] 5100 ± 70 4.60 −0.05 ± 0.46 [49]
K GJ 2006 A GJ 2006 A M3.5V 6.959[3] −32.552 [3] 34.89 ± 0.09 [14] 0.55 [12] 0.56 ± 0.02 [12] 3150 ± 18 4.69 −0.5 ± 0.1 [3]
L GJ 551 Proxima Cen M5.5V 217.43[3] −62.68 [3] 1.3 ± 0.003 [14] 0.12 [64] 0.15 ± 0.004 [64] 2990 ± 44 5.16 −0.07 ± 0.14 [3]
S Sun G2V 4.8E–06 1 1 5772 [21] 4.44 log(Fe/H) = −4.49 [54]

Notes. Columns 1–13 provide the assigned ID, HD/GJ ID, SIMBAD ID, spectral type, RA, Dec, distance, mass, radius, effective temperature, surface gravity, and metallicity of each star with references numbered inside [ ]. Spectral types are obtained from SIMBAD, unless specified and Teff s from Soubiran et al. (2016). log g is computedusing mass and radius. Check the caption of Table 2 for references.

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