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 ) .