## 6 Results  
In our first set of simulations for \(R=7000\) km, we obtain the different parallax light curves for each varying \(\Phi\) as shown in Figure 7, with the figure legend shown in Figure 8. The photometric curve without parallax, labeled as Original, is also shown for comparison. We perform 100 Monte Carlo simulations for each time sample. For each R value, we show % error in peak magnification value between each parallax photometric curve as well as the difference in time shift for the peak magnification. The average CS reconstruction error for R = 7000 km is shown in Table 4. Tables 5 and 6 show the error at peak magnification and the time difference in hours at peak magnification for R = 7000 km, respectively. Microlensing parallax provides a \(\Delta u_{0}\), which shows the change in magnification amplitude, as well as a \(\Delta t_{0}\), which shows a change in \(t_{0}\) location. The higher the \(R\) value, the greater the \(\Delta\). \begin{table}
\begin{tabular}{c c c c} \hline R & \(t_{E}\) & **Cadence** & **Observation Time** \\ \hline
7000 km & 1 day & 48 min & 1 day \\
42,000 km & 1 day & 48 min & 1 day \\
1 AU & 1 day & 5.02 days & 150.5 days \\ \hline \end{tabular}
\end{table} 
Table 3: Simulation setup parameters. \begin{table}
\begin{tabular}{c c c c c c c c c} \hline \hline \(\Phi\) & **0** & \(\pi\) & \(\pi\) & \(3\pi\) & \(\pi\) & \(5\pi\) & \(3\pi\) & \(7\pi\) \\  & & \(\overline{8}\) & \(\overline{4}\) & \(\overline{8}\) & \(\overline{2}\) & \(\overline{8}\) & \(\overline{4}\) & \(\overline{8}\) \\ \hline Avg \% Err & 0.175 & 0.230 & 0.088 & 0.109 & 0.163 & 0.161 & 0.240 & 0.098 \\ \hline Avg \% Err at peak & 0.075 & 0.06 & **1.07** & 0.068 & **1.09** & 0.076 & 0.081 & 0.073 \\ \hline Std dev. \% Err at peak & 0.057 & 0.064 & **9.94** & 0.056 & **9.94** & 0.086 & 0.070 & 0.068 \\ \hline \hline \end{tabular}
\end{table} 
Table 4: Percent Error for CS reconstruction for each \(\Phi\) for R = 7000 km. The second row shows average % error over all time samples, the third row shows average % error at peak magnification, and the last row shows the standard deviation of the % error at peak magnification. Figure 8: Legend for Figure 7.  
Figure 7: Photometric curves generated by different parallax values, shown with its corresponding CS reconstructed curve for R = 7000 km. Figure 10: Legend for Figure 9. \begin{table}
\begin{tabular}{c c c c c c c c c} \hline \hline \(\mathbf{\Phi}\) & \(\mathbf{0}\) & \(\dfrac{\pi}{\mathbf{8}}\) & \(\dfrac{\pi}{\mathbf{4}}\) & \(\dfrac{3\pi}{\mathbf{8}}\) & \(\dfrac{\pi}{\mathbf{2}}\) & \(\dfrac{5\pi}{\mathbf{8}}\) & \(\dfrac{3\pi}{\mathbf{4}}\) & \(\dfrac{7\pi}{8}\) \\ \hline Avg \% Err & 0.108 & 0.110 & 0.182 & 0.110 & 0.191 & 0.208 & 0.173 & 0.201 \\ \hline Avg \% Err at peak & **1.07** & 0.059 & 0.091 & **1.07** & 0.086 & 0.063 & 0.062 & 0.071 \\ \hline Std dev. \% Err at peak & **9.94** & 0.041 & 0.205 & **9.94** & 0.094 & 0.049 & 0.062 & 0.057 \\ \hline \hline \end{tabular}
\end{table} 
Table 7: Percent Error for CS reconstruction for each \(\Phi\) for R = 42,000 km. The second row shows average % error over all time samples, the third row shows average % error at \(t_{0}\), and the last row shows the standard deviation of the % error at \(t_{0}\). Figure 9: Photometric curves generated by different parallax values, shown with its corresponding CS reconstructed curve for R = 42,000 km. The original photometric curve without any microlensing effects is shown in red for comparison. Figure 11 shows the microlensing parallax curves for R = 1 AU. In this figure, we do not show the microlensing curve without parallax (Original curve in Figures 7 and 9) for comparison, as the \(\Delta\) in \(u_{0}\) and \(t_{0}\) are significantly high and will not be clearly readable with the given sampling cadence and observation window. Figure 12 is the corresponding legend. In Table 10, we show the % error due to CS reconstruction in the photometric curves. Tables 11 and 12 show % error at peak magnification and time difference in days at peak magnification, respectively.