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Table 3.

Photometric properties of the new 16 quasars.

Name i z Y J H Ks W1 W2 zml χBD2/χquasars2
LS J1451−0445 23.69 ± 0.17 20.83 ± 0.01 20.94 ± 0.23 20.63 ± 0.17 20.21 ± 0.19 20.02 ± 0.06 20.02 ± 0.14 6.1 4.37
LS J2301−1530 24.75 ± 0.80 20.65 ± 0.03 20.16 ± 0.08 20.07 ± 0.10 19.74 ± 0.18 19.78 ± 0.05 19.91 ± 0.13 6.37 2.89
LS J0208−6647 23.44 ± 0.14 20.17 ± 0.01 20.72 ± 0.10 19.85 ± 0.14 19.18 ± 0.02 18.82 ± 0.03 6.11 5.53
LS J2223−3815 23.56 ± 0.20 20.57 ± 0.03 19.84 ± 0.04 19.77 ± 0.12 19.92 ± 0.05 19.92 ± 0.11 6.30 2.25
LS J0006−7935 23.60 ± 0.09 20.57 ± 0.02 20.58 ± 0.16 20.56 ± 0.17 20.21 ± 0.27 19.95 ± 0.04 19.92 ± 0.08 6.10 5.87
LS J0104−6857 23.75 ± 0.21 20.50 ± 0.02 20.83 ± 0.19 20.89 ± 0.22 19.81 ± 0.19 19.90 ± 0.04 19.33 ± 0.05 6.11 3.71
LS J1035−0515 23.34 ± 0.22 20.14 ± 0.01 20.51 ± 0.15 19.68 ± 0.07 19.14 ± 0.07 18.55 ± 0.05 18.32 ± 0.01 18.19 ± 0.03 6.43 2.16
LS J1130+1420 24.66 ± 0.39 21.05 ± 0.03 21.13 ± 0.21 20.61 ± 0.20 20.48 ± 0.24 20.31 ± 0.08 20.20 ± 0.16 6.20 21.09
LS J1332+1102 24.17 ± 0.36 20.80 ± 0.04 20.50 ± 0.13 20.29 ± 0.11 20.03 ± 0.13 19.85 ± 0.12 19.95 ± 0.05 20.38 ± 0.18 6.22 2.92
LS J1435−1053 24.64 ± 0.53 21.27 ± 0.04 20.49 ± 0.21 20.51 ± 0.09 21.22 ± 0.42 6.21 1.24
LS J1141+1006 24.08 ± 0.31 21.14 ± 0.02 21.19 ± 0.22 20.95 ± 0.27 20.58 ± 0.22 20.93 ± 0.14 21.50 ± 0.56 6.07 2.70
LS J1330−4025 22.80 ± 0.08 20.13 ± 0.01 20.58 ± 0.25 19.94 ± 0.25 19.72 ± 0.04 19.46 ± 0.07 6.03 11.61
LS J2011−4436 23.90 ± 0.26 20.95 ± 0.03 20.44 ± 0.10 19.59 ± 0.10 19.32 ± 0.03 19.26 ± 0.06 6.31 2.90
LS J2037−5152 25.55 ± 0.70 21.08 ± 0.04 21.00 ± 0.17 20.32 ± 0.21 20.40 ± 0.08 19.75 ± 0.09 6.18 1.30
LS J2155−5111 25.45 ± 0.34 21.35 ± 0.03 21.05 ± 0.22 20.65 ± 0.09 20.41 ± 0.16 6.24 2.51
LS J0139−5209 23.24 ± 0.08 20.65 ± 0.01 20.71 ± 0.12 20.27 ± 0.23 20.35 ± 0.07 20.64 ± 0.19 6.05 1.83

Notes. Col. (1): Abbreviated quasar name; Cols. (2)–(3): optical magnitudes from LS DR10, Cols. (4)–(7): NIR magnitudes from UKIDSS DR11, VHS DR5 or UHS DR2; Cols. (8)–(9): MIR magnitudes from WISE; Col. (10): maximum-likelihood photometric redshift estimated by eazy-py; Col. (11): stellar contaminant-to-quasar χ2 ratio used for the prioritization of the candidates.

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