\begin{table}%t5
    \caption{\label{t5}Absolute magnitudes and spectrophotometric distances for confirmed 
nearby dwarfs not known to be binaries.}
    %\centering
\par
\begin{tabular}{lllll}
   \hline 
   \hline\\[-3mm]
  DENIS name  &   SpT  &  $M_{\rm J}$  &  Distance (pc) &  Distance error    \\
 (1)        &   (2)  &  (3)    &  (4)           &  (5)               \\                       
   \hline
J0000286$-$124514 & dM9.5 & 11.65 & 19.2 & 3.6  \\ %1
J0006579$-$643654 & dL0   & 11.83 & 20.9 & 3.8  \\ %2
J0014554$-$484417 & dL2.5 & 12.74 & 17.7 & 3.1  \\ %3
J0028554$-$192716 & dL0.5 & 12.01 & 24.4 & 5.4  \\ %4
J0031192$-$384035 & dL2.5 & 12.74 & 18.7 & 3.4  \\ %5
J0050244$-$153818 & dL0.5 & 12.01 & 21.4 & 3.9  \\ %6
J0053189$-$363110 & dL2.5 & 12.74 & 19.7 & 3.8  \\ %7
J0055005$-$545026 & dM8.5 & 11.28 & 31.0 & 7.1  \\ %8
J0116529$-$645557 & dL1   & 12.19 & 28.1 & 5.2  \\ %9
J0128266$-$554534 & dL1   & 12.19 & 21.0 & 4.1  \\ %10 
J0206566$-$073519 & dM8.5 & 11.28 & 40.9 & 7.7  \\ %13
J0213371$-$134322 & dM9   & 11.47 & 36.5 & 7.7  \\ %14
J0224120$-$763320 & dL0   & 11.83 & 50.8 & 11.2 \\ %15
J0227102$-$162446 & dL0   & 11.83 & 23.3 &  4.5 \\ %16
J0230450$-$095305 & dL0   & 11.83 & 37.2 &  8.2 \\ %17
J0240121$-$530552 & dM9.5 & 11.65 & 34.7 &  6.4 \\ %18
J0301488$-$590302 & dM9   & 11.47 & 24.7 &  4.3 \\ %19 
J0314352$-$462341 & dL2   & 12.56 & 28.9 &  6.0 \\ %20
J0325293$-$431229 & dM8.5 & 11.28 & 37.6 &  6.9 \\ %21 
J0427271$-$112713 & dM7   & 10.92 & 33.3 &  5.8 \\ %23
J0428510$-$225322 & dL0.5 & 12.01 & 19.4 &  3.4 \\ %24 
J0436360$-$295947 & dM8   & 11.10 & 55.2 & 11.2 \\ %25
J0443373$+$000205 & dM9.5 & 11.65 & 15.0 &  2.8 \\ %26
J0529572$-$200300 & dM9   & 11.47 & 39.9 &  6.0 \\ %27 
J0608528$-$275358 & dM9.5 & 11.65 & 25.5 &  4.6 \\ %28 
J0610008$-$472741  & dM8.5 & 11.28 & 43.2 &  8.5 \\ %29
J0620165$-$430010  & dM8   & 11.10 & 59.1 & 11.7 \\ %30
J0719317$-$505141 & dL1   & 12.19 & 23.0 &  4.1 \\ %31 
J0921141$-$210445 & dL3   & 12.92 &  9.7 &  1.7 \\ %32
J0953213$-$101420 & dL0   & 11.83 & 21.8 &  3.8 \\ %33  
J1004283$-$114648 & dM8   & 11.10 & 56.2 & 11.6 \\%34
J1004403$-$131818 & dL0   & 11.83 & 36.8 &  9.2 \\ %35
J1019245$-$270717 & dL0.5 & 12.01 & 20.5 &  3.6 \\ %36
J1115297$-$242934 & dM8   & 11.10 & 28.5 &  4.9 \\ %37
J1206501$-$393725 & dL2   & 12.56 & 22.4 &  4.1 \\ %38 
J1216121$-$125731 & dM8   & 11.10 & 63.6 & 16.4 \\ %39 
J1234018$-$112407 & dM9.5 & 11.65 & 39.5 &  7.8 \\ %41 
J1256569$+$014616 & dL1.5 & 12.38 & 25.8 &  4.6 \\ %42 
J1359551$-$403456 & dL2   & 12.56 & 17.6 &  3.2 \\ %43 
J1411051$-$791536 & dM8.5 & 11.28 & 23.4 &  4.1 \\ %44 
J1622326$-$120719 & dM9.5 & 11.65 & 22.0 &  3.8 \\ %52
J1633131$-$755322 & dM9.5 & 11.65 & 19.5 &  3.3 \\ %53
J1707252$-$013809 & dL0.5 & 11.47 & 54.8 & 10.1 \\ %55
J1753452$-$655955 & dL2   & 12.56 & 21.4 &  3.9 \\ %57 
J1907440$-$282420 & dM9   & 11.47 & 37.7 &  7.3 \\ %59
J1926005$-$650006 & dM9   & 11.47 & 41.4 &  8.0 \\ %60 
J1934511$-$184134 & dM8.5 & 11.28 & 39.7 &  7.5 \\ %61
J1956460$-$774717 & dM9.5 & 11.65 & 32.1 &  6.1 \\ %63
J2013108$-$124244 & dL1.5 & 12.38 & 26.8 &  5.6 \\%64
J2030412$-$363509 & dM8   & 11.10 & 43.8 &  7.9 \\ %65
J2045024$-$633206 & dM9.5 & 11.65 & 15.9 &  3.1 \\ %66 
J2126340$-$314322 & dM9.5 & 11.65 & 20.4 &  4.0 \\ %67
J2139136$-$352950 & dL0   & 11.83 & 33.7 &  6.4 \\ %68
J2143510$-$833712 & dM9.5 & 11.65 & 20.4 &  3.4 \\ %69 
J2150133$-$661036 & dL0   & 11.83 & 23.4 &  4.1 \\ %70
J2150149$-$752035 & dL1   & 12.19 & 22.3 &  4.0 \\ %71
J2243169$-$593219 & dM9   & 11.47 & 33.3 &  6.1 \\ %72
J2308113$-$272200 & dL1.5 & 12.38 & 27.6 &  6.0 \\ %73
J2322468$-$313323 & dL1   & 12.19 & 18.7 &  3.7 \\ %74
J2329343$-$540854  & dL3   & 12.92 & 25.6 &  4.9 \\ %75
J2330226$-$034717 & dL0.5 & 12.01 & 30.2 &  6.3 \\ %76
J2345390$+$005514 & dM9   & 11.47 & 28.2 &  5.6 \\ %77 
J2354599$-$185221 & dL2   & 12.56 & 21.5 &  3.9 \\ %78 
    \hline 
   \end{tabular}
\tablefoot{Column 1: DENIS name. 
Column 2: spectral type adopted in this paper. 
Column 3: absolute $J$-band magnitude estimated from
the absolute magnitude vs. $I-J$ color relationship 
given in Phan-Bao et al. (\cite{Phan2008}). 
Column 4: spectrophometric distance in parsecs.}
\end{table}