## 6 Results
\begin{table}
\begin{tabular}{c c c c c c c c} \hline  & **0** & \(\dfrac{\pi}{8}\) & \(\dfrac{\pi}{4}\) & \(\dfrac{3\pi}{8}\) & \(\dfrac{\pi}{2}\) & \(\dfrac{5\pi}{8}\) & \(\dfrac{3\pi}{4}\) & \(\dfrac{7\pi}{8}\) \\ \hline
0 & - & 22.1 & 7.50 & 109 & 215 & 25.1 & 59.7 & 70.9 \\ \hline \(\dfrac{\pi}{8}\) & 28.3 & - & 18.7 & 168 & 305 & 3.85 & 48.3 & 62.6 \\ \hline \(\dfrac{\pi}{4}\) & 8.11 & 15.8 & - & 126 & 241 & 19.0 & 56.5 & 68.5 \\ \hline \(\dfrac{3\pi}{8}\) & 52.1 & 62.7 & 55.7 & - & 51.0 & 64.1 & 80.7 & 86.1 \\ \hline \(\dfrac{\pi}{2}\) & 68.3 & 75.3 & 70.7 & 33.8 & - & 76.2 & 87.2 & 90.8 \\ \hline \(\dfrac{5\pi}{8}\) & 33.5 & 4.00 & 23.5 & 179 & 321 & - & 46.2 & 61.1 \\ \hline \(\dfrac{3\pi}{4}\) & 148 & 93.4 & 130 & 418 & 682 & 86.0 & - & 27.7 \\ \hline \(\dfrac{7\pi}{8}\) & 243 & 168 & 218 & 617 & 982 & 157 & 38.3 & - \\ \hline \end{tabular}
\end{table} 
Table 8: Percent error at peak magnification between a microlensing photometric curve with \(\Phi\) shown in the first row, compared to the photometric curve with \(\Phi\) in the first column. Error values for R = 42,000 km. Values in bold underline show where % error between the two curves is less than 10%. \begin{table}
\begin{tabular}{c c c c c c c c} \hline  & **0** & \(\dfrac{\pi}{8}\) & \(\dfrac{\pi}{4}\) & \(\dfrac{3\pi}{8}\) & \(\dfrac{\pi}{2}\) & \(\dfrac{5\pi}{8}\) & \(\dfrac{3\pi}{4}\) & \(\dfrac{7\pi}{8}\) \\ \hline
0 & - & 1.66 & 4.14 & 6.62 & 9.10 & 10.8 & 10.8 & 10.8 \\ \hline \(\dfrac{\pi}{8}\) & 1.66 & - & 2.48 & 4.97 & 7.45 & 9.10 & 9.10 & 9.10 \\ \hline \(\dfrac{\pi}{4}\) & 4.14 & 2.48 & - & 2.48 & 4.97 & 6.62 & 6.62 & 6.62 \\ \hline \(\dfrac{3\pi}{8}\) & 6.62 & 4.97 & 2.48  
Our results show that there is no significant error for a microlensing parallax event using CS techniques. For all the photometric curves, the average error is less than 0.5% for all CS reconstructed curves and less than 1.1% at peak magnification time. From our simulations, we note that the parallax curves get more distinguished for higher \(R\) values, that is, the time separation and amplitude separation between the photometric curves is higher. From our simulations, we show that the error due to CS reconstruction is less than the error between any two microlens parallax curves. However, we can use Tables 5, 8 and 11 as a basis to determine the optimal orbital phases to choose for satellite placement. Although CS reconstruction results show average error within the % error for the two curves, a better placement, if using less than eight satellites, would be to choose orbital phases which have a greater microlensing detectability. \begin{table}
\begin{tabular}{c c c c c c c c c} \hline  & **0** & \(\dfrac{\boldsymbol{\pi}}{\boldsymbol{8}}\) & \(\dfrac{\boldsymbol{\pi}}{\boldsymbol{4}}\) & \(\dfrac{\boldsymbol{3\pi}}{\boldsymbol{8}}\) & \(\dfrac{\boldsymbol{\pi}}{\boldsymbol{2}}\) & \(\dfrac{\boldsymbol{5\pi}}{\boldsymbol{8}}\) & \(\dfrac{\boldsymbol{3\pi}}{\boldsymbol{4}}\) & \(\dfrac{\boldsymbol{7\pi}}{\boldsymbol{8}}\) \\ \hline
0 & - & 12.7 & 27.2 & 43.7 & 18.7 & 276 & 217 & 167 \\ \hline \(\dfrac{\pi}{\boldsymbol{8}}\) & 11.3 & - & 12.8 & 27.5 & \(\underline{\boldsymbol{5.34}}\) & 234 & 181 & 137 \\ \hline \(\dfrac{\pi}{\boldsymbol{4}}\) & 21.4 & 11.4 & - & 13.0 & \(\underline{\boldsymbol{6.65}}\) & 196 & 149 & 110 \\ \hline \(\dfrac{3\pi}{\boldsymbol{8}}\) & 30.4 & 21.5 & 11.5 & - & 17.4 & 162 & 121 & 85.6 \\ \hline \(\dfrac{\pi}{\boldsymbol{2}}\) & 15.8 & \(\underline{\boldsymbol{5.07}}\) & \(\underline{\boldsymbol{7.12}}\) & 21.0 & - & 217 & 167 & 125 \\ \hline \(\dfrac{5\pi}{\boldsymbol{8}}\) & 73.4 & 70.0 & 66.2 & 61.8 & 68.4 & - & 15.7 & 29.1 \\ \hline \(\dfrac{3\pi}{\boldsymbol{4}}\) & 68.5 & 64.4 & 59.9 & 54.7 & 62.5 & 18.6 & - & 15.9 \\ \hline \(\dfrac{7\pi}{\boldsymbol{8}}\) & 62.5 & 57.7 & 52.3 & 46.1 & 55.5 & 41.0 & 18.9 & - \\ \hline \end{tabular}
\end{table} 
Table 11: Percent error at peak between a microlensing photometric curve with \(\Phi\) shown in the first row, compared to the photometric curve with \(\Phi\) in the first column.