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Table 2:

Photometric data of UKIDSS matched L dwarf candidates.
SDSS Name SDSS r SDSS i SDSS z 2MASS J 2MASS H 2MASS K UKIDSS Y UKIDSS J UKIDSS H UKIDSS K Sp. Typea
  J004759.59+135332.0b 24.78 $\pm$ 0.88 22.11 $\pm$ 0.28 19.61 $\pm$ 0.10 16.81 $\pm$ 0.16 16.10 $\pm$ 0.17 15.51 $\pm$ 0.19 18.03 $\pm$ 0.03 17.22 $\pm$ 0.03 16.52 $\pm$ 0.03 16.00 $\pm$ 0.03 L3.5
  J015141.04-005156.5c 22.23 $\pm$ 0.15 19.70 $\pm$ 0.03 17.61 $\pm$ 0.02 15.10 $\pm$ 0.05 14.27 $\pm$ 0.04 13.59 $\pm$ 0.05 16.24 $\pm$ 0.01 15.02 $\pm$ 0.00 14.29 $\pm$ 0.00 13.65 $\pm$ 0.00 L2
J022927.95-005328.5 24.19 $\pm$ 0.64 21.54 $\pm$ 0.11 19.41 $\pm$ 0.07 16.49 $\pm$ 0.10 15.75 $\pm$ 0.10 15.18 $\pm$ 0.14 ... 16.62 $\pm$ 0.02 15.82 $\pm$ 0.02 15.15 $\pm$ 0.02 L3.5
J073241.77+264558.9 24.31 $\pm$ 0.46 22.40 $\pm$ 0.18 19.83 $\pm$ 0.08 17.37 $\pm$ 0.21 16.81 $\pm$ 0.25 15.64 $\pm$ 0.19 ... 17.55 $\pm$ 0.02 ... ... L4.5
J074436.02+251330.5 24.28 $\pm$ 0.49 21.23 $\pm$ 0.07 18.77 $\pm$ 0.03 17.17 $\pm$ 0.25 16.04 $\pm$ 0.21 15.66 $\pm$ 0.22 ... 16.68 $\pm$ 0.01 ... ... L1
J075754.16+221604.9 23.34 $\pm$ 0.36 21.45 $\pm$ 0.10 19.41 $\pm$ 0.06 16.61 $\pm$ 0.13 16.10 $\pm$ 0.22 15.30 $\pm$ 0.14 ... 16.87 $\pm$ 0.01 ... ... L2.5
J081303.96+243355.9 23.41 $\pm$ 0.38 21.32 $\pm$ 0.08 19.30 $\pm$ 0.05 16.67 $\pm$ 0.12 15.63 $\pm$ 0.12 14.97 $\pm$ 0.09 ... 16.57 $\pm$ 0.01 ... ... L3
J081409.45+260250.4 25.06 $\pm$ 0.67 21.88 $\pm$ 0.15 19.69 $\pm$ 0.10 17.18 $\pm$ 0.18 16.50 $\pm$ 0.21 15.76 $\pm$ 0.19 ... 17.25 $\pm$ 0.02 ... ... L2
  J083613.45+022106.2c 22.36 $\pm$ 0.16 19.12 $\pm$ 0.02 17.09 $\pm$ 0.01 14.76 $\pm$ 0.04 14.17 $\pm$ 0.04 13.71 $\pm$ 0.04 15.73 $\pm$ 0.01 14.72 $\pm$ 0.00 14.18 $\pm$ 0.00 13.68 $\pm$ 0.00 L0.5
J092745.81+010640.4 24.03 $\pm$ 0.68 21.34 $\pm$ 0.10 19.21 $\pm$ 0.06 16.97 $\pm$ 0.20 16.18 $\pm$ 0.21 15.37 $\pm$ 0.21 18.05 $\pm$ 0.03 17.11 $\pm$ 0.01 16.55 $\pm$ 0.02 15.99 $\pm$ 0.03 L1
J094624.37+344639.8 23.40 $\pm$ 0.30 20.92 $\pm$ 0.05 18.82 $\pm$ 0.03 16.44 $\pm$ 0.10 15.79 $\pm$ 0.13 15.14 $\pm$ 0.12 ... 16.33 $\pm$ 0.01 ... ... L1
J095941.47+114146.0 23.51 $\pm$ 0.38 21.30 $\pm$ 0.08 19.29 $\pm$ 0.05 16.43 $\pm$ 0.14 15.66 $\pm$ 0.13 15.24 $\pm$ 0.19 ... ... ... 15.27 $\pm$ 0.01 L3
J121238.73+000721.6 24.02 $\pm$ 0.66 20.85 $\pm$ 0.09 18.25 $\pm$ 0.03 15.81 $\pm$ 0.10 15.01 $\pm$ 0.09 14.46 $\pm$ 0.09 ... 15.69 $\pm$ 0.01 ... ... L3.5
J133131.70+122531.4 24.62 $\pm$ 0.66 21.32 $\pm$ 0.10 19.32 $\pm$ 0.05 16.78 $\pm$ 0.16 15.72 $\pm$ 0.17 15.28 $\pm$ 0.15 17.83 $\pm$ 0.03 16.72 $\pm$ 0.01 16.03 $\pm$ 0.02 15.46 $\pm$ 0.01 L2.5
J134531.43+001551.2 24.14 $\pm$ 0.51 21.59 $\pm$ 0.11 19.47 $\pm$ 0.08 16.94 $\pm$ 0.21 15.98 $\pm$ 0.14 15.55 $\pm$ 0.23 18.19 $\pm$ 0.03 16.95 $\pm$ 0.02 16.19 $\pm$ 0.02 15.60 $\pm$ 0.02 L2.5
J150153.00-013507.1 22.71 $\pm$ 0.25 20.80 $\pm$ 0.07 18.62 $\pm$ 0.05 16.08 $\pm$ 0.09 14.95 $\pm$ 0.07 14.26 $\pm$ 0.09 ... ... 15.02 $\pm$ 0.01 14.25 $\pm$ 0.01 L3.5
J154236.26-004545.9 24.71 $\pm$ 0.79 21.78 $\pm$ 0.15 19.35 $\pm$ 0.06 16.71 $\pm$ 0.13 15.98 $\pm$ 0.14 15.41 $\pm$ 0.20 18.07 $\pm$ 0.02 16.83 $\pm$ 0.02 16.21 $\pm$ 0.02 15.64 $\pm$ 0.02 L3.5
J154432.77+265551.2 23.22 $\pm$ 0.23 21.31 $\pm$ 0.07 19.10 $\pm$ 0.04 16.22 $\pm$ 0.10 15.24 $\pm$ 0.10 14.64 $\pm$ 0.10 ... 16.23 $\pm$ 0.01 ... ... L4.5
J154740.16+053208.3 23.39 $\pm$ 0.30 20.57 $\pm$ 0.04 18.57 $\pm$ 0.03 16.18 $\pm$ 0.10 15.58 $\pm$ 0.11 15.11 $\pm$ 0.16 17.25 $\pm$ 0.01 16.18 $\pm$ 0.01 15.58 $\pm$ 0.01 15.02 $\pm$ 0.01 L0.5
J161711.68+322249.5 24.80 $\pm$ 0.88 21.25 $\pm$ 0.12 19.03 $\pm$ 0.06 16.56 $\pm$ 0.13 15.69 $\pm$ 0.15 15.42 $\pm$ 0.16 ... 16.68 $\pm$ 0.01 ... ... L2
J232715.71+151730.4 23.26 $\pm$ 0.28 21.31 $\pm$ 0.09 19.13 $\pm$ 0.05 16.29 $\pm$ 0.11 15.35 $\pm$ 0.09 14.77 $\pm$ 0.13 17.54 $\pm$ 0.02 16.20 $\pm$ 0.01 15.36 $\pm$ 0.01 14.68 $\pm$ 0.01 L5
J234040.33-003337.2 23.54 $\pm$ 0.35 21.45 $\pm$ 0.10 19.35 $\pm$ 0.06 17.06 $\pm$ 0.16 16.34 $\pm$ 0.23 15.52 $\pm$ 0.20 17.94 $\pm$ 0.03 17.03 $\pm$ 0.02 16.46 $\pm$ 0.02 16.01 $\pm$ 0.04 L1
J234513.85+002441.6 24.80 $\pm$ 0.71 22.63 $\pm$ 0.29 19.56 $\pm$ 0.08 16.78 $\pm$ 0.16 15.90 $\pm$ 0.20 15.55 $\pm$ 0.19 17.67 $\pm$ 0.03 ... 16.21 $\pm$ 0.02 15.59 $\pm$ 0.02 L8.5
Notes: UKIDSS magnitude limits for Y, J, H and K bands are 20.5, 20.0, 18.8 and 18.4 respectively. All magnitudes here are Vega based. We use 0.1 $^{\prime\prime}$ as a typical position error for UKIDSS. Error ellipses of 2MASS and SDSS overlap for some objects for which proper motion angle errors are not listed; a spectral types are based on the relationship between spectral type and SDSS and 2MASS colors (i-z, i-J, i-H, i-K are used largely and r-i, z-J, z-H, z-K with less weight); b It is merged with a nearby faint galaxy in 2MASS image, so its 2MASS photometric data is not reliable. The spectral type is based on SDSS-UKIDSS colors (i-J, i-H and i-K) according to Eq. (9). c Data errors of J, H, K bands are less than 0.005.

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