  The FCRAO Survey of the Taurus Molecular Cloud observed the 12CO and 13CO
J=1-0 emission from 98 square degrees of this important, nearby star forming
region. This set of data with 45" resolution comprises the highest spatial
dynamic range image of an individual molecular cloud constructed to date, and
provides valuable insights to the molecular gas distribution, kinematics, and
the star formation process. In this contribution, we describe the observations,
calibration, data processing, and characteristics of the noise and line
emission of the survey. The angular distribution of 12CO and 13CO emission over
1 km/s velocity intervals and the full velocity extent of the cloud are
presented. These reveal a complex, dynamic medium of cold, molecular gas.
