  Debris disks are intimately linked to planetary system evolution since the
rocky material surrounding the host stars is due to secondary generation from
the collisions of planetesimals. With the conclusion and lack of future large
scale infrared excess survey missions, it is time to summarize the history of
using excess emission in the infrared as a tracer of debris. We have compiled a
catalog of infrared excess stars from peer reviewed articles and performed an
extensive search for new debris disks by cross correlating the Tycho 2 and
AllWISE catalogs. This study will examine each debris disk stars parameters
obtained through high resolution spectroscopy at various facilities. We will
maintain a webpage devoted to these infrared excess sources and provide various
resources related to our catalog creation, SED fitting, and data reduction.
