\documentstyle[twoside, epsf]{article}

\input ibvs2.sty
\input ibvst.sty

\begin{document}

\IBVShead{4928}{21 July 2000}

\IBVStitle{New Eclipsing Variable in the Field of QS Geminorum}

\IBVSauth{Carroll, David D.; Hintz, Eric G.}

\IBVSinsto{Brigham Young University, Dept.\ of Physics and Astronomy, Provo, Utah 84602, USA\\ \indent e-mail: doctor@tardis.byu.edu}

\SIMBADobj{GSC 01342-01261}

\begintext

\vskip-6pt
\IBVSTnam{GSC 01342-01261}

\IBVSTcoo{6\hr46\mm43\sec}{+20\deg53\arcm21\arcs}{2000}

\IBVSTobs{Observations made with the 0.4-m David Derrick Telescope of the Orson Pratt Observatory on the campus of Brigham Young University.}

\IBVSTdet{Pictor 416 XT CCD at the Newtonian focus which gives a plate scale of 0.93 arcsec/pixel}

\IBVSTfil{Johnson $V$ (Bessel, 1990)}

\IBVSTcomp{HD 263542 (GSC 01342-01109, $V = 9.72$)\\
& HD 48995 (GSC 01342-00517, $V = 8.61$)}

\IBVSTsys{Johnson}{The two stars listed above}

\IBVSTdata{Upon request from the authors}

\IBVSTtyp{ EA (Algol variable) --- this is only a guess }

\IBVSTrem{
These observations were primarily to observe the delta Scuti star QS
Gem.  Since the magnitude of QS Gem is 8.847 compared to the new
variables 11.29 the errors are fairly large.  We also note that we only
saw one complete secondary minimum and only part of one primary
minimum.  The true nature of the star is yet to be determined. However,
we estimate a period of 1.32 d, with a the secondary minimum having a
drop of 0.18 mag and the primary having a drop of greater that 0.5
mag.}

\IBVSfig{5.5cm}{4928-f1.eps}{GSC 1342-1261 is labeled as No.\ 3}

\IBVSfig{6.75cm}{4928-f2.eps}{}

\IBVSfig{6.75cm}{4928-f3.eps}{}

\vskip-33pt
\reference

Bessell, M.S., 1990, {\it PASP}, {\bf 102}, 1181

\endreferences

\end{document}
