Brandon Bear

TL;DR: In this article, the authors reported the detection of giant pulse (GP) emission from PSR B0950+08 in 24 hours of observations made at 39.4 MHz, with a bandwidth of 16 MHz, using the first station of the LWA.

TL;DR: In this article, the authors detected 119 giant pulses from PSR B0950+08 (at its dispersion measure), which they defined as having SNRs at least 10 times larger than for the mean pulse in their data set.

TL;DR: In this article, the authors explore opportunities for multi-messenger astronomy using gravitational waves (GWs) and prompt, transient low-frequency radio emission to study highly energetic astrophysical events, highlighting proposed mechanisms that lead to a short-duration, high-flux radio pulse originating from the merger of two neutron stars or from a superconducting cosmic string cusp.

TL;DR: In this article, the authors reported the detection of giant pulse emission from PSR~B0950+08 in 12 hours of observations made simultaneously at 42 and 74~MHz, using the first station of the Long Wavelength Array, LWA1.

TL;DR: In this article, the authors reported the detection of giant pulse emission from PSR~B0950+08 in 12 hours of observations made simultaneously at 42~MHz and 74~MHz, using the first station of the Long Wavelength Array, LWA1.