I. Introduction
The direct far-field antenna measurement technique is favored for its ability to obtain far-field antenna pattern data with relative ease and simplicity [1]. Multipath reflections in antenna test environments often contribute significantly to measurement errors within a facility's specified error budget. In particular, direct collimation ranges can be more susceptible to the influence of these undesired elements [2]. In the past, the mathematical absorber reflection suppression (MARS) technique has been employed for an extended duration in the context of spherical [3], [4], [5], cylindrical [6], [7], [8], and planar [9], [10], [11] near-field antenna measurement systems, compact antenna test ranges [12], as well as far-field [1] measurement facilities. The primary purpose of MARS is to detect and mitigate spurious scattering effects. It is a unique measurement and mathematical post-processing technique that only requires minimal detailed information about the antenna under test (AUT), the probe, and the measurement geometry structure [7].