TSAI_poster Searches for Radio Transients using the Long Wavelength Array

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The abstract: "We report the detection of giant pulse emissions from pulsars at 40 MHz and 70 MHz using the first station of the Long Wavelength Array - LWA1. Compared with the normal pulse, Giant pulses of pulsars have shorter temporal durations, higher intensities, and their cumulative distributions of pulse strength follow a power law, which is much less steep than would be expected if we were observing the tail of a Gaussian distribution of normal pulses. We also searched radio transients from nearby galaxies M31and M81, but no detection with S/N > 7 (177 Jy) was found in a large dispersion measure range from 1.0 to 5000 pc cm^-3."

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