\begin{table}%t1 \caption{\label{table_charac}Important characteristics of the sample stars.} \small%\centerline { \begin{tabular}{lllrrcccc} \hline\hline Name & Sp. type & Var. type & $P$ [days] & $K$ [mag] & $J-K$ [mag] & Ref. & $M_{\rm{bol}}$ & [12]--[25] \\ \hline \object{U Cet} & M4 & M & 234.76 & 2\fm73 & 1\fm11 & 1 & $-4\fm60$ & $-$1.14 \\ \object{W Cet} & S7 & M & 351.31 & 2\fm14 & 1\fm23 & 1 & $-5\fm07$ & $-$1.32 \\ \object{V441~Cyg}& M4S & SRA & 288.00 & 1\fm69 & 1\fm39 & 3 & $-5\fm66$ & $-$1.28 \\ \object{W Eri} & M7 & M & 376.63 & 1\fm78 & 1\fm42 & 1 & $-5\fm08$ & $-$0.90 \\ \object{S Gru} & M7 & M & 401.51 & 0\fm54 & 1\fm22 & 1 & $-5\fm35$ & $-$0.87 \\ \object{R Hor} & M7 & M & 407.60 & $-$0\fm88 & 1\fm24 & 1 & $-5\fm35$ & $-$0.92 \\ \object{T Hor} & M5 & M & 217.60 & 3\fm34 & 1\fm13 & 1 & $-4\fm44$ & $-$1.15 \\ \object{TW Hor} & C5(N) & SRB & 158.00 & 0\fm19 & 1\fm46 & 3 & $-4\fm89$ & $-$1.03 \\ \object{R Hya} & M7 & M & 388.87 & $-$2\fm52 & 1\fm24 & 1 & $-5\fm28$ & $-$1.08 \\ \object{RU Hya} & M6 & M & 331.50 & 1\fm60 & 1\fm18 & 1 & $-5\fm07$ & $-$0.74 \\ \object{Y Lib} & M5 & M & 275.70 & 3\fm16 & 1\fm21 & 1 & $-4\fm72$ & $-$0.73 \\ \object{U Mic} & M6 & M & 334.29 & 1\fm80 & 1\fm22 & 1 & $-5\fm00$ & $-$0.69 \\ \object{Y Scl} & M5 & SRB & 79.36 & 0\fm35 & 1\fm27 & 2 & $-4\fm24$ & $-$0.94 \\ \object{T Tuc} & M4 & M & 250.30 & 2\fm96 & 1\fm18 & 2 & $-4\fm58$ & $-$1.08 \\ \object{ER Vir} & M4 & SRB & 55.00 & 1\fm44 & 1\fm10 & 4 & $-4\fm03$ & $-$1.41 \\ \object{EV Vir} & M4 & SRB & 120.00 & 1\fm55 & 1\fm15 & 4 & $-5\fm08$ & $-$1.34 \\ \object{RS Vir} & M7 & M & 353.35 & 1\fm15 & 1\fm31 & 1 & $-5\fm09$ & $-$0.56 \\ \object{S Vir} & M7 & M & 378.01 & 0\fm30 & 1\fm27 & 1 & $-5\fm21$ & $-$0.98 \\ \hline \end{tabular}} \smallskip References for near infrared data: 1:~\citet{Catchpole}; 2:~\citet{Fouquet}; 3:~\citet{KH94}; 4:~\citet{K95}. \end{table}