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\newcommand{\pasa}{Pub. Astron. Soc. Australia}
\newcommand{\caa}{Chinese Astron. Astrophys.}
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\tablecaption{VARIABLE STARS}
\label{tab:var}
\tablehead{\colhead{(1)} & \colhead{(2)} & \colhead{(3)} & \colhead{(4)} & \colhead{(5)} & \colhead{(6)} & \colhead{(7)} & \colhead{(8)} & \colhead{(9)} & \colhead{(10)} & \colhead{(11)} & \colhead{(12)} & \colhead{(13)} & \colhead{(14)}\\
\colhead{Field} & \colhead{ID} & \colhead{R.A.} & \colhead{Dec.} & \colhead{Unfilter} & \colhead{Av} & \colhead{Amplitude} & \colhead{$J_s$} & \colhead{Period(TNTS)} & \colhead{Src$^{b}$}  & \colhead{Period(VSX)} & \colhead{$T_0^{c}$} & \colhead{Type$^{d}$} & \colhead{Note$^{e}$}\\
\colhead{     } & \colhead{  } & \multicolumn{2}{c}{(J2000.0)$^{a}$} & \multicolumn{3}{c}{(mag)} & \colhead{ } & \colhead{(d)} & \colhead{  } & \colhead{(d)} & \colhead{($HJD$-2456000)} & \colhead{    } & \colhead{    }}
\startdata
S007 & 424 & 22:47:55.16 & +25:46:59.60 & 13.88 & 0.19  & 0.33 & 0.89 & 0.382994 & (LS) & 0.382989 & 196.824 & EC & V,C \\
S008 & 1839 & 22:51:42.89 & +25:32:21.01 & 14.59 & 0.35  & 0.45 & 1.59 & 0.354250 & (LS) & 0.354265 & 196.650 & RRC & V,C \\
S008 & 542 & 22:53:00.98 & +25:43:48.03 & 14.84 & 0.34  & 0.23 & 1.23 & 46.094477 & (LS) &      & 214.880 & SR & N \\
S008 & 729 & 22:53:18.25 & +25:42:40.00 & 14.35 & 0.35  & 1.11 & 8.48 & 0.471269 & (LS) & 0.471272 & 196.318 & RRAB & V \\
S008 & 8407 & 22:54:12.33 & +24:38:07.03 & 15.41 & 0.26  & 1.02 & 2.46 & 0.608931 & (LS) & 0.608926 &      & RRAB & V,C \\
S008 & 8461 & 22:54:18.92 & +24:37:59.08 & 13.59 & 0.26  & 0.25 & 0.77 & 13.345449 & (LS) &      & 190.193 & SR & N \\
S009 & 9362 & 23:01:39.04 & +24:26:04.04 & 14.97 & 0.43  & 0.41 & 1.20 & 0.359450 & (PDM) & 0.359444 & 196.675 & RRC & V,C \\
S011 & 4138 & 23:11:27.60 & +25:08:42.01 & 17.18 & 0.18  & 1.04 & 0.85 & 0.546095 & (LS) & 0.546052 & 196.395 & RRAB & V,C \\
S012 & 9389 & 23:18:25.72 & +24:25:54.09 & 15.57 & 0.20  & 0.46 & 1.35 & 0.305437 & (LS) & 0.305435 & 196.489 & RRC & V,C \\

\enddata
\tablecomments{\\
  $^a$: Based on the TNTS reference images. \\
  $^b$: L-S: Lomb-Scargle method; PDM: Phase Dispersion Minimization method; VSX: from VSX catalogs. \\
  $^c$: Epoch when primary eclipse or minimum light occurs. \\
  $^d$: ACEP= Anomalous Cepheids; RS= RS Canum Venaticorum; EC= contact binary; ES= semi-detached binary; ED= detached binary; CWA= W Virginis; RR= RR~Lyrae variable; BL= ``Blazhko effect''; CEP= Cepheids ; GDOR= Gamma Doradus star; DSCT= Delta Scuti star; SR= Semiregular pulsator; M= Mira variable; LPV= long period variable; L= slow irregular variable \\
  $^e$: V= AAVSO VSX variable; C= CSS variable; L= LINEAR variable; N= New variable.}

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