  We present sources selected from their Wide-field Infrared Survey Explorer
(WISE) colors that merit future observations to image for disks and possible
exoplanet companions. Introducing a weighted detection method, we eliminated
the enormous number of specious excess seen in low signal to noise objects by
requiring greater excess for fainter stars. This is achieved by sorting through
the 747 million sources of the ALLWISE database. In examining these dim stars,
it can be shown that a non-Gaussian distribution best describes the spread
around the main-sequence polynomial fit function. Using a gamma Probability
Density Function (PDF), we can best mimic the main sequence distribution and
exclude natural fluctuations in IR excess. With this new methodology we
re-discover 25 IR excesses and present 14 new candidates. One source
(J053010.20-010140.9), suggests a 8.40 $\pm$ 0.73 AU disk, a likely candidate
for possible direct imagining of planets that are likely fully formed. Although
all of these sources are well within the current flux ratio limit of
$\sim$10$^{-6}$ (Wyatt 2008), J223423.85+403515.8 shows the highest bolometric
flux ratio ($f_d$=0.0694) between disk and host star, providing a very good
candidate for direct imaging of the circumstellar disk itself. In re-examining
the Kepler candidate catalog (original study preformed by Kennedy and Wyatt
2012), we found one new candidate that indicates disk like characteristics (TYC
3143-322-1).
