A Heavily Scattered Fast Radio Burst Is Viewed Through Multiple Galaxy Halos

We present a multi-wavelength study of the apparently non-repeating, heavily scattered fast radio burst, FRB 20221219A, detected by the Deep Synoptic Array 110 (DSA-110). The burst exhibits a moderate dispersion measure (DM) of 706. 7^+0. 6-₀. ₆ pc~cm^-3 and an unusually high scattering timescale of ₎₁ₒ = 19. 2-₂. ₇^+2. 7 ms at 1. 4 GHz. We associate the FRB with a Milky Way-like host galaxy at z₇₎ₒₓ = 0. 554 of stellar mass log₁₀ (M, ₇₎ₒₓ) = 10. 20^+0. 04-₀. ₀₃ ~M_. We identify two intervening galaxy halos at redshifts z₈₆₇₁ = 0. 492 and z₈₆₇₂ = 0. 438, with low impact parameters, b₈₆₇₁ = 43. 0-₁₁. ₃^+11. 3 kpc and b₈₆₇₂ = 36. 1-₁₁. ₃^+11. 3 kpc, and intermediate stellar masses, log₁₀ (M, ₈₆₇₁) = 10. 01^+0. 02-₀. ₀₂ ~M_ and log₁₀ (M, ₈₆₇₂) = 10. 60^+0. 02-₀. ₀₂ ~M_. The presence of two such galaxies suggests that the sightline is significantly overcrowded compared to the median sightline to this redshift, as inferred from the halo mass function. We perform a detailed analysis of the sightline toward FRB 20221219A, constructing both DM and scattering budgets. Our results suggest that, unlike most well-localized sources, the host galaxy does not dominate the observed scattering. Instead, we posit that an intersection with a single partially ionized cloudlet in the circumgalactic medium of an intervening galaxy could account for the substantial scattering in FRB 20221219A and remain in agreement with typical electron densities inferred for extra-planar dense cloud-like structures in the Galactic and extragalactic halos (e. g. , high-velocity clouds).