3 papers
astro-ph.HE2026
Synchrotron Emission from Cooled Particle Distributions
Ross Ferguson, Ben Margalit
Synchrotron emitting electrons can lose energy (`cool') through various processes including radiative losses (e.g., synchrotron or inverse-Compton cooling) and adiabatic expansion.…
astro-ph.HE2025
Numerical Modeling of Relativistic Effects in Synchrotron-Emitting Shocks
Ross Ferguson, Ben Margalit
Synchrotron emission is seen in a vast array of astrophysical transients, such as gamma-ray bursts (GRBs), radio supernovae, neutron star (NS) mergers, tidal disruption events (TDE…
astro-ph.HE2025
RRAT-like behaviour of PSR B0656+14 observed with I-LOFAR
S. C. Susarla, R. Ferguson, O. A. Johnson +5
Single pulse studies offer vital insights into the emission physics of pulsars, particularly in the case of young, nearby sources where intrinsic variability is often pronounced. P…