\begin{table}%t1
%\begin{center}
%\par
%  \caption{continued.  } 
%{
% $$
%   \begin{tabular}{lllllllllllllll}
%     \hline\hline
%     \noalign{\smallskip}   
%$Var Name$ & $HIP$ & P$(days)$ & T_{0}$-2~400~000$ & $Type$ & $Sp$ & $CCDM no$ & \rho $(\arcsec)$ & L_{3} & a_{1} & a_{2} & a_{4} & \Sigma({\rm O-C})^{2} & $EX$ & $Ref.$^{{*}} \\
%$(1)$ & $(2)$ & $(3)$ & $(4)$ & $(5)$ & $(6)$ & $(7)$ & $(8)$ & $(9)$ & $(10)$ & $(11)$ & $(12)$ & $(13)$ & $(14)$ & $(15)$ \\
%     \noalign{\smallskip}
%     \hline 
%     \noalign{\smallskip}
     \object{V2357 Oph}	&	082967	&	0.415568$^{{b}}$	&	52050.2364$^{{b}}$	&	EW$^{{a}}$	&	G5V$^{{a}}$	&		&		&		&	+0.005(4)	&	-0.053(4)	&	-0.001(4)	&	0.021	&		&	1,33 \\
\object{V2377 Oph}	&	085944	&	0.425401	&	48500.0316	&	EW$^{{a}}$	&	G0/1V$^{{a}}$	&		&		&		&	-0.011(2)	&	-0.055(2)	&	+0.001(1)	&	0.010	&		&	1,7 \\
\object{V2388 Oph}	&	087655	&	0.802298	&	48500.1200	&	EW$^{{a}}$	&	F3V$^{{a}}$	&	J17542+1108A	&	0.088	&	0.167	&	-0.011(1)	&	-0.126(1)	&	-0.016(1)	&	0.010	&		&	1,21,23,25 \\
\object{V1363 Ori}	&	023809	&	0.431915	&	48500.0343	&	EW?	&	F8	&		&		&		&	+0.007(5)	&	-0.076(4)	&	-0.003(4)	&	0.019	&		&	1,3 \\
\object{V386 Pav}	&	103320	&	0.551841	&	48500.2722	&	EW	&	A9V	&		&		&		&	-0.006(1)	&	-0.049(1)	&	-0.000(1)	&	0.042	&		&	1 \\
\object{PU Peg}	&	110464	&	0.862023	&	48500.0487	&	EB	&	F0	&	J22226+0956A	&	91	&	--	&	-0.008(1)	&	-0.041(1)	&	+0.003(1)	&	0.013	&		&	1,3 \\
\object{V335 Peg}	&	112960	&	0.810746	&	48500.3591	&	E	&	F5	&		&		&		&	-0.010(1)	&	-0.014(1)	&	-0.001(1)	&	0.004	&		&	1 \\
\object{V351 Peg}	&	115627	&	0.593297$^{{b}}$	&	48500.4930$^{{b}}$	&	EW$^{{a}}$	&	A8V$^{{a}}$	&		&		&		&	-0.008(2)	&	-0.122(2)	&	-0.015(2)	&	0.004	&		&	1,3,5 \\
\object{V357 Peg}	&	117185	&	0.578452	&	48500.3159	&	EW	&	F5	&		&		&		&	+0.006(2)	&	-0.163(2)	&	-0.030(2)	&	0.012	&		&	1,17,22,24,35 \\
\object{V592 Per}	&	022050	&	0.715722	&	48500.2430	&	EB	&	F2	&	J04445+3953A	&	0.206	&	0.314	&	-0.009(9)	&	-0.174(8)	&	-0.028(9)	&	0.026	&		&	1 \\
     \object{BL Phe}	&	000883	&	0.810352	&	48500.3370	&	EB	&	F6IV/V	&	J00108-5729A	&	3.21	&	0.336	&	-0.064(2)	&	-0.134(2)	&	-0.044(2)	&	0.032	&	EA	&	1 \\
\object{BM Phe}	&	001507	&	0.413627	&	48500.2010	&	EW	&	F3/F5V	&		&		&		&	-0.002(2)	&	-0.103(3)	&	-0.010(3)	&	0.036	&		&	1 \\
\object{VW Pic}	&	023196	&	0.4257631	&	48500.0070	&	EB	&	F3V	&	J04595-4928A	&	9.887	&	0.138	&	+0.000(1)	&	-0.046(1)	&	-0.010(1)	&	0.010	&	EA	&	1 \\
\object{XY Pic}	&	027170	&	0.2972608	&	48500.1131	&	EB?	&	F0III/IV	&		&		&		&	+0.000(1)	&	-0.021(1)	&	+0.002(1)	&	0.005	&		&	1 \\
\object{CP Psc}	&	004593	&	0.684014	&	48500.4656	&	EB?	&	--	&		&		&		&	-0.029(5)	&	-0.064(5)	&	-0.036(5)	&	0.042	&	EA	&	1 \\
\object{VY PsA}	&	109884	&	0.633889	&	48500.5510	&	EB	&	F3V	&		&		&		&	-0.019(1)	&	-0.059(2)	&	-0.011(2)	&	0.005	&	EA	&	1 \\
\object{BD Scl}	&	002550	&	0.566287	&	48500.5040	&	EB	&	F2	&		&		&		&	-0.048(4)	&	-0.090(4)	&	-0.007(4)	&	0.013	&	EB	&	1 \\
\object{BE Scl}	&	006350	&	0.422901	&	48500.2670	&	EW	&	F8	&		&		&		&	-0.010(3)	&	-0.149(3)	&	-0.026(3)	&	0.054	&		&	1 \\
\object{V1055 Sco}	&	080603	&	0.363673	&	48500.2734	&	EB	&	G3V	&	J16274-3729A	&	0.2	&	0.420	&	-0.028(4)	&	-0.176(3)	&	-0.050(4)	&	0.034	&	EB	&	1 \\
     \object{OU Ser}	&	075269	&	0.2967645	&	48500.2780	&	EW	&	F9/G0V$^{\rm{a}}$	&		&		&		&	-0.002(2)	&	-0.076(2)	&	-0.007(2)	&	0.030	&		&	1,4,12,31 \\
\object{V1123 Tau}	&	016706	&	0.399957	&	48500.3570	&	EB	&	G0	&	J03350+1743A	&	4.268	&	0.169	&	-0.010(3)	&	-0.161(3)	&	-0.032(4)	&	0.030	&		&	1 \\
\object{V1128 Tau}	&	017878	&	0.3053732	&	48500.0620	&	EB	&	G0	&	J03495+1255A	&	12.09	&	--	&	-0.015(5)	&	-0.173(4)	&	-0.038(5)	&	0.035	&		&	1 \\
\object{QW Tel}	&	090026	&	0.411928	&	48500.1940	&	EB	&	F8/G0	&	J18222-5534A	&	31.1	&	--	&	-0.010(3)	&	-0.061(3)	&	-0.003(3)	&	0.012	&		&	1 \\
\object{DX Tuc}	&	118096	&	0.377111	&	48500.2540	&	EW	&	F7IV/V	&		&		&		&	-0.003(4)	&	-0.112(4)	&	-0.019(4)	&	0.097	&		&	1 \\
\object{HH UMa}	&	054165	&	0.3754937$^{{b}}$   &	52368.3979$^{{b}}$	&	EW$^{{a}}$	&	F8	&		&		&		&	+0.003(3)	&	-0.075(4)	&	-0.006(4)	&	 0.024	&		&	1,37 \\
\object{HN UMa}	&	055030	&	0.382608	&	48500.0781	&	EW$^{{a}}$	&	F8V$^{{a}}$	&		&		&		&	-0.000(2)	&	-0.047(2)	&	-0.004(2)	&	0.008	&		&	1,33 \\
\object{HX UMa}	&	058648	&	0.379156	&	48500.3720	&	EW$^{{a}}$	&	F4V$^{{a}}$	&	J12021+4304A	&	0.626	&	0.045	&	-0.003(2)	&	-0.076(2)	&	-0.004(2)	&	0.042	&		&	1,33 \\
\object{II UMa}	&	061237	&	0.82522	&	48500.0830	&	EW	&	F5III$^{{a}}$	&	J12329+5448A	&	0.872	&	0.145	&	-0.001(2)	&	-0.139(2)	&	-0.013(2)	&	0.042	&		&	1,25 \\
\object{TV UMi}	&	073474	&	0.415546	&	48500.2744	&	EB	&	F8	&		&		&		&	-0.006(1)	&	-0.034(1)	&	-0.002(1)	&	0.003	&		&	1,34 \\
\object{V362 Vel}	&	054112	&	0.445177	&	48500.2560	&	EB	&	F3V	&		&		&		&	-0.002(2)	&	-0.104(2)	&	-0.015(2)	&	0.100	&		&	1 \\
\object{LV Vir}	&	066078	&	0.409439	&	48500.1744	&	EB	&	F6V	&	J13328-1746A	&	1.181	&	0.413	&	-0.001(3)	&	-0.121(3)	&	-0.002(3)	&	0.012	&		&	1 \\
\object{MS Vir}	&	068881	&	0.312440	&	48500.1960	&	EB	&	K0/K1III/IV	&		&		&		&	-0.020(7)	&	-0.095(6)	&	-0.002(6)	&	0.042	&		&	1 \\
\object{NN Vir}	&	070020	&	0.480690$^{{b}}$	&	50595.3452$^{{b}}$	&	EW$^{{a}}$	&	F0/1V$^{{a}}$	&		&		&		&	+0.004(5)	&	-0.147(4)	&	-0.011(4)	&	0.024	&		&	1,27,28 \\
   \object{DX Tuc}	&	118096	&	0.377111	&	48500.2540	&	EW	&	F7IV/V	&		&		&		&	-0.003(4)	&	-0.112(4)	&	-0.019(4)	&	0.097	&		&	1 \\
\object{HH UMa}	&	054165	&	0.3754937$^{{b}}$   &	52368.3979$^{{b}}$	&	EW$^{{a}}$	&	$F8$	&		&		&		&	+0.003(3)	&	-0.075(4)	&	-0.006(4)	&	 0.024	&		&	1,37 \\
\object{HN UMa}	&	055030	&	0.382608	&	48500.0781	&	EW$^{{a}}$	&	F8V$^{{a}}$	&		&		&		&	-0.000(2)	&	-0.047(2)	&	-0.004(2)	&	0.008	&		&	1,33 \\
\object{HX UMa}	&	058648	&	0.379156	&	48500.3720	&	EW$^{{a}}$	&	F4V$^{{a}}$	&	J12021+4304A	&	0.626	&	0.045	&	-0.003(2)	&	-0.076(2)	&	-0.004(2)	&	0.042	&		&	1,33 \\
\object{II UMa}	&	061237	&	0.82522	&	48500.0830	&	EW	&	F5III$^{{a}}$	&	J12329+5448A	&	0.872	&	0.145	&	-0.001(2)	&	-0.139(2)	&	-0.013(2)	&	0.042	&		&	1,25 \\
\object{TV UMi}	&	073474	&	0.415546	&	48500.2744	&	EB	&	F8	&		&		&		&	-0.006(1)	&	-0.034(1)	&	-0.002(1)	&	0.003	&		&	1,34 \\
\object{V362 Vel}	&	054112	&	0.445177	&	48500.2560	&	EB	&	F3V	&		&		&		&	-0.002(2)	&	-0.104(2)	&	-0.015(2)	&	0.100	&		&	1 \\
\object{LV Vir}	&	066078	&	0.409439	&	48500.1744	&	EB	&	F6V	&	J13328-1746A	&	1.181	&	0.413	&	-0.001(3)	&	-0.121(3)	&	-0.002(3)	&	0.012	&		&	1 \\
\object{MS Vir}	&	068881	&	0.312440	&	48500.1960	&	EB	&	K0/K1III/IV	&		&		&		&	-0.020(7)	&	-0.095(6)	&	-0.002(6)	&	0.042	&		&	1 \\
\object{NN Vir}	&	070020	&	0.480690$^{{b}}$	&	50595.3452$^{{b}}$	&	EW$^{{a}}$	&	F0/1V$^{{a}}$	&		&		&		&	+0.004(5)	&	-0.147(4)	&	-0.011(4)	&	0.024	&		&	1,27,28 \\
     \noalign{\smallskip}
     \hline
  \end{tabular}
%     $$ }%\end{center}
%\par
\smallskip
%\begin{itemize}
%\item [
{\bf Note:} %] 
Columns: (1) Name of the variable; (2) {\it HIPPARCOS} identifier; (3) variability period in days;
(4) Epoch in HJD for the systems marked with~$^{b}$ and in~BJD for the remaining; (5) variability type; (6) spectral type;
(7)~CCDM identifier for systems with close visual or spectroscopic companions (Catalogue of Components of Double and Multiple Stars, Dommanget \& Nys \cite{domman}); (8) separation between the visual or spectroscopic components in arcseconds; (9) third light 
contribution from the visual or spectroscopic component in light units; (10)--(12) the Fourier cosine coefficients in light units obtained 
by Fourier decomposition of the light curves, the numbers in parentheses are standard errors in units of last decimal places; (13) Sum of 
squared residuals for the Fourier fits as a goodness of fit parameter; (14) Systems excluded among the genuine W~UMa-type
systems by "Fourier filter'' as described in text, EA = detached systems eliminated by $a_{2}-a_{4}$ filter, EB = $\beta$  Lyr-type systems
eliminated by $a_{2}-a_{1}$ filter; (15) coded key references on the literature for the corresponding system.
\\
%
%\item [
$^{{*}}$ %] 
1. Kazarovets et~al. (\cite{kaza}), 2. Eggen (\cite{eggen}), 
3. Gomez-Forrellad et~al. (\cite{gomez1}), 4. Rucinski et~al. (\cite{ruc3}), 
5. Rucinski et~al. (\cite{ruc4}), 6. Pribulla et~al. (\cite{pribul2}), 7. Lu et~al. 
(\cite{lu}), 8. Dumitrescu (\cite{dumi}), 9. \"{O}zdemir et~al. (\cite{ozdem1}), 
10. Gothard et~al. (\cite{goth}), 11. Samec et~al. (\cite{samec}), 12. Pribulla \& Vanko 
(\cite{pribul1}), 13. Vanko et~al. (\cite{vanko1}), 14. Erdem et~al. (\cite{erdem}), 15.
Pribulla et~al. (\cite{pribul3}), 16. Sipahi et~al. (\cite{sipahi}), 17. 
Keskin et~al. (\cite{keskin}), 18. \"{O}zdemir et~al. (\cite{ozdem2}), 19. \"{O}zdemir et~al. 
(\cite{ozdem3}), 20. \c{C}i\c{c}ek et~al. (\cite{cicek}), 21. Yakut \& \.{I}bano\~{g}lu 
(\cite{yakut}), 22. Ya\c{s}arsoy et~al. (\cite{yasar}), 23. Rodriguez et~al. 
(\cite{rodri}), 24. Ali\c{s} et~al. (\cite{alis}), 25. Rucinski et~al. (\cite{ruc5}),
26. Soydugan et~al. (\cite{soydu}), 27. Gomez-Forrellad \& Garcia-Melendo (\cite{gomez2}),
28. Rucinski \& Lu (\cite{ruc6}), 29. Vanko \& Pribulla (\cite{vanko2}), 30. Strohmeier (\cite{stroh1}),
31. Ye\c{s}ilyaprak C. (\cite{yesil}), 32. Strohmeier \& Knigge (\cite{stroh2}),
33. Rucinski et~al. (\cite{ruc7}), 34. De\~{g}irmenci et~al. (\cite{degir}), 35. Tanr{\i}verdi et~al.
(\cite{tanri}), 36. Karska \& Maciejewski (\cite{karska}), 37. Pribulla et~al. (\cite{pribul6}).
\\
%\smallskip
%\item [
$^{{a}}$ %] 
Values are changed according to the literature.
\\
%\smallskip
%\item [
$^{{b}}$ %] 
Type of variability was changed from pulsating to EW in the literature and light elements are updated accordingly.
%\end{itemize}
      \end{table}