\documentstyle[twoside, epsf]{article}

\input ibvso.sty
\input ibvs2.sty

\begin{document}

\IBVShead{5599}{7 February 2005}

\IBVStitle{Observations of variables}

\IBVSabs{New observations of, and new information on known variable stars.}

\begintext


The last but one issue of the volume publishes new observations, and
results on known variable stars. Figures and data files are available
electronically.

\bigskip
\bigskip

The Editors

\bigskip
\bigskip
\bigskip



\IBVSOobs{2 February 2004}
{
Bedient, J. - University of Hawaii, bedient@hawaii.edu \\ %email
Richwine, P. - University of Arizona, pebbler@email.arizona.edu \\ %email
}{1}

\GCVSobj{NSV 12374}
\SIMBADobj{SV* R 321}

\IBVSOobj{
NSV 12374 }
{
NSV 12374 is found to be a Mira-type variable star using
archived CCD images and ASAS-3 data.
The period is 265 days and range 13.0 -- $<$15 (V).
Cross-identifications made: NSV 12374 = SV* R 321 = IRAS 19429-0526 = USNO-B1.0 0846-0566062 = 2MASS J19453923-0519183
}
{
light curve, \IBVSefigure{5599-f1.eps}
\IBVSfigKey{5599-f1.eps}{NSV 12374}{light curve}
phase diagram, \IBVSefigure{5599-f2.eps}
\IBVSfigKey{5599-f2.eps}{NSV 12374}{phased light curve}
data file \IBVSedata{5599-t1.txt}
\IBVSdataKey{5599-t1.txt}{NSV 12374}{photometry}
}{1}


\IBVSOobs{12 February 2004}
{
Ignatieva, T.I. - Sternberg Astronomical Institute, Moscow, Russia \\
Antipin, S.V. - Sternberg Inst. and Instr. of Astr., RAS, Moscow, Russia, antipin@sai.msu.ru \\ %email
}{2}

\IBVSecomment{GCVS:}
\GCVSobj{V1543 Cyg} 

\IBVSecomment{SIMBAD:} 
\SIMBADobj{V1543 Cyg}

\IBVSOobj{
V1543 Cyg }
{
V1543 Cyg, an SR: star in the GCVS, is actually a classical Cepheid.
JDmax = 2443343.07 + 2.03029d $\times$ E.
}
{
phased light curve, \IBVSefigure{5599-f3.eps}
\IBVSfigKey{5599-f3}{V1543 Cyg}{phased light curve}
data file \IBVSedata{5599-t2.txt}
\IBVSdataKey{5599-t2.txt}{V1543 Cyg}{photometry}
}{2}

\vfill\eject

\IBVSOobs{2 April 2004}
{
Dumitrescu, A. - Astronomical Institute of the Romanian Academy, alex@aira.astro.ro \\ %email
Iliev, L. - Astronomical Institute of the Bulgarian Academy, liliev@astro.bas.bg \\ %email
Tudose, V. - Astronomical Institute of the Romanian Academy, vtudose@aira.astro.ro \\ %email
}{3}

\IBVSecomment{SIMBAD:} 
\SIMBADobj{V376 And}

\IBVSOobj{
V376 And = HIP 12039 = HD 15922}
{
We report BV observations of the eclipsing binary system V376 And. Six times of minima are presented.
}
{
phased light curve, \IBVSefigure{5599-f4.ps}
\IBVSfigKey{5599-f4}{V376 And}{light curve}
data file \IBVSedata{5599-t3.txt}
\IBVSdataKey{5599-t3.txt}{V376 And}{photometry ; times of minima}
}{3}

\IBVSOobs{16 April 2004}
{
Otero, S. - Grupo Wezen 1 88 \& CEA, Argentina, varsao@fullzero.com.ar \\ %email
Pojmanski, G. - ASAS, {\tt http://www.astrouw.edu.pl/\~{}gp/asas} \\ %email
}{4}

\IBVSecomment{GCVS:}
\GCVSobj{NSV 12236}

\IBVSecomment{SIMBAD:} 
\SIMBADobj{SV* BV 1713}

\IBVSOobj{
NSV 12236 = ASAS 193907-2049.2 = GSC 6311 1034 = SV* BV 1713 = 2MASS J19390656-2049140}
{
NSV 12236 is a CWA star with the following elements: HJDmax 2452001.10 + 14.279 $\times$ E. Range in V= 11.35 -- 12.55 according to ASAS-3 data.
}
{
phased light curve, \IBVSefigure{5599-f5.ps}
\IBVSfigKey{5599-f5}{NSV 12236}{light curve}
ASAS-3 data \IBVSshortlink{http://www.astrouw.edu.pl/cgi-asas/asas_lc/193907-2049.2}{ASAS 193907-2049.2}
}{4}

\IBVSecomment{GCVS:}
\GCVSobj{NSV 05356}

\IBVSecomment{SIMBAD:} 
\SIMBADobj{HD 310803}

\IBVSOobj{
NSV 05356 = ASAS 114920-6600.6 = HD 310803 = SV* BV 726 = CPD $-$65 01725 = CoD $-$65 01151 = GSC 8985 2113 = 2MASS J11491992-6600387}
{
SIMBAD cross-identifications are correct but the position given is wrong due to a typographic error in the DEC that was written as $-$06 degrees instead of $-$66.
Tycho-2 position is 11\hr 49\mm 19\fsec944 $-$66\deg 00\arcm 38\farcs65 (2000.0)
SIMBAD wrongly puts the star at 11\hr 49\mm 42\sec $-$06\deg 00\farcm6 (2000.0)
NSV 05356 is a short period DCEP star (HD spectrum G0) with the following elements: HJDmax 2452056.529 + 1.39143 $\times$ E. Range in V= 9.89 -- 10.33 according to ASAS-3 data.
}
{
phased light curve, \IBVSefigure{5599-f6.ps}
\IBVSfigKey{5599-f6}{NSV 05356}{light curve}
ASAS-3 data \IBVSshortlink{http://www.astrouw.edu.pl/cgi-asas/asas_lc/114920-6600.6}{ASAS 114920-6600.6}
}{5}

\IBVSecomment{GCVS:}
\GCVSobj{NSV 10164}

\IBVSecomment{SIMBAD:} 
\SIMBADobj{NSV 10164}

\IBVSOobj{
NSV 10164 = ASAS 180601-4731.5 = GSC 8361 1107 = CPD $-$47 8688 = CD $-$47 12046 = SV* BV 1217 = 2MASS J18060173-4731272}
{
RVA variable star with elements: HJDmax 2452057.0 + 108.71 $\times$ E. V range is 9.84 -- 12.76 (ASAS-3 data).
}
{
phased light curve, \IBVSefigure{5599-f7.ps}
\IBVSfigKey{5599-f7}{NSV 10164}{light curve}
ASAS-3 data \IBVSshortlink{http://www.astrouw.edu.pl/cgi-asas/asas_lc/180601-4731.5}{ASAS 180601-4731.5}
}{6}

\vfill\eject

\IBVSOobs{27 April 2004}
{
Bernhard, K. - Linz, Austria, kl.bernhard@aon.at \\ %email
Kiyota, S. - Tsukuba, Japan, skiyota@nias.affrc.go.jp \\ %email
Moschner, W. - Lennestadt, Germany, wolfgang.moschner@t-online.de \\ %email
}{5}

\IBVSecomment{SIMBAD:} 
\SIMBADobj{GSC 0752-0542}

\IBVSOobj{
GSC 0752.0542 = Brh V39}
{
GSC 0752.0542 (RA: 07\hr 01\mm 00\fsec4 +10\deg 03\arcm 46\arcs, J2000) can be called as an 
anomalous RRab star, because of a period, which is typical for an RRab star 
and a folded light curve with a rather low amplitude, which looks more 
like an RRc star. This star shows a clear light curve variation, but a period
analysis of the available data does not point to any consistent solution. 
Max = HJD 2452306.468 + 0.71240 $\times$ E .
}
{
folded light curve (3/2000), \IBVSefigure{5599-f8.ps}
\IBVSfigKey{5599-f8}{GSC 0752-0542}{light curve}
folded light curve (10/2001-2/2002), \IBVSefigure{5599-f9.ps}
\IBVSfigKey{5599-f9}{GSC 0752-0542}{light curve}
folded light curve (3/2004), \IBVSefigure{5599-f10.ps}
\IBVSfigKey{5599-f10}{GSC 0752-0542}{light curve}
data file \IBVSedata{5599-t4.txt}
\IBVSdataKey{5599-t4.txt}{GSC 0752-0542}{photometry}
}{7}

\IBVSOobs{24 June 2004}
{
Krajci, Tom - 3933 Stockton Loop, SE Albuquerque, NM 87118-1104, loukrajci@comcast.net \\ %email
}{6}

\IBVSecomment{SIMBAD:} 
\SIMBADobj{V718 Her}

\IBVSOobj{
V718 Her}
{
V718 Her is currently listed in the GCVS as type EW/KW. Recent unfiltered 
observations from Tashkent show that it is in fact type RRc. Initial data 
indicate the following ephemeris for time of maximum:
HJDmax = 2453163.6535(8) + 0.297626(5) $\times$ E .
Note that the period is significantly different from the GCVS value of 
0.4588788, which is assessed as an aliasing effect.
}
{
folded light curve, \IBVSefigure{5599-f11.ps}
\IBVSfigKey{5599-f11}{V718 Her}{light curve}
data file \IBVSedata{5599-t5.txt}
\IBVSdataKey{5599-t5.txt}{V718 Her}{photometry}
}{8}

\IBVSecomment{SIMBAD:}
\SIMBADobj{BH UMa}

\IBVSOobj{
BH UMa}
{
BH UMa is currently listed in the GCVS as type EW/KE. Recent unfiltered 
observations from Tashkent show that the star is in fact type RRc. Initial data
indicate the following ephemeris for time of maximum:
HJDmax = 2453053.6545(5) + 0.349350(3) $\times$ E .
}
{
folded light curve, \IBVSefigure{5599-f12.ps}
\IBVSfigKey{5599-f12}{BH UMa}{light curve}
data file \IBVSedata{5599-t6.txt}
\IBVSdataKey{5599-t6.txt}{BH UMa}{photometry}
}{9}


\IBVSOobs{4 August 2004}
{
Sahin, T. - Akdeniz University, Turkey \\
Yesilyaprak, C. - Akdeniz University, Turkey \\
}{7}

\IBVSecomment{SIMBAD:}
\SIMBADobj{V2129 Cyg}

\IBVSOobj{
V2129 Cyg}
{
V2129 Cyg was discovered  by the Hipparcos Satellite as a low amplitude delta Scuti type star. Modulation of the light curve is suspected.
}
{
folded light curve, \IBVSefigure{5599-f13.ps}
\IBVSfigKey{5599-f13}{V2129 Cyg}{light curve}
data files \IBVSedata{5599-t7.txt}
\IBVSdataKey{5599-t7.txt}{V2129 Cyg}{photometry}
\IBVSedata{5599-t8.txt}
\IBVSdataKey{5599-t8.txt}{V2129 Cyg}{photometry}
\IBVSedata{5599-t9.txt}
\IBVSdataKey{5599-t9.txt}{V2129 Cyg}{photometry}
}{10}


\IBVSOobs{1 September 2004}
{
Frank, P.- BAV, Germany, frank.velden@t-online.de \\ %email
Bernhard, K.-  BAV, Austria, kl.bernhard@aon.at \\ %email
Quester, W.- BAV, Germany, wquester@aol.com \\ %email
Lloyd, C. - Rutherford Appleton Laboratory, UK, cl@astro1.bnsc.rl.ac.uk \\ %email
}{8}

\IBVSecomment{SIMBAD:}
\SIMBADobj{GSC 1927-0862}

\IBVSOobj{
GSC 1927-0862 = Brh V130}
{
GSC 1927-0862 (RA: 08\hr 08\mm 15\fsec9 DEC: +23\deg 04\arcm 10\arcs, J2000) is a W UMa star 
with the ephemeris: HJDminI = 2452707.522 + 0.536435 $\times$ E, range 
(unfiltered, near V): 12.7 -- 13.1  
}
{
folded light curve, \IBVSefigure{5599-f14.ps}
\IBVSfigKey{5599-f14}{GSC 1927-0862}{light curve}
data file, \IBVSedata{5599-t10.txt}
\IBVSdataKey{5599-t10.txt}{GSC 1927-0862}{photometry}
ROTSE1 data  \IBVSshortlink{http://skydot.lanl.gov/nsvs/star.php?num=7316757&mask=32004}{NSVS 7316757}
}{11}

\IBVSecomment{SIMBAD:}
\SIMBADobj{GSC 4992-0663}

\IBVSOobj{
GSC 4992-0663 = Brh V134}
{
GSC 4992.0663 (RA: 14\hr 36\mm 28\fsec4 DEC: $-$05\deg 36\arcm 22\arcs, J2000) is a W UMa star 
with the ephemeris: HJDminI = 2452811.400 +  0.242075 $\times$ E, range 
(unfiltered, near V): 12.6 -- 13.1  
}
{
folded light curve, \IBVSefigure{5599-f15.ps}
\IBVSfigKey{5599-f15}{GSC 4992-0663}{light curve}
data file, \IBVSedata{5599-t11.txt}
\IBVSdataKey{5599-t11.txt}{GSC 4992-0663}{photometry}
ASAS3data \IBVSshortlink{http://www.astrouw.edu.pl/cgi-asas/asas_cgi_get_data?143628-0536.4,asas3}{ASAS 143628-0536.4}
}{12}


\IBVSecomment{SIMBAD:}
\SIMBADobj{GSC 5749-1622}

\IBVSOobj{
GSC 5749-1622 = Brh V137}
{
Though W UMa stars often can be identified with an X-ray source, an entry in the
ROSAT All-Sky Bright Source Catalogue (1RXS) is quite rare. GSC 5749-1622 
(RA: 20\hr 19\mm 49\fsec6 DEC: $-$12\deg 30\arcm 38\arcs, J2000) can be identified with 
1RXS J201950.0-123037, 
the Tycho-2 Spectral Type Catalog gives the spectral type F8/G0 V, 
corresponding to an effective temperature of 6200 K. 
Ephemeris: HJDminI = 2452909.387 + 0.418895 $\times$ E, range (unfiltered, near V): 
9.7 -- 10.3 .
}
{
folded light curve, \IBVSefigure{5599-f16.ps}
\IBVSfigKey{5599-f16}{GSC 5749-1622}{light curve}
data file, \IBVSedata{5599-t12.txt}
\IBVSdataKey{5599-t12.txt}{GSC 5749-1622}{photometry}
ASAS3data \IBVSshortlink{http://www.astrouw.edu.pl/cgi-asas/asas_cgi_get_data?201950-1230.6,asas3}{ASAS 201950-1230.6}
}{13}


\IBVSOobs{2 September 2004}
{
Z{\l}oczewski, K. - Warsaw University Astronomical Observatory, kzlocz@astrouw.edu.pl \\ %email
}{9}

\IBVSecomment{SIMBAD:} 
\SIMBADobj{TU Tri}

\IBVSOobj{
TU Tri}
{
An outburst (14.6 mag)
was reported by M. Simonsen on January 1 2003. The last reported possible
outburst was in 1998, further two outbursts were recorded in 1995. K.
Torii confirmed that it was still in outburst on January 4 2003, and the
resultant light curve showed no superhumps (vsnet-campaign-dn 3237,
3262). Our light curve on January 1/2 2003 shows clear superhumps with
period 0.0745d estimated from the two observed minima. VAR$-$COMP denotes
the difference of the magnitude of the variable and the magnitude corresponding
to the sum of intensities of the comparisons. A small variation is found 
between C1 and C2 (up to 0.05 mag., see fig. 5599-f19), however, 
this does not affect the result we found on TU Tri.
}
{
finding chart, \IBVSefigure{5599-f17.ps}
\IBVSfigKey{5599-f17}{TU Tri}{finding chart}
light curves, \IBVSefigure{5599-f18.ps}
\IBVSfigKey{5599-f18}{TU Tri}{light curve}
\IBVSefigure{5599-f19.ps}
\IBVSfigKey{5599-f19}{TU Tri}{light curve}
data files \IBVSedata{5599-t13.txt}
\IBVSdataKey{5599-t13.txt}{TU Tri}{photometry}
\IBVSedata{5599-t14.txt}
\IBVSdataKey{5599-t14.txt}{TU Tri}{photometry}
}{14}

\IBVSOobs{3 November 2004}
{
Baranov, A. - Moscow Astronomy Club (c/o Sternberg Astron. Inst.) \\
}{10}

\IBVSecomment{SIMBAD:} 
\SIMBADobj{KP Dra}
\IBVSecomment{GCVS:} 
\GCVSobj{KP Dra}

\IBVSOobj{
KP Dra}
{
Min(I)=JD2448122.49+2.012415 $\times$ E. Bpg=12.8 -- 16.0.
}
{
light curve, \IBVSefigure{5599-f20.eps}
\IBVSfigKey{5599-f20}{KP Dra}{light curve}
data file \IBVSedata{5599-t15.txt}
\IBVSdataKey{5599-t15.txt}{KP Dra}{photometry}
}{15}

\IBVSOobs{9 November 2004}
{
Bernhard, K.-  BAV, Austria, klaus.bernhard@liwest.at \\ %email
Frank, P.- BAV, Germany, frank.velden@t-online.de \\ %email
Moschner, W. - BAV, Germany, wolfgang.moschner@t-online.de \\ %email
Proksch, W. - BAV, Germany, willi.proksch@t-online.de \\ %email
}{11}

\IBVSecomment{SIMBAD:} 
\SIMBADobj{GSC 2144-1499}

\IBVSOobj{
GSC 2144.1499 = Brh V152}
{
GSC 2144.1499 (RA: 19\hr 55\mm 11\fsec6 DEC: +24\deg 57\arcm 10\arcs, J2000) is a WUMa star 
with the ephemeris: HJDminI = 2453284.307 + 0.36424 $\times$ E, range 
(unfiltered, near V): 13.1 -- 13.6
}
{
light curve, \IBVSefigure{5599-f21.ps}
\IBVSfigKey{5599-f21}{GSC 2144-1499}{light curve}
data file, \IBVSedata{5599-t16.txt}
\IBVSdataKey{5599-t16.txt}{GSC 2144-1499}{photometry}
ROTSE data   \IBVSshortlink{http://skydot.lanl.gov/nsvs/star.php?num=8399096&mask=32004}{NSVS 8399096}
}{16}

\IBVSecomment{SIMBAD:} 
\SIMBADobj{GSC 1830-1432}

\IBVSOobj{
GSC 1830.1432 = Brh V129}
{
GSC 1830.1432 (RA: 04\hr 43\mm 41\fsec3 DEC: +22\deg 53\arcm 38\arcs, J2000) is a WUMa star 
with the ephemeris: HJDminI = 2452928.5399 +  0.271825 $\times$ E, range 
(unfiltered, near V): 11.5 -- 11.8  
}
{
light curve, \IBVSefigure{5599-f22.ps}
\IBVSfigKey{5599-f22}{GSC 1830-1432}{light curve}
data file, \IBVSedata{5599-t17.txt}
\IBVSdataKey{5599-t17.txt}{GSC 1830-1432}{photometry}
ROTSE data   \IBVSshortlink{http://skydot.lanl.gov/nsvs/star.php?num=6780089&mask=32004}{NSVS 6780089}
}{17}

\IBVSecomment{SIMBAD:} 
\SIMBADobj{GSC 1419-0091}

\IBVSOobj{
GSC 1419.0091 = Brh V132}
{
GSC 1419.0091 (RA: 10\hr 11\mm 59\fsec2 DEC: +16\deg 52\arcm 30\arcs, J2000) is a WUMa star 
with the ephemeris: HJDminI = 2452754.4602 + 0.266727 $\times$ E, range 
(unfiltered, near V): 11.4 -- 11.7 
}
{
light curve, \IBVSefigure{5599-f23.ps}
\IBVSfigKey{5599-f23}{GSC 1419-0091}{light curve}
data file, \IBVSedata{5599-t18.txt}
\IBVSdataKey{5599-t18.txt}{GSC 1419-0091}{photometry}
ROTSE data   \IBVSshortlink{http://skydot.lanl.gov/nsvs/star.php?num=10269934&mask=32004}{NSVS 10269934}
}{18}

\vfill\eject

\IBVSOobs{9 November 2004}
{
Pejcha, Ondrej - Nicholas Copernicus Observatory and Planetarium, Brno, Czech Republic, pejcha@astro.sci.muni.cz \\ %email
Mikulasek, Zdenek - Institute of Theoretical Physics and Astrophysics, Masaryk University in Brno, Kotlarska 2, 611 37 Brno, Czech Republic \\
Hroch, Filip - Institute of Theoretical Physics and Astrophysics, Masaryk University in Brno, Kotlarska 2, 611 37 Brno, Czech Republic \\
}{12}

\IBVSecomment{SIMBAD:} 
\SIMBADobj{GSC 02652-01324}

\IBVSOobj{
TrES-1 = GSC 02652-01324}
{
Using a simple model of exoplanet transit and a new robust method for O$-$C 
determination (both will be elaborated thoroughly elsewhere - 
Mikulasek et al., 2005) we have derived mid-transit timings for TrES-1 
exoplanet transits on two dates. Namely, 
JD$_{\rm hel}$ = 2 453 253.4685(6) (open circles)
JD$_{\rm hel}$ = 2 453 256.4985(18) (V - dots, Rc - open squares)
The O$-$C with respect to Alonso et al. (2004) ephemeris are (0.0012 $\pm$ 0.0007) 
and (0.0010 $\pm$ 0.0018), respectively. 
}
{
light curve, \IBVSefigure{5599-f24.ps}
\IBVSfigKey{5599-f24}{GSC 02652-01324}{light curve}
data files \IBVSedata{5599-t19.txt}
\IBVSdataKey{5599-t19.txt}{GSC 02652-01324}{photometry}
\IBVSedata{5599-t20.txt}
\IBVSdataKey{5599-t20.txt}{GSC 02652-01324}{photometry}
}{19}


\IBVSOobs{10 November 2004}
{
Khruslov, A.V., Tula, Russia, khruslov@bk.ru \\ %email
SkyDOT team - http://skydot.lanl.gov \\
Pojmanski, G., - ASAS, {\tt http://www.astrouw.edu.pl/\~{}gp/asas} \\
}{13}

\IBVSecomment{GCVS:}
\GCVSobj{V523 Aur}
\IBVSecomment{SIMBAD:}
\SIMBADobj{V523 Aur}

\IBVSOobj{
V523 Aur = GSC 2965-00210 =  NSVS 4705573 = Mis V0002}
{
V523 Aur , an E: star in the GCVS, is a W UMa star with the elements:
JDminI  = 2451518.32 + 0.33043 d $\times$ E , range  13.4 -- 14.2(R) according to
ROTSE1 data.
}
{
phased light curve,  \IBVSefigure{5599-f25.ps}
\IBVSfigKey{5599-f25}{V523 Aur}{light curve}
ROTSE1 data  \IBVSshortlink{http://skydot.lanl.gov/nsvs/star.php?num=4705573&mask=32004}{NSVS 4705573}
}{20}

\IBVSecomment{GCVS:}
\GCVSobj{FT Boo}
\IBVSecomment{SIMBAD:}
\SIMBADobj{FT Boo}

\IBVSOobj{
FT Boo = GSC 3465-00188 = NSVS 5115340 =  Tmz V042}
{
FT Boo is currently listed in the GCVS as type L:. According to ROTSE1 data,
it is an RRAB star with the following elements:
JDmax  = 2451422.190 + 0.458775 d $\times$ E,  range 13.4 -- 14.6 (R), M--m ~ 0.15 P
}
{
phased light curve, \IBVSefigure{5599-f26.ps}
\IBVSfigKey{5599-f26}{FT Boo}{light curve}
ROTSE1 data  \IBVSshortlink{http://skydot.lanl.gov/nsvs/star.php?num=5115340&mask=32004}{NSVS 5115340}
}{21}

\IBVSecomment{GCVS:}
\GCVSobj{FU Boo}
\IBVSecomment{SIMBAD:}
\SIMBADobj{FU Boo}

\IBVSOobj{
FU Boo = GSC 1472.01141 = NSVS 10517999 = ASAS 142254+1932.2 =  Tmz V734}
{
FU Boo , an LB: star in the GCVS, is an RRAB star with the elements:
JDmax = 2451432.74 + 0.65357 d $\times$ E , range 13.6 -- 14.6 (R), 13.2 -- 14.6 (V),
M--m ~ 0.18 P according to ROTSE1 and ASAS-3 data.
}
{
phased light curve, \IBVSefigure{5599-f27.ps}
\IBVSfigKey{5599-f27}{FU Boo}{light curve}
ROTSE1 data, \IBVSshortlink{http://skydot.lanl.gov/nsvs/star.php?num=10517999&mask=32004}{NSVS 10517999}
ASAS3 data \IBVSshortlink{http://www.astrouw.edu.pl/cgi-asas/asas_lc/142254+1932.2}{ASAS 142254+1932.2}
}{22}

\vfill\eject

\IBVSecomment{GCVS:}
\GCVSobj{CF Cam}
\IBVSecomment{SIMBAD:}
\SIMBADobj{CF Cam}

\IBVSOobj{
CF Cam = GSC 3728.01092 =  NSVS 1965946 = IRAS 03314+5804}
{
CF Cam , a DCEP: star in the GCVS, is a classical Cepheid with the elements:
JDmax  = 2451366.0 + 9.44 d $times$ E, range  11.2 -- 11.7 (R) according to ROTSE1
data.
}
{
phased light curve, \IBVSefigure{5599-f28.ps}
\IBVSfigKey{5599-f28}{CF Cam}{light curve}
ROTSE1 data  \IBVSshortlink{http://skydot.lanl.gov/nsvs/star.php?num=1965946&mask=32004}{NSVS 1965946}
}{23}

\IBVSecomment{GCVS:}
\GCVSobj{GW Cnc}
\IBVSecomment{SIMBAD:}
\SIMBADobj{GW Cnc}

\IBVSOobj{
GW Cnc = GSC 1399.01081 = NSVS 10127789 =ASAS  084813+2107.2 =  Tmz V003}
{
GW Cnc , an L: star in the GCVS , is actually an EW star with the elements:
JDminI =2451554.023 + 0.281415 d $\times$ E, range in 12.6 -- 13.2 -- 13.1 (R),
12.3 -- 13.2 -- 13.2 (V) according to ROTSE1 and ASAS-3 data.
}
{
phased light curve,  \IBVSefigure{5599-f29.ps}
\IBVSfigKey{5599-f29}{GW Cnc}{light curve}
ROTSE1 data,  \IBVSshortlink{http://skydot.lanl.gov/nsvs/star.php?num=10127789&mask=32004}{NSVS 10127789}
ASAS3 data \IBVSshortlink{http://www.astrouw.edu.pl/cgi-asas/asas_cgi_get_data?084813+2107.2,asas3}{ASAS 084813+2107.2}
}{24}

\IBVSecomment{GCVS:}
\GCVSobj{V602 Cyg}
\IBVSecomment{SIMBAD:}
\SIMBADobj{V602 Cyg}

\IBVSOobj{
V602 Cyg = TYC 3190.00950  = NSVS 5904647}
{
V602 Cyg is an L: star (spectral type G7) in the GCVS. According to NSVS data,
it is an SRD star with the elements:
JDmax = 2451260. + 34.5 d $\times$ E, range 10.3 -- 10.6 (R).
}
{
phased light curve,  \IBVSefigure{5599-f30.ps}
\IBVSfigKey{5599-f30}{V602 Cyg}{light curve}
ROTSE1 data  \IBVSshortlink{http://skydot.lanl.gov/nsvs/star.php?num=5904647&mask=32004}{NSVS 5904647}
}{25}

\IBVSecomment{GCVS:}
\GCVSobj{DR Lyn}
\IBVSecomment{SIMBAD:}
\SIMBADobj{DR Lyn}

\IBVSOobj{
DR Lyn = GSC 3421.02216 = NSVS 4785816 =  Tmz V023}
{
DR Lyn is an EA star in the GCVS without light elements. Light elements are:
JDminI = 2451483.98 + 1.78080 d $\times$ E , range  12.4 --  14.5 -- 12.6 (R),
D = 0.17 P according to ROTSE1 data.
}
{
phased light curve,  \IBVSefigure{5599-f31.ps}
\IBVSfigKey{5599-f31}{DR Lyn}{light curve}
ROTSE1 data  \IBVSshortlink{http://skydot.lanl.gov/nsvs/star.php?num=4785816&mask=32004}{NSVS 4785816}
}{26}

\IBVSecomment{GCVS:}
\GCVSobj{V344 Ser}
\IBVSecomment{SIMBAD:}
\SIMBADobj{V344 Ser}

\IBVSOobj{
V344 Ser = GSC 0347.00695 = NSVS 13419554 = ASAS 151159+0602.3 = Tmz V044}
{
V344 Ser , an L star in the GCVS , is actually an RRAB star with the elements:
JDmax = 24 51416.837 + 0.46506  d $\times$ E , range 13.1 -- 14.3 (R), 12.7 -- 14.5 (V),
M--m ~ 0.1 P according to ROTSE1 and ASAS-3 data.
}
{
phased light curve,  \IBVSefigure{5599-f32.ps}
\IBVSfigKey{5599-f32}{V344 Ser}{light curve}
ROTSE1 data,  \IBVSshortlink{http://skydot.lanl.gov/nsvs/star.php?num=13419554&mask=32004}{NSVS 13419554}
ASAS3 data \IBVSshortlink{http://www.astrouw.edu.pl/cgi-asas/asas_cgi_get_data?151159+0602.3,asas3}{ASAS 151159+0602.3}
}{27}

\IBVSecomment{GCVS:}
\GCVSobj{KQ UMa}
\IBVSecomment{SIMBAD:}
\SIMBADobj{KQ UMa}

\IBVSOobj{
KQ UMa = GSC 4376.01629 = NSVS 782942 = Tmz V083}
{
KQ UMa is an L: star in the GCVS. The star actually belongs to the RRAB
type with the following elements: JDmax = 2451493.21 + 0.48635 d $\times$ E,
range 14.0 -- 15.2 (R), M--m ~ 0.1 P according to ROTSE1 data.
}
{
phased light curve,  \IBVSefigure{5599-f33.ps}
\IBVSfigKey{5599-f33}{KQ UMa}{light curve}
ROTSE1 data  \IBVSshortlink{http://skydot.lanl.gov/nsvs/star.php?num=782942&mask=32004}{NSVS 782942}
(NSVS 782942 = NSVS 2496194)
}{28}

\IBVSecomment{GCVS:}
\GCVSobj{OQ Vir}
\IBVSecomment{SIMBAD:}
\SIMBADobj{OQ Vir}

\IBVSOobj{
OQ Vir = GSC 0306.00750 = NSVS 13266152 =  ASAS 132543+0603.4 =  Tmz V747}
{
OQ Vir , an SR: star in the GCVS, is actually an RRAB star with the
elements:  JDmax = 2451475.75 + 0.603915 d $\times$ E, range 13.6 -- 14.7 (R),
13.1 -- 14.5 (V), M--m ~ 0.2 P according to ROTSE1 and ASAS-3 data.
}
{
phased light curve,  \IBVSefigure{5599-f34.ps}
\IBVSfigKey{5599-f34}{OQ Vir}{light curve}
ROTSE1 data,  \IBVSshortlink{http://skydot.lanl.gov/nsvs/star.php?num=13266152&mask=32004}{NSVS 13266152}
ASAS3 data \IBVSshortlink{http://www.astrouw.edu.pl/cgi-asas/asas_cgi_get_data?132543+0603.4,asas3}{ASAS 132543+0603.4}
}{29}

\IBVSOobs{22 November 2004}
{
Hoogeveen, G.J. - Bottelaarpassage 43, Almere 1315 EP, Netherlands, gertho@xs4all.nl \\ %email
}{14}

\IBVSecomment{SIMBAD:}
\SIMBADobj{VX Dra} 
\SIMBADobj{FU Dra}

\IBVSOobj{
VX Dra}
{
We argue that VX Dra is identical to FU Dra, despite
considerable difference in coordinates.
}
{
finding chart,  \IBVSefigure{5599-f35.ps}
\IBVSfigKey{5599-f35}{VX Dra}{finding chart}
detailed description \IBVSetable{5599-t21.tex}
}{30}

\IBVSOobs{27 January 2005}
{
N\'emeth, P. - University of Szeged, Hungary, pnemeth@titan.physx.u-szeged.hu \\ %email
Kiss, L.L. - University of Sydney 2006, NSW Australia \\
S\'arneczky, K. - University of Szeged, Hungary \\
}{15}

\IBVSecomment{SIMBAD:}
\SIMBADobj{HS 0705+6700}

\IBVSOobj{
HS 0705+6700 = GSC 4123-265
}
{
New observations in Johnson V and Cousins I bands are presented for the 
pre-cataclysmic binary HS 0705+6700. The new ephemeris, improved by 
seven new epochs of minimum, is HJD(min)=2453071.42845 + 0.095646783(8)E.
}
{
phased light curve,  \IBVSefigure{5599-f36.eps}
\IBVSfigKey{5599-f36}{HS 0705+6700}{light curve}
times of minima, \IBVSedata{5599-t22.txt}
\IBVSdataKey{5599-t22.txt}{HS 0705+6700}{times of minima}
data files \IBVSedata{5599-t23.txt}
\IBVSdataKey{5599-t23.txt}{HS 0705+6700}{photometry}
\IBVSedata{5599-t24.txt}
\IBVSdataKey{5599-t24.txt}{HS 0705+6700}{photometry}
}{31}

\references

Alonso, R., Brown, T.M., Torres, G., Latham, D.W., Sozzetti, A.,
Mandushev, G., Belmonte, J.A., Charbonneau, D., Deeg, H.J.,
Dunham, E.W., O'Donovan, F.T., Stefanik, R.P., 2004, {\it ApJL},
{\bf 613}, L153

Mikulasek, Z., et al., 2005, in preparation

\end{document}

