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.

Cone search capability for table J/AJ/166/101/table2 (*SFF01 Emission-Line Objects)

Cone search capability for table J/AJ/166/101/table3 (*SFF10 Emission-Line Objects)

Cone search capability for table J/AJ/166/101/table4 (*SFF15 Emission-Line Objects)