Fewer than a dozen gamma-ray pulsars were known when the Fermi Gamma-ray Space
Telescope was launched on 2008 June 11, and the extent and diversity of the population …

Magnetars are neutron stars with extremely strong magnetic fields (1013 to 1015 gauss),,
which episodically emit X-ray bursts approximately 100 milliseconds long and with energies …

Time-domain and multimessenger astronomy (TDAMM) involves the study of transient and
time-variable phenomena across various wavelengths and messengers. The Astro2020 …

Magnetars are strongly magnetized, isolated neutron stars,–with magnetic fields up to
around 1015 gauss, luminosities of approximately 1031–1036 ergs per second and rotation …

Context. There has been significant technological and scientific progress in our ability to
detect, monitor, and model the physics of γ-ray bursts (GRBs) over the 50 years since their …

The contemporaneous detection of gravitational waves and gamma rays from
GW170817/GRB 170817A, followed by kilonova emission a day after, confirmed compact …

Magnetars are slowly rotating neutron stars that possess the strongest magnetic fields
known in the cosmos (10 14− 10 15 G). They display a range of transient high-energy …

Magnetars are neutron stars characterized by strong surface magnetic fields generally
exceeding the quantum critical value of 44.1 TG. High-energy photons propagating in their …

The physical origin of fast radio bursts (FRBs) remains unclear. Finding multiwavelength
counterparts of FRBs can provide a breakthrough for understanding their nature. In this …

Fast radio bursts (FRBs) are a class of highly energetic, mostly extragalactic radio transients
lasting for∼ milliseconds. While over 600 FRBs have been published so far, their origins are …