Table 8
substellar candidates and background sources observed during the IDPS.
| Star | α | δ | ρ | θ | δρ = ρδθ | Δm | Filter | M | mmin,max | aproj | Date | Tel. | # | Status |
| (J2000.0) | (J2000.0) | (") | (deg) | (mas) | (MJup) | (AU) | ||||||||
|
|
||||||||||||||
| HR9 | 00:06:50.09 | −23:06:27.14 | 19.691 | 337.347 | 40 | – | Kp | – | – | 770.1 ± 13.0 | 2001-12-01 | KE | 1 | ? |
| HIP 682 | 00:08:25.74 | +06:37:00.48 | 5.472 | 268.037 | 14 | 15.47 ± 0.49 | Ks | – | – | – | 2012-09-04 | KE | 1 | B |
| 4.945 | 267.774 | 12 | 14.73 ± 0.31 | Kp | – | – | – | 2006-07-18 | KE | 1 | B | |||
Notes. In the status column, “A” stands for associated with the star, whereas “B” is for background object and “F” for false detection. The flag “B?"’ means that the errors bars are larger than parallax and proper motion, but given the displacement of all the candidates between the two epochs, we are confident the object is background.
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