  We have compiled photometry at 3.4, 4.6, 12 and 22 $\mu$m from the all-sky
survey performed by the Wide-field Infrared Survey Explorer (WISE) for all
known members of the Taurus complex of dark clouds. Using these data and
photometry from the Spitzer Space Telescope, we have identified members with
infrared excess emission from circumstellar disks and have estimated the
evolutionary stages of the detected disks, which include 31 new full disks and
16 new candidate transitional, evolved, evolved transitional, and debris disks.
We have also used the WISE All-Sky Source Catalog to search for new
disk-bearing members of Taurus based on their red infrared colors. Through
optical and near-infrared spectroscopy, we have confirmed 26 new members with
spectral types of M1 - M7. The census of disk-bearing stars in Taurus should
now be largely complete for spectral types earlier than $\sim$M8 ($M \gtrsim
0.03$ $M_\odot$).
