the target list using the same methods outlined in @2005ApJ...624.1010B. We started by simulating $10^5$ exoEarths around a Sun-like star at 1 pc using the planet parameters listed in Table \[exoearth\_params\_table\]. For each synthetic exoEarth, we calculated the projected angular separation of the planet and star, $s_{\rm p}$, and the flux ratio of the planet to the star, expressed as $$\Delta {\rm mag}_{\rm p} = -2.5 \log{\frac{f_{\rm p}}{f_{\star}}},$$ where $f_{\rm p}$ is the flux from the planet and $f_{\star}$ is the flux from the star.

[ccl]{} $\eta_{\earth}$ & $0.1$ & Fraction of stars with an exoEarth candidate\
$R_{\rm p}$ & $1$ $R_{\earth}$ & Planet radius\
$a$ & $[0.7,1.5]$ AU & Semi-major axis (uniform distribution)\
$e$ & $[0,0.35]$ & Eccentricity (uniform distribution)\
$\cos{i}$ & $[-1,1]$ & Cosine of inclination (uniform distribution)\
$\omega$ & $[0,2\pi)$ & Argument of pericenter (uniform distribution)\
$M$ & $[0,2\pi)$ & Mean anomaly (uniform distribution)\
$\Phi$ & Lambert & Phase function\
$A_G$ & $0.2$ & Geometric albedo (corresponds to spherical albedo $A_B = 0.3$)\
$z$ & 23 mag arcsec$^{-2}$ & Surface brightness of zodiacal light\
$x$ & 22 mag arcsec$^{-2}$ & Surface brightness of 1 zodi of exozodiacal dust\
$n$ & $3$ & Number of zodis for all 