Overview
- FRB 20240304B has been spectroscopically localized to a host at redshift 2.148, confirming it as the most distant FRB with a secure identification.
- The burst resides in a clumpy, low-mass dwarf galaxy with active star formation and 10–20% solar metallicity, consistent with a young magnetar source.
- An observed dispersion measure of ∼2,458 pc/cm³ and high linear polarization fraction of 49% reveal the density and magnetic field structure of the intervening intergalactic medium.
- By doubling the redshift reach of localized FRBs, the discovery enables these flashes to chart ionized baryons through roughly 80% of cosmic history.
- Combining sensitive radio detection at MeerKAT with deep imaging and spectroscopy from JWST highlights a cross-facility approach to unraveling FRB origins.