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We present the status of the development of a Cherenkov telescope to be flownon a long-duration balloon flight, the Extreme Universe Space Observatory SuperPressure Balloon 2 (EUSO-SPB2). EUSO-SPB2 is an approved NASA balloon missionthat is planned to fly in 2023 and is a precursor of the Probe of ExtremeMulti-Messenger Astrophysics (POEMMA), a candidate for an Astrophysicsprobe-class mission. The purpose of the Cherenkov telescope on-board EUSOSPB2is to classify known and unknown sources of backgrounds for future space-basedneutrino detectors. Furthermore, we will use the Earth-skimming technique tosearch for Very-High-Energy (VHE) tau neutrinos below the limb (E > 10 PeV) andobserve air showers from cosmic rays above the limb. The 0.785 m^2 Cherenkovtelescope is equipped with a 512-pixel SiPM camera covering a 12.8{\deg} x6.4{\deg} (Horizontal x Vertical) field of view. The camera signals aredigitized with a 100 MS/s readout system. In this paper, we discuss the statusof the telescope development, the camera integration, and simulation studies ofthe camera response.

Overview of Cherenkov Telescope on-board EUSO-SPB2 for the Detection of Very-High-Energy Neutrinos