\documentstyle[epsf, twoside, ibvst, ibvs2]{article}

\begin{document}

\IBVShead{5532}{26 May 2004}

\IBVStitletl{New Elements for 80 Eclipsing Binaries III.}

\IBVSauth{Otero, Sebasti\'an A.}

\IBVSinsto{Centro de Estudios Astron\'omicos (CEA), Grupo Wezen 1 88, Buenos Aires, Argentina; \\e-mail: varsao@fullzero.com.ar}

\IBVStyp{ EA EB EW }

\IBVSkey{variable stars, eclipsing binary, periods}

\IBVSabs{This research presents new elements for 80 eclipsing binaries found}
\IBVSabs{with the help of the ASAS-3 and Hipparcos databases.}


\begintext

The publicly available ASAS-3 (Pojmanski, 2002) and Hipparcos (Perryman et al., 1997) databases have been used to prepare this third list presenting new elements for eclipsing binaries.
Three catalogues have been used to detect the candidates for this study:
the Hipparcos Catalogue, the New Catalogue of Suspected Variable Stars (NSV) (Kukarkin and Kholopov, 1982) and its supplement (NSVS) (Kazarovets et al., 1998).
For more details on the selection of the candidate eclipsing binaries and data analysis, see Otero (2003).
Elements were found with AVE (Barber\'a, 1999) and a Microsoft Excel period search utility kindly provided by Patrick Wils (Wils, 2003).
Hipparcos observations have been transformed to V using a table by the author published electronically in IBVS No. 5482 (Otero, 2003b).
Table 1 shows the list of variables. The first column gives the variable star designation according to the GCVS. The following columns give another identifier; the brightness range of the variable, with the magnitude of secondary eclipse between brackets; the epoch of minimum light derived from the complete dataset; the period; the variability class and the spectral type with a note to the spectral type source.


\begin{table}[!hb]
\small
\centerline{{\bf Table 1}. New elements for 80 eclipsing binary stars.}
\begin{center}
\begin{tabular}{ccc@{$-$}ccccc}
\multicolumn{2}{c}{Star Name} & \multicolumn{2}{c}{Magnitude range}&   Epoch &     Period  &  Type    &   Spectral type\\
 Variable &   Other ID  &   \multicolumn{2}{c}{(V)}    &      (HJD2440000+)& (days)  &&\\
CE Cir    &	HIP 068750     &	7.93 &	8.11 (8.08)  &	8219.079  &	13.9324    &	EA   &     B9IV/V (1)\\
NSV 00763 &	GSC 7009 0216 &	10.58 &	11.17(10.82) &	12129.860   &	6.11384   &	EA&\\
NSV 01175 &	GSC 8873 0040 &	10.83 &	11.2 (11.2:) &	12134.878   &	4.63963   &	EA &       G5V(e?)(31)\\
NSV 01708 &	GSC 7592 0778 &	12.27 &	13.1 (12.95) &	12215.706   &	3.6521    &	EA&\\
NSV 03489 &	GSC 5965 2026 &	11.13 &	11.60(11.53) &	12215.795   &	2.53153   &	EA & \\
NSV 03725* &	HIP 037763     &	8.31 &	8.68 (8.60:) &	13042.680  &	12.3192    &	EA  &      B8/B9III (1)\\
NSV 03870 &	HD  066436     &	9.43 &	10.07(10.02) &	12723.645   &	0.446394  &	EW     &   F3V (2)\\
NSV 04226 &	GSC 6024 2103 &	12.28 &	14.7 (12.36) &	12645.761   &	3.4331    &	EA&\\
NSV 04426 &	GSC 5470 0214 &	12.7 &	14.1:(12.85:) &	12031.470   &	1.89439   &	EA&\\
NSV 04677 &	GSC 6053 1042 &	10.04 &	10.76(10.10) &	11932.715   &	2.2110    &	EA&\\
NSV 04686 &	GSC 8610 2627 &	12.16 &	12.66(12.54) &	13018.820   &	7.1362    &	EA&\\
NSV 04711 &	GSC 9214 0576 &	12.6  &	13.3:(12.8:) &	13018.786   &	0.79995   &	EA&\\
NSV 04941 &	GSC 8210 2662 &	12.72 &	<14.5(12.85:) &	12810.482   &	3.76173   &	EA&\\
NSV 05156 &	GSC 7734 0221 &	11.96 &	12.66(12.11) &	12736.612   &	1.81033   &	EA&\\
NSV 05177 &	GSC 8217 0730 &	12.32 &	<13.6(12.45:) &	12934.800   &	2.63205   &	EA&\\
NSV 05487 &	GSC 8241 1098 &	11.72 &	<13.7(11.85) &	12759.622   &	1.95074   &	EA&\\
NSV 06061 &	GSC 8258 0787 &	11.24 &	13.05(11.43) &	12738.740   &	3.5116    &	EA&\\
\end{tabular}
\end{center}
\end{table}

\begin{table}
\small
\centerline{{\bf Table 1}. New elements for 80 eclipsing binary stars.}
\begin{center}
\begin{tabular}{ccc@{$-$}ccccc}
\multicolumn{2}{c}{Star Name} & \multicolumn{2}{c}{Magnitude range}&   Epoch &     Period  &  Type    &   Spectral type\\
 Variable &   Other ID  &   \multicolumn{2}{c}{(V)}    &      (HJD2440000+)& (days)  &&\\
NSV 06091 &	HD  113764    &	10.30 &	11.02(10.99) &	12116.460   &	1.04222   &	EA/KE &    A1/A2V (3)\\
NSV 06144 &	GSC 5543 1285 &	11.53 &	12.22(11.85) &	12879.487   &	0.454857  &	EW/KW&\\
NSV 06150 &	GSC 9521 0323 &	11.88 &	12.6 (12.5) &	12404.915   &	0.288906  &	EW/KW&\\
NSV 06208 &	GSC 8248 1062 &	11.81 &	12.61(12.03) &	12793.568   &	0.740645  &	EA&\\
NSV 06218* &	HIP 065403     &	9.08 &	9.44:(9.42:) &	12014.643   &	5.7945    &	EA  &      G5V (3)\\ 
NSV 06354 &	HD  118532     &	9.71 &	9.93 (9.87) &	11984.818   &	0.793856  &	EB/KE&     A6IV (2)\\
NSV 06488 &	GSC 6148 0142 &	11.75 &	12.43(11.85) &	13090.714   &	0.81672   &	EA&\\
NSV 06592 &	GSC 9252 1620 &	12.19 &	13.3:(12.33) &	11903.842   &	2.74188   &	EA & \\   
NSV 06714* &	GSC 8691 2843 &	11.49 &	11.9:(11.9:) &	11954.777   &	2.09093   &	EA&\\
NSV 06746* &	GSC 7814 1992 &	11.26 &	11.87(11.77) &	12452.523   &	1.14153   &	EW/KE:&\\
NSV 06800 &	GSC 9007 4133 &	12.30 &	13.85(12.45) &	12643.849   &	2.43419   &	EA&\\
NSV 06921* &	HD  133473     &	9.82 &	10.4:(10.4:) &	11930.798   &	6.20673   &	EA  &      F5/F6V (2)\\
NSV 06933* &	HD  133674     &	9.92 &	10.55(10.40) &	12414.589   &	4.61052   &	EA   &     B9IV (3)\\
NSV 07038 &	GSC 9513 2469 &	12.37 &	13.17(13.10) &	12809.693   &	0.448784  &	EW&\\
NSV 07044 &	HD  136591     &	9.99 &	10.51(10.43) &	13011.851   &	0.386773  &	EW&        F8 (1)\\
NSV 07763* &	HD  328368     &	9.99 &	10.45(10.10) &	12452.575   &	1.78686   &	EA:&       B5 (9)\\
NSV 07847* &	HD  149450     &	8.17 &	8.51 (8.26) &	12040.789   &	1.108897  &	EA  &      B3III (2)\\
NSV 07871* &	HD  149647     &	9.17 &	9.6: (9.5:) &	12860.710   &	7.9935    &	EA   &     A2mA3-A7 (1)\\
NSV 08564 &	GSC 9276 2787 &	11.50 &	12.39(11.68) &	11950.843   &	5.3275    &	EA&\\
NSV 09348 &	GSC 8729 0831 &	11.27 &	12.07(12.06) &	12563.539   &	1.05333   &	EA&\\
NSV 09482 &	GSC 8355 2072 &	12.4  &	 13.4 (12.7) &	11994.792   &	0.524694  &	EB/KW&\\
NSV 09948 &	GSC 9067 0173 &	11.32 &	11.90(11.89) &	12467.440   &	0.327111  &	EW&\\
NSV 10425 &	GSC 9290 1725 &	12.37 &	13.9: (12.6) &	12055.753   &	5.0543    &	EA&\\
NSV 10789* &	GSC 8363 3070 &	11.60 &	12.92(11.90) &	11981.962   &	6.23975   &	EA & \\   
NSV 11114 &	GSC 8368 0719 &	12.38 &	14.6  (12.5) &	12811.846   &	2.76857   &	EA&\\
NSV 11217 &	GSC 7927 0894 &	10.68 &	11.51(10.80) &	12712.879   &	1.00545   &	EA&\\
NSV 11381* &	HD  174245     &	9.78 &	10.81(10.20:) &	12922.518   &	2.63743   &	EA: &      B8 (24)\\
NSV 11425 &	GSC 8385 0036 &	12.7  &	14.5:(13.2:) &	12831.888   &	0.88483   &	EA&\\
NSV 11764 &	GSC 8379 1399 &	11.37 &	12.13(11.44) &	12875.681   &	2.67524   &	EA&\\
NSV 11807 &	GSC 7427 0358 &	11.76 &	12.30(12.23:) &	12740.875   &	0.948834  &	EA&\\
NSV 12215 &	GSC 0479 0823 &	10.61 &	11.15(11.07) &	12481.639   &	0.531737  &	EW/KW &    K2 (14)\\
NSV 12710 &	GSC 5746 0936 &	11.68 &	12.3 (11.9:) &	12213.521   &	1.14177   &	EA&\\
NSV 13404* &	HD  199063    &	10.64 &	11.25(10.93) &	12175.543   &	0.597959  &	EB/KE &    A2/A3V: (2)\\
NSV 13527 &	GSC 8793 0788 &	12.15 &	14.12(12.35) &	12930.544   &	2.85739   &	EA&\\
NSV 13605 &	HD  201964     &	8.38 &	8.84 (8.77:) &	12104.716   &	2.69592   &	EA &       A2mA7/8-A8/9 (2)\\
NSV 13608 &	GSC 9469 0599 &	12.66 &	 13.7 (13.0) &	12085.710   &	0.510696  &	EB&\\
NSV 13711 &	GSC 7482 0186 &	11.31 &	12.68(11.44) &	12500.634   &	1.86244   &	EA &\\
NSV 13717 &	GSC 7991 0677 &	10.91 &	11.34(11.00) &	12831.720   &	0.801683  &	EA&\\
NSV 13766 &	GSC 9322 0006 &	12.05 &	12.7 (12.7) &	12900.626   &	0.390816  &	EW&\\
NSV 13890* &	HD  207570     &	9.28 &	9.56(9.54:) &	12844.790   &	0.373882  &	EW &       F6V(+A/F) (3)\\
NSV 14003 &	GSC 7995 0354 &	11.79 &	12.42(12.24) &	12996.535   &	0.601954  &	EB/KE&\\
NSV 14163 &	GSC 9340 0292 &	12.6  &	13.4 (12.93) &	12563.625   &	0.832102  &	EA&\\
NSV 14164 &	HD  212936     &	9.53 &	9.97 (9.87) &	12770.852   &	3.64523   &	EA   &     F0IV/V (1)\\
NSV 14384* &	GSC 9338 1173 &	11.5  &	11.95(11.85) &	11869.540 & 121.21      &	EB/GS&\\
NSV 14532 &	HD  214505     &	9.37 &	10.04(10.02) &	12992.612   &	0.336029  &	EW/KW &    K1V (29)\\
NSV 17233 &	HIP 033274     &	7.88 &	 7.98 (7.98)  &	8323.304   &	3.01351   &	EA     &   B8III (4)\\
NSV 17258* &	HIP 033538     &	8.71 &	8.86 (8.77)  &	8701.550 & 50.363     &	EA     &   Fm del Del (5)\\
NSV 17336* &	HIP 034262     &	8.25 &	8.43 (8.34) &	13067.651   &	2.98260   &	EA &       B3V (4)\\
NSV 18132* &	HIP 044550     &	8.89 &	9.06 (9.05)  &	8311.779  &	10.31168   &	EA/DM&     G3V (2)\\
NSV 18183* &	HIP 045945     &	8.45 &	8.55 (8.55) &	12764.617   &	6.64046   &	EA     &   A0V (3)\\
NSV 18424 &	GSC 8956 1910 &	12.5  &	13.3:(13.1:) &	11919.730   &	2.87362   &	EA    &    B8V (14)\\
NSV 19453* &	HD  110116    &	10.06 &	10.5:(10.32) &	12135.445 & 15.493     &	EA   &     B9IV (1)\\
NSV 19983 &	GSC 1473 1049 &	10.25 &	10.59(10.57) &	12751.746   &	0.53152   &	EW   &     F0 (28)\\
NSV 20009* &	HIP 068339     &	8.42 &	8.62(8.62:)  &	7917.350 & 15.5543    &	EA/DM &    B9V (1)\\
NSV 20245 &	GSC 6769 0476 &	11.07 &	11.70(11.33) &	11996.772   &	0.782983  &	EA:&\\
NSV 20721* &	HIP 081604     &	7.61 &	7.80 (7.77:)  &	8180.587 & 20.9659    &	EA&        A2IV (1)\\ 
\end{tabular}
\end{center}
\end{table}

\begin{table}
\small
\centerline{{\bf Table 1}. New elements for 80 eclipsing binary stars.}
\begin{center}
\begin{tabular}{ccc@{$-$}ccccc}
\multicolumn{2}{c}{Star Name} & \multicolumn{2}{c}{Magnitude range}&   Epoch &     Period  &  Type    &   Spectral type\\
 Variable &   Other ID  &   \multicolumn{2}{c}{(V)}    &      (HJD2440000+)& (days)  &&\\
NSV 24926 &	GSC 6903 0105 &	10.76 &	11.08(10.95) &	12529.568   &	0.80681   &	EB&\\
NSV 25992* &	HIP 113654     &	8.13 &	8.19 (8.19)  &	8560.500   &	1.424797  &	EA:/KE:   &A8V (27)\\
V0362 Pup* &	HIP 034659     &	7.49 &	7.66 (7.66:)  &	8258.268   &	9.26581   &	EA      &  A2Vs (2)\\
V0920 Her &	HIP 082390     &	7.87 &	 7.98 (7.97)  &	7954.497   &	6.92644   &	EA       & A0 (28)\\
V1000 Cen* &	HIP 069980     &	8.40 &	8.67 (8.63:) &	12102.514 & 16.6336    &	EA     &   B8IV (1)\\
V1375 Ori &	HIP 025902     &	6.66 &	6.85 (6.72)  &	7915.300 & 146.33      &	EA/GS    & K0/1III (5)\\
V1384 Ori &	HIP 028142     &	7.21 &	 7.45 (7.29)  &	8702.336   &	3.28023   &	EA &       B2V (30)\\
\end{tabular}
\end{center}
Sources of spectral type: (1) Houk and Cowley, 1975. (2) Houk, 1978. (3) Houk, 1982. (4) Houk and Smith-Moore, 1988. (5) Houk and Swift, 1999. (9) Nesterov et al., 1995. (14) Kholopov et al., 2003. (24) Ochsenbein, 1980. (27) Grenier et al., 1999. (28) Kharchenko, 2001. (29) Metanomski et al., 1998. (30) Guetter, 1968. (31) Torres et al., 2000.
\end{table}

Notes on individual stars:\\
NSV 03725 = Eccentric system.\\
NSV 06218 = One HIP eclipse recorded but not classified as variable in the HIP catalogue. Period might be half the value given.\\
NSV 06714 = Primary eclipse might be the secondary.\\
NSV 06746 = Might be EB-type.\\
NSV 06921 = Period might be half the value given.\\
NSV 06933 = Very eccentric system.\\
NSV 07763 = EB-like.\\
NSV 07847 = Bright peak in the middle of Min II. Strong reflection effect.\\
NSV 07871 = Uncertain eclipse depths.\\
NSV 10789 = O'Connell effect. Max. II $V= 11\fmm63$.\\
NSV 11381 = EB-like.\\
NSV 13404 = Strong O'Connell effect. Max II $V= 10\fmm70$.\\
NSV 13890 = Classified as DSCT:/EW: by Piquard (2001) with a period of 0.373868 d.\\
NSV 14384 = Tycho-2 $B-V= 1\fmm57$.\\
NSV 17233 = Period might be half the value given. Min I might be min II. Visual binary. $A= 8\fmm1; B= 9\fmm7$ Hp. Sep. 0\farcs29 (Perryman et al., 1997)\\
NSV 17258 = Slightly eccentric system.\\
NSV 17336 = Eccentric binary. Visual binary (sep. 2\farcs66) made Hipparcos data completely useless.\\
NSV 18132 = Period might be half the value given. Visual binary 9\farcs4 (Dommanget \& Nys, 2002)\\
NSV 18183 = Period might be half the value given.\\
NSV 19453 = Eccentric system.\\
NSV 20009 = Period might be half the value given. Visual triple. $A= 8\fmm5; B= 11\fmm4$ Hp. Sep. 7\farcs32 (Perryman et al., 1997). $C= 12\fmm8$ B (Egret et al., 1992). The AC sep. is 44\arcs\ (Worley and Douglass, 1997).\\
NSV 20721 = Period might be half the value given.\\
NSV 25992 = Min I might be Min II. Visual binary. $A= 8\fmm5; B= 9\fmm9$ Hp. Sep. 3\farcs96 (Perryman et al., 1997). Koen and Eyer (2002) give per= 0.7124 d.\\
V0362 Pup = Visual binary. $A= 7\fmm8; B= 9\fmm4$ Hp. Sep. 0\farcs69 (Perryman et al., 1997).\\
V1000 Cen = Eccentric system. Primary eclipse might be the secondary.\\

\clearpage



{\it Acknowledgements:} The author wants to thank John Greaves for his collaboration and suggestions and Patrick Wils for providing his period search utility. This research has made use of the SIMBAD and VizieR databases operated at the Centre de Donn\'ees Astronomiques (Strasbourg) in France.
This publication also makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation.

\IBVSetable{5532-t2.tex}
\IBVSecomment{The table with light curve links}

\vspace*{2cm}


\IBVSfig{10cm}{5532-f1.eps}{Lightcurve of NSV 04677 showing ASAS-3 data.}
\IBVSfigKey{5532-f1.eps}{NSV 04677}{light curve}

\IBVSfig{10cm}{5532-f2.eps}{Lightcurve of NSV 06933 showing ASAS-3 data.}
\IBVSfigKey{5532-f2.eps}{NSV 06933}{light curve}

\IBVSfig{10cm}{5532-f3.eps}{Lightcurve of NSV 07847 showing ASAS-3 data.}
\IBVSfigKey{5532-f3.eps}{NSV 07847}{light curve}

% (Fig. 4)
\IBVSfig{10cm}{5532-f4.eps}{Lightcurve of NSV 11381 showing ASAS-3 data.}
\IBVSfigKey{5532-f4.eps}{NSV 11381}{light curve}

% (Fig. 5)  
\IBVSfig{10cm}{5532-f5.eps}{Lightcurve of NSV 13404 showing ASAS-3 data.}
\IBVSfigKey{5532-f5.eps}{NSV 13404}{light curve}


\clearpage
\references


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Dommanget, J., Nys, O., 2002, {\it Observations et Travaux}, {\bf 54}, 5, Catalogue of the Components of Double and Multiple Stars (CCDM)
%%(2002yCat.1274....0D)

Egret, D., Didelon P., McLean B.J., Russell J.L., Turon C., 1992, {\it A\&A}, {\bf 258}, 217, Tycho Input Catalogue, Revised version 
%%(1992A\&A...258..217E)

Grenier, S., et al., 1999, {\it A\&AS}, {\bf 137}, 451, Radial velocities. IX. Measurements of 2800 B2-F5 stars for Hipparcos 
%%(1999A\&AS..137..451G) 

Guetter, H.H., 1968, {\it PASP}, {\bf 80}, 197, Spectral classification of 239 early-type stars 
%%(1968PASP...80..197G)


Houk, N., 1978, Dept. of Astronomy, Univ. of Michigan Ann Arbor, {\it Catalogue of two dimensional spectral types for the HD stars}, {\bf Vol. 2} 
%%(1978MSS...C02....0H)

Houk, N., 1982, Dept. of Astronomy, Univ. of Michigan Ann Arbor, {\it Catalogue of two-dimensional spectral types for the HD stars}, {\bf Vol. 3} 
%%(1982MSS...C03....0H)

Houk, N., Cowley, A.P., 1975, Dept. of Astronomy, Univ. of Michigan Ann Arbor, {\it Catalogue of two dimensional spectral types for the HD stars}, {\bf Vol. 1} 
%%(1975MSS...C01....0H)

Houk, N., Smith-Moore M., 1988, Dept. of Astronomy, Univ. of Michigan Ann Arbor, {\it Catalogue of two-dimensional spectral types for the HD stars}, {\bf Vol. 4}
%%(1988MSS...C04....0H)

Houk N., Swift C., 1999, Dept. of Astronomy, Univ. of Michigan Ann Arbor, {\it Catalogue of two-dimensional spectral types for the HD stars}, {\bf Vol. 5} 
%%(1999mctd.book.....H)

Kazarovets, V., Samus, N.N., Durlevich, O.V., 1998, {\it IBVS}, No. 4655, New Catalogue of Suspected Variable Stars. Supplement - Version 1.0 
%%(1998IBVS.4655....1K)

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%%(2001KFNT...17..409K)

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%%(2002MNRAS.331...45K)

Kukarkin, B.V., Kholopov, P.N., 1982, Moscow: Publication Office "Nauka", {\it New Catalogue of Suspected Variable Stars}
%%(1982ncsv.book.....K)

Mermilliod, J.-C., Hauck, B., Mermilliod M., 1997, {\it A\&AS}, {\bf 124}, 349, General Catalogue of Photometric Data (GCPD) II 
%%(1997A%26AS..124..349M)

Metanomski, A.D.F., Pasquini, L., Krautter, J., Cutispoto, G., Fleming, T.A., 1998, {\it A\&AS}, {\bf 131}, 197, F, G and K stars in the ROSAT all-sky survey. I. Photometry 
%%(1998A\&AS..131..197M)

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%%(1995A\&AS..110..367N)

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%%(1980BICDS..19...74O)

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Otero, S., 2003b, {\it IBVS}, No. 5482 ({\tt http://www.konkoly.hu/pub/ibvs/5401/5482-t2.txt})

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%%(1997A\&A...323L..49P)

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%%(2001yCat.2233....0P)

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%%(2002AcA....52..397P)

Torres, C.A.O., et al., 2000, {\it AJ}, {\bf 120}, 1410 
%%(2000AJ....120.1410T)

Wils, P., 2003, private communication.

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%%(1997A\&AS..125..523W)

\endreferences

\vfill\eject

%From: IBVS 5725
\IBVSerratum{5532}

Geert Hoogeveen reported the following error:

\begin{table}[h!]
\begin{tabular}{c l l l}
\hline
IBVS No. & item & printed & correct \\
\hline
5532 & identifier (NSV 14532) & HD 214505 & HD 220345 \\
\hline
\end{tabular}
\end{table}

\end{document}
