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![\begin{figure}
\par\includegraphics[width=0.49\textwidth,clip]{aa14015f3a.eps}\i...
...3c.eps}\includegraphics[width=0.49\textwidth,clip]{aa14015f3d.eps}
\end{figure}](/articles/aa/olm/2010/03/aa14015-10/img44.png)
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Figure 4:
Different captions of the ASAS light curve of V1247 Ori.
Data points that deviate less and more than 3 |
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from the
iteratively-``cleaned'' light curve are plotted with small (blue) dots and open
(red) circles, respectively. Top left panel: full time and magnitude ranges. The horizontal dashed line marks the value V = 10.25 mag.
Top right panel: full time range. Only magnitudes brighter than V
= 10.25 mag are shown. The vertical dashed lines indicate the
enlargement areas in the bottom panels, corresponding to the two main
occultation events. Bottom panels: full magnitude ranges, 200 d-wide time intervals around
the 2002 Dec. ( left) and 2004 Feb. ( right) occultation events.
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