Open Access

Table 1

Content of the catalogue of inferred masses for the Orbital300 sample.

GaiaDR3 source_id 1,med 1,lo 1,up 2,med 2,lo 2,lo ap σ(ap) T σ(T) log10(f1/f2)
() () () () () () (au) (au) (days) (days)
1729398647131392 0.5001 0.4867 0.5493 0.1170 0.0035 0.1753 0.3118 0.0043 538.083 8.575 1.9576
2488955023504768 0.4488 0.4248 0.4525 0.0775 0.0694 0.0878 0.2136 0.0154 441.589 4.821 2.1656
3205080690546176 0.8473 0.7602 0.8642 0.0325 0.0035 0.5583 0.4405 0.0127 879.223 64.436 4.9103
3679313799492864 0.3648 0.3588 0.3882 0.1232 0.0811 0.1259 0.0897 0.0035 1074.243 56.782 1.1449
4016657710743168 1.4086 1.1721 1.5381 0.4151 0.0132 0.4474 0.4196 0.0192 822.289 26.599 2.7579
5168082607675520 0.6835 0.6479 0.7370 0.3085 0.2906 0.4449 0.1792 0.0051 711.032 4.757 1.5329
7326187710462720 1.0944 0.8926 1.1955 0.2941 0.0141 0.3830 0.1891 0.0035 300.369 1.320 2.5974
7623811764175616 0.7208 0.7176 0.7258 0.1176 0.1135 0.1241 0.1723 0.0180 241.112 1.492 2.7660
8499499760858368 0.8426 0.7643 0.8837 0.4637 0.2747 0.5320 0.2381 0.0094 448.716 0.957 1.4428
8628662312765440 0.6880 0.6622 0.7278 0.1152 0.0038 0.4162 0.1884 0.0067 1243.326 33.863 2.7783

Notes. 1,med is the median mass of the primary; 1,lo and 1,up are the 16th and 84th percentiles of the mass posterior, representing the lower and upper uncertainties, respectively; and the same is the case for the secondary, ℳ2. The table also includes the photometric SMA ap, the period T, and their 1σ uncertainties. The final column is log-base 10 of the G-band flux ratio at the median parameters. The electronic version of this table lists all 20 334 systems sorted by increasing source_id, with precise fields reported (no rounding). There are no missing data. The full table is available at the CDS.

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