Table 3
List of estimated parameters for the Gaia astrometric asteroid binary candidates.
| ID | Wobble period(h) | Wobble amplitude (mas) | Separation (km) 1st interval | Mass ratio 1st interval | Separation (km) 2nd interval | Mass ratio 2nd interval | Taxonomy correction |  |
|---|---|---|---|---|---|---|---|---|
| KNOWN BINARIES | ||||||||
| 317 | 127.56 ± 64.57 | 2.38 ± 1.69 | (5.08 ± 4.79)e+02 | (1.21 ± 1.11)e-02 | (5.27 ± 5.27)e+04 | (7.36 ± 2.63)e-01 | * | |
| 1509 | > 84.06 | – | – | – | – | – | – | – |
| 2871 | 20.69 ± 4.63 | 0.45 ± 0.07 | (1.56 ± 0.18)e+01 | (1.18 ± 0.25)e-02 | (1.43 ± 0.16)e+01 | (6.00 ± 0.38)e-01 | * | |
| 4337 | 35.93 ± 6.36 | 0.61 ± 0.07 | (6.57 ± 0.66)e+01 | (2.40 ± 0.40)e-03 | (5.99 ± 0.62)e+01 | (8.18 ± 0.17)e-01 | * | |
| 5817 | > 144.11 | – | – | – | – | – | – | – |
| 18301 | 139.82 ± 70.02 | 3.10 ± 1.92 | (7.61 ± 1.38)e+01 | (9.78 ± 3.19)e-03 | (6.95 ± 1.24)e+01 | (6.35 ± 0.56)e-01 | * | * |
| OBJECTS WITH TWO SOLUTIONS | ||||||||
| 10.02 ± 0.02 | 0.74 ± 0 | |||||||
| 542 | 10.04 ± 0.04 | 0.56 ± 0.01 | (7.64 ± 0.20)e+01 | (2.30 ± 0.10)e-03 | (6.90 ± 0.19)e+01 | (8.20 ± 0.05)e-01 | * | * |
| 14.37 ± 0.19 | 0.48 ± 0.01 | |||||||
| 2219 | 13.56 ± 0.36 | 0.74 ± 0.06 | (5.59 ± 1.10)e+01 | (2.50 ± 0.80)e-03 | (5.08 ± 0.99)e+01 | (8.16 ± 0.33)e-01 | * | * |
| 63.47 ± 13.54 | 0.68 ± 0.05 | |||||||
| 9573 | 57.59 ± 3.56 | 0.99 ± 0.05 | (3.37 ± 0.57)e+01 | (1.08 ± 0.33)e-02 | (3.08 ± 0.50)e+01 | (6.18 ± 0.53)e-01 | * | |
| 10.33 ± 0.13 | 0.56 ± 0.05 | |||||||
| 10766 | 73.57 ± 9.51 | 0.87 ± 0.55 | (1.17 ± 0.24)e+02 | (4.99 ± 1.70)e-03 | (1.07 ± 0.22)e+02 | (7.36 ± 0.48)e-01 | * | |
| OBJECTS WITH ONE SOLUTION | ||||||||
| 53 | 9.08 ± 0.01 | 1.42 ± 0.01 | (2.39 ± 0.96)e+02 | (2.50 ± 1.50)e-03 | (2.54 ± 1.25)e+02 | (8.34 ± 0.76)e-01 | * | |
| 203 | 23.89 ± 0.27 | 0.88 ± 0.01 | (2.32 ± 0.03)e+02 | (1.00 ± 0)e-03 | (5.94 ± 3.71)e+02 | (9.35 ± 0.39)e-01 | * | |
| 217 | 12.70 ± 0.04 | 0.88 ± 0.02 | (1.84 ± 0.82)e+02 | (2.75 ± 1.75)e-03 | (2.19 ± 1.25)e+02 | (8.33 ± 0.88)e-01 | * | |
| 238 | 9.85 ± 0.01 | 2.23 ± 0.02 | (3.23 ± 1.07)e+02 | (2.00 ± 1.00)e-03 | (3.92 ± 1.96)e+02 | (8.59 ± 0.66)e-01 | * | |
| 247 | 12.10 ± 0.06 | 0.55 ± 0.02 | (1.46 ± 0.05)e+02 | (1.00 ± 0)e-03 | (4.41 ± 2.38)e+02 | (9.53 ± 0.24)e-01 | * | |
| ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ |
Notes. The grey lines represent the objects with density constrained by taxonomy, and the magenta lines indicate the best candidates accounting for the taxonomic correction and a strong detection with 
. The objects with orange ID represent those that were selected as binary candidates but with periods larger than the length of the observation window, therefore the period given as the minimum is the length of the observation window used. This is an extract of the full table, which is available at the CDS.
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