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Table 4.

Most reliable gravitationally lensed quasar candidates found with the “Multiplets” method described in the text.

ID RA Dec Multiplets Num. of Separation Notes
( (± type matches (arcsec)
KIDSJ0000−3502 00:00:57.10 −35:02:54.15 QSO 2 1.0 Low-separation double
KIDSJ0139−3103 01:39:59.08 −31:03:35.06 QSO 2 1.6 Low-separation double
KIDSJ0201−3208 02:01:15.44 −32:08:34.57 QSO 2 1.6 Low-separation double
KIDSJ1334−0120 13:34:11.18 −01:20:52.22 QSO 2 1.1 Low-separation double

KIDSJ0008−3237 00:08:16.01 −32:37:15.80 GAL 3 2.7 Gravitational arc
KIDSJ0106−2917 01:06:49.80 −29:17:12.20 GAL 2 3.4 Double with large shear
KIDSJ0206−2855 02:06:30.86 −28:55:42.22 GAL 2 1.2 Low-separation double
KiDSJ0208−3203 02:08:53.16 −32:02:03.51 GAL 3 2.0 Cross Quad candidate
KIDSJ0215−2909 02:15:14.4 −29:09:25.6 GAL 3 3.2 Fold Quad candidate
KIDSJ1204+0034 12:04:56.58 +00:34:06.02 GAL 3 4.6 Large-separation double
KiDSJ1346+0017 13:46:12.38 +00:17:20.18 GAL 4 2.8 Double with large shear
KIDSJ1359+0129 13:59:43.98 +01:28:13.90 GAL 2 0.9 Low-separation double

Notes. Cutouts of the candidates are shown in Fig. 11. We highlight in the table the number of matches found for each system in the BEXGO catalogue. In groups where the number of detections is smaller than the total number of objects visible from the cutout, most probably these objects are fainter than the magnitude threshold we set for the input catalogue. We double checked that these missing matches were not objects classified as stars. The last column before the notes indicates the separation between the multiple QSO images.

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