Table 1.
Solutions from the combination of Gaia NSS astrometric solutions with SB9 double-lined spectroscopy.
Gaia DR3 ID | q | σq | ℳ1 | σℳ1 | ℳ2 | σℳ2 | β | σβ | F2 | Ref. |
---|---|---|---|---|---|---|---|---|---|---|
48197783694869760 | 0.6771 | 0.0124 | 0.9707 | 0.0423 | 0.6573 | 0.0190 | 0.0936 | 0.0030 | 1.32 | 1 |
69883417170175488 | 0.9793 | 0.0224 | 0.8271 | 0.0289 | 0.8100 | 0.0273 | 0.3976 | 0.0084 | −0.03 | 2 |
308256610357824640 | 0.6970 | 0.0099 | 0.4283 | 0.2000 | 0.2985 | 0.1393 | 0.2770 | 0.0232 | −0.15 | 3 |
478996438146017280 | 0.9212 | 0.0064 | 0.8112 | 0.0249 | 0.7473 | 0.0228 | 0.3879 | 0.0030 | 1.25 | 4 |
544027809281308544 | 0.8336 | 0.0178 | 0.9465 | 0.0510 | 0.7890 | 0.0317 | 0.1363 | 0.0072 | 0.01 | 5 |
595390807776621824 | 0.8822 | 0.0061 | 0.7877 | 0.0105 | 0.6948 | 0.0066 | 0.3123 | 0.0017 | −0.03 | 6 |
660622010858088320 | 0.8707 | 0.0367 | 0.7304 | 0.0607 | 0.6360 | 0.0341 | 0.2252 | 0.0081 | 1.01 | 5 |
827608625636174720 | 0.9403 | 0.0129 | 0.7357 | 0.0392 | 0.6917 | 0.0367 | 0.4076 | 0.0045 | 0.29 | 7 |
882872210352301568 | 0.5027 | 0.0026 | 1.0044 | 0.0123 | 0.5049 | 0.0036 | 0.0257 | 0.0038 | −0.07 | 8 |
1067685718250692352 | 0.8884 | 0.0036 | 1.0279 | 0.0125 | 0.9132 | 0.0101 | 0.3035 | 0.0048 | 0.10 | 9 |
1074883087005896320 | 0.9388 | 0.0261 | 0.6640 | 0.0393 | 0.6233 | 0.0326 | 0.3977 | 0.0068 | 1.11 | 10 |
1324699172583973248 | 0.8839 | 0.0087 | 1.3136 | 0.0476 | 1.1611 | 0.0376 | 0.3167 | 0.0039 | 0.40 | 11 |
1441993625629660800 | 0.8344 | 0.0128 | 1.1033 | 0.0455 | 0.9205 | 0.0293 | 0.0706 | 0.0132 | −0.10 | 12 |
1480959875337657088 | 0.9351 | 0.0771 | 0.8679 | 0.1330 | 0.8116 | 0.0925 | 0.2884 | 0.0180 | 0.77 | 13 |
1517219363639758976 | 0.8198 | 0.0062 | 1.0650 | 0.0405 | 0.8731 | 0.0313 | 0.1576 | 0.0075 | 1.55 | 14 |
1517927895803742080 | 0.9076 | 0.0148 | 0.6354 | 0.0251 | 0.5767 | 0.0183 | 0.3546 | 0.0037 | 1.75 | 7 |
1528045017687961856 | 0.6793 | 0.0029 | 1.1179 | 0.0285 | 0.7593 | 0.0185 | 0.0623 | 0.0045 | 2.30 | 15 |
1615450866336763904 | 0.7864 | 0.0106 | 1.0138 | 0.0396 | 0.7973 | 0.0261 | 0.1317 | 0.0044 | 0.14 | 16 |
1918953867019478144 | 0.9308 | 0.0007 | 1.0465 | 0.0050 | 0.9741 | 0.0047 | 0.3866 | 0.0014 | 0.63 | 17 |
2012218158438964224 | 0.9486 | 0.0150 | 2.3368 | 0.1644 | 2.2168 | 0.1509 | 0.3589 | 0.0064 | 0.92 | 18 |
2035577729682322176 | 0.9024 | 0.0089 | 0.7027 | 0.0417 | 0.6341 | 0.0374 | 0.3227 | 0.0056 | −0.16 | 19 |
2067948245320365184 | 0.7863 | 0.0006 | 0.8374 | 0.0023 | 0.6584 | 0.0017 | 0.1521 | 0.0014 | 0.48 | 17 |
2129771310248902016 | 0.9071 | 0.0183 | 0.7408 | 0.0399 | 0.6720 | 0.0302 | 0.3184 | 0.0048 | −0.16 | 10 |
2185171578009765632 | 0.9629 | 0.0082 | 1.2178 | 0.0299 | 1.1727 | 0.0333 | 0.4436 | 0.0033 | 1.28 | 17 |
2198442167969655296 | 0.7508 | 0.0152 | 0.9844 | 0.0416 | 0.7391 | 0.0189 | 0.1963 | 0.0033 | 0.65 | 10 |
3283823387685219328 | 0.7419 | 0.0004 | 0.9864 | 0.0112 | 0.7319 | 0.0083 | 0.1478 | 0.0031 | 0.37 | 20 |
3312631623125272448 | 0.7062 | 0.0024 | 0.9920 | 0.0304 | 0.7005 | 0.0215 | 0.1249 | 0.0051 | 1.54 | 21 |
3366718833479009408 | 0.6407 | 0.0022 | 1.0494 | 0.0102 | 0.6724 | 0.0051 | 0.0155 | 0.0028 | 0.18 | 8 |
3409686270424363008 | 0.7076 | 0.0031 | 0.7927 | 0.0139 | 0.5610 | 0.0087 | 0.1086 | 0.0028 | 2.07 | 17 |
3427930123268526720 (a) | 0.3311 | 0.0047 | 0.8066 | 0.0760 | 0.2671 | 0.0248 | 0.0616 | 0.0066 | 5.23 | 3 |
3536759371865789568 | 0.8392 | 0.0212 | 1.6490 | 0.0899 | 1.3838 | 0.0492 | 0.2000 | 0.0061 | 0.62 | 22 |
3549833939509628672 | 0.9406 | 0.0195 | 0.9450 | 0.0384 | 0.8889 | 0.0249 | 0.3567 | 0.0051 | 0.19 | 22 |
3931519127529822208 | 0.7750 | 0.0260 | 1.0791 | 0.0762 | 0.8363 | 0.0342 | 0.1403 | 0.0045 | 1.19 | 23 |
3935131126305835648 | 0.7039 | 0.0022 | 1.4860 | 0.0744 | 1.0460 | 0.0523 | 0.1374 | 0.0052 | 0.08 | 20 |
3954536956780305792 | 0.9053 | 0.0094 | 0.7713 | 0.7626 | 0.6982 | 0.6904 | 0.3262 | 0.0600 | 0.49 | 5 |
3964895043508685312 | 0.8650 | 0.0084 | 0.7531 | 0.1654 | 0.6514 | 0.1426 | 0.2201 | 0.0196 | −0.09 | 17 |
4145362250759997952 | 0.6960 | 0.0216 | 0.9414 | 0.0611 | 0.6552 | 0.0261 | 0.0757 | 0.0046 | 0.16 | 24 |
4228891667990334976 | 0.8629 | 0.0057 | 1.0907 | 0.0588 | 0.9412 | 0.0502 | 0.2872 | 0.0038 | 4.10 | 25 |
4354357901908595456 | 0.5832 | 0.0194 | 0.7005 | 0.0509 | 0.4085 | 0.0177 | 0.0606 | 0.0041 | 0.18 | 26,27 |
4589258562501677312 | 0.8201 | 0.0317 | 0.6679 | 0.0628 | 0.5478 | 0.0395 | 0.2924 | 0.0085 | −0.13 | 5 |
5762455439477309440 | 0.8041 | 0.0327 | 0.8058 | 0.0674 | 0.6480 | 0.0333 | 0.1768 | 0.0076 | 0.20 | 5 |
6244076338858859776 | 0.8820 | 0.0076 | 0.7730 | 0.0135 | 0.6818 | 0.0101 | 0.2943 | 0.0023 | 0.86 | 10 |
6799537965261994752 | 0.9000 | 0.0017 | 0.9036 | 0.0092 | 0.8132 | 0.0083 | 0.3267 | 0.0024 | 1.32 | 24 |
Notes.
q is the mass ratio, ℳ1 is the mass of the primary, ℳ2 is the mass of the secondary (in ℳ⊙) and β is the flux fraction of the secondary. σq, σℳ1, σℳ2 and σβ are their associated uncertainties. F2 is the goodness-of-fit estimator. Ref gives the reference of the raw radial velocity data used in the fit, as provided by SB9. High F2, removed from the Sect. 5 study. Full table including the correlations and the orbital parameters is available at the CDS.
References. (1) Tomkin (2005); (2) Mermilliod et al. (2009); (3) Baroch et al. (2018); (4) Fekel et al. (1994); (5) Goldberg et al. (2002); (6) Griffin (2009); (7) Sperauskas et al. (2019); (8) Fekel et al. (2015); (9) Ginestet & Carquillat (1995); (10) Halbwachs et al. (2018); (11) Griffin (2011); (12) Griffin (1990); (13) Halbwachs et al. (2012); (14) Griffin (2008); (15) Kiefer et al. (2016); (16) Griffin (2013); (17) Kiefer et al. (2018); (18) Griffin (1993); (19) Imbert (2006); (20) Halbwachs et al. (2020); (21) Tomkin (2007); (22) Griffin (2006); (23) Griffin (2012); (24) Tokovinin (2019); (25) Griffin (2014); (26) Mazeh et al. (1997); (27) Mayor & Turon (1982).
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