  The KPNO International Spectroscopic Survey (KISS) is an objective-prism
survey designed to detect extragalactic emission-line objects. It combines many
of the features of previous slitless spectroscopic surveys with the advantages
of modern CCD detectors, and is the first purely digital objective-prism survey
for emission-line galaxies (ELGs). Here we present the third list of ELG
candidates selected from our red spectral data, which cover the wavelength
range 6400 to 7200 A. In most cases, the detected emission line is H-alpha. The
current survey list covers the region of the NOAO Deep Wide-Field Survey
(NDWFS). This survey covers two fields; the first is 3 x 3 degrees square and
located at RA = 14h 30m, DEC = 34.5 deg (B1950), the second is 2.3 x 4.0
degrees and centered at RA = 2h 7.5m, DEC = -4.75 deg. A total area of 19.65
deg^2 is covered by the KISS data. A total of 261 candidate emission-line
objects have been selected for inclusion in the survey list (13.3 per deg^2).
We tabulate accurate coordinates and photometry for each source, as well as
estimates of the redshift, emission-line flux and line equivalent width based
on measurements of the digital objective-prism spectra. The properties of the
KISS ELGs are examined using the available observational data. When combined
with the wealth of multi-wavelength data already available for the NDWFS
fields, the current list of KISS ELGs should provide a valuable tool for
studying star-formation and nuclear activity in galaxies in the local universe.
