\begin{table}%tA.4
  \caption{Stellar parameters relevant for the Hertzsprung-Russell Diagram of all objects. 
The objects are grouped by type and sorted by right ascension. For the objects in Taurus, a~distance of~$140~{\rm pc}$ is assumed, for~MBM12 $90~{\rm pc}$. The color excess that was used to calculate the extinction~$A_{V}$ is given in the neighboring column. To get the real colors of the objects we used the spectral type~-- color conversion from \citet{1995ApJS..101..117K} for early spectral types and \citet{1992ApJS...82..351L} for type~M0 and later. The masses and ages are interpolated from pre main sequence models by \citet{1994ApJS...90..467D}. The apparent magnitudes in~$V$ for objects observed in Run~I was determined by absolute photometry ourselves. For Run~II objects we had to rely on~VizieR \citep{2000AAS..143...23O} values~-- we averaged all available values. For more details see text.}\label{tab:hrd}
%\centerline
{
  \begin{tabular}{l|rlcllllll}
  \hline\hline
Object name             & $\log L_{{\rm bol}}$ & $\log T_{{\rm eff}}$ & $T_{{\rm eff}}$  & $M_{{\rm bol}}$ & $V$ & $A_{V}$ & Determination $A_{V}$ & \multicolumn{1}{c}{$M/M_{\odot}$} & $\log {\rm Age}$ \\
\hline
Classical TTS:&&&&&&&&&\\
Lk\Ha{}263&              --0.870& 3.519&  3300&    6.91&   14.90& 0.62&     $E(V-R,I,J;R-I)$          &0.20&6.35\\
Lk\Ha{}262&                 --1.162& 3.585&  3850&    7.65&   14.83&1.16&    $E(V-R,I,J;R-I)$                  &0.60&7.25\\
Lk\Ha{}264&                 --0.570& 3.638&  4350&    6.17&   13.74&2.08&    $E(V-I,J;R-I)$            &0.90&7.20\\
\hline
Weak-line TTS:&&&&&&&&&\\
RX J0255.4+2005        &  --0.656& 3.624 &   4205&    6.38&   12.23&0.26&    $E(V-I,J,H,K;R-I)$          &0.82&  7.30\\
E0255.3+2018          &  --0.195& 3.662 &   4590&    5.23&   11.84&1.29&    $E(V-J,H,K;R-I)$            &1.10&  6.94\\
RX J0312.8-0414NW     &  0.054  &3.780 &   6030&    4.61&   10.86&0.35&    $E(R-I)$                        &1.12&  7.60\\
RX J0312.8-0414SE     &  --0.176& 3.742 &   5520&    5.18&    11.62&0.46&    $E(R-I)$                        &0.95&  7.60\\
RX J0324.4+0231       &  --0.788& 3.638 &   4350&    6.71&    12.69&0.0 &   $E(R-I)$                        &0.71&  7.65\\
RX J0333.1+1036       &  --0.410& 3.675 &   4730&    5.77&    12.15&0.15&    $E(R-I)$                        &0.90&  7.40\\
RX J0344.8+0359       &  --0.539& 3.675 &   4730&    6.09&    12.74&0.42&    $E(R-I)$                        &0.80&  7.60\\
RX J0351.4+0953W      &  --0.600& 3.699 &   5000&    6.24&    12.64&0.30&    $E(R-I)$                        &0.79&  7.88\\
RX J0403.4+1725       &  0.000  &3.675 &   4730&    4.74&    11.69&0.72&    {\citep{2000AAS..145..187C}} &1.33&  6.80\\
RX J0406.8+2541       &  0.518  &3.597 &   3955&    3.45&    11.72&1.46&    {\citep{2000AAS..145..187C}} &0.55&  5.00$^9$\\
RX J0407.3+0113S      &  --0.506& 3.675 &   4730&    5.97&    13.85&1.73&    $E(R-I)$                        &0.83&  7.55\\
RX J0407.3+0113N      &  --0.157& 3.763 &   5800&    5.13&    12.80&1.73&    $E(R-I)$                        &1.00&  7.70\\
RX J0409.3+1716       &  --0.336& 3.571 &   3720&    5.58&    13.30&0.56&    {\citep{2000AAS..145..187C}} &0.50&  6.16\\
RX J0434.3+0226       &  --0.362& 3.662 &   4590$^1$&    5.64&    12.46&0.54&    $E(R-I)$                        &0.76&  7.20\\
RX J0439.4+3332A      &  0.158  &3.638 &   4350&    4.34&    11.31&0.52&    $E(V-I)$                        &0.90&  6.07\\
RX J0445.5+1207       &  --0.399& 3.609 &   4060&    5.74&    13.03&0.64&    $E(R-I)$                        &0.80&  6.70\\
RX J0450.0+0151       &  --0.218& 3.675 &   4730&    5.28&    11.96&0.02&    $E(R-I)$                        &1.02&  7.20\\
RX J0452.8+1621       &  --0.158& 3.662 &   4590&    5.14&    11.57&0.16&    $E(B-V)$                        &1.13&  6.88\\
RX J0528.9+1046       &  --0.658& 3.675 &   4730$^2$&    6.38&    13.22&0.61&    $E(R-I)$                        &0.74&  7.80\\
RX J0529.3+1210       &  --0.602& 3.597 &   3955$^3$&    6.25&   13.26&0.20&    $E(J-K),E(V-I)$                 &0.54&  6.90\\
RX J0530.7-0434       &  --0.015& 3.675 &   4730&    4.78&    11.62&0.60&    $E(V-J,R-I)$                    &1.32&  6.80\\
\hline
Ke stars: &&&&&&\\
RX J0408.2+1956       &  --0.307& 3.690&   4900&    5.51&    13.04&1.38&    $E(R-I)$                         &0.93&  7.38\\
RX J0457.1+3142       &  --0.066& 3.690&   4900&    4.91&    11.80&0.74&    $\varnothing$ Tau-Aur {\citep{2000AAS..145..187C}}  &1.18&  7.02\\
\hline
Zero Age Main Sequence:&&&&&&&\\
RX J0407.9+1750       &  --0.060& 3.662&   4590&    4.89&   11.27& 0.1&      {\citep{2000AAS..145..187C}}  &1.19&  6.75\\
RX J0422.9+0141       &  0.107 & 3.792&   6200$^4$&    4.47&   11.79& 1.43&    $E(B-V)$                         &1.11&  7.60\\
RX J0444.7+0813       &  --0.318& 3.675&  4730&    5.54&   13.23&0.38&    $E(R-I)$                          &0.96&  7.25\\
RX J0447.9+2755       &  --0.445& 3.720&  5250&    5.85&    12.34&0.45&    $E(J-K)$                          &0.85&  7.80\\
RX J0455.8+1742       &  0.012 & 3.675&  4730&    4.71&    11.29&0.35&    $E(V-J,V-H,V-K,V-R)$          &1.27&  6.75\\
\hline
Unknown type: &&&&&&&\\
GSC2.2~N3022313162    &  --0.848& 3.829&   6740&    6.86&
13.27& 0.56&    same as neighbor             &--   &  --   \\
1RXS J044534.0+120917 &  --0.763& 3.720&  5250&    6.65&    13.23&0.54&    $E(R-I)$, SpTy(K0) from $V-K$        &--   &  --   \\
IRAS 04451+2750       &   0.294& 3.690&   4900&    4.00&   11.70&
1.55&    $E$({\tiny all filters}), SpTy(K2) by adjustment &1.53&  6.50\\
\hline
\end{tabular}}
\medskip
$^1$~\citet{Torres2002}: $T_{\rm eff}^{\rm A}=$ 5050;
$^2$~\citet{Torres2002}  $T_{\rm eff}^{\rm A,B}=$ 4800, 4550;
$^3$~\citet{Torres2002}  $T_{\rm eff}^{\rm A}=$ 4350;
$^4$~\citet{Torres2002}  $T_{\rm eff}^{\rm A,B}=$ 4550, 6300. \\
\changed{$^9$ Note that this age is not consistent with the Lithium-Test (classified as ZAMS). However, in lower resolution spectra by \citet{1999AA...342..173M} the \WLi\
 was given as 590~m\AA.}
\end{table}