ABSTRACT. We report on the detection of giant pulses from the Crab Nebula pulsar at a frequency of 200 MHz using the field deployment system designed for the Mileura Widefield Array's Low Frequency Demonstrator (MWA-LFD). Our observations are among the first high-quality detections at such low frequencies. The measured pulse shapes are deconvolved for interstellar pulse broadening, yielding a pulse-broadening time of 670 ± 100 μs, and the implied strength of scattering (scattering measure) is the lowest that is estimated toward the Crab Nebula from observations made so far. The sensitivity of the system is largely dictated by the sky background, and our simple equipment is capable of detecting pulses that are brighter than ~9 kJy in amplitude. The brightest giant pulse detected in our data has a peak amplitude of ~50 kJy, and the implied brightness temperature is 10^31.6 K. We discuss the giant pulse detection prospects with the full MWA-LFD system. With a sensitivity over 2 orders of magnitude larger than the prototype equipment, the full system will be capable of detecting such bright giant pulses out to a wide range of Galactic distances; from ~15 to ~30 kpc depending on the frequency. The MWA-LFD will thus be a highly promising instrument for the studies of giant pulses and other fast radio transients at low frequencies.

Subject headings: ISM: individual (Crab Nebula); ISM: structure; pulsars: general; pulsars: individual (Crab pulsar); scattering

Print publication: Issue 1 (2007 August 10)
Received 2007 March 24, accepted for publication 2007 April 30