\documentstyle[twoside, epsf]{article}

\input ibvsn.sty
\input ibvs2.sty

\begin{document}

\IBVShead{6100}{13 March 2014}

\IBVStitle{Reports on New Discoveries}

\IBVSabs{List of newly discovered variables.}

%Previous reports can be found in \IBVSshortlink{http://www.konkoly.hu/cgi-bin/IBVS?5998}{IBVS No. 5998}.

\IBVSnews{27 September 2011}
{
Monninger, G. - Bundesdeutsche Arbeitsgemeinschaft f\"ur Ver\"anderliche Sterne e.V. (BAV), Munsterdamm 90, DE-12169 Berlin, Germany, gerold.monninger@online.de \\ %email
}{1}

\IBVSnstar{
22 07 15.50 }
{ +41 11 56.9 }
{DSCT }
{11.93 (Vmag - GSC2.3)}
{ 0.07855(1) d }
{2455805.4193(7) }
{ GSC 3202-0370 =
 USNO-A2.0 1275-17055482 =
 USNO-B1.0 1311-0458390 =
 Tycho-2 3202-00370-1 =
 2MASS 22071548+4111573 =
 GSC2.3 N2XB000049
 }
{finding chart, \IBVSefigure{6100-f1.ps}
\IBVSfigKey{6100-f1.ps}{GSC 3202-0370}{finding chart}
light curve, \IBVSefigure{6100-f2.ps}
\IBVSfigKey{6100-f2.ps}{GSC 3202-0370}{light curve}
data file \IBVSedata{6100-t1.txt}
\IBVSdataKey{6100-t1.txt}{GSC 3202-0370}{photometry}
}{1}

\IBVSnews{8 December 2011}
{
Liakos, A. - Department of Astrophysics, Astronomy and Mechanics, National and Kapodistrian University of Athens, Panepistimioupolis, GR-157 84, Zografos, Athens, Hellas, alliakos@phys.uoa.gr \\ %email
Niarchos, P. - Department of Astrophysics, Astronomy and Mechanics, National and Kapodistrian University of Athens, Panepistimioupolis, GR-157 84, Zografos, Athens, Hellas, pniarcho@phys.uoa.gr \\ %email
}{2}

Remark: Detected in the FoV of V482 Per.

\IBVSnstar{
04 15 44.8 }
{ +47 29 18.2 }
{DSCT }
{B=10.677 mag (The Hipparcos and Tycho Catalogues)}
{ 1.08095 h }
{- }
{ GSC 3332-0388 = TYC 3332-0388-1 = USNO-A2.0 1350-04385880
 }
{finding chart, \IBVSefigure{6100-f3.eps}
\IBVSfigKey{6100-f3.eps}{GSC 3332-0388}{finding chart}
light curve, \IBVSefigure{6100-f4.eps}
\IBVSfigKey{6100-f4.eps}{GSC 3332-0388}{light curve}
data file \IBVSedata{6100-t2.txt}
\IBVSdataKey{6100-t2.txt}{GSC 3332-0388}{photometry}
}{2}

Remark: Detected in the FoV of TW Lac and V413 Lac

\IBVSnstar{
22 30 02.3 }
{ +54 46 57.9 }
{DSCT }
{B=13.9 mag (The USNO-A2.0 Catalogue)}
{ 1.27973 h }
{- }
{ GSC 3987-1298 = USNO-A2.0 1425-13529111
 }
{finding chart, \IBVSefigure{6100-f5.eps}
\IBVSfigKey{6100-f5.eps}{GSC 3987-1298}{finding chart}
light curve, \IBVSefigure{6100-f6.eps}
\IBVSfigKey{6100-f6.eps}{GSC 3987-1298}{light curve}
data file \IBVSedata{6100-t3.txt}
\IBVSdataKey{6100-t3.txt}{GSC 3987-1298}{photometry}
}{3}

Remark:  Detected in the FoV of QX And

\IBVSnstar{
01 57 12.04 }
{ +37 54 35.9 }
{DSCT }
{R=15.5 mag (The USNO-A2.0 Catalogue)}
{ 2.792904 h }
{- }
{ USNO-A2.0 1275-01165814
 }
{finding chart, \IBVSefigure{6100-f7.eps}
\IBVSfigKey{6100-f7.eps}{USNO-A2.0 1275-01165814}{finding chart}
light curve, \IBVSefigure{6100-f8.eps}
\IBVSfigKey{6100-f8.eps}{USNO-A2.0 1275-01165814}{light curve}
data file \IBVSedata{6100-t4.txt}
\IBVSdataKey{6100-t4.txt}{USNO-A2.0 1275-01165814}{photometry}
}{4}


\IBVSnews{13 January 2012}
{
Martignoni, Massimiliano - Stazione Astronomica Betelgeuse, Magnago, Milano,
Italy, massimiliano.martignoni@alice.it \\ %email
}{3}

Remark: UCAC3 276-106147 is an EW type eclipsing binary in the field of view of
 TV Lyn.
 

\IBVSnstar{
07 34 16.6 }
{ 47 54 02.4 }
{EW }
{14.15-14.75 (V)}
{ 0.3150905d }
{2455933.5083 }
{ UCAC3 276-106147
 }
{finding chart, \IBVSefigure{6100-f9.ps}
\IBVSfigKey{6100-f9.ps}{UCAC3 276-106147}{finding chart}
light curve, \IBVSefigure{6100-f10.ps}
\IBVSfigKey{6100-f10.ps}{UCAC3 276-106147}{light curve}
data file \IBVSedata{6100-t5.txt}
\IBVSdataKey{6100-t5.txt}{UCAC3 276-106147}{photometry}
data file \IBVSedata{6100-t6.txt}
\IBVSdataKey{6100-t6.txt}{UCAC3 276-106147}{minima/maxima times}
}{5}

\IBVSnews{20 February 2012}
{
Monninger, G. - Bundesdeutsche Arbeitsgemeinschaft f\"ur Ver\"anderliche Sterne e.V. (BAV), Munsterdamm 90, DE-12169 Berlin, Germany, gerold.monninger@online.de \\ %email
}{4}

Remark: In the field of the high amplitude delta scuti variable (HADS) 
GSC 01924-01134 (this IBVS issue, Monninger, 2011).
USNO-B1.0 1191-0155860 is listed in the Catalogue of SDSS BHB candidates
(Smith et al., 2010). A modulation in the light curve was observed.

\IBVSnstar{
07 44 07.84 }
{ +29 08 20.12 }
{ RRab }
{15.92 (Vmag - GSC2.3)}
{ 0.45283(1) d }
{2455887.611(1) }
{ USNO-B1.0 1191-0155860 = USNO-A2.0 1125-05322478 = 2MASS 07440785+2908199 = GSC2.3 N8R3014149
 }
{finding chart, \IBVSefigure{6100-f11.ps}
\IBVSfigKey{6100-f11.ps}{USNO-B1.0 1191-0155860}{finding chart}
light curve, \IBVSefigure{6100-f12.ps}
\IBVSfigKey{6100-f12.ps}{USNO-B1.0 1191-0155860}{light curve}
data file \IBVSedata{6100-t7.txt}
\IBVSdataKey{6100-t7.txt}{USNO-B1.0 1191-0155860}{photometry}
}{6}

\IBVSnews{4 June 2012}
{
H\"ummerich, Stefan - Bundesdeutsche Arbeitsgemeinschaft f\"ur Ver\"anderliche Sterne e.V. (BAV), Munsterdamm 90, DE-12169 Berlin, Germany, 
ernham@rz-online.de \\ %email
Bernhard, Klaus - Bundesdeutsche Arbeitsgemeinschaft f\"ur Ver\"anderliche Sterne e.V. (BAV), Munsterdamm 90, DE-12169 Berlin, Germany, 
klaus.bernhard@liwest.at \\ %email
}{5}

Remark: GSC 02504-01101 (2MASS J-K = 0.264) has been identified as a double-mode RR Lyrae (RRd) star by analysis of CRTS data (Drake et al., 2009) with Period04 (Lenz et al., 2005):\\
\\
\begin{tabular}{llll}
\hline
    &   frequency (c/d)&  semi-amplitude (mag) & \\
\hline
F1  &   2.9274089      &  0.1759               &  (first overtone)\\
F2  &   2.1747158      &  0.1423               &  (fundamental)\\
F3  &   5.1021296      &  0.0564               &  (F1+F2)\\
F4  &   4.3494536      &  0.0419               &  (2F2)\\
\hline
\end{tabular}
\\
\\
With a fundamental period of 0.4598 d, the star is near the lower edge of known RRd stars in the Petersen diagram; the ratio F2/F1=0.743 is in agreement with other RRd variables. GSC 02504-01101 is listed in the Catalogue of SDSS BHB candidates (Smith et al., 2010).\\

\IBVSnstar{
09 40 51.026 }
{ +34 52 05.32 }
{ RRd }
{14.69 (Vmag - GSC)}
{ 0.4598 d }
{- }
{ GSC 02504-01101 = USNO-B1.0 1248-0174773 = 2MASS J09405102+3452053 = WISE J094051.03+345205.3 = CSS\_J094051.0+345205
 }
{finding chart, \IBVSefigure{6100-f13.ps}
\IBVSfigKey{6100-f13.ps}{GSC 02504-01101}{finding chart}
light curve, \IBVSefigure{6100-f14.ps}
\IBVSfigKey{6100-f14.ps}{GSC 02504-01101}{light curve}
data file \IBVSedata{6100-t8.txt}
\IBVSdataKey{6100-t8.txt}{GSC 02504-01101}{photometry}
}{7}

\IBVSnews{12 June 2012}
{
Bernhard, Klaus - Bundesdeutsche Arbeitsgemeinschaft f\"ur Ver\"anderliche Sterne e.V. (BAV), Munsterdamm 90, DE-12169 Berlin, Germany, 
klaus.bernhard@liwest.at \\ %email
H\"ummerich, Stefan - Bundesdeutsche Arbeitsgemeinschaft f\"ur Ver\"anderliche Sterne e.V. (BAV), Munsterdamm 90, DE-12169 Berlin, Germany, 
ernham@rz-online.de \\ %email
}{6}

Remark: USNO-B1.0 1221-0206959 (2MASS J-K = 0.119) has been identified as a 
double-mode RR Lyrae (RRd) star by analysis of CRTS data (Drake et al., 2009) 
with Period04 (Lenz et al., 2005):
\\
\begin{tabular}{llll}
\hline
      & frequency (c/d) & semi-amplitude (mag) & \\
\hline
F1    & 2.66122         & 0.1944               & (first overtone) \\
F2    & 1.98192         & 0.1006               & (fundamental) \\
F3    & 5.32245         & 0.0424               & (2F1) \\
F4    & 4.64316         & 0.0443               & (F1+F2) \\
\hline
\end{tabular}
\\
\\
Analysis and folded lightcurves were based on CRTS data from HJD 2453481 to 
2455358 as the period is possibly variable.
With a fundamental period of 0.50456 d, the star is situated in the middle of 
the Petersen diagram; the ratio F1/F2=0.745 is in agreement with other RRd 
variables. USNO-B1.0 1221-0206959 is listed in the Catalogue of SDSS BHB 
candidates (Smith et al., 2010).

\IBVSnstar{
 09 30 44.097 }
{ +32 09 16.83 }
{ RRd }
{15.27 (Vmag - NOMAD)}
{ 0.50456 d }
{- }
{ USNO-B1.0 1221-0206959 = UCAC3 245-100368 = 2MASS J09304409+3209168 = WISE J093044.10+320917.1 = CSS\_J093044.1+320916
 }
{finding chart, \IBVSefigure{6100-f15.ps}
\IBVSfigKey{6100-f15.ps}{USNO-B1.0 1221-0206959}{finding chart}
light curve, \IBVSefigure{6100-f16.ps}
\IBVSfigKey{6100-f16.ps}{USNO-B1.0 1221-0206959}{light curve}
data file \IBVSedata{6100-t9.txt}
\IBVSdataKey{6100-t9.txt}{USNO-B1.0 1221-0206959}{photometry}
}{8}

\IBVSnews{23 July 2012}
{Nelson, R.H. - Sylvester Robotic Observatory, Prince George, BC, Canada,
bob.nelson@shaw.ca \\ %email
Lubcke, G. - 1400 E Washington Ave, Madison, WI 53703,
lubcke@tds.net \\ %email
}{7}

Remark: In the vicinity of V471 Cas.

\IBVSnstar{
 01 32 32.8 }
{ +55 15 26.23 }
{ EW }
{13.43 (R mag = GSC2.3)}
{ 0.2409532(2) }
{ 2455937.5483(12) }
{ GSC 3674-1587
 }
{finding chart, \IBVSefigure{6100-f17.ps}
\IBVSfigKey{6100-f17.ps}{GSC 3674-1587}{finding chart}
light curve, \IBVSefigure{6100-f18.ps}
\IBVSfigKey{6100-f18.ps}{GSC 3674-1587}{light curve}
light curve, \IBVSefigure{6100-f19.ps}
\IBVSfigKey{6100-f19.ps}{GSC 3674-1587}{light curve}
light curve, \IBVSefigure{6100-f20.ps}
\IBVSfigKey{6100-f20.ps}{GSC 3674-1587}{light curve}
data file \IBVSedata{6100-t10.txt}
\IBVSdataKey{6100-t10.txt}{GSC 3674-1587}{photometry}
}{9}

\IBVSnews{15 August 2012}
{
Bernhard, Klaus - Bundesdeutsche Arbeitsgemeinschaft f\"ur Ver\"anderliche Sterne e.V. (BAV), Munsterdamm 90, DE-12169 Berlin, Germany, 
klaus.bernhard@liwest.at \\ %email
H\"ummerich, Stefan - Bundesdeutsche Arbeitsgemeinschaft f\"ur Ver\"anderliche Sterne e.V. (BAV), Munsterdamm 90, DE-12169 Berlin, Germany, 
ernham@rz-online.de \\ %email
}{8}

Remark: USNO-B1.0 1220-0275842 (2MASS J-K = 0.193) has been identified as a double-mode RR Lyrae (RRd) star by analysis of CRTS data (Drake et al., 2009) with Period04 (Lenz et al., 2005):
\\
\begin{tabular}{llllll}
\hline
    & frequency (c/d)& period (d) & semi-amplitude (mag) & epoch (max)  & \\
\hline
F1  &   2.857841     &  0.349914  &     0.196            & 2456018.599  & (first overtone) \\
F2  &   2.124844     &  0.470622  &     0.170            & 2456018.684  & (fundamental) \\
\hline
\end{tabular}
\\
\\
With a fundamental period of 0.470622 d, the star is near the lower edge of known RRd stars in the Petersen diagram; the ratio F2/F1=0.7435 is in agreement with other RRd variables.
No linear combination modes could be found in the data. USNO-B1.0 1220-0275842 is listed in the Catalogue of SDSS BHB candidates (Smith et al., 2010).\\

\IBVSnstar{
15 16 09.239 }
{ +32 00 07.27 }
{ RRd }
{15.77 - 16.45 (CV - CRTS)}
{ 0.470622 d }
{- }
{ USNO-B1.0 1220-0275842 = UCAC4 611-051459 = 2MASS J15160921+3200073 = WISE J151609.21+320007.3 = CSS\_J151609.2+320007
 }
{finding chart, \IBVSefigure{6100-f21.ps}
\IBVSfigKey{6100-f21.ps}{USNO-B1.0 1220-0275842}{finding chart}
light curve, \IBVSefigure{6100-f22.ps}
\IBVSfigKey{6100-f22.ps}{USNO-B1.0 1220-0275842}{light curve}
data file \IBVSedata{6100-t11.txt}
\IBVSdataKey{6100-t11.txt}{USNO-B1.0 1220-0275842}{photometry}
}{10}

\IBVSnews{15 August 2012}
{
H\"ummerich, Stefan - Bundesdeutsche Arbeitsgemeinschaft f\"ur Ver\"anderliche Sterne e.V. (BAV), Munsterdamm 90, DE-12169 Berlin, Germany, 
ernham@rz-online.de \\ %email
Bernhard, Klaus - Bundesdeutsche Arbeitsgemeinschaft f\"ur Ver\"anderliche Sterne e.V. (BAV), Munsterdamm 90, DE-12169 Berlin, Germany, 
klaus.bernhard@liwest.at \\ %email
}{9}

Remark: GSC 02015-00233 (2MASS J-K = 0.225) has been identified as a double-mode RR Lyrae (RRd) star by analysis of CRTS data (Drake et al., 2009) with Period04 (Lenz et al., 2005):
\\
\begin{tabular}{llllll}
\hline
    & frequency (c/d)& period (d) & semi-amplitude (mag) & epoch (max)  & \\
\hline
F1  &   2.709041     &  0.369134  &     0.187            & 2456042.399  & (first overtone) \\
F2  &   2.01935      &  0.495208  &     0.062            & 2456042.233  & (fundamental) \\
\hline
\end{tabular}
\\
\\
With a fundamental period of 0.495208 d, the star is situated in the middle of known RRd stars in the Petersen diagram; the ratio F2/F1=0.745 is in agreement with other RRd variables.
No linear combination modes could be found in the data. GSC 02015-00233 is listed in the Catalogue of SDSS BHB candidates (Smith et al., 2010).\\

\IBVSnstar{
14 31 30.858 }
{ +22 50 23.37 }
{ RRd }
{15.34 - 15.87 (CV - CRTS)}
{ 0.495208 d }
{- }
{ GSC 02015-00233 = USNO-B1.0 1128-0282033 = UCAC4 565-051392 = 2MASS J14313085+2250234 = WISE J143130.85+225023.3 = CSS\_J143130.9+225023
 }
{finding chart, \IBVSefigure{6100-f23.ps}
\IBVSfigKey{6100-f23.ps}{GSC 02015-00233}{finding chart}
light curve, \IBVSefigure{6100-f24.ps}
\IBVSfigKey{6100-f24.ps}{GSC 02015-00233}{light curve}
data file \IBVSedata{6100-t12.txt}
\IBVSdataKey{6100-t12.txt}{GSC 02015-00233}{photometry}
}{11}

\IBVSnews{15 August 2012}
{
H\"ummerich, Stefan - Bundesdeutsche Arbeitsgemeinschaft f\"ur Ver\"anderliche Sterne e.V. (BAV), Munsterdamm 90, DE-12169 Berlin, Germany, 
ernham@rz-online.de \\ %email
Drake, A.J. - Catalina Real-Time Transient Survey \\
}{10}

Remark: UCAC4 position. J-K=0.216 (2MASS). Rise duration: 39\%.
USNO-B1.0 1185-0218778 is listed in the Catalogue of SDSS BHB candidates 
(Smith et al., 2010).

\IBVSnstar{
14 20 31.084 }
{ +28 31 25.59 }
{ RRc }
{ 14.98 - 15.50 (CV) }
{ 0.291608 d }
{ 2453479.80 }
{ USNO-B1.0 1185-0218778 = UCAC4 593-052447 = 2MASS J14203110+2831255 = WISE J142031.08+283125.6 = CSS\_J142031.1+283125
 }
{finding chart, \IBVSefigure{6100-f25.ps}
\IBVSfigKey{6100-f25.ps}{USNO-B1.0 1185-0218778}{finding chart}
light curve, \IBVSefigure{6100-f26.ps}
\IBVSfigKey{6100-f26.ps}{USNO-B1.0 1185-0218778}{light curve}
data file \IBVSedata{6100-t13.txt}
\IBVSdataKey{6100-t13.txt}{USNO-B1.0 1185-0218778}{photometry}
}{12}

Remark: UCAC4 position. J-K=0.339 (2MASS). Rise duration: 11\%.
USNO-B1.0 1047-0235244 is listed in the Catalogue of SDSS BHB candidates 
(Smith et al., 2010).

\IBVSnstar{
14 36 37.890 }
{ +14 47 49.16 }
{ RRab }
{ 15.17 - 16.13 (CV) }
{ 0.523764 d }
{ 2455365.745 }
{ USNO-B1.0 1047-0235244 = UCAC4 524-056277 = 2MASS J14363788+1447491 = WISE J143637.88+144749.1 = CSS\_J143637.9+144749
 }
{finding chart, \IBVSefigure{6100-f27.ps}
\IBVSfigKey{6100-f27.ps}{USNO-B1.0 1047-0235244}{finding chart}
light curve, \IBVSefigure{6100-f28.ps}
\IBVSfigKey{6100-f28.ps}{USNO-B1.0 1047-0235244}{light curve}
data file \IBVSedata{6100-t14.txt}
\IBVSdataKey{6100-t14.txt}{USNO-B1.0 1047-0235244}{photometry}
}{13}

Remark: UCAC4 position. J-K=0.556 (2MASS). Rise duration: 13\%.
USNO-B1.0 1014-0232010 is listed in the Catalogue of SDSS BHB candidates (Smith
 et al., 2010).

\IBVSnstar{
14 45 59.525 }
{ +11 28 07.26 }
{ RRab }
{ 15.52 - 16.60 (CV) }
{ 0.499028 d }
{ 2454515.932 }
{ USNO-B1.0 1014-0232010 = UCAC4 508-058222 = 2MASS J14455953+1128071 = WISE J144559.53+112807.1 = CSS\_J144559.5+112807
 }
{finding chart, \IBVSefigure{6100-f29.ps}
\IBVSfigKey{6100-f29.ps}{USNO-B1.0 1014-0232010}{finding chart}
light curve, \IBVSefigure{6100-f30.ps}
\IBVSfigKey{6100-f30.ps}{USNO-B1.0 1014-0232010}{light curve}
data file \IBVSedata{6100-t15.txt}
\IBVSdataKey{6100-t15.txt}{USNO-B1.0 1014-0232010}{photometry}
}{14}

Remark: 2MASS position. J-H=0.084 (2MASS; J-H value given as Kmag is flagged as 
being of bad quality.) Rise duration: 15\%.
USNO-B1.0 1138-0226755 is listed in the Catalogue of SDSS BHB candidates (Smith
et al., 2010).

\IBVSnstar{
15 35 21.609 }
{ +23 53 50.07 }
{ RRab }
{ 15.60 - 16.62 (CV) }
{ 0.526759 d }
{ 2453560.740 }
{ USNO-B1.0 1138-0226755 = 2MASS J15352160+2353500 = WISE J153521.60+235350.1 = CSS\_J153521.6+235350
 }
{finding chart, \IBVSefigure{6100-f31.ps}
\IBVSfigKey{6100-f31.ps}{USNO-B1.0 1138-0226755}{finding chart}
light curve, \IBVSefigure{6100-f32.ps}
\IBVSfigKey{6100-f32.ps}{USNO-B1.0 1138-0226755}{light curve}
data file \IBVSedata{6100-t16.txt}
\IBVSdataKey{6100-t16.txt}{USNO-B1.0 1138-0226755}{photometry}
}{15}

Remark: UCAC4 position. J-K=0.277 (2MASS). Rise duration: 14\%.
USNO-B1.0 1060-0220956 is listed in the Catalogue of SDSS BHB candidates (Smith
et al., 2010).

\IBVSnstar{
14 26 44.107 }
{ +16 04 57.82 }
{ RRab }
{ 15.00 - 16.14 (CV) }
{ 0.457791 d }
{ 2455351.779 }
{ USNO-B1.0 1060-0220956 = UCAC4 531-055289 = 2MASS J14264411+1604579 = WISE J142644.11+160457.8 = CSS\_J142644.1+160457
 }
{finding chart, \IBVSefigure{6100-f33.ps}
\IBVSfigKey{6100-f33.ps}{USNO-B1.0 1060-0220956}{finding chart}
light curve, \IBVSefigure{6100-f34.ps}
\IBVSfigKey{6100-f34.ps}{USNO-B1.0 1060-0220956}{light curve}
data file \IBVSedata{6100-t17.txt}
\IBVSdataKey{6100-t17.txt}{USNO-B1.0 1060-0220956}{photometry}
}{16}

Remark: UCAC4 position. J-K=0.291 (2MASS). Rise duration: 13\%.
USNO-B1.0 1360-0241542 is listed in the Catalogue of SDSS BHB candidates (Smith
et al., 2010).

\IBVSnstar{
14 47 06.527 }
{ +46 02 13.79 }
{ RRab }
{ 14.49 - 15.66 (CV) }
{ 0.481240 d }
{ 2454905.952 }
{ USNO-B1.0 1360-0241542 = UCAC4 681-055635 = 2MASS J14470651+4602136 = WISE J144706.53+460213.7 = CSS\_J144706.6+460213
 }
{finding chart, \IBVSefigure{6100-f35.ps}
\IBVSfigKey{6100-f35.ps}{USNO-B1.0 1360-0241542}{finding chart}
light curve, \IBVSefigure{6100-f36.ps}
\IBVSfigKey{6100-f36.ps}{USNO-B1.0 1360-0241542}{light curve}
data file \IBVSedata{6100-t18.txt}
\IBVSdataKey{6100-t18.txt}{USNO-B1.0 1360-0241542}{photometry}
}{17}

\IBVSnews{14 January 2013}
{
H\"ummerich, S. - Bundesdeutsche Arbeitsgemeinschaft f\"ur Ver\"anderliche Sterne e.V. (BAV), Munsterdamm 90, DE-12169 Berlin, Germany, ernham@rz-online.de \\ %email
}{11}

Remark: GSC 00330-01491 has been identified as an RRc star by analysis of 
CRTS data (Drake et al., 2009).
UCAC4 position. $J-K=0.073$ (2MASS; Skrutskie et al., 2006). Rise duration: 47%.
GSC 00330-01491 is listed in the Catalogue of SDSS BHB candidates (Smith et al.,
 2010).
 
\IBVSnstar{
14 59 54.942 }
{ +04 44 26.04 }
{ RRc }
{ 14.26 - 14.67 (CV) }
{ 0.352039 d }
{ 2453904.783 }
{ GSC 00330-01491 = USNO-B1.0 0947-0233808 = UCAC4 474-052391 = 2MASS J14595492+0444259 = WISE J145954.93+044425.9 = CSS\_J145954.9+044426
 }
{finding chart, \IBVSefigure{6100-f37.ps}
\IBVSfigKey{6100-f37.ps}{GSC 00330-01491}{finding chart}
light curve, \IBVSefigure{6100-f38.ps}
\IBVSfigKey{6100-f38.ps}{GSC 00330-01491}{light curve}
data file \IBVSedata{6100-t19.txt}
\IBVSdataKey{6100-t19.txt}{GSC 00330-01491}{photometry}
}{18}

Remark: USNO-B1.0 0994-0247663 has been identified as an RRc star by analysis 
of CRTS data (Drake et al., 2009). UCAC4 position. 
$J-K$=0.265 (2MASS; Skrutskie et al., 2006). Rise duration: 39%.
USNO-B1.0 0994-0247663 is listed in the Catalogue of SDSS BHB candidates (Smith 
et al., 2010).

\IBVSnstar{
15 47 24.001 }
{ +08 44 34.63 }
{ RRab }
{ 14.72 - 15.83 (CV) }
{ 0.501280 d }
{ 2453818.922 }
{ USNO-B1.0 0994-0247663 = UCAC4 498-063752 = 2MASS J15060750+0926369 = WISE J150607.50+092636.9 = CSS\_J150607.5+092636
 }
{finding chart, \IBVSefigure{6100-f39.ps}
\IBVSfigKey{6100-f39.ps}{USNO-B1.0 0994-0247663}{finding chart}
light curve, \IBVSefigure{6100-f40.ps}
\IBVSfigKey{6100-f40.ps}{USNO-B1.0 0994-0247663}{light curve}
data file \IBVSedata{6100-t20.txt}
\IBVSdataKey{6100-t20.txt}{USNO-B1.0 0994-0247663}{photometry}
}{19}

Remark: USNO-B1.0 1049-0245939 has been identified as an RRc star by analysis 
of CRTS data (Drake et al., 2009). UCAC4 position. 
$J-K$=0.183 (2MASS; Skrutskie et al., 2006). Rise duration: 40%.
USNO-B1.0 1049-0245939 is listed in the Catalogue of SDSS BHB candidates (Smith 
et al., 2010).

\IBVSnstar{
15 37 26.810 }
{ +14 56 58.31 }
{ RRc }
{ 15.18 - 15.64 (CV) }
{ 0.362629 d }
{ 2454346.644 }
{ USNO-B1.0 1049-0245939 = UCAC4 525-059342 = 2MASS J15372680+1456583 = WISE J153726.79+145658.2 = CSS\_J153726.8+145658
 }
{finding chart, \IBVSefigure{6100-f41.ps}
\IBVSfigKey{6100-f41.ps}{USNO-B1.0 1049-0245939}{finding chart}
light curve, \IBVSefigure{6100-f42.ps}
\IBVSfigKey{6100-f42.ps}{USNO-B1.0 1049-0245939}{light curve}
data file \IBVSedata{6100-t21.txt}
\IBVSdataKey{6100-t21.txt}{USNO-B1.0 1049-0245939}{photometry}
}{20}



\IBVSnews{7 February 2013}
{
Martignoni, Massimiliano - "Stazione Astronomica Betelgeuse", Magnago, Milano, Italy, massimiliano.martignoni@alice.it \\ %email
}{12}

Remark: TYC 5378-1590-1 is an EA type eclipsing binary in the field of view of DV Mon.
It was observed with a 0.25m Schmidt-Cassegrain Telescope (f/10) of the "Stazione Astronomica Betelgeuse" in Magnago, Italy equipped with a 512x512 pixels 
Kodak KAF261E CCD cooled to (typ.) -20°C; 1.6 arcsec per pixel (1x1 binning); 
14'x14' field of view, with a V photometric filter.
Reduction to standard photometric system was performed.
As comparison and check stars were used UCAC4 406-017649 (V=11.47) and UCAC4 406-017634 (V=12.79).
Using also V magnitude data coming from the All Sky Automated Survey (ASAS), 
a total of 916 measures were collected.
The star shows a secondary minimum approximately at phase 0.70.

\IBVSnstar{
06 45 43.95 }
{ -08 50 35.6 }
{ EA }
{ 10.85-11.50 (V) }
{ 3.73235d }
{ 2456263.980 }
{ TYC 5378-1590-1 = UCAC4 406-017746
 }
{finding chart, \IBVSefigure{6100-f43.ps}
\IBVSfigKey{6100-f43.ps}{TYC 5378-1590-1}{finding chart}
light curve, \IBVSefigure{6100-f44.ps}
\IBVSfigKey{6100-f44.ps}{TYC 5378-1590-1}{light curve}
data file \IBVSedata{6100-t22.txt}
\IBVSdataKey{6100-t22.txt}{TYC 5378-1590-1}{photometry}
}{21}

\IBVSnews{25 March 2013}
{
Nelson, R.H. - 1393 Garvin St., Prince George, BC, V2M 3Z1 Canada, bob.nelson@shaw.ca \\ %email
Lubcke, Gil - 6816 South Avenue, Middleton, Wisconsin, 53562.  USA, lubcke@tds.net \\ %email
Molnar, Larry - Calvin College, Grand Rapids, MI, 49546-4403, lmolnar@calvin.edlu \\ %email
}{13}

Remark: Star was discovered to be variable by R.H. Nelson on 2012-10-10 while 
observing GSC 4267-0682.  He obtained a light curve around a primary minimum 
in R (Cousins).  Follow-up data was acquired by G. Lubcke and L. Molnar.  
The latter discovered the period and obtained a largely full light curve 
in R (Cousins) with some additional data in V.

\IBVSnstar{
22 05 43.480 }
{ +61 55 18.835 }
{ EA }
{ B mag = 11.06, V mag = 10.81 (SIMBAD) }
{ 2.6334576 d }
{ 2456297.54746 }
{ GSC 4267-0588 = TYC 4267-588-1 = 2MASS J22054347+6155189
 }
{finding chart, \IBVSefigure{6100-f45.ps}
\IBVSfigKey{6100-f45.ps}{GSC 4267-0588}{finding chart}
light curve, \IBVSefigure{6100-f46.ps}
\IBVSfigKey{6100-f46.ps}{GSC 4267-0588}{light curve}
light curve, \IBVSefigure{6100-f47.ps}
\IBVSfigKey{6100-f47.ps}{GSC 4267-0588}{light curve}
data file, \IBVSedata{6100-t23.txt}
\IBVSdataKey{6100-t23.txt}{GSC 4267-0588}{photometry}
data file \IBVSedata{6100-t24.txt}
\IBVSdataKey{6100-t24.txt}{GSC 4267-0588}{photometry}
}{22}

\IBVSnews{23 August 2013}
{
Srdoc, Gregor - Sarsoni 90 Viskovo, Croatia, gregor@vip.hr \\ %email
Frank, Peter - Bundesdeutsche Arbeitsgemeinschaft f\"ur Ver\"anderliche Sterne e.V. (BAV), Munsterdamm 90, DE-12169 Berlin, Germany, frank.velden@t-online.de \\ %email
H\"ummerich, Stefan - Bundesdeutsche Arbeitsgemeinschaft f\"ur Ver\"anderliche Sterne e.V. (BAV), Munsterdamm 90, DE-12169 Berlin, Germany, ernham@rz-online.de \\ %email
Bernhard, Klaus - Bundesdeutsche Arbeitsgemeinschaft f\"ur Ver\"anderliche Sterne e.V. (BAV), Munsterdamm 90, DE-12169 Berlin, Germany, Klaus.Bernhard@liwest.at \\ %email
}{14}

Remark: GSC 02075-01605 has been discovered as a candidate variable star by 
investigation of light curves from the SuperWASP public archive (Butters 
et al., 2010). Follow-up observations by G. Srdoc ($V$ filter; 19 nights; 
black circles in folded light curve) and P. Frank ($-IR$ filter; 2 nights; 
grey circles) indicate that GSC 02075-01605 is a DSCT variable. $J-K$=0.101 
(2MASS; Skrutskie et al., 2006).  Positional information was drawn from the 
UCAC4 catalogue (Zacharias et al., 2013). The difference in mean magnitude 
between the two datasets results from the use of different filters and 
telescope systems. The given magnitude range has been derived from G. Srdoc's 
observations because of the use of a $V$-filter.

\IBVSnstar{
17 28 31.533 }
{ +22 34 18.93 }
{ RRab }
{ 13.15 - 13.45 (CV) }
{ 0.049113 d }
{ 2456462.4354 }
{ GSC 02075-01605 = UCAC4 563-061083 = 2MASS 17283152+2234189
 }
{finding chart, \IBVSefigure{6100-f48.eps}
\IBVSfigKey{6100-f48.eps}{GSC 02075-01605}{finding chart}
light curve, \IBVSefigure{6100-f49.eps}
\IBVSfigKey{6100-f49.ps}{GSC 02075-01605}{light curve}
data file \IBVSedata{6100-t25.txt}
\IBVSdataKey{6100-t25.txt}{GSC 02075-01605}{photometry}
}{23}

\IBVSnews{9 September 2013}
{
Nelson, Robert H. - Sylvester Robotic Observatory, Prince George, BC, Canada  bob.nelson@shaw.ca \\ %email
Buchheim, Robert - Altimira Observatory (minor planet center observatory code G76) Bob@kbuchheim.org \\ %email
}{15}

Remark: Minima Determination:  Fourier 5-term fit (Nelson), Kwee \& van Woerden (both).

\IBVSnstar{
23 00 07.0183 }
{ +30 39 17.709 }
{ EA }
{ 14.07 (USNO A2.0:  B=15.2,  R=13.8) }
{ 0.47187 (2) d }
{ 2456530.5060(6) }
{ GSC 2750-0054 = USNO A2.0 1200-19628029
 }
{finding chart, \IBVSefigure{6100-f50.eps}
\IBVSfigKey{6100-f50.eps}{GSC 2750-0054}{finding chart}
O-C diagram, \IBVSefigure{6100-f51.eps}
\IBVSfigKey{6100-f51.eps}{GSC 2750-0054}{O-C diagram}
clear light curve (Nelson), \IBVSefigure{6100-f52.eps}
\IBVSfigKey{6100-f52.ps}{GSC 2750-0054}{light curve}
B light curve (Buchheim), \IBVSefigure{6100-f53.eps}
\IBVSfigKey{6100-f53.ps}{GSC 2750-0054}{light curve}
V light curve (Buchheim), \IBVSefigure{6100-f54.eps}
\IBVSfigKey{6100-f54.ps}{GSC 2750-0054}{light curve}
R light curve (Buchheim), \IBVSefigure{6100-f55.eps}
\IBVSfigKey{6100-f55.ps}{GSC 2750-0054}{light curve}
data file (Buchheim), \IBVSedata{6100-t26.txt}
\IBVSdataKey{6100-t26.txt}{GSC 2750-0054}{photometry}
data file (Nelson), \IBVSedata{6100-t27.txt}
\IBVSdataKey{6100-t27.txt}{GSC 2750-0054}{photometry}
}{24}


\IBVSnews{25 September 2013}
{
Nelson, Robert H. - Sylvester Robotic Observatory, Prince George, BC, Canada  bob.nelson@shaw.ca \\ %email
Buchheim, Robert - Altimira Observatory (minor planet center observatory code G76) Bob@kbuchheim.org \\ %email
}{16}

\IBVSnstar{
23 00 00.8628 }
{ +30 39 00.458 }
{ EB? }
{ 13.58 (USNO A2.0: B=14.5, R=13.1) }
{ 0.2991 (1) d }
{ 56529.9697 (36) }
{ GSC 2750-1476 = USNO A2.0 1200-19626931
 }
{
finder chart, \IBVSefigure{6100-f56.eps}
\IBVSfigKey{6100-f56.eps}{GSC 2750-1476}{finding chart}
O-C diagram, \IBVSefigure{6100-f57.eps}
\IBVSfigKey{6100-f57.eps}{GSC 2750-1476}{O-C diagram}
clear light curve (Nelson), \IBVSefigure{6100-f58.eps}
\IBVSfigKey{6100-f58.eps}{GSC 2750-1476}{light curve}
B light curve (Buchheim), \IBVSefigure{6100-f59.eps}
\IBVSfigKey{6100-f59.eps}{GSC 2750-1476}{light curve}
V light curve (Buchheim), \IBVSefigure{6100-f60.eps}
\IBVSfigKey{6100-f60.eps}{GSC 2750-1476}{light curve}
R light curve (Buchheim), \IBVSefigure{6100-f61.eps}
\IBVSfigKey{6100-f61.eps}{GSC 2750-1476}{light curve}
data file (Nelson), \IBVSedata{6100-t28.txt}
\IBVSdataKey{6100-t28.txt}{GSC 2750-1476}{photometry}
data file (Buchheim), \IBVSedata{6100-t29.txt}
\IBVSdataKey{6100-t29.txt}{GSC 2750-1476}{photometry}
}{25}

\IBVSnews{17 January 2014}
{
Martignoni, Massimiliano - Stazione Astronomica Betelgeuse, Magnago, Milano, Italy, massimiliano.martignoni@alice.it \\ %email
}{17}

\IBVSnstar{
22 10 27.06 }
{ +55 09 29.7 }
{ EB }
{13.17 (0.04) $\pm$ 0.02 (V) } { 0.181378 d }
{ 2 456 185.220 }
{ UCAC4 726-082768 }
{finding chart, \IBVSefigure{6100-f62.eps}
\IBVSfigKey{6100-f62.eps}{UCAC4 726-082768}{finding chart}
light curve, \IBVSefigure{6100-f63.eps}
\IBVSfigKey{6100-f63.eps}{UCAC4 726-082768}{light curve}
data file \IBVSedata{6100-t30.txt}
\IBVSdataKey{6100-t30.txt}{UCAC4 726-082768}{photometry}
}{26}

Remark: UCAC4 726-082768 is an EB type eclipsing binary type variable star in the field of view of KM Cep. 
It was observed with a 0.25\,m Schmidt-Cassegrain telescope (f/10) of the Stazione Astronomica Betelgeuse in Magnago, Italy equipped with a 512$\times$512 pixels 
Kodak KAF261E CCD cooled to (typ.) $-$20$\deg$C; 1.6 arcsec per pixel (1$\times$1 binning); $14\arcm$$\times$$14\arcm$
field of view, with {\it V} photometric filter.
As comparison and check stars were used UCAC4 726-082801 and UCAC4 726-082806.
A total of 380 measures in {\it V} band were collected; reduction to the standard photometric system was not performed.


\IBVSnews{29 January 2014}
{
Martignoni, Massimiliano - Stazione Astronomica Betelgeuse, Magnago, Milano, Italy, massimiliano.martignoni@alice.it \\ %email
}{18}

\IBVSnstar{
22 10 29.04 }
{ +55 09 01.2 }
{ L: }
{14.5: (0.5:) (V) } {  }
{  }
{ UCAC4 726-082786 }
{finding chart, \IBVSefigure{6100-f64.eps}
\IBVSfigKey{6100-f64.eps}{UCAC4 726-082768}{finding chart}
light curve, \IBVSefigure{6100-f65.eps}
\IBVSfigKey{6100-f65.eps}{UCAC4 726-082768}{light curve}
data file \IBVSedata{6100-t31.txt}
\IBVSdataKey{6100-t31.txt}{UCAC4 726-082768}{photometry}
}{27}


Remark: UCAC4 726-082786 is an L: type variable star in the field of view of KM Cep. 
It was observed with a 0.25\,m Schmidt-Cassegrain telescope (f/10) of the Stazione Astronomica Betelgeuse in Magnago, Italy equipped with a 512$\times$512 pixels Kodak KAF261E CCD cooled to (typ.) $-$20$\deg$C; 1.6 arcsec per pixel (1$\times$1 binning); $14\arcm$$\times$$14\arcm$, with {\it V} photometric filter. 
As comparison and check stars were used UCAC4 726-082801 and UCAC4 726-082806.
A total of 396 measures in {\it V} band were collected; reduction to the standard photometric system was not performed.


\IBVSnews{27 February 2014}
{
Liakos, A. - National Observatory of Athens, Institute for Astronomy \& Astrophysics, Space Applications \& Remote Sensing, I.\ Metaxa \& Vas.\ Pavlou St., \linebreak GR-152 36, Palaia Penteli, Athens, Greece, alliakos@noa.gr \\ %email
Niarchos, P. - Department of Astrophysics, Astronomy and Mechanics, National and Kapodistrian University of Athens, Panepistimioupolis, GR-157 84, Zografos, Athens, Greece, pniarcho@phys.uoa.gr \\ %email
}{19}

\IBVSnstar{
18 42 29 }
{ +08 58 35 }
{ CV or SR }
{ 11.2 (V) } {  }
{ Multiperiodic }
{ GSC 1025-0798 = TYC 1025-798-1 = 2MASS J18422913+0858346 }
{finding chart, \IBVSefigure{6100-f66.eps}
\IBVSfigKey{6100-f66.eps}{GSC 1025-0798}{finding chart}
light curve, \IBVSefigure{6100-f67.eps}
\IBVSfigKey{6100-f67.eps}{GSC 1025-0798}{light curve}
light curve, \IBVSefigure{6100-f68.eps}
\IBVSfigKey{6100-f68.eps}{GSC 1025-0798}{light curve}
light curve, \IBVSefigure{6100-f69.eps}
\IBVSfigKey{6100-f69.eps}{GSC 1025-0798}{light curve}
data file \IBVSedata{6100-t32.txt}
\IBVSdataKey{6100-t32.txt}{GSC 1025-0798}{photometry}
}{28}


Remark: Detected in the FoV of V456 Oph.



\IBVSnstar{
07 38 20.2 }
{ $-$02 48 04.8 }
{ EW }
{ 13.6 (V) } { 0.4245(1) }
{ 2455939.383(9) }
{ GSC 4835-1716 = USNO A2.0 0825-05281746 = 2MASS 07382020-0248044 = \linebreak NOMAD1 0871-0207620   }
{finding chart, \IBVSefigure{6100-f70.eps}
\IBVSfigKey{6100-f70.eps}{GSC 4835-1716}{finding chart}
light curve, \IBVSefigure{6100-f71.eps}
\IBVSfigKey{6100-f71.eps}{GSC 4835-1716}{light curve}
data file \IBVSedata{6100-t33.txt}
\IBVSdataKey{6100-t33.txt}{GSC 4835-1716}{photometry}
}{29}


Remark: Detected in the FoV of V868 Mon.

\IBVSnews{5 March 2014}
{
Liakos, A. - National Observatory of Athens, Institute for Astronomy \& Astrophysics, Space Applications \& Remote Sensing, I.\ Metaxa \& Vas.\ Pavlou St., \linebreak GR-152 36, Palaia Penteli, Athens, Greece, alliakos@noa.gr \\ %email
Niarchos, P. - Department of Astrophysics, Astronomy and Mechanics, National and Kapodistrian University of Athens, Panepistimioupolis, GR-157 84, Zografos, Athens, Greece, pniarcho@phys.uoa.gr \\ %email
}{20}

\IBVSnstar{
01 57 54.9 }
{ +37 47 53.4 }
{ EC }
{ 14.0 (B) } { }
{ }
{ GSC 2816-2000 = USNO 1275-01172833 = 2MASS 01575487+3747534 = NOMAD1 1277-0038470 }
{finding chart, \IBVSefigure{6100-f72.eps}
\IBVSfigKey{6100-f72.eps}{GSC 2816-2000}{finding chart}
light curve, \IBVSefigure{6100-f73.eps}
\IBVSfigKey{6100-f73.eps}{GSC 2816-2000}{light curve}
data file \IBVSedata{6100-t34.txt}
\IBVSdataKey{6100-t34.txt}{GSC 2816-2000}{photometry}
}{30}


Remark: Detected in the FoV of QX And and GSC 2816-0743 (= NGC 752 170; discovered by Zhang et al. (2009)). The C-K light curve is given for direct comparison with the V-C one. 


\IBVSnstar{
18 28 39.6 }
{ +06 46 00.9 }
{ EC }
{ 12.3 ($V_T$) } { }
{ }
{ GSC 0445-0903 = TYC 445-903-1 = 2MASS 18283962+0645598}
{finding chart, \IBVSefigure{6100-f74.eps}
\IBVSfigKey{6100-f74.eps}{GSC 0445-0903}{finding chart}
light curve, \IBVSefigure{6100-f75.eps}
\IBVSfigKey{6100-f75.eps}{GSC 0445-0903}{light curve}
data file \IBVSedata{6100-t35.txt}
\IBVSdataKey{6100-t35.txt}{GSC 0445-0903}{photometry}
}{31}


Remark:  Detected in the FoV of V2612 Oph. The minimum in I-filter is deeper than the one in V-filter. Therefore, it corresponds to the secondary minimum of the binary's light curve. This suggests Algol-type variability. The C-K light curves are given for direct comparison with the V-C ones. 


\IBVSnstar{
20 19 35.2 }
{ +33 47 26.5 }
{ EC }
{ 12.2 (B) } { }
{ }
{ GSC 2680-1387 = USNO 1200-14916877 = 2MASS 20193521+3347262 = NOMAD1 1237-0465366 }
{finding chart, \IBVSefigure{6100-f76.eps}
\IBVSfigKey{6100-f76.eps}{GSC 2680-1387}{finding chart}
light curve, \IBVSefigure{6100-f77.eps}
\IBVSfigKey{6100-f77.eps}{GSC 2680-1387}{light curve}
light curve, \IBVSefigure{6100-f78.eps}
\IBVSfigKey{6100-f78.eps}{GSC 2680-1387}{light curve}
data file \IBVSedata{6100-t36.txt}
\IBVSdataKey{6100-t36.txt}{GSC 2680-1387}{photometry}
}{32}


Remark: Detected in the FoV of MY Cyg. The C-K light curve is given for direct comparison with the V-C one.  



\IBVSnstar{
 08 10 54.2 }
{ +57 40 01.3 }
{ EC }
{ 11.6 (V) } { }
{ }
{ GSC 3802-1680 = TYC 3802-1680-1 = USNO-A2.0 1425-07102186 = NOMAD1 1476-0238610 }
{finding chart, \IBVSefigure{6100-f79.eps}
\IBVSfigKey{6100-f79.eps}{GSC 3802-1680}{finding chart}
light curve, \IBVSefigure{6100-f80.eps}
\IBVSfigKey{6100-f80.eps}{GSC 3802-1680}{light curve}
light curve, \IBVSefigure{6100-f81.eps}
\IBVSfigKey{6100-f81.eps}{GSC 3802-1680}{light curve}
data file \IBVSedata{6100-t37.txt}
\IBVSdataKey{6100-t37.txt}{GSC 3802-1680}{photometry}
}{33}


Remark: Detected in the FoV of SX Lyn and GSC 3802-1986 (discovered by Liakos \& Niarchos (2011)).


\IBVSnstar{
 02 34 46.6 }
{ +71 31 21.4 }
{ EA }
{  9.7 (B) } { }
{ }
{ GSC 4320-1033 = TYC 4320-1033-1 = USNO-A2.0 1575-01428060 = 2MASS 02344652+7131209 }
{finding chart, \IBVSefigure{6100-f82.eps}
\IBVSfigKey{6100-f82.eps}{GSC 4320-1033}{finding chart}
light curve, \IBVSefigure{6100-f83.eps}
\IBVSfigKey{6100-f83.eps}{GSC 4320-1033}{light curve}
light curve, \IBVSefigure{6100-f84.eps}
\IBVSfigKey{6100-f84.eps}{GSC 4320-1033}{light curve}
data file \IBVSedata{6100-t38.txt}
\IBVSdataKey{6100-t38.txt}{GSC 4320-1033}{photometry}
}{34}

Remark: Detected in the FoV of AB Cas and V663 Cas.


\IBVSnstar{
 07 09 34.9 }
{ +12 10 37.2 }
{ EA }
{  13.8 (I) } { }
{ 2455537.4735(5) }
{ USNO-A2.0~0975-04711370 = NOMAD1 1021-0151694 = 2MASS  07093486 \linebreak+1210369 = UCAC4 511-036297 }
{finding chart, \IBVSefigure{6100-f85.eps}
\IBVSfigKey{6100-f85.eps}{USNO-A2.0 0975-04711370}{finding chart}
light curve, \IBVSefigure{6100-f86.eps}
\IBVSfigKey{6100-f86.eps}{USNO-A2.0 0975-04711370}{light curve}
light curve, \IBVSefigure{6100-f87.eps}
\IBVSfigKey{6100-f87.eps}{USNO-A2.0 0975-04711370}{light curve}
data file \IBVSedata{6100-t39.txt}
\IBVSdataKey{6100-t39.txt}{USNO-A2.0 0975-04711370}{photometry}
}{35}

Remark:  Detected in the FoV of AV CMi, 2MASS J07083972+1214429 (discovered by Liakos \& Niarchos 2010), GSC 0770-0523 (discovered by Liakos \& Niarchos 2010), and USNO-A2.0 0975-04721840 (discovered by Liakos \& Niarchos 2011).



\IBVSnstar{
 20 20 56.8 }
{ +18 26 12.4 }
{ EA }
{ 14.1 (B) } { 8.935 }
{ 2455856.289 }
{ USNO A2.0 1050-17346460 = 2MASS 20205676+1826120 = NOMAD1 1084-0573113   }
{finding chart, \IBVSefigure{6100-f88.eps}
\IBVSfigKey{6100-f88.eps}{USNO A2.0 1050-17346460}{finding chart}
light curve, \IBVSefigure{6100-f89.eps}
\IBVSfigKey{6100-f89.eps}{USNO A2.0 1050-17346460}{light curve}
light curve, \IBVSefigure{6100-f90.eps}
\IBVSfigKey{6100-f90.eps}{USNO A2.0 1050-17346460}{light curve}
data file \IBVSedata{6100-t40.txt}
\IBVSdataKey{6100-t40.txt}{USNO A2.0 1050-17346460}{photometry}
}{36}

Remark:  Detected in the FoV of BX Del and BW Del. The reference time of minimum as given in the ephemeris (2455856.289) was assumed and it is not a true minimum time. The period is also uncertain, but the value given describes the data in the most sufficient way. The system may have eccentric orbit. 


\IBVSnstar{
 04 16 10.6 }
{ +47 38 14.9 }
{ EC }
{  15.1 (R) } { }
{  }
{ USNO A2.0 1350-04394387 = 2MASS 04161058+4738146 = NOMAD1 1376-0126986  }
{finding chart, \IBVSefigure{6100-f91.eps}
\IBVSfigKey{6100-f91.eps}{USNO A2.0 1350-04394387}{finding chart}
light curve, \IBVSefigure{6100-f92.eps}
\IBVSfigKey{6100-f92.eps}{USNO A2.0 1350-04394387}{light curve}
light curve, \IBVSefigure{6100-f93.eps}
\IBVSfigKey{6100-f93.eps}{USNO A2.0 1350-04394387}{light curve}
data file \IBVSedata{6100-t41.txt}
\IBVSdataKey{6100-t41.txt}{USNO A2.0 1350-04394387}{photometry}
}{37}

Remark:  Detected in the FoV of V482 Per. The period is probably between 4.66 and 13.99 days, but more times of minima are needed for its determination.





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\end{document}
