Star Formation Across Cosmic Time (SFACT) is a new narrowband (NB) survey designed to detect faint emission-line galaxies (ELGs) and QSOs over a broad range of redshifts. Here we present the first list of SFACT candidates from our pilot-study fields. Using the WIYN 3.5m telescope, we are able to achieve good image quality with excellent depth and routinely detect ELGs to r=25.0. The limiting line flux of the survey is ~1.0x10^-16^erg/s/cm^2^. SFACT targets three primary emission lines: H{alpha}, [OIII] {lambda}5007, and [OII] {lambda}3727. The corresponding redshift windows allow for the detection of objects at z~0-1. With a coverage of 1.50deg^2^ in our three pilot-study fields, a total of 533 SFACT candidates have been detected (355 candidates deg-2). We detail the process by which these candidates are selected in an efficient and primarily automated manner, then tabulate accurate coordinates, broadband photometry, and NB fluxes for each source.