A survey conducted with the seven-beam Arecibo L-Band Feed Array (ALFA) at the Arecibo Observatory, at frequencies near 1.4 GHz. Primarily concentrated in those areas of the plane which can be seen from Arecibo, this survey is ongoing, having started in 2004. Originally using the WAPP autocorrelators as backend and now using the Mock spectrometers, which allows about 300 MHz of bandwidth. Website: http://www2.naic.edu/alfa/pulsar/.