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 m2 light-collection surface and the ability to rotate in azimuth. It has a field of view measuring 5 deg by 60 deg, which is equipped with a silicon photomultiplier camera with a resolution of 0.3 deg. Utilizing the design of Trinity One, we present performance calculations in relation to various source classes.
A. N. Otte (Wed,) studied this question.