Fast radio bursts (FRBs) are flashes of unknown physical origin. The majority of FRBs have
been seen only once, although some are known to generate multiple flashes,. Many models …

Fast radio bursts (FRBs) are brief, bright, extragalactic radio flashes,. Their physical origin
remains unknown, but dozens of possible models have been postulated. Some FRB sources …

The binary neutron star merger event GW170817 was detected through both
electromagnetic radiation and gravitational waves. Its afterglow emission may have been …

Fast radio bursts are millisecond-duration, bright radio signals (fluence 0.1–100 Jy ms)
emitted from extragalactic sources of unknown physical origin. The recent CHIME/FRB and …

Fast radio bursts (FRBs) are extragalactic radio flashes of unknown physical origin. Their
high luminosities and short durations require extreme energy densities, such as those found …

Very-long-baseline interferometry (VLBI) is a challenging observational technique, which
requires in-depth knowledge about radio telescope instrumentation, interferometry, and the …

Fast radio bursts (FRBs) are bright, coherent, short-duration radio transients of as-yet
unknown extragalactic origin. FRBs exhibit a variety of spectral, temporal and polarimetric …

The millisecond-duration radio flashes known as fast radio bursts (FRBs) represent an
enigmatic astrophysical phenomenon. Recently, the sub-arcsecond localization (∼ 100 mas …

Very long baseline interferometric (VLBI) localizations of repeating fast radio bursts (FRBs)
have demonstrated a diversity of local environments: from nearby star-forming regions to …

We monitored the position of the close-by (about 370 Mpc) gamma-ray burst GRB 190829A,
which originated from a massive star collapse, through very long baseline interferometry …