The KPNO International Spectroscopic Survey (KISS) is an objective-prism survey for extragalactic emission-line objects. It combines many of the features of previous slitless spectroscopic surveys with the advantages of modern CCD detectors, and it is the first purely digital objective-prism survey for emission-line galaxies. Here we present the first list of emission-line galaxy candidates selected from our blue spectral data, which cover the wavelength range 4800 5500 A. In most cases, the detected emission line is O III lambda5007. The current survey list covers a 1degrees-wide strip located delta = 29degrees30/ (B1950.0) and spanning the right ascension range 8(h)30(m) to 17(h)0(m). An area of 116.6 deg(2) is covered. A total of 223 candidate emission-line objects have been selected for inclusion in the survey list (1.91 deg(-2)). We tabulate accurate coordinates and photometry for each source, as well as estimates of the redshift, emission-line flux, and equivalent width based on measurements of the digital objective-prism spectra. The median apparent magnitude of the sample is B = 18.2, and galaxies with redshifts approaching z = 0.1 are detected. The properties of the KISS emission-line galaxies are examined using the available observational data and compared with previous surveys carried out with photographic plates, as well as with the Halpha-selected portion of KISS. References: 35
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