Astronomy & Astrophysics

All Figures

$\begin{figure} \par\includegraphics[width=7cm,clip]{8221fig1.eps}\end{figure}$ Figure 1: APO g' image of the quasar system Q2237+0305.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=7cm,clip]{8221fig2.eps} \end{figure}$ Figure 2: Top panel: black squares show the APO g'-band light curve (relative to the faintest data point) of the high magnification event seen in image C of Q2237+0305 in 1999. For comparison, in light gray, the OGLE V-band light curve sampling this event is shown. Middle panel: APO r'-band light curve for the event (black squares) and the OGLE V-band light curve plotted in light gray. Bottom panel: APO g'-r' color curve. The dashed line is shown to guide the eye.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=7.5cm,clip]{8221fig3.eps} \end{figure}$ Figure 3: Example track for a 0.05 E_R (10 pixel) FWHM g'-band source size and a source size ratio $\sigma _{r'}/\sigma _{g'}=1.48$ . In the top panels the fitted track is shown in a $1.0 E_R \times 1.0 E_R$ section of the microlensing patterns. In the middle panel we plot the fitted difference light curve (solid line) and the observed OGLE difference light curve. In the lower panel the best-fitting color curve (solid line) and the APO g'-r' color curve are shown.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=15.5cm,clip]{NEW-8221fig4.eps} \end{figure}$ Figure 4: Probability histograms for g' or V source size, r'/g' source size ratio and transverse velocity (projected to the lens plane), respectively. The dotted line shows the best-fitting values (or average of the 68 percent confidence region if no single best-fitting value is found). The error bars describe the 68 percent confidence limits.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=7cm,clip]{8221fig1.eps}\end{figure}$	Figure 1: APO g' image of the quasar system Q2237+0305.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=15.5cm,clip]{NEW-8221fig4.eps} \end{figure}$	Figure 4: Probability histograms for g' or V source size, r'/g' source size ratio and transverse velocity (projected to the lens plane), respectively. The dotted line shows the best-fitting values (or average of the 68 percent confidence region if no single best-fitting value is found). The error bars describe the 68 percent confidence limits.
Open with DEXTER