Table 1.
Physical parameters for our eight dual AGN candidates.
| Primary component |
Secondary component |
||||
|---|---|---|---|---|---|
| Source ID | D | Nb detections | G | Nb detections | G |
| [mas] | [mag] | [mag] | |||
| (1) | (2) | (3) | (4) | (5) | (6) |
| 413107379 | 318.08 | 82 | 19.3 ± 0.1 | 50 | 19.7 ± 0.1 |
| 709923047 | 239.37 | 28 | 17.4 ± 0.1 | 14 | 18.5 ± 0.1 |
| 185414449 | 402.79 | 102 | 19.6 ± 0.1 | 10 | 20.5 ± 0.1 |
| 372100463 | 130.65 | 28 | 19.5 ± 0.2 | 8 | 19.6 ± 0.2 |
| 502675674 | 143.90 | 53 | 19.3 ± 0.1 | 8 | 19.3 ± 0.1 |
| 481987315 | 369.48 | 64 | 18.7 ± 0.1 | 40 | 19.7 ± 0.1 |
| 451971551 | 349.72 | 42 | 19.4 ± 0.1 | 32 | 19.8 ± 0.1 |
| 666080784 | 221.52 | 31 | 18.9 ± 0.1 | 15 | 19.9 ± 0.1 |
Notes. (1): First digits of the object identifier in the Gaia DR3 catalog. (2): Angular separation between the components. (3): Number of Gaia detections inside the first component. (4): Magnitude of the first component in the G band. (5): Number of Gaia detections inside the second component. (6): Magnitude of the second component in the G band. The uncertainties correspond to the standard deviation of the quantities, derived from the measures made for each observational point.
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