TAROGE-M is a radio antenna array atop $\sim2.7$ km-high Mt.~Melbourne in Antarctica for detecting ultra-high energy (UHE, $E> 10^{17}$ eV) air showers in near-horizontal directions. Besides the detection of cosmic rays and Earth-skimming tau neutrinos, its primary goal is to reproduce the discovery and verify the origin of so-called ANITA anomalous events, having feature of upward-going UHE air showers but cannot be explained by tau neutrinos. The detection concept takes advantages of a high altitude for a broad view toward the horizon; strong and near-vertical geomagnetic field for enhancing the radio signal; and quiet radio environment in Antarctica. Its relatively simple design and high duty cycle make it easily to be extended and thus to achieve an exposure competitive with ANITA experiments within a few years.


The first TAROGE-M station operating at 180--450 MHz frequencies deployed in 2020 detected seven UHE cosmic ray events within $25.3$-day livetime. The events have a mean energy of $\sim 1$ EeV and an estimated flux consistent with other experiments, and validate the station as an UHE particle detector. In 2022--2023 season, the system was upgraded for a robust long-term operation, with a more detailed calibration with a drone-borne pulser. We also discuss the planned upgrade, including the implementation of interferometric trigger, which is expected to increase the cosmic ray and tau neutrino acceptances by a factor of 10 at $0.1$ EeV, corresponding to a lower energy threshold by a factor of 3.