The spectrography is accomplished with filters effectively
covering enough channels to produce the spectral resolution: they
are linearly variable filters, which vary in the band
they allow across one direction. The sky is to be continuously
scanned so that at any instant, portions of the captured image are
capturing different wavelengths. The spacecraft design minimizes
moving parts.
It is aimed at a number of scientific goals for which such a survey
is useful, including more data regarding the history of large scale structures and
galaxy formation as well as measurement of the water in
molecular clouds that could contribute to habitableextra-solar planets. It is expected that it will uncover some
gravitational lensing, and that cross correlation with data
from other surveys will confirm Sunyaev-Zel'dovich effects and gravitational
lensing effects,
and correlation-efforts will produce new information about large
scale structure.