  The Star Formation Across Cosmic Time (SFACT) survey is a new narrowband
survey designed to detect emission-line galaxies (ELGs) and quasi-stellar
objects (QSOs) over a wide range of redshifts in discrete redshift windows. The
survey utilizes the WIYN 3.5m telescope and the Hydra multifiber positioner to
perform efficient follow-up spectroscopy on galaxies identified in the imaging
part of the survey. Since the objects in the SFACT survey are selected by their
strong emission lines, it is possible to obtain useful spectra for even the
faintest of our sources (r ~ 25). Here we present the 453 objects that have
spectroscopic data from the three SFACT pilot-study fields, 415 of which are
confirmed ELGs. The methodology for processing and measuring these data is
outlined in this paper and example spectra are displayed for each of the three
primary emission lines used to detect objects in the survey (H-alpha, [O
III]5007, and [O II]3727). Spectra of additional QSOs and non-primary
emission-line detections are also shown as examples. The redshift distribution
of the pilot-study sample is examined and the ELGs are placed in different
emission-line diagnostic diagrams in order to distinguish the star-forming
galaxies from the active galactic nuclei.
