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\input ibvs2.sty
\input ibvse.sty
\input epsf.sty

\begin{document}
\IBVShead{5282}{31 May 2002}

\IBVStitletl{Erratum to IBVS No.~4855 and Times of Minima}{ of the Eclipsing Binary V357 Pegasi}

\IBVSauth{Alis, Sinan$^{1,2}$; Keskin, M. Mustafa$^{3}$; Atay, M. Eray$^{1}$}

\IBVSinst{University of Istanbul, Faculty of Science, Department of Astronomy and Space Sciences, 34452 Universite-Istanbul, Turkey, email: sinanali@yahoo.com}
\IBVSinst{Eyuboglu Twin Observatories, Namik Kemal Mah, Dr. Rustem Eyuboglu Sok, No:3 81240, Umraniye-Istanbul, Turkey}
\IBVSinst{Ege University, Science Faculty, Astronomy and Space Sciences Department, 35100, Bornova - Izmir, Turkey}


\SIMBADobj{V357 Peg}

\IBVStyp{ Binaries: eclipsing }
\IBVSkey{photoelectric photometry}
\IBVSabs{We present new photoelectric minima for V357 Pegasi.}


\begintext


\IBVSEobs{16\arcs\ Cassegrain telescope at TUBITAK$^{\dagger}$ National Observatory.} 

\IBVSEdet{SSP-5A photoelectric photometer, Hamamatsu 4457 pmt.}

\IBVSEred{Reduction of the data were made in the usual way.}

\IBVSfoot{TUBITAK : The Scientific and Technical Research Council of Turkey}

\IBVSEmethod{Times of minima were determined by the method of Kwee and van Woerden}


{\small
\IBVSEstars{V357 Peg & EW & 23 45 35 & +25 28 52 & HIP 116688 & 48500.3159 & 0.578452 & 1 \\}  
}


\IBVSEsource{1. The Hipparcos \& Tycho Catalogues (ESA, 1997)}

\IBVSEmin{
V357 Peg & 51810.4986 & 0.0004 &  II  &	$U,B,V,R$  &  $-$0.0007   &   This work\\
         & 51812.5233 & 0.0005 &  I   &	$U,B,V,R$  &  $-$0.0006   &   This work\\
         & 51817.4412 & 0.0010 &  II  &	$U,B,V,R$  &     0.0005   &   This work\\
         & 51819.4662 & 0.0010 &  I   &	$U,B,V,R$  &     0.0009   &   This work\\
}


\IBVSErem{
There is an error in Table 1 in Keskin et al. (2000), in the minima types 
(primary or secondary) of the V357 Peg. Type I (as primary  min.) should have 
been  type II (as secondary min.) and vice versa. The results of 
this error are: a)~the light elements for min I given in Table 2 in Keskin et
al. (2000) should have been for Min II b) this confusion of minima types caused Yasarsoy et al. (2000) to reach a wrong conclusion to point out that the 
secondary minima of the system are deeper than the primary minima. The authors 
have admitted the confusion that they committed in private communications. 
}


\IBVSEack{SA and MMK are grateful to Prof. Zeynel Tunca for his guidance and helpful comments about the manuscript. The authors would like to thank to the TUBITAK National Observatory (TUG) for their kind (partial financial and equipment) support. This work was also supported by the Research  Fund of Istanbul University, Project No: OR-104/07032000.}



\references

ESA, 1997, {\it The Hipparcos \& Tycho Catalogues}, ESA SP--1200

Keskin, V., Yasarsoy, B., Sipahi, E., 2000, {\it IBVS}, No.\,4855

Kwee, K. K. and van Woerden, H., 1956, {\it B.A.N.}, {\bf 12}, 330

Yasarsoy, B., Sipahi, E., Keskin, V., 2000, {\it IBVS}, No.\,4866

\endreferences

\end{document}

