Image Details
Caption: Figure 12.
1D power spectrum from the analysis of 96 hr of MeerKAT interferometer data at z = 0.32 and z = 0.44. The mitigation of residual RFI (as discussed in Section 4) is achieved through the implementation of two distinct approaches: BLF (Section 4.2) and UVDF (Section 4.3).
© 2026. The Author(s). Published by the American Astronomical Society.