The Trinity-One PeV-Neutrino Telescope

Following the Trinity Demonstrator, Trinity One will be the first of the 18 Cherenkov telescopes that make up the Trinity PeV-Neutrino Observatory. Located on Frisco Peak in Utah, Trinity One can observe 64% of the sky, allowing it to detect potential neutrino point sources with unprecedented sensitivity, ranging from 1 PeV to 10 EeV. We outline the design of Trinity One, which features a 60 m${}^2$ light-collection surface and the ability to rotate in azimuth. It has a field of view measuring $5^{\circ }$ by ${60}^{\circ }$, which is equipped with a silicon photomultiplier camera with a resolution of ${0.3}^{\circ }$. Utilizing the design of Trinity One, we present performance calculations in relation to various source classes.