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Table 1

Properties of the WISSH QSOs considered in this paper.

SDSS name RA Dec zSDSS u g r i z J H K E(BV)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13)
J0801+5210 08:01:17.79 +52:10:34.5 3.217 19.73 17.26 16.90 16.76 16.69 15.71 15.34 14.61 0.0
J0958+2827 09:58:41.21 +28:27:29.5 2.120 20.95 18.50 17.84 17.71 17.51 16.31 16.04 15.41 0.0
J1106+6400 11:06:10.72 +64:00:09.6 2.205 16.44 16.11 16.01 15.98 15.81 15.06 14.55 13.95 0.0
J1111+1336 11:11:19.10 +13:36:03.9 3.462 22.26 18.11 17.30 17.18 17.05 15.89 15.51 15.03 0.0
J1157+2724 11:57:47.99 + 27:24:59.6 2.214 19.98 19.11 18.25 17.77 17.31 16.14 15.43 14.48 0.2
J1201+0116 12:01:44.36 +01:16:11.6 3.240 19.50 17.72 17.39 17.32 17.27 15.90 15.88 14.84 0.0
J1236+6554 12:36:41.45 +65:54:42.1 3.358 20.52 17.81 17.29 17.19 16.96 16.00 15.47 15.31 0.0
J1421+4633 14:21:23.97 +46:33:18.0 3.404 21.96 17.97 17.38 17.22 17.09 16.28 15.49 14.89 0.0
J1422+4417 14:22:43.02 +44:17:21.2 3.605 23.45 19.36 18.15 17.57 17.11 15.81 15.21 14.46 0.1
J1521+5202 15:21:56.48 +52:02:38.5 2.195 16.44 15.90 15.60 15.44 15.33 14.64 14.06 13.35 0.0
J1538+0855 15:38:30.55 +08:55:17.0 3.551 24.14 18.17 17.17 17.00 16.84 15.67 15.48 14.72 0.0
J2123−0050 21:23:29.46 −00:50:52.9 2.269 17.16 16.63 16.42 16.34 16.10 15.18 14.62 13.90 0.0
J2346−0016 23:46:25.66 −00:16:00.4 3.489 21.24 18.69 17.91 17.75 17.56 16.87 16.13 15.30 0.0

J0745+4734a 07:45:21.78 +47:34:36.1 3.214 19.56 16.63 16.35 16.29 16.19 15.08 14.61 13.95 0.0
J0900+4215a 09:00:33.50 +42:15:47.0 3.297 22.97 17.11 16.74 16.69 16.58 15.37 14.68 14.00 0.0
J1201+1206a 12:01:47.90 +12:06:30.3 3.495 20.77 18.31 17.41 17.31 17.18 15.87 15.25 14.61 0.0
J1326−0005a 13:26:54.95 −00:05:30.1 3.307 22.83 20.90 20.54 20.02 19.28 17.39 16.75 15.31 0.3
J1549+1245a 15:49:38.71 +12:45:09.1 2.386 20.23 18.67 17.84 17.38 16.90 15.86 14.56 13.52 0.1

Notes. Columns give the following information: (1) SDSS name, (2–3) celestial coordinates, (4) redshift from SDSS DR10, (5–9) SDSS DR10 photometric data, (10–12) 2MASS photometric data, and (13) colour excess E(BV) (Duras et al., in prep.). (a)See Paper I for the analysis of the LBT/LUCI spectra of these objects.

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