The Camera and Readout for the Trinity Demonstrator and the EUSO-SPB2 Cherenkov Telescope
Mahdi Bagheri, Srikar Gadamsetty, Eliza Gazda, Eleanor Judd, Evgeny, Kuznetsov, A. Nepomuk Otte, Mathew Potts, Oscar Romero Matamala, Noah, Shapera, Joshua Sorell, Svanik Tandon, Andrew Wang

TL;DR
This paper presents the development and characterization of modular silicon photomultiplier cameras designed for detecting high-energy neutrinos using Cherenkov imaging, with applications in the Trinity and EUSO-SPB2 projects.
Contribution
It introduces two new SiPM cameras with advanced electronics and cooling, tailored for high-energy neutrino detection in atmospheric Cherenkov experiments.
Findings
Successful characterization and calibration of SiPMs
Effective bench testing of the camera systems
Demonstrated camera performance for neutrino detection
Abstract
We developed a modular silicon photomultiplier camera to detect Earth-skimming PeV to EeV tau neutrinos with the imaging atmospheric Cherenkov technique. We built two cameras, a 256-pixel camera with S14161-6050HS SiPMs for the Trinity Demonstrator located on Frisco Peak, Utah, and a 512-pixel camera with S14521-6050AN SiPMs for the EUSO-SPB2 Cherenkov Telescope. The front-end electronics are based on the eMUSIC ASIC, and the camera signals are sampled and digitized with the 100MS/s and 12-bit AGET system. Both cameras are liquid-cooled. We detail the camera concept and the results from characterizing the SiPMs, bench testing, and calibrating the two cameras.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsParticle Detector Development and Performance · Radiation Detection and Scintillator Technologies · Astrophysics and Cosmic Phenomena
