  The Transiting Exoplanet Survey Satellite (TESS) is a NASA Astrophysics
Explorer mission. Following its scheduled launch in 2017, TESS will focus on
detecting exoplanets around the nearest and brightest stars in the sky, for
which detailed follow-up observations are possible. TESS will, as the NASA
Kepler mission, include a asteroseismic program that will be organized within
the TESS Asteroseismic Science Consortium (TASC), building on the success of
the Kepler Asteroseismic Science Consortium (KASC). Within TASC data for
asteroseismic analysis will be prepared by the TASC Working Group 0 (WG-0), who
will facilitate data to the community via the TESS Asteroseismic Science
Operations Center (TASOC), again building on the success of the corresponding
KASOC platform for Kepler. Here, we give an overview of the steps being taken
within WG-0 to prepare for the upcoming TESS mission.
