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This project is a visual search for field dwarf galaxies using Second PalomarSky Survey photographic plates. A morphologically selected sample of 310objects yielded 145 detections of true dwarfs within a redshift search windowof 0 to 10,000 km sec^-1. We confirm the low mass, dwarf nature of the same bycomparison of luminosity, isophotal size, HI mass and HI profile widthdistribution of other dwarf samples. The goal of this project is to use thesenewly discovered dwarf galaxies to map large scale structure as a test ofbiased galaxy formation. Initial indicators are that the large scaledistribution of dwarf galaxies is identical to bright, high mass galaxies, incontradiction to theory using biasing. The full analysis of the sample will bereported in the final paper of our series.

Gas‐rich Dwarfs from the Second Palomar Sky Survey. I. Catalog and Characteristics