\documentstyle[twoside,epsf]{article}
\input ibvs2.sty

\begin{document}

\IBVShead{6062}{4 July 2013}

\IBVStitletl{New light elements for 63 long period}{variable stars from ASAS-3 database}

\IBVSauth{Mina, Federico D.} 

\IBVSinsto{Grupo de Astrometr\'ia y Fotometr\'ia, Observatorio Astron\'omico C\'ordoba, Argentina}
\IBVSinsto{Facultad de Filosof\'ia y Humanidades, Universidad Nacional de C\'ordoba, Argentina}
\IBVSinsto{email: fede\_mina@hotmail.com}


\IBVSkey{variable stars, periods, times of maxima}

\IBVSabs{New light elements, times of maxima and O-C diagrams }
\IBVSabs{for 63 long period variable stars form ASAS-3 databases. }


\begintext

We present new light elements of 63 long period variable stars in the southern hemisphere ($-83\deg  < {\rm DEC}  < -15\deg$). All observations were obtained from the ASAS-3 database. The observations were made between 2001 and 2009. An average of 400 data points was available for each star, and never less than 100. All observations were made in the V-band (Pojmanski 2002, 2003).

The names, alternative names and positions of Table 1 were obtained from the VSX catalog (Watson et al. 2006). Almost all the stars studied were classified as Mira-type variables in VSX. In some particular cases, we refine the periods already in VSX.

When enough data points were available, we also calculated 287 times of maxima of these variable stars. The method used for these calculations was to adjust the best bi-gaussian profile for each period (see Buys and De Clerk 1972 for a complete description of bi-gaussian profiles), which showed better results than the method of bisected chords (Knott et al. 1863), especially when there were few or none observations near maximum. This was performed by Origin 8.6.0 software (OriginLab, Northampton, MA). These times of extrema were used both to determine the epoch and to build an O$-$C diagram for the stars. Potentially interesting O$-$C diagrams are presented in Figures 1 to 4, and were made with a spreadsheet made by the author.

The periods were determined using Scargle Periodogram in the AVE software (Barber\'a, 1999). In some cases, the period was refined using the O$-$C diagrams for each star.



\begin{table}[h]
\small
\centerline{{\bf Table 1.} New elements for 63 variables.}
\begin{center}
\begin{tabular}{rlcc@{\hskip2mm}c@{\hskip2mm}c@{\hskip2mm}c}
\ Star & Name & Position RA & Position DEC & Epoch & Period & Spectral type \\ Variable & Other ID & J2000 & J2000 & (HJD2450000+) & (days) & \\
\hline
OV Pup &  & 07 33 51.50 & $-$28 23 45.8 & 2912.3 & 138.0 & M8:e (1) \\
V0470 Pup &  & 07 40 42.81 & $-$22 10 35.6 & 1959.8 & 108.9 & M8-M9 (2) \\
NR Pup &  & 07 59 42.63 & $-$50 08 34.1 & 4261.9 & 174.9 & Me (1) \\
II Pup &  & 08 03 25.75 & $-$27 55 26.0 & 2605.1 & 153.1 & M8-M9 (4) \\
OY Pup &  & 08 06 08.18 & $-$37 17 46.6  & 3405.6 & 217.3 & Me (1) \\
DP Pup & NSVS J0810431-151944 & 08 10 43.09 & $-$15 19 46.9 & 2755.0 & 322.0 & M8e (5) \\
LZ Pup &  & 08 12 10.82 & $-$23 43 48.5  & 2974.2 & 132.1 & M8 (4) \\
FT Pup & ASAS J082543-2337.3 & 08 25 42.70 & $-$23 37 14.1 & 2925.7 & 266.0 & S (1) \\


\hline
\end{tabular}
\end{center}
\end{table}

\newpage
\begin{table}
\small
\centerline{{\bf Table 1.} New elements for 63 variables (cont).}
\begin{center}
\begin{tabular}{rlcc@{\hskip2mm}c@{\hskip2mm}c@{\hskip2mm}c}
\ Star & Name & Position RA & Position DEC & Epoch & Period & Spectral type \\ Variable & Other ID & J2000 & J2000 & (HJD2450000+) & (days) & \\
\hline
WY Pyx & ASAS J083649-3627.7 & 08 36 48.98 & $-$36 27 36.4 & 2515.6 & 362.6 & Me (2) \\
UU Pyx &  & 08 43 12.06 & $-$33 05 45.1 & 2690.5 & 162.3 & Me (1) \\
RU Cha &  & 10 14 29.93 & $-$81 19 44.0 & 2010.4 & 104.2 &  \\
XZ Cha & ASAS J111209-7854.7 & 11 12 08.82 & $-$78 54 39.8  & 1949.5 & 231.0 &  \\
CK Cha & ASAS J113324-7727.4 & 11 33 23.75 & $-$77 27 21.7 & 2082.2 & 203.0 & Me (1) \\
AK Cha & ASAS J120841-8235.3 & 12 08 43.65 & $-$82 35 16.4 & 2964.6 & 186.1 &  \\
OS Mus & ASAS J120846-6545.5 & 12 08 46.00 & $-$65 45 30.0 & 2954.0 & 611.4 & M4 (1) \\
AM Cha &  & 12 12 02.18 & $-$77 00 34.9 & 2463.0 & 106.6 &  \\
AO Cha & ASAS J121611-8045.0 & 12 16 10.63 & $-$80 45 01.2 & 3068.1 & 214.0 &  \\
CH Mus & ASAS J122046-7532.9 & 12 20 45.75 & $-$75 32 52.8  & 2067.1 & 343.4 & Me (1) \\
AV Cha &  & 12 37 09.07 & $-$77 18 17.7  & 1894.8 & 86.3 &  \\
CO Cha & ASAS J124007-8031.9 & 12 40 08.14 & $-$80 31 55.2 & 2014.7 & 209.8 &  \\
CS Mus &  & 13 02 59.73 & $-$74 12 00.6 & 3410.3 & 191.0 &  \\
BU Cha & ASAS J134300-7947.7 & 13 43 00.02 & $-$79 47 41.6 & 2076.7 & 185.0 & Me (1) \\
VZ Cir & ASAS J142402-6605.9 & 14 24 02.00 & $-$66 05 54. & 2082.5 & 81.8 & M6 (2) \\
TBR V0151 &  & 14 44 30.90 & $-$59 51 57.0 & 3555.6 & 143.0 &  \\
TBR V0200 &  & 14 48 59.20 & $-$68 36 20.0 & 1970.0 & 429.5 &  \\
CT Cir &  & 14 58 41.16 & $-$57 51 04.0 & 1958.6 & 40.0 & M4III (6) \\
FF Lup & ASAS J151138-4354.7 & 15 11 37.80 & $-$43 54 41.9 & 3152.8 & 218.2 & Me (1) \\
AS Cir & ASAS J151339-6020.3 & 15 13 39.51 & $-$60 20 18.3 & 2621.2 & 517.9 & C (1) \\
FG Lup & ASAS J151508-3641.1 & 15 15 08.05 & $-$36 40 57.2 & 2874.4 & 148.7 &  \\
FM Lup & ASAS J152022-3735.3 & 15 20 21.67 & $-$37 35 15.7 & 1972.3 & 162.6 & Me (1) \\
MW Aps &  & 15 21 51.71 & $-$74 33 49.9 & 2700.1 & 196.4 & Me (2) \\
AQ Lup & ASAS J152218-4905.7 & 15 22 18.66 & $-$49 05 39.2 & 2435.0 & 150.3 &  \\
GN Lup & ASAS J152409-3302.7 & 15 24 08.39 & $-$33 02 41.5 & 2792.1 & 324.0 & S3,8 (1) \\
TBR V0116 &  & 15 26 06.20 & $-$60 49 47.0   & 1939.2 & 282.3 &  \\
GP Lup &  & 15 28 35.61 & $-$37 34 02.1 & 3843.3 & 70.4 & Me (1) \\
V0344 Nor &  & 15 40 30.64 & $-$51 12 55.6 & 2064.5 & 91.2 & M2/5e (2) \\
AW Aps &  & 15 48 32.17 & $-$73 28 16.3  & 2125.8 & 158.6 &  \\
IR TrA & ASAS J155247-6441.8 & 15 52 47.14 & $-$64 41 52.6 & 2090.6 & 223.6 & Me (1) \\
NU Lup &  & 15 57 33.91 & $-$30 08 27.9  & 1944.5 & 219.4 &  \\
BE Aps &  & 16 06 07.10 & $-$79 34 55.2 & 3778.9 & 389.0 & Me (3)  \\
BO Nor & ASAS J160648-5934.0 & 16 06 48.19 & $-$59 34 04.3  & 2856.2 & 58.1 &  \\
NSV 7536 &  & 16 14 14.23 & $-$53 34 47.3 & 2725.6 & 302.2 &  \\
CR Nor &  & 16 14 17.50 & $-$58 34 44.7 & 3482.8 & 271.5 &  \\
ER TrA & ASAS J161602-6312.4 & 16 16 01.78 & $-$63 12 21.4   & 2054.3 & 352. & Me (1) \\
NSV 7610 & ASAS J162058-6711.6 & 16 20 57.79 & $-$67 11 33.2 & 1983.9 & 205.5 &  \\
PV Nor &  & 16 21 02.08 & $-$55 18 15.4 & 3451.6 & 208.3 &  \\
IX Nor & ASAS J162216-5528.6 & 16 22 14.62 & $-$55 28 40.7  & 2165.1 & 254.8 &  \\
EX TrA & ASAS J162242-6124.7 & 16 22 42.65 & $-$61 24 36.3   & 3572.4 & 212.7 & Me (1) \\
X Nor & ASAS J162526-5155.6 & 16 25 25.76 & $-$51 55 37.3 & 2715.2 & 520.2 & C(Nb) (1) \\
NW Nor &  & 16 29 47.32 & $-$57 40 52.4  & 3147.5 & 251.9 &  \\
CC Aps &  & 16 31 18.86 & $-$79 51 28.8  & 2165.3 & 141.1 &  \\
LO Nor &  & 16 33 21.13 & $-$56 04 02.4  & 2118.4 & 281.6 &  \\
NSV 7825 &  & 16 36 36.89 & $-$70 09 01.8  & 2066.9 & 289.4 &  \\
FV Aps &  & 16 37 40.90 & $-$75 08 24.6  & 2076.8 & 114.0 &  \\
V0356 Ara &  & 16 40 10.47 & $-$55 17 41.9  & 4201.1 & 222.9 &  \\
FW Aps &  & 16 54 27.08 & $-$75 11 12.9 & 2901.4 & 256.5 & Me  (3) \\
DH Aps & ASAS J170914-7338.8 & 17 09 13.50 & $-$73 38 46.9 & 2107.4 & 188.8 &  \\
DX Aps &  & 17 27 32.91 & $-$76 38 47.2 & 1992.4 & 103.7 &  \\
EO Aps &  & 17 38 24.01 & $-$74 27 58.0 & 4741.9 & 79.2 & Me (3) \\
DG Pav & ASAS J183627-6756.0 & 18 36 26.81 & $-$67 56 01.4  & 2104.1 & 268.4 & Me (1) \\
DI Pav & ASAS J193720-5657.9 & 19 37 20.09 & $-$56 57 51.4 & 2696.1 & 256.0 & Me (1) \\
NO Pav & ASAS J195905-6216.9 & 19 59 05.26 & $-$62 16 51.2  & 3372.7 & 425.9 & Me (1) \\
DM Pav &  & 21 20 53.88 & $-$61 34 27.7 & 2521.3 & 143.4 & M8 (2) \\

\hline
\end{tabular}
\end{center}
Sources of spectral type:\\
~\\
(1) GCVS, Samus et al.  (2013), (2) Skiff (2013), (3) Stock et al. (1972), (4) MacConnell (1993), (5) Vyssotsky (1943), (6) Kharchenko et al. (2009)
\end{table}


\clearpage
Notes on individual stars:\\
DP Pup = Period from the VSX \\
FT Pup = Period from the VSX \\
WY Pyx = Wrong period of 353 days in VSX \\
XZ Cha = Wrong period of 226 days in VSX \\
CK Cha = The period is from VSX \\
AK Cha = The period is from VSX \\
OS Mus = Wrong period of 734.56 days in VSX \\
AO Cha = Period of 212.83 days in VSX is not completely accurate \\
CH Mus = Period of 344.89 days in VSX is slightly inaccurate \\
CO Cha = Period of 209.09 days in VSX is slightly inaccurate \\
BU Cha = The period is from VSX \\
VZ Cir = The epoch is from VSX but the period of 78.864 in VSX is slightly inaccurate \\
FF Lup = Wrong period of 224.97 days in VSX \\
AS Cir = Wrong period of 532.14 days in VSX \\
FG Lup = Wrong period of 169.8 days in VSX \\
FM Lup = Period of 164.05 days in VSX is slightly inaccurate \\
AQ Lup = The epoch is from VSX but the period of 148.96 in VSX is slightly inaccurate \\
GN Lup = Period of 323.44 days in VSX is slightly inaccurate \\
IR TrA = Wrong period of 219.03 days in VSX \\
BO Nor = Period of 59.072 days in VSX is slightly inaccurate \\
ER TrA = The period is from VSX \\
NSV 7610 = Wrong period of 106.76 days in VSX \\
IX Nor = Period of 253.99 days in VSX is slightly inaccurate \\
EX TrA = Period of 209.61 days in VSX is slightly inaccurate \\
X Nor = Wrong period of 526.57 days in VSX \\
DH Aps= Wrong period of 184.66 days in VSX \\
DG Pav = Period of 266.01 days in VSX is slightly inaccurate \\
DI Pav = Period of 260.31 days in VSX is slightly inaccurate \\
~\\


\IBVSetable{6062-t3.tex}
\IBVSecomment{Table 1. with figure links}

\begin{table}
\begin{center}
\small
\centerline{{\bf Table 2.} New Times of Maxima}
\begin{tabular}{lllllccccc}
\ Star Name & Time of Maxima & Standard Error \\ & HJD (+2450000) & \\
\hline
OV Pup & 2912.3 & 0.6 & \\
 & 3462.0 & 0.6 & \\
 & 3742.5 & 0.7 & \\
 & 4579.0 & 2.4 & \\
 & 4847.5 & 5.7 & \\
 & 5121.6 & 1.2 & \\
V470 Pup & 1959.9 & 1.0 & \\
 & 2939.4 & 0.8 & \\
 & 4575.1 & 0.6 & \\
NR Pup & 4262.0 & 1.6 & \\
II Pup & 2605.2 & 2.4 & \\
 & 3066.5 & 1.1 & \\
 & 3517.7 & 1.8 & \\
 & 4447.6 & 1.4 & \\
OY Pup & 2551.6 & 1.9 & \\
 & 2986.8 & 1.1 & \\
 & 3405.6 & 0.5 & \\
 & 3837.6 & 0.6 & \\
 & 4274.0 & 3.7 & \\
LZ Pup & 2974.2 & 1.8 & \\
 & 3757.0 & 1.4 & \\
 & 4164.7 & 1.4 & \\
 & 4559.4 & 0.4 & \\
FT Pup & 2925.7 & 3.8 & \\
 & 3158.6 & 2.4 & \\
 & 3486.7 & 3.3 & \\
 & 4543.4 & 4.7 & \\
 & 4798.4 & 7.4 & \\
WY Pyx & 2145.9 & 6.0 & \\
 & 2515.6 & 7.7 & \\
 & 2879.2 & 4.8 & \\
 & 5054.5 & 8.7 & \\
UU Pyx & 2690.5 & 0.3 & \\
 & 3030.5 & 0.6 & \\
 & 3669.9 & 1.3 & \\
 & 4969.3 & 1.9 & \\
RU Cha & 2010.4 & 0.9 & \\
 & 2842.5 & 2.5 & \\
 & 3063.2 & 0.8 & \\
 & 3482.0 & 0.8 & \\
 & 3702.1 & 3.3 & \\
 & 4308.4 & 1.5 & \\
 & 4524.1 & 0.9 & \\
 & 4927.0 & 0.6 & \\
XZ Cha & 1949.5 & 0.7 & \\
 & 2174.2 & 2.3 & \\
 & 2852.6 & 0.8 & \\
 & 3097.9 & 0.5 & \\
 & 3565.4 & 1.2 & \\
 & 4257.3 & 0.8 & \\
 & 4493.8 & 0.7 & \\
 & 4730.5 & 3.8 & \\
 & 4955.7 & 0.7 & \\
CK Cha & 2082.2 & 0.8 & \\
 & 2494.7 & 2.0 & \\
 & 3127.0 & 2.8 & \\
 & 4307.9 & 1.6 & \\
 & 4511.3 & 0.9 & \\
AK Cha & 2212.0 & 0.8 & \\
 & 2794.7 & 1.4 & \\
 & 2964.6 & 2.3 & \\
 & 3535.5 & 1.1 & \\

\hline
\end{tabular}
\end{center}
\end{table}

\begin{table}
\begin{center}
\small
\centerline{{\bf Table 2.} New Times of Maxima (cont.)}
\begin{tabular}{lllllccccc}
\ Star Name & Time of Maxima & Standard Error \\ & HJD (+2450000) & \\
\hline
AK Cha (cont.)& 4284.1 & 0.9 & \\
 & 4457.0 & 0.6 & \\
 & 4632.7 & 0.4 & \\
AO Cha & 2007.0 & 1.4 & \\
 & 2648.2 & 2.6 & \\
 & 2846.7 & 2.4 & \\
 & 3068.1 & 1.4 & \\
 & 3494.8 & 1.1 & \\
 & 4140.8 & 1.1 & \\
 & 4561.7 & 1.1 & \\
 & 4990.5 & 0.9 & \\
CH Mus & 2067.1 & 0.5 & \\
 & 2758.6 & 1.4 & \\
 & 3098.5 & 0.6 & \\
 & 3443.4 & 0.5 & \\
 & 3786.4 & 0.8 & \\
 & 4123.3 & 1.9 & \\
 & 4468.4 & 0.8 & \\
 & 4814.8 & 1.6 & \\
AV Cha & 1894.8 & 1.2 & \\
 & 3457.3 & 2.5 & \\
 & 4481.2 & 1.7 & \\
CO Cha & 2014.7 & 1.2 & \\
 & 2643.3 & 1.3 & \\
 & 3062.1 & 2.5 & \\
 & 3471.2 & 0.8 & \\
 & 4326.1 & 1.0 & \\
 & 4529.0 & 0.5 & \\
 & 4952.6 & 0.8 & \\
CS Mus & 3410.3 & 2.0 & \\
 & 3791.8 & 1.6 & \\
 & 4165.4 & 0.6 & \\
 & 4941.9 & 1.1 & \\
BU Cha & 2076.7 & 1.5 & \\
 & 2465.1 & 4.0 & \\
 & 2822.5 & 1.3 & \\
 & 3556.1 & 1.4 & \\
 & 3746.2 & 4.5 & \\
 & 4304.5 & 2.8 & \\
 & 4484.9 & 4.2 & \\
 & 4665.4 & 2.7 & \\
 & 5039.1 & 4.2 & \\
VZ Cir & 2473.6 & 1.1 & \\
 & 3819.8 & 2.8 & \\
 & 3883.8 & 2.3 & \\
 & 4532.7 & 4.7 & \\
 & 4693.2 & 1.5 & \\
TBR V0151 & 3555.6 & 1.4 & \\
 & 4842.3 & 1.6 & \\
TBR V0200 & 1970.0 & 0.8 & \\
 & 2818.4 & 1.4 & \\
 & 4975.9 & 1.6 & \\
CT Cir & 1958.6 & 1.9 & \\
 & 3120.5 & 4.8 & \\
FF Lup & 2057.5 & 1.1 & \\
 & 2502.9 & 2.0 & \\
 & 2709.9 & 0.9 & \\
 & 3152.8 & 1.3 & \\
 & 3589.5 & 1.4 & \\
 & 3806.9 & 1.2 & \\
 & 4250.4 & 1.5 & \\
 & 4895.9 & 1.2 & \\
\hline
\end{tabular}
\end{center}
\end{table}


\begin{table}
\begin{center}
\small
\centerline{{\bf Table 2.} New Times of Maxima (cont.)}
\begin{tabular}{lllllccccc}
\ Star Name & Time of Maxima & Standard Error \\ & HJD (+2450000) & \\
\hline
AS Cir & 2621.2 & 3.9 & \\
 & 3154.5 & 1.2 & \\
 & 3671.6 & 8.6 & \\
 & 4168.3 & 2.5 & \\
 & 4716.4 & 5.7 & \\
FG Lup & 1999.6 & 1.4 & \\
 & 2874.4 & 0.7 & \\
 & 3170.2 & 1.4 & \\
 & 3459.4 & 1.4 & \\
 & 4653.0 & 1.5 & \\
 & 4953.6 & 2.0 & \\
FM Lup & 1972.3 & 1.5 & \\
 & 2786.3 & 1.6 & \\
 & 3432.7 & 1.0 & \\
 & 4244.4 & 1.9 & \\
 & 5050.0 & 4.7 & \\
 & 4872.7 & 0.8 & \\
MW Aps & 2700.2 & 1.7 & \\
 & 3079.1 & 0.9 & \\
 & 3453.6 & 1.2 & \\
 & 4638.4 & 0.6 & \\
 & 5051.1 & 0.5 & \\
AQ Lup & 2131.8 & 1.4 & \\
 & 2734.7 & 0.9 & \\
 & 3033.1 & 2.7 & \\
 & 3633.8 & 1.0 & \\
 & 4236.1 & 1.4 & \\
 & 4534.0 & 1.1 & \\
GN Lup & 2455.0 & 0.9 & \\
 & 2792.1 & 1.0 & \\
 & 3117.4 & 1.9 & \\
 & 3435.4 & 1.2 & \\
 & 3764.7 & 1.5 & \\
 & 5061.2 & 1.3 & \\
TBR V0116 & 1939.2 & 2.0 & \\
 & 2502.7 & 2.6 & \\
 & 2777.2 & 2.8 & \\
 & 3068.9 & 4.1 & \\
GP Lup & 2876.2 & 2.2 & \\
 & 3574.2 & 2.3 & \\
 & 3843.3 & 1.1 & \\
V0344 Nor & 2064.5 & 3.8 & \\
 & 2894.0 & 1.6 & \\
 & 3433.5 & 1.2 & \\
 & 4527.0 & 1.9 & \\
 & 5075.4 & 1.9 & \\
AW Aps & 2125.9 & 1.6 & \\
 & 3077.8 & 3.3 & \\
 & 3405.9 & 3.9 & \\
 & 4343.7 & 2.0 & \\
 & 4657.3 & 6.0 & \\
IR TrA & 2090.6 & 1.4 & \\
 & 2536.2 & 1.6 & \\
 & 2753.1 & 0.5 & \\
 & 3419.8 & 0.7 & \\
 & 3642.0 & 0.9 & \\
 & 3864.5 & 1.1 & \\
 & 4317.0 & 0.9 & \\
 & 4547.4 & 0.9 & \\
 & 4995.5 & 1.6 & \\
\hline
\end{tabular}
\end{center}
\end{table}

\begin{table}
\begin{center}
\small
\centerline{{\bf Table 2.} New Times of Maxima (cont.)}
\begin{tabular}{lllllccccc}
\ Star Name & Time of Maxima & Standard Error \\ & HJD (+2450000) & \\
\hline
NU Lup & 1944.5 & 2.1 & \\
 & 2836.1 & 1.6 & \\
 & 3055.4 & 4.6 & \\
 & 3479.4 & 1.6 & \\
 & 4562.9 & 1.0 & \\
 & 4998.5 & 1.2 & \\
BE Aps & 3778.9 & 2.1 & \\
 & 4553.2 & 1.2 & \\
 & 4950.0 & 5.7 & \\
BO Nor & 2856.2 & 2.2 & \\
 & 3153.5 & 6.6 & \\
 & 4364.1 & 10.5 & \\
 & 4543.8 & 15.4 & \\
CR Nor & 3482.8 & 2.9 & \\
 & 4569.1 & 3.1 & \\
ER TrA & 2054.3 & 5.5 & \\
 & 2753.7 & 1.5 & \\
 & 3099.0 & 1.4 & \\
 & 3819.6 & 5 & \\
 & 4174.2 & 2.6 & \\
 & 4858.1 & 6.5 & \\
NSV 7610 & 1983.9 & 1.4 & \\
 & 2081.7 & 2.4 & \\
 & 2819.5 & 1.3 & \\
 & 3829.0 & 3.5 & \\
 & 4241.6 & 3.4 & \\
 & 4655.5 & 2.9 & \\
PV Nor & 3451.6 & 2.4 & \\
 & 4284.9 & 2.8 & \\
IX Nor & 2165.1 & 4.8 & \\
 & 2674.7 & 2.0 & \\
 & 3436.8 & 3.5 & \\
 & 4213.1 & 3.6 & \\
 & 4712.6 & 1.4 & \\
EX TrA & 2077.4 & 8.0 & \\
 & 2516.5 & 2.1 & \\
 & 2726.4 & 2.4 & \\
 & 3572.4 & 3.4 & \\
 & 4628.7 & 2.2 & \\
 & 5064.7 & 5.7 & \\
X Nor & 2715.2 & 0.8 & \\
 & 4278.8 & 1.4 & \\
 & 4792.9 & 2.4 & \\
 & 5053.4 & 2.2 & \\
CC Aps & 2165.3 & 0.8 & \\
 & 2727.6 & 1.2 & \\
 & 3578.2 & 1.3 & \\
 & 3854.6 & 1.3 & \\
 & 4706.5 & 1.7 & \\
 & 4988.4 & 6.7 & \\
LO Nor & 2118.4 & 4.4 & \\
NSV 7825 & 2066.9 & 0.6 & \\
 & 3805.8 & 2.5 & \\
 & 4381.0 & 3.2 & \\
 & 4967.0 & 16.4 & \\
FV Aps & 2076.9 & 0.7 & \\
 & 2528.6 & 0.7 & \\
 & 2764.3 & 0.9 & \\
 & 3443.7 & 0.7 & \\
 & 4126.9 & 1.1 & \\
 & 4358.5 & 0.9 & \\
 & 4596.1 & 4.4 & \\
V0356 Ara & 4201.1 & 6.2 & \\
\hline
\end{tabular}
\end{center}
\end{table}

\begin{table}
\begin{center}
\small
\centerline{{\bf Table 2.} New Times of Maxima (cont.)}
\begin{tabular}{lllllccccc}
\ Star Name & Time of Maxima & Standard Error \\ & HJD (+2450000) & \\
\hline
FW Aps & 2901.4 & 6.8 & \\
 & 3412.4 & 3.5 & \\
DH Aps & 2107.5 & 1.1 & \\
 & 2520.6 & 2.0 & \\
 & 2920.1 & 6.0 & \\
 & 3059.5 & 2.8 & \\
 & 3477.5 & 1.7 & \\
 & 3842.3 & 1.4 & \\
 & 4237.3 & 2.4 & \\
 & 4374.9 & 1.7 & \\
 & 4566.7 & 1.2 & \\
 & 4972.4 & 2.9 & \\
DX Aps & 1992.4 & 4.7 & \\
 & 2183.2 & 1.3 & \\
 & 3431.9 & 0.8 & \\
 & 3650.3 & 3.0 & \\
 & 3862.2 & 8.2 & \\
 & 4892.6 & 4.3 & \\
EO Aps & 3545.0 & 2.7 & \\
 & 4255.6 & 4.7 & \\
 & 4741.9 & 2.6 & \\
DG Pav & 2104.1 & 0.7 & \\
 & 2913.8 & 0.7 & \\
 & 3454.0 & 0.9 & \\
 & 4268.4 & 1.6 & \\
 & 5058.5 & 0.7 & \\
DI Pav & 2185.4 & 0.4 & \\
 & 2945.1 & 0.5 & \\
 & 4242.1 & 0.7 & \\
 & 4750.7 & 0.6 & \\
 & 5009.1 & 0.9 & \\
NO Pav & 2090.4 & 0.8 & \\
 & 2510.5 & 1.3 & \\
 & 2942.2 & 0.8 & \\
 & 4222.9 & 1.6 & \\
DM Pav & 2521.3 & 1.8 & \\
 & 2796.7 & 1.0 & \\
 & 3114.1 & 7.3 & \\
 & 3663.3 & 1.1 & \\
 & 5102.4 & 3.9 & \\

\hline
\end{tabular}
\end{center}
\end{table}

\IBVSfig{7cm}{6062-f1.eps}{O$-$C diagram of XZ Cha.}
\IBVSfigKey{6062-f1.eps}{XZ Cha}{O-C diagram}

\IBVSfig{7cm}{6062-f2.eps}{O$-$C diagram of CK Cha.}
\IBVSfigKey{6062-f2.eps}{CK Cha}{O-C diagram}

\IBVSfig{7cm}{6062-f3.eps}{O$-$C diagram of MW Aps.}
\IBVSfigKey{6062-f3.eps}{MW Aps}{O-C diagram}

\IBVSfig{7cm}{6062-f4.eps}{O$-$C diagram of IR TrA.}
\IBVSfigKey{6062-f4.eps}{IR TrA}{O-C diagram}



\newpage
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\end{document}
