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%\{\tiny .}
\footnotesize

\footnotesize
\begin{table}
\caption[  ]{Photometry and evolutionary classification of the sample}
\begin{tabular}{lrccccrrrrll}
\hline
    Name         &    HD  &  (U-B)&(B-V) &(V-R)$_{\rm j}$&(R-I)$_{\rm j}$&D& V & Mv(d,V) & Lum &  Sp.type    &Comments\\
     (1)         &   (2)  &   (3)   &   (4)   &   (5)   &    (6)  &  (7)  &   (8)   &    (9)  &  (10)   &(11)&(12)   \\
\hline      
13 Cet A   p  &     3196   &  0.080  & 0.570  & 0.470  & 0.290  &    21.3  &   5.200  &   3.558  &   off & \{F7V/\}     & a,kc      \\  
13 Cet A   s  &     3196   &   --    &  --    &  --    &  --    &    21.3  &    --    &    --    &   MS  &    --        &           \\  
CF Tuc     s  &     5303   &  0.180  &  --    &  --    &  --    &    54.0  &    --    &   4.4    &   MS  &   G0V        & c,j       \\  
CF Tuc     p  &     5303   &   --    & 0.735  & 0.626  & 0.472  &    54.0  &    --    &   3.748  &   off &   K4IV       & a,kc      \\  
BQ Hyi     p  &    14643   &  0.380  & 0.850  & 0.696  & 0.483  &    77.0  &   8.190  &   3.758  &   off &    G1Vp      & a,kc      \\  
UX For     p  &    17084   &  0.210  & 0.730  & 0.640  & 0.458  &    --    &   7.990  &   5.3    &   MS  &    G5-8V     & a,kc,j    \\  
VY Ari     p  &    17433   &  0.630  & 0.960  & 0.610  & 0.554  &    21.0  &   6.900  &   5.289  &   off &   K3-4V-IV   & a,kc      \\  
V471 Tau   p  &     --     &  0.410  & 0.870  & 0.750  & 0.520  &    59.0  &   9.710  &   5.886  &   MS  &      K2V     & a,d,i     \\  
AG Dor     p  &    26354   &  0.630  & 0.950  & 0.794  & 0.544  &    --    &   8.670  &   6.15   &   MS  &    K1Vp      & a,kc,j    \\  
EI Eri     p  &    26337   &  0.140  & 0.670  & 0.610  & 0.390  &    75.0  &   6.960  &   2.585  &   off &    G5IV      & a         \\  
V818 Tau   p  &    27130   &  0.330  & 0.775  &  --    & 0.254  &    44.7  &   8.313  &   5.158  &   MS  &     G6V      & a,i       \\  
V818 Tau   s  &    27130   &   --    &  --    &  --    &  --    &    44.7  &    --    &   7.73   &   MS  &     K6V      & j         \\  
BD+14 690  p  &    27691   &  0.090  & 0.560  &  --    & 0.330  &    --    &   7.000  &   4.4    &   MS  &    G0V       & a,j       \\  
 vB 69     p  &    28291   &  0.335  & 0.746  &  --    &  --    &    --    &   8.590  &   5.9    &   MS  &    K0V       & a,j       \\  
V833 Tau   p  &   283750   &  0.950  & 1.085  & 0.947  & 0.738  &    16.7  &   8.160  &   7.046  &   MS  &    dK5e      & a,kc      \\  
V808 Tau   1  &   283882   &  0.920  & 1.060  &  --    & 0.420  &    42.0  &  10.423  &   7.307  &   MS  &     K3V      & b         \\  
V808 Tau   2  &   283882   &  0.920  & 1.060  &  --    & 0.420  &    42.0  &  10.423  &   7.307  &   MS  &     K3V      & b         \\  
BD+64 487  1  &    30957   &   --    &  --    &  --    &  --    &    --    &   9.353  &   6.4    &   MS  &     K2V      & j         \\  
BD+64 487  2  &    30957   &   --    &  --    &  --    &  --    &    --    &   9.353  &   6.4    &   MS  &     K2V      & j         \\  
V1198 Ori  p  &    31738   &  0.200  & 0.710  &  --    &  --    &    60.0  &   7.120  &   3.229  &   off &    G5IV      & a         \\  
YY Gem        &      --    &  1.040  & 1.350  & 1.340  &  1.06  &    13.7  &   9.823  &   9.139  &   MS  &    dM1e      & b         \\
HR2814     p  &    57853   &  0.050  & 0.590  &  --    &  --    &    26.0  &   6.600  &   4.525  &   MS  &     F9.5V    & a         \\  
54 Cam     p  &    65626   &  0.165  & 0.620  &  --    &  --    &    38.0  &   6.500  &   2.5    &   off &     F9IV     & a,d,k     \\  
54 Cam     s  &    65626   &   --    &  --    &  --    &  --    &    38.0  &    --    &   2.88   &   off &     G5IV     & k         \\  
TY Pyx     p  &    77137   &  0.260  & 0.720  & 0.550  &  --    &    55.0  &   6.835  &   3.9    &   off &      G5IV    & a,d,e,h   \\  
TY Pyx     s  &    77137   &   --    & 0.760  &  --    &  --    &    55.0  &    --    &   3.8    &   off &      G5IV    & h         \\  
$\xi$ UMa B p &    98230   &  0.220  & 0.590  &  --    &  --    &     7.9  &   4.870  &   5.382  &   MS  &     G5V      & a         \\  
DF UMa     p  &     --     &   --    & 0.890  &  --    &  --    &    22.7  &  10.140  &   8.389  &   MS  &    dM0e      & a,i       \\  
DF UMa     s  &     --     &   --    &  --    &  --    &  --    &    22.7  &    --    &   12.3   &   MS  &    [dM5]     & j         \\  
CD-38 7259 s  &   101309   &   --    &  --    &  --    &  --    &    62.0  &    --    &   5.1    &   MS  &    G5V       & j         \\  
IL Com     1  &   108102   & -0.010  & 0.510  & 0.400  & 0.300  &    86.0  &   8.833  &   4.161  &   MS  &     F8V      & b         \\  
IL Com     2  &   108102   & -0.010  & 0.510  & 0.400  & 0.300  &    86.0  &   8.833  &   4.161  &   MS  &     F8V      & b         \\  
RS CVn     s  &   114519   &  0.090  & 0.420  &  --    &  --    &   180.0  &    --    &   2.6    &   off &     F4IV     & c,h       \\  
MS Ser     p  &   143313   &  0.630  & 0.940  &  --    &  --    &    30.0  &    --    &   6.215  &   MS  &     K2V      & d,e,i     \\  
MS Ser     s  &   143313   &  1.150  & 1.230  &  --    &  --    &    30.0  &    --    &   7.725  &   MS  &     K6V      & j         \\  
$\sigma$$^2$ CrB s  &   146361   &  0.000  & 0.470  & 0.500  &  --    &    21.0  &   5.700  &   4.089  &   MS  &     F6V      & a         \\  
$\sigma$$^2$ CrB p  &   146361   &   --    &  --    &  --    &  --    &    21.0  &    --    &   4.4    &   MS  &     G0V      & j         \\  
WW Dra     s  &   150708   &  0.040  & 0.600  &  --    &  --    &   180.0  &    --    &   2.304  &   off &     G2IV     & d,m       \\  
V792 Her   s  &   155638   &   --    & 0.450  &  --    &  --    &   310.0  &    --    &   2.349  &   off &    F2IV      & m         \\  
 Z Her     p  &   163930   &   --    & 0.590  &  --    &  --    &   100.0  &   7.230  &   2.9    &   off &     F4V-IV   & g,h       \\  
 Z Her     s  &   163930   &   --    &  --    &  --    &  --    &   100.0  &    --    &   3.5    &   off &      K0IV    & h         \\  
V772 Her   Aa &   165590   &  0.130  & 0.590  &  --    &  --    &    41.7  &    --    &   4.4    &   MS  &     G0V      & d,e,h     \\  
V772 Her   B  &   165590   &   --    &  --    &  --    &  --    &    41.7  &    --    &   5.1    &   MS  &     G5V      & h         \\  
ADS 11060C p  &   165590   &  1.130  & 1.360  &  --    &  --    &    41.7  &  11.373  &   8.272  &   MS  &     K7V      & b         \\  
ADS 11060C s  &   165590   &  1.130  & 1.360  &  --    &  --    &    41.7  &  11.373  &   8.272  &   MS  &     K7V      & b         \\  
V815 Her   p  &   166181   &  0.130  & 0.720  & 0.540  &  --    &    31.0  &   7.660  &   5.222  &   MS  &      G5V     & a,i       \\  
V815 Her   s  &   166181   &   --    &  --    &  --    &  --    &    31.0  &    --    &   9.6    &   MS  &    [M1-2V]   & j         \\  
BY Dra     p  &   234677   &  1.000  & 1.221  & 1.100  & 0.780  &    15.6  &   8.070  &   7.4    &   MS  &     K4V      & a,d,h     \\  
BY Dra     s  &   234677   &   --    &  --    &  --    &  --    &    15.6  &    --    &   8.6    &   MS  &    K7.5V     & h         \\  
V478 Lyr   p  &   178450   &  0.210  & 0.740  & 0.650  & 0.430  &    26.0  &   7.680  &   5.605  &   MS  &     G8V      & a         \\  
HR 7578    1  &   188088   &  0.940  & 1.050  & 0.830  & 0.480  &    15.0  &   6.913  &   6.753  &   MS  &    K2-3V     & b         \\  
HR 7578    2  &   188088   &  0.940  & 1.050  & 0.830  & 0.480  &    15.0  &   6.913  &   6.753  &   MS  &    K2-3V     & b         \\  
V1396 Cyg  p  &    --      &  1.080  & 1.517  &  --    & 0.910  &    15.9  &  10.130  &   9.280  &   MS  &     M2V      & a,d,i     \\  
V1396 Cyg  s  &    --      &   --    &  --    &  --    &  --    &    15.9  &    --    &   11.3   &   MS  &     M4Ve     & j         \\  
ER Vul     p  &   200391   &   --    & 0.680  &  --    &  --    &    46.0  &   7.270  &   4.62   &   MS  &     G0V      & a,d,h     \\  
ER Vul     s  &   200391   &   --    &  --    &  --    &  --    &    46.0  &    --    &   4.74   &   MS  &     G5V      & h         \\  
42 Cap     p  &   206301   &  0.200  & 0.650  &  --    & 0.240  &    34.0  &   5.170  &   2.513  &   off &    G2IV      & a         \\  
KZ And     p  &   218738   &  0.550  & 0.893  &  --    &  --    &    --    &   8.733  &   6.4    &   MS  &    dK2       & b,j       \\  
KZ And     s  &   218738   &  0.550  & 0.893  &  --    &  --    &    --    &   8.733  &   6.4    &   MS  &    dK2       & b,j       \\  
SZ Psc     s  &   219113   &  0.000  & 0.440  &  --    &  --    &   125.0  &    --    &   3.3    &   MS  &    F8IV      & h         \\  
KT Peg     p  &   222317   &  0.160  & 0.670  &  --    &  --    &    22.5  &   7.040  &   5.394  &   MS  &    G5V       & a,l,m     \\  
KT Peg     s  &   222317   &   --    &  --    &  --    &  --    &    22.5  &    --    &   7.820  &   MS  &    K6V       & l,m       \\  
\hline
\end{tabular}
$\,$ \\
Spectral type between brackets are asumed from the photometry.
a.- The color indices include the contribution of the secondary, except when the color for the secondary is given.
b.- Two equal stars: (U-B)$_p$=(U-B)$_s$=(U-B)$_{obs}$, V$_p$=V$_s$=V$_{obs}$+0.753.
c.- The hot component dominates (U-B).
d.- There is also available M$_V^p$, M$_V^s$.
e.- It is posible to deconvolve the photometry in V.
f.- Combined M$_V$.
g.- The hot component dominates (B-V).
h.- M$_V$(hot/cool) were calculated independently during the eclipses.
i.- M$_V$(primary) were calculated by a deconvolution with the M$_V$(total) and M$_V$(secondary):
V$_{\rm p}$ = V$_{\rm s}$ - 2.5 Log [10$^{\rm -(V_{\rm total}-V_{s})/2.5}$ - 1].
j.- M$_V$ assumed from the spectral type.
k.- From the Strassmeier et al. catalogue.
l.- Distance from M$_V$, V.
m.- M$_V$ from R, T$_{\rm eff}$, CB.
\end{table}

                  







	



\setcounter{table}{1}
\footnotesize
\begin{table*}
\caption[  ]{\footnotesize Equivalent widths and corrections for the observed stars (in m\AA).}
\begin{tabular}{lrccccccl}
\hline
 Name           &     HD & Teff &Radius    &EW(Li+Fe)& EW(Fe) &
EW(Li) & CCF(c/h)& Comments  \\
                &        & (K)&(R$_{\odot}$)& (m\AA)  & (m\AA)&
(m\AA) &         &    \\
     (1)         &    (2) &  (3) &    (4)  &    (5)  &   (6)  &  
(7)   &    (8)  &   (9)   \\
\hline                                                            
                                                       
  13 Cet A       &   3196 & 6023 &     --  &      89 &
4$^{calc}$&85$^{calc}$&      -- &        \\ 

  VY Ari         &  17433 & 4831 &     --  &      62
&23$^{calc}$&39$^{calc}$&      -- &        \\ 

  EI Eri         &  26337 & 5555 &     --  &      67 &     11 &   
 55 &      -- &        \\ 

  BD+64 487      &  30957 & 4900 &     --  &      54 &     16 &   
 38 & 2.000   &   3    \\ 

  BD+64 487      &  30957 & 4900 &     --  &    13.5 &      3 &   
 13 & 2.000   &   3    \\ 

  V1198 Ori      &  31738 & 5517 &     --  &      13 &      3 &   
 11 &      -- &        \\ 

  V1198 Ori      &  31738 &   -- &     --  &      -- &     -- &   
 -- &      -- &        \\ 

  YY Gem         &  --    & 3185 &     --  &      43 &
7$^{calc}$&36$^{calc}$& 2.000   &   3    \\ 

  YY Gem         &  --    & 3185 &     --  &      -- &     -- &   
 -- & 2.000   &   3    \\ 

$\xi$ UMa B       &  98230 & 5948 &     --  &      44 &      1 &   
 33 &      -- &        \\ 

  DF UMa         &  --    & 5117 &     --  &      68
&14$^{calc}$&52$^{calc}$& 1.027   &   3    \\ 

  DF UMa         &  --    & 3240 &     --  
 &  --    &    --     &  --       & 37.678  &   3    \\
%&      27&16$^{calc}$&11$^{calc}$& 37.678  &   3    \\ 

  MS Ser         & 143313 & 4989 &     --  &      46
&40$^{calc}$& 7$^{calc}$& 1.249   &   3    \\ 


  MS Ser         & 143313 & 4275 &     --  &      -- &     -- &   
 -- & 5.018   &   3    \\ 

$\sigma$$^2$ CrB     & 146361 & 6444 &   1.22  &     30* &
4$^{calc}$&18$^{calc}$& 1.777   &   1    \\ 

$\sigma$$^2$ CrB     & 146361 & 6030 &   1.21  &     60* &
7$^{calc}$&30$^{calc}$& 2.287   &   1    \\ 

  WW Dra         & 150708 & 5910 &   2.12  &      87* &      4 &   
 34 & 2.158   &   1    \\ 

  WW Dra         & 150708 & 4580 &   3.9   &      21 &     13 &   
  7 & 1.863   &   1,4  \\    %%%%%% Evolved

  V772 Her       & 165590 & 5948 &   1.0   &      -- &     --
&105$^{calc}$&1.536   &   1    \\ 

  V772 Her       & 165590 & 5770 &   0.6   &      -- &     --
&83$^{calc}$& 2.926   &   1    \\ 

  ADS 11060C     & 165590 & 3979 &     --  &      43
&33$^{calc}$&10$^{calc}$& 2.000   &   3    \\ 

  ADS 11060C     & 165590 & 3979 &     --  &      -- &     -- &   
 -- & 2.000   &   3    \\ 

  V815 Her       & 166181 & 5496 &   0.97  &     202
&10$^{calc}$&192$^{calc}$&1.040   &   1    \\ 

  V815 Her       & 166181 & 3648 &   0.525 &      -- &     -- &   
 -- & 26.113  &   1    \\ 

  V1396 Cyg      &     -- & 3752 &   0.4   &      52 &     40 &   
 12 & 1.383   &   1    \\ 

  V1396 Cyg      &     -- & 3370 &   0.3426&      -- &     -- &   
 -- & 3.611   &   1    \\ 

  KZ And         & 218738 & 5117 &     --  &      29 &
7$^{calc}$&27$^{calc}$& 2.000   &   3    \\ 

  KZ And         & 218738 & 5117 &     --  &      34 &
7$^{calc}$&36$^{calc}$& 2.000   &   3    \\ 

  KT Peg         & 222317 & 5528 &   0.93  &      17 &     12 &   
  4 & 1.168   &   1    \\ 

  KT Peg         & 222317 & 4178 &   0.72  &      -- &     -- &   
 -- & 6.937   &   1    \\ 
\hline                           
\end{tabular}    
$\,$\\
$*$ Line blended with others.
$^{1}$ CCF from Equation 2 and 3. 
$^{2}$ CCF from Equation 2 and 4.
$^{3}$ We deconvolved the magnitude of the primary from the total
magnitude and an estimation of the magnitude of the secondary by
using the spectral type.  
$^{4}$ Evolved components.
\end{table*}    
\footnotesize



\setcounter{table}{2}

\footnotesize
\begin{table*}
\begin{flushleft}
\caption[ ]{\footnotesize Final abundances, where Log N(Li)=12$+$Log\{N(Li)/N(H)\},
 and other parameters for CABS}
\begin{tabular}{lrccrcllc}
\hline
  Name         &     HD &T$_{\rm eff}$&EW(Li)$_{\rm cor}$&N(Li)&  
Mass         & P$_{\rm orb}$   &P$_{\rm phot}$& Log Age        \\
                 &          &    (K)  &  (m\AA)   &           & 
(M$_\odot$)   &      (d)        &     (d)      &  (yr)     \\     
    (1)          &    (2)   &    (3)  &    (4)   &     (5)   &    
 (6)       &       (7)       &      (8)     &        (9)     \\
\hline
 13 Cet A p      &    3196  &   6023  &  85      &    
2.84&$\sim1.60^{\rm CM}$&2.08200 &$\sim2.08^{\rm Porb}$ &
9.221$^{\rm M}$\\  
 13 Cet A s      &    3196  &   5700  &$\le$1    & $\le$0.0  &   
--          & 2.08200 &$\sim2.08^{\rm Porb}$&$\sim9.22^{\rm P}$\\  
 CF Tuc   s      &    5303  &   6030  &  61.29   &     2.59  &   
1.057       &    2.79786      &    2.798     &      9.892     \\  
 CF Tuc   p      &    5303  &   5097  &  73.49   &     1.87  &   
1.205       &    2.79786      &    2.798     &      9.812   \\  
 BQ Hyi   p      &   14643  &   5140  &  26.64   &     1.27
&$\sim1.32^{\rm CM}$& 18.379        &    18.24 & $\sim9.454^{\rm
M}$\\  
 UX For   p      &   17084  &   5357  &  24.49   &     1.45  &   
--          &    0.95479      &    0.957     &      --       \\  
 VY Ari   p      &   17433  &   4831  &  39      &     1.10
&$\sim0.80^{\rm CM}$& 13.198        &    16.42 & $\sim10.059^{\rm
M}$\\  
 V471 Tau p      &    --    &   4752  &  218.7   &     2.72  &   
0.8         &    0.52119299   &    0.5197    &       Hyades   \\  
 AG Dor   p      &   26354  &   4964  &  16.46   &     0.82 
&$\le$0.80       &    2.562        &    2.533     &     --      \\  
 EI Eri   p      &   26337  &   5555  &  25.65   &     1.67  &   
--          &    1.947227     &    1.945     &      --       \\  
 vB22     p      &   27130  &   5542  &  67.3    &     2.28  &   
1.086       &5.609198 &$\sim5.61^{\rm Porb}$ &       Hyades   \\  
 vB22     s      &   27130  &   4366  &  --      &     --    &   
0.776       &5.609198 &$\sim5.61^{\rm Porb}$ &       Hyades  \\  
 vB40A    p      &   27691  &   6225  &  122.3   &     3.46  &   
--          &4.00000  &$\sim4.00^{\rm Porb}$ &       Hyades  \\  
 vB 69    p      &   28291  &   5539  &  11.8    &     1.28
&$\sim0.96^{\rm CM}$&  41.66        &    --        &       Hyades \\  
 V833 Tau p      &  283750  &   4540  &  16.2    &     0.23  &   
0.8         &    1.787797     &    1.797     &       Hyades   \\  
 vB117    p      &  283882  &   4650  &$\le$4.2  &$\le$-0.25
&$\sim0.79^{\rm Msin^3i}$& 11.9293 &    6.82      &       Hyades  \\  
 vB117    s      &  283882  &   4520  &$\le$2.6  &$\le$-0.65
&$\sim0.77^{\rm Msin^3i}$& 11.9293 &    6.82      &       Hyades  \\  
 BD+64 487 1     &   30957  &   4900  &  76      &     1.64 
&$\le$0.80       &    44.38        &    --        &      --    \\  
 BD+64 487 2     &   30957  &   4900  &  27      &     0.98 
&$\le$0.80       &    44.38        &    --        &      --    \\  
 V1198 Ori p     &   31738  &   5517  &  11      &     1.23 
&$\sim1.84^{\rm CM}$&    --        &    4.55   &$\sim9.059^{\rm
M}$\\  
 HR 2814   p     &   57853  &   5948  &  101.54  &     2.93  &    
--         &    122.169      &    --        &        --      \\  
 YY Gem          &   --     &   3185  &   65     &     0.11  &   
0.62        &    0.8142822    &    0.8143    &      --       \\
 54 Cam    p     &   65626  &   5829  &  65.70   &     2.47  &   
1.64        &    11.06803     &    10.163 &$\sim9.194^{\rm
M}$\\  
 54 Cam    s     &   65626  &   5460  &  116.57  &     2.71  &   
1.61        &    11.06803     &    10.163 &$\sim9.217^{\rm
M}$ \\  
 TY Pyx    p     &   77137  &   5438  &  4.53    &     0.75  &   
1.22        &    3.198548     &    3.32      &      9.730    \\  
 TY Pyx    s     &   77137  &   5390  &  7.05    &     0.89  &   
1.20        &    3.198548     &    3.32      &      9.796  \\  
$\xi$ UMa B  p     &   98230  &   5948  &  33      &     2.14  &    
--         &    3.9805  &$\sim3.98^{\rm Porb}$&      --      \\  
 DF UMa    p     &    --    &   5117  &  53      &     1.60  &   
0.56        &    1.033824&$\sim1.03^{\rm Porb}$&    --       \\  
 DF UMa    s     &    -     &   3240  &  --      &      --   &   
0.3         &    1.033824&$\sim1.00^{\rm Porb}$&    --       \\  
 CD-38 7259 s    &  101309  &   5770  &  41.54   &     2.13  &    
--         &    11.710       &    11.66     &        --      \\  
 IL Com    p     &  108102  &   6266  &  22      &     2.25  &   
0.85        &    0.9616       &    0.82      &      10.054   \\  
 IL Com    s     &  108102  &   6266  &  28      &     2.37  &   
0.82        &    0.9616       &    0.82      &      10.121   \\  
 RS CVn    s     &  114519  &   6700  &  --      & $\sim$3   &   
1.41        &    4.797851     &    4.7912    &      9.410    \\  
 MS Ser    p     &  143313  &   4989  &   9      &     0.57  &   
--          &    9.01490      &    9.60      &       --       \\  
 MS Ser    s     &  143313  &   4275  &  --      &     --    &   
--          &    9.01490      &    9.60      &       --      \\  
$\sigma$$^2$ CrB s    &  146361  &   6444  &  30      &     2.61  &   
1.12        &    1.139791     &    1.1687    &      9.611     \\  
$\sigma$$^2$ CrB p    &  146361  &   6030  &  69      &     2.67  &   
1.14        &    1.139791     &    1.1687    &      9.648    \\  
 WW Dra    s     &  150708  &   5910  &  73      &     2.61  &   
1.36        &    4.629617     &    4.63      &      9.575   \\  
 V792 Her  s     &  155638  &   6539  &  81      &     2.4   &   
1.41        &    27.5368      &    27.07     &      9.422   \\  
 Z Her     p     &  163930  &   5948  & --       &    --     &   
1.61        &    3.992801     &    3.962     &      9.012   \\  
 Z Her     s     &  163930  &   5000  & --       &    --     &   
1.31        &    3.992801     &    3.962     &      9.675  \\  
 V772 Her  Aa    &  165590  &   5948  &  158     &     3.19  &   
1.04        &    0.879504     &    0.878     &      9.465   \\  
 V772 Her  B     &  165590  &   5770  &  243     &     3.60  &   
0.88        &    7391.25      &    --        &      9.465   \\  
 ADS 11060C p    &  165590  &   3979  &  16      &    -0.43 
&$\sim0.70^{\rm Msin^3i}$ & 25.762 &    --        &     V772 Her  \\  
 ADS 11060C s    &  165590  &   3979  &  --      &     --   
&$\sim0.67^{\rm Msin^3i}$ & 25.762 &    --        &     V772 Her  \\  
 V815 Her  p     &  166181  &   5496  &  201     &     3.63 
&$\sim0.86^{\rm RT}$& 1.809837     &    1.819   &$\sim9.972^{\rm
M}$\\  
 V815 Her  s     &  166181  &   3648  &  --      &     --    &   
--          &    1.809837     &    1.819   &$\sim9.972^{\rm P}$ \\  
 BY Dra    p     &  234677  &   4300  &  7       &    -0.42 
&$\sim$0.55      &    5.975112     &    3.827     &      --       \\  
 BY Dra    s     &  234677  &   4021  &  8       &    -0.65  &   
0.44        &    5.975112     &    3.827     &      --        \\  
 V478 Lyr  p     &  178450  &   5395  &  59      &     1.97 
&$\sim0.83^{\rm RT}$& 2.130514     &    2.13    &$\sim10.014^{\rm
M}$\\  
 HR 7578   1     &  188088  &   4839  &  4.91    &     0.1  
&$\ge$0.80       &    46.815       &    16.5      & $\le$9.966 \\  
 HR 7578   2     &  188088  &   4839  &  4.91    &     0.1  
&$\ge$0.80       &    46.815       &    16.5      & $\le$9.966    \\  
 V1396 Cyg p     &   --     &   3752  &  17      &    -0.60  &   
0.42        &    3.276188 &$\sim3.28^{\rm Porb}$&     --     \\  
 V1396 Cyg s     &   --     &   3370  &  --      &     --    &   
0.27        &    3.276188 &$\sim3.28^{\rm Porb}$&     --     \\  
 ER Vul    p     &  200391  &   5602  &$\le$8    &$\le$1.15  &   
1.10        &    0.6980951    &    0.6942    &      9.569     \\  
 ER Vul    s     &  200391  &   5770  &$\le$9    &$\le$1.35  &   
1.05        &    0.6980951    &    0.6942    &      9.748     \\  
 42 Cap    p     &  206301  &   5710  &  42.07   &  2.09 
&$\sim2.58^{\rm CM}$& 13.1740 &$\sim13.17^{\rm
Porb}$&$\sim8.649^{\rm M}$\\  
 KZ And    p     &  218738  &   5117  &  58      &    
1.65&$\sim0.66^{\rm Msin^3i}$& 13.1740   &    3.03      &    --    \\  
 KZ And    s     &  218738  &   5117  &  62      &     1.68  &   
0.63        &    3.032867     &    3.03      &    --          \\  
 SZ Psc    s     &  219113  &   6500  & 75.50    &     3.31  &   
1.28        &    3.032867     &    3.955     &      9.496     \\  
 KT Peg    p     &  222317  &   5528  &  4       &     0.87  &   
0.93        &    6.201986     &    6.092     &      9.926    \\  
 KT Peg    s     &  222317  &   5528  &  --      &     --    &   
0.62        &    6.201986     &    6.092  &$\sim9.926^{\rm P}$ \\  
\hline
\end{tabular}
$\,$\\
\footnotesize
CM.- Mass estimated from the color--magnitud diagram.
Porb.- Photometric period similar to the orbital value.
M.- Age estimated from the mass--age realtionship.
P.- Age of the secondary equal to the computed age for the primary.
Msin$^3$i.- Mass computed from  M$\times$sin$^3$i.
RT.- Mass estimated from  Radii--T$_{\rm eff}$ plane. 
\end{flushleft}
\end{table*}

\end{document}

