  The Askaryan Radio Array (ARA) is an in-ice ultrahigh energy (UHE, $>10$ PeV)
neutrino experiment at the South Pole that aims to detect radio emissions from
neutrino-induced particle cascades. ARA has five independent stations which
together have collected nearly 24 station-years of data. Each of these stations
search for UHE neutrinos by burying in-ice clusters of antennas $\sim 200$ m
deep in a roughly cubical lattice with side length $\sim 15$ m. Additionally,
the fifth ARA station (A5) has a beamforming trigger, referred to as the Phased
Array (PA), consisting of a trigger array of 7 tightly packed
vertically-polarized antennas. In this proceeding, we will present a neutrino
search with the data of this "hybrid" station, emphasizing its capabilities for
improved analysis efficiencies, background rejection, and neutrino vertex
reconstruction. This is enabled by combining the closely packed trigger
antennas with the long-baselines of the outrigger antennas. We will also place
the A5 analysis into the context of the broader five station analysis program,
including efforts to characterize and calibrate the detector, model and
constrain backgrounds, and reject noise across the entire array. We anticipate
this full neutrino search to set world-leading limits above 100 PeV, and inform
the next generation of neutrino detection experiments.
