\begin{table}%t2
\par
 \caption{\label{tab2}Photometric data of UKIDSS matched L dwarf
candidates.}
 %\centerline
 {
 \begin{tabular}{c c c c c c c c
c c c l} \hline\hline
SDSS Name & SDSS {\it r} & SDSS {\it i} & SDSS {\it z} & 2MASS {\it J} & 2MASS {\it H} & 2MASS {\it K} & UKIDSS {\it Y} & UKIDSS {\it J} & UKIDSS {\it H} & UKIDSS {\it K} & Sp. Type$^{{a}}$ \\
\hline
~~J004759.59$+$135332.0$^{{b}}$ & 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$-$005156.5$^{{c}}$ & 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$~0.02 & ... & ... & L2 \\
~~J083613.45$+$022106.2$^{{c}}$ & 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$~0.02 & L8.5 \\
\hline
\end{tabular}}
\par
\smallskip
Notes: UKIDSS magnitude limits for {\it Y}, {\it J}, {\it H} and
{\it K}~bands are~20.5, 20.0, 18.8 and~18.4 respectively. All
magnitudes here are Vega based. We use~0.1$^{\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 ({\it i-z}, {\it i-J}, {\it i-H},
{\it i-K} are used largely and
{\it r-i}, {\it z-J}, {\it z-H}, {\it 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
({\it i-J, i-H} and {\it i-K}) according to Eq.~(9).
$^{{c}}$ Data errors of {\it J, H, K}~bands are less
than~0.005.
\end{table}