\begin{table}%ta1
\caption{\label{sample}Pleiades spectroscopic sample of 45 low-mass stars and brown dwarfs.}
\par
{ { 
\begin{tabular}{l c c c c c c c c c}
\hline\hline \noalign{\smallskip}
Object & SpT & $\alpha$\tablefootmark{a} ~$\delta$\tablefootmark{a} & $I_{\rm C}$ & $Z$\tablefootmark{b} & $Y$\tablefootmark{b} & $J$\tablefootmark{b} & $H$\tablefootmark{b} & $K$\tablefootmark{b} & Ref.\tablefootmark{c} \\ 
&     & &  (mag)      &(mag)&(mag)&(mag)&(mag)&(mag)& \\ 
\hline	 
\object{HHJ~2}           &  M6.5 & 03 38 27.52~~~25 30 18.1 &  17.30 &  16.591 $\pm$ 0.011   &  15.938 $\pm$ 0.007   &  15.284 $\pm$ 0.007   &  14.747 $\pm$ 0.005   &  14.355 $\pm$ 0.006   & 1,--,1,7  \\ 
\object{HHJ~3}           &  M6.0 & 03 48 50.45~~~22 44 29.9 &  17.51 &  16.562 $\pm$ 0.010   &  15.825 $\pm$ 0.006   &  15.098 $\pm$ 0.006   &  14.531 $\pm$ 0.005   &  14.141 $\pm$ 0.004   & 1,--,1,7  \\ 
\object{HHJ~6}           &  M6.5 & 03 41 42.41~~~23 54 57.1 &  17.00 &  16.171 $\pm$ 0.007   &  15.464 $\pm$ 0.006   &  14.709 $\pm$ 0.004   &  14.124 $\pm$ 0.004   &  13.760 $\pm$ 0.050   & 1,--,1,7  \\ 
\object{HHJ~7}           &  M6.0 & 03 57 49.37~~~22 08 31.0 &  17.00 &  16.149 $\pm$ 0.007   &  15.498 $\pm$ 0.005   &  14.831 $\pm$ 0.005   &  14.286 $\pm$ 0.005   &  13.884 $\pm$ 0.003   & 1,--,1,7  \\ 
%martin1996
\object{PPl~1}           &  M6.5 & 03 45 41.27~~~23 54 09.8 &  18.21 &  17.166 $\pm$ 0.014   &  16.189 $\pm$ 0.008   &  15.360 $\pm$ 0.006   &  14.782 $\pm$ 0.005   &  14.305 $\pm$ 0.006   & 4,8,7,5   \\ 
\object{PPl~14}          &  M5.5 & 03 44 34.30~~~23 51 24.6 &  17.43 &  16.920 $\pm$ 0.011   &  16.157 $\pm$ 0.007   &  15.438 $\pm$ 0.007   &  14.884 $\pm$ 0.005   &  14.478 $\pm$ 0.006   & 4,2,7,1   \\ 
\object{PPl~15}          &  M6.5 & 03 48 04.66~~~23 39 30.2 &  17.91 &  17.014 $\pm$ 0.012   &  16.054 $\pm$ 0.007   &  15.283 $\pm$ 0.006   &  14.704 $\pm$ 0.005   &  14.256 $\pm$ 0.006   & 4,2,7,2   \\ 
\object{Calar~3}         &  M8.0 & 03 51 25.57~~~23 45 21.3 &  19.00 &         ...         &         ...         &  16.083 $\pm$ 0.010   &  15.478 $\pm$ 0.009   &  15.009 $\pm$ 0.011   & 4,3,5,3   \\ 
\object{Teide~1}         &  M8.0 & 03 47 17.92~~~24 22 31.7 &  19.26 &  18.174 $\pm$ 0.029   &  17.067 $\pm$ 0.013   &  16.215 $\pm$ 0.010   &  15.591 $\pm$ 0.009   &  15.096 $\pm$ 0.011   & 4,3,5,2   \\ 
%cossburn1997
\object{PIZ~1}           &  M9.0 & 03 48 31.52~~~24 34 37.3 &  20.00 &  19.218 $\pm$ 0.065   &  17.883 $\pm$ 0.025   &  16.715 $\pm$ 0.015   &  15.977 $\pm$ 0.012   &  15.357 $\pm$ 0.014   & 5,--,7,6  \\ 
%zapateroosorio1997b
\object{Roque~4}\tablefootmark{d}   &  M9.0 & 03 43 53.55~~~24 31 11.6 &  20.25 &  18.970 $\pm$ 0.054   &  17.709 $\pm$ 0.025   &  16.649 $\pm$ 0.016   &  15.942 $\pm$ 0.016   &  15.260 $\pm$ 0.040   & 6,--,--,5 \\ 
\object{Roque~11}        &  M8.0 & 03 47 12.08~~~24 28 31.7 &  19.06 &         ...         &  16.988 $\pm$ 0.013   &  16.174 $\pm$ 0.087   &  15.505 $\pm$ 0.009   &  15.048 $\pm$ 0.012   & 6,--,8,2  \\ 
\object{Roque~13}        &  M7.5 & 03 45 50.66~~~24 09 03.5 &  18.67 &  17.478 $\pm$ 0.017   &  16.582 $\pm$ 0.010   &  15.705 $\pm$ 0.008   &  15.095 $\pm$ 0.006   &  14.580 $\pm$ 0.008   & 6,8,7,5   \\ 
\object{Roque~14}        &  M7.0 & 03 46 42.98~~~24 24 50.7 &  18.27 &  17.484 $\pm$ 0.018   &  16.403 $\pm$ 0.009   &  15.550 $\pm$ 0.066   &  14.890 $\pm$ 0.006   &  14.391 $\pm$ 0.007   & 6,--,8,7  \\ 
\object{Roque~16}        &  M6.0 & 03 47 39.02~~~24 36 22.2 &  17.91 &  17.112 $\pm$ 0.013   &  16.271 $\pm$ 0.008   &  15.548 $\pm$ 0.007   &  14.992 $\pm$ 0.006   &  14.570 $\pm$ 0.008   & 6,8,7,3   \\ 
\object{Roque~17}        &  M6.5 & 03 47 23.97~~~22 42 37.4 &  17.87 &         ...         &  16.123 $\pm$ 0.008   &  15.354 $\pm$ 0.007   &  14.809 $\pm$ 0.006   &  14.402 $\pm$ 0.007   & 6,--,2,7  \\ 
%martin1998a
\object{Teide~2}         &  M6.0 & 03 52 06.72~~~24 16 00.5 &  18.02 &  17.079 $\pm$ 0.013   &  16.255 $\pm$ 0.009   &  15.515 $\pm$ 0.008   &  14.971 $\pm$ 0.008   &  14.507 $\pm$ 0.008   & 7,7,7,3   \\ 
%stauffer1998a
\object{CFHT~9}          &  M6.5 & 03 49 15.12~~~24 36 22.5 &  17.71 &  16.847 $\pm$ 0.011   &  16.059 $\pm$ 0.007   &  15.371 $\pm$ 0.006   &  14.890 $\pm$ 0.005   &  14.433 $\pm$ 0.007   & 8,8,7,3   \\ 
\object{CFHT~10}         &  M6.5 & 03 44 32.32~~~25 25 18.0 &  17.78 &  16.994 $\pm$ 0.012   &  16.209 $\pm$ 0.009   &  15.450 $\pm$ 0.008   &  14.883 $\pm$ 0.007   &  14.476 $\pm$ 0.007   & 8,8,7,3   \\ 
\object{CFHT~12}         &  M8.0 & 03 53 55.12~~~23 23 36.2 &  17.97 &  16.947 $\pm$ 0.012   &  16.027 $\pm$ 0.007   &  15.172 $\pm$ 0.006   &  14.569 $\pm$ 0.005   &  14.088 $\pm$ 0.005   & 8,8,3,3   \\ 
\object{CFHT~15}         &  M7.0 & 03 55 12.60~~~23 17 37.3 &  18.62 &  17.842 $\pm$ 0.022   &  16.877 $\pm$ 0.012   &  15.977 $\pm$ 0.010   &  15.348 $\pm$ 0.009   &  14.842 $\pm$ 0.010   & 8,8,3,3   \\ 
\object{MHObd~3 }        &  M8.0 & 03 41 54.16~~~23 05 04.7 &  18.27 &  17.349 $\pm$ 0.016   &  16.376 $\pm$ 0.010   &  15.522 $\pm$ 0.008   &  14.975 $\pm$ 0.007   &  14.415 $\pm$ 0.007   & 8,8,7,4   \\ 
%festin1998b
\object{NPL~26}          &  M5.0 & 03 47 07.89~~~24 23 37.9 &  15.70 &  15.094 $\pm$ 0.004   &  14.598 $\pm$ 0.003   &  13.954 $\pm$ 0.003   &  13.415 $\pm$ 0.002   &  13.080 $\pm$ 0.002   & 9,--,4,2 \\ 
\object{NPL~34}          &  M6.0 & 03 48 55.65~~~24 21 40.1 &  17.05 &  16.220 $\pm$ 0.007   &  15.636 $\pm$ 0.005   &  14.963 $\pm$ 0.005   &  14.416 $\pm$ 0.004   &  14.055 $\pm$ 0.005   & 9,--,1,2 \\ 
\object{NPL~36}          &  M7.5 & 03 48 19.02~~~24 25 12.7 &  18.66 &  17.655 $\pm$ 0.020   &  16.668 $\pm$ 0.011   &  15.930 $\pm$ 0.009   &  15.365 $\pm$ 0.008   &  14.935 $\pm$ 0.011   & 9,--,7,2 \\ 
\object{NPL~38}          &  M8.0 & 03 47 50.41~~~23 54 47.9 &  19.18 &  18.179 $\pm$ 0.028   &  17.138 $\pm$ 0.014   &  16.311 $\pm$ 0.011   &  15.622 $\pm$ 0.009   &  15.093 $\pm$ 0.012   & 9,--,8,2 \\ 
%stauffer1998b
\object{MHObd~1}         &  M7.0 & 03 44 52.42~~~24 36 49.5 &  17.95 &  17.147 $\pm$ 0.014   &  16.294 $\pm$ 0.008   &  15.487 $\pm$ 0.059   &  14.948 $\pm$ 0.006   &  14.525 $\pm$ 0.007   & 10,10,--,4 \\ 
%martin1998b
\object{Roque~5}         &  M9.0 & 03 44 22.44~~~23 39 01.3 &  20.19 &  19.107 $\pm$ 0.064   &  17.857 $\pm$ 0.025   &  16.874 $\pm$ 0.017   &  16.254 $\pm$ 0.016   &  15.666 $\pm$ 0.018   & 11,--,7,5 \\ 
%martin2000
\object{CFHT~1}          &  M4.9 & 03 51 51.56~~~23 34 49.1 &  16.10 &  15.431 $\pm$ 0.005   &  14.857 $\pm$ 0.004   &  14.260 $\pm$ 0.003   &  13.768 $\pm$ 0.003   &  13.385 $\pm$ 0.003   & 12,--,3,3 \\ 
\object{CFHT~2}          &  M4.9 & 03 52 44.29~~~23 54 15.0 &  16.61 &  15.738 $\pm$ 0.005   &  15.184 $\pm$ 0.004   &  14.554 $\pm$ 0.004   &  14.000 $\pm$ 0.004   &  13.654 $\pm$ 0.004   & 12,--,3,3 \\ 
\object{CFHT~5}          &  M5.5 & 03 48 44.69~~~24 37 23.5 &  17.02 &  16.260 $\pm$ 0.008   &  15.584 $\pm$ 0.005   &  14.911 $\pm$ 0.005   &  14.419 $\pm$ 0.004   &  14.002 $\pm$ 0.005   & 12,--,7,3 \\ 
%CFHT~6_pmnotmemb & M6.9 & 03 52 07.88~~~23 59 13.1 &  17.11 &  16.169 $\pm$ 0.007   &  15.371 $\pm$ 0.005   &  14.636 $\pm$ 0.005   &  14.066 $\pm$ 0.004   &  13.640 $\pm$ 0.004   & 12,--,7,3 \\ 
\object{CFHT~7}          &  M5.6 & 03 52 05.83~~~24 17 31.0 &  17.34 &  16.512 $\pm$ 0.009   &  15.860 $\pm$ 0.007   &  15.176 $\pm$ 0.006   &  14.618 $\pm$ 0.006   &  14.251 $\pm$ 0.007   & 12,--,7,3 \\ 
\object{CFHT~16}         &  M9.3 & 03 44 35.16~~~25 13 42.8 &  18.66 &  17.656 $\pm$ 0.020   &  16.584 $\pm$ 0.010   &  15.662 $\pm$ 0.007   &  14.985 $\pm$ 0.006   &  14.448 $\pm$ 0.008   & 12,12,7,3 \\ 
\object{CFHT~17}         &  M7.9 & 03 43 00.17~~~24 43 52.3 &  18.80 &  17.791 $\pm$ 0.021   &  16.841 $\pm$ 0.013   &  16.022 $\pm$ 0.010   &  15.425 $\pm$ 0.010   &  15.070 $\pm$ 0.060   & 12,--,3,3 \\ 
\object{CFHT~25}         &  M9.0 & 03 54 05.35~~~23 33 59.3 &  19.69 &  18.651 $\pm$ 0.041   &  17.573 $\pm$ 0.024   &  16.647 $\pm$ 0.018   &  15.964 $\pm$ 0.016   &  15.434 $\pm$ 0.017   & 12,--,3,3 \\ 
%CFHT~26_?       & M7.1 & 03 54 01.41~~~24 44 46.7 &  20.21 &  19.768 $\pm$ 0.124   &  18.534 $\pm$ 0.053   &  17.775 $\pm$ 0.042   &  17.194 $\pm$ 0.045   &  16.809 $\pm$ 0.055   & 12,--,--,3 \\ 
\object{NPL~40}          &  M9.8 & 03 48 49.03~~~24 20 25.4 &  20.55 &  19.222 $\pm$ 0.069   &  18.227 $\pm$ 0.035   &  17.237 $\pm$ 0.023   &  16.569 $\pm$ 0.020   &  16.059 $\pm$ 0.029   & 12,--,8,2 \\ 
\object{Roque~7}         &  M8.3 & 03 43 40.31~~~24 30 11.2 &  19.50 &  18.552 $\pm$ 0.038   &  17.490 $\pm$ 0.021   &  16.494 $\pm$ 0.014   &  15.853 $\pm$ 0.015   &  15.470 $\pm$ 0.020   & 12,--,3,3 \\ 
\object{Roque~25}        &  L0.1 & 03 48 30.75~~~22 44 50.4 &  21.80 &  20.389 $\pm$ 0.193   &  18.936 $\pm$ 0.065   &  17.714 $\pm$ 0.039   &  16.861 $\pm$ 0.035   &  16.251 $\pm$ 0.027   & 12,--,9,5 \\ 
%pinfield2003
\object{BPL~327}         &  M7.1 & 03 55 23.08~~~24 49 04.9 &  18.07 &  17.087 $\pm$ 0.014   &  16.311 $\pm$ 0.009   &  15.528 $\pm$ 0.008   &  15.013 $\pm$ 0.007   &  14.595 $\pm$ 0.008   & 13,--,6,5 \\ 
%BPL~45_nopminfo &  M8.1 & 03 42 48.17~~~24 04 01.2 &  18.87 &  17.739 $\pm$ 0.020   &  16.847 $\pm$ 0.012   &  16.038 $\pm$ 0.010   &  15.466 $\pm$ 0.011   &  14.936 $\pm$ 0.010   & 13,--,--,5 \\ 
%this study
\object{BRB~17}          &  L0.0 & 03 54 07.98~~~23 54 27.9 &  20.92 &  19.841 $\pm$ 0.111   &  18.451 $\pm$ 0.050   &  17.408 $\pm$ 0.033   &  16.628 $\pm$ 0.030   &  16.028 $\pm$ 0.029   & 14,--,5,6  \\ 
\object{PLIZ~28}         &  L0.0 & 03 54 14.06~~~23 17 52.0 &  21.20 &  20.028 $\pm$ 0.136   &  18.873 $\pm$ 0.062   &  17.601 $\pm$ 0.035   &  16.818 $\pm$ 0.031   &  16.138 $\pm$ 0.030   & 14,--,5,6  \\ 
\object{PLIZ~35}         &  L2.0 & 03 52 39.16~~~24 46 29.5 &  21.46 &  20.292 $\pm$ 0.030   &  19.271 $\pm$ 0.100   &  18.066 $\pm$ 0.055   &  17.106 $\pm$ 0.042   &  16.509 $\pm$ 0.042   & 14,--,5,6  \\ 
\object{BRB~21}          &  L3.0 & 03 54 10.27~~~23 41 40.2 &  21.68 &  20.215 $\pm$ 0.030   &  19.260 $\pm$ 0.101   &  18.143 $\pm$ 0.062   &  17.171 $\pm$ 0.046   &  16.393 $\pm$ 0.040   & 14,--,5,6  \\ 
\object{BRB~23}          &  L3.5 & 03 50 39.54~~~25 02 54.7 &  22.03 &         ...         &  19.786 $\pm$ 0.112   &  18.225 $\pm$ 0.044   &  17.358 $\pm$ 0.038   &  16.563 $\pm$ 0.043   & 14,--,5,6  \\ 
\object{BRB~29}          &  L4.5 & 03 54 01.43~~~23 49 57.7 &  22.84 &         ...         &         ...         &  18.686 $\pm$ 0.103   &  17.711 $\pm$ 0.081   &  16.999 $\pm$ 0.070   & 14,--,5,6  \\ 
\hline                  
\end{tabular}}}
\vspace*{-1.5mm}
\tablefoot {\tablefoottext{a}{Coordinates from UKIDSS Galaxy Cluster Survey DDR6.} \tablefoottext{b}{$ZYJHK$-band photometry from UKIDSS Galaxy Cluster Survey DDR6, except for the
measurements at $Z$~band of PLIZ~35 and BRB~21 \citep{casewell2007}, MKO
$K$~band of HHJ~6, Roque~4, CFHT~17, and Roque~7 \citep{pinfield2003}, and
$J$~band of MHObd~1 (2MASS, converted to UKIDSS photometric system).}
\tablefoottext{c}{References for the quadruplet (SpT,Li,$\mu$,$I_{\rm C}$): {\it Spectral type or lithium test}: 1)~\citet{steele1995a}; 2)~\citet{basri1996}; 3)~\citet{rebolo1996}; 4)~\citet{martin1996}; 5)~\citet{cossburn1997}; 6)~\citet{zapateroosorio1997b}; 7)~\citet{martin1998a}; 8)~\citet{stauffer1998a}; 9)~\citet{festin1998b}; 10)~\citet{stauffer1998b}; 11)~\citet{martin1998b}; 12)~\citet{martin2000}; 13)~\citet{pinfield2003}; 14)~this study. Spectral type uncertainties for our \mbox{L-type} targets are listed in Table~\ref{log}; for the other objects the uncertainties are typically of half a subclass. {\it Proper motion}: 1)~\citet{hambly1993}; 2)~\citet{pinfield2000}; 3)~\citet{moraux2001}; 4)~\citet{deacon2004}; 5)~\citet{bihain2006};  6)~\citet{casewell2007}; 7)~\citet{lodieu2007}; 8)~\citet{stauffer2007}; 9) this study. {\it $I_{\rm C}$-band photometry}: 1)~\citet{stauffer1994}; 2)~\citet{festin1998a}; 3)~\citet{bouvier1998}; 4)~\citet{stauffer1998b}; 5) \citet{jameson2002}; 6)~\citet{bihain2006}; 7)~\citet{stauffer2007}. Magnitude errors are of 0.05--0.1~mag.} \tablefoottext{d}{Roque~4 has radial velocity and spectral features consistent with cluster membership \citep{zapateroosorio1997b,kirkpatrick2008}.}}
\vspace*{-1.5mm}
\end{table}