  Localisation of fast radio bursts (FRBs) to arcsecond and sub-arcsecond
precision maximizes their potential as cosmological probes. To that end, FRB
detection instruments are deploying triggered complex-voltage capture systems
to localize FRBs, identify their host galaxy and measure a redshift. Here, we
report the discovery and localisation of two FRBs (20220717A and 20220905A)
that were captured by the transient buffer system deployed by the MeerTRAP
instrument at the MeerKAT telescope in South Africa. We were able to localize
the FRBs to a precision of $\sim$1 arc-second that allowed us to unambiguously
identify the host galaxy for FRB 20220717A (posterior probability$\sim$0.97).
FRB 20220905A lies in a crowded region of the sky with a tentative
identification of a host galaxy but the faintness and the difficulty in
obtaining an optical spectrum preclude a conclusive association. The bursts
show low linear polarization fractions (10--17$\%$) that conform to the large
diversity in the polarization fraction observed in apparently non-repeating
FRBs akin to single pulses from neutron stars. We also show that the host
galaxy of FRB 20220717A contributes roughly 15$\%$ of the total dispersion
measure (DM), indicating that it is located in a plasma-rich part of the host
galaxy which can explain the large rotation measure. The scattering in FRB
20220717A can be mostly attributed to the host galaxy and the intervening
medium and is consistent with what is seen in the wider FRB population.
