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Pulsar Science: Arecibo 327 MHz Drift Scan Processing

Friday, November 8, 2013: 11:00 AM - 1:00 PM
Napoleon B3-C3 (Sheraton New Orleans Hotel)
Nathan Tehrani , West Virginia University
Pulsars are the hot, extremely massive and compact remnants of long-dead stars. They can be detected at radio frequencies using large radio telescopes. This poster details the processing of a decade-long pulsar survey using the Arecibo Telescope in Puerto Rico, including the discovery of two new pulsars.