2–6 Dec 2025
Biblioteca Salaborsa
Europe/Rome timezone
Proceedings submission deadline is ___ 24 March 2026 ___

Preliminary characterization of the 64-channel MIZAR ASIC for Cherenkov light detection

3 Dec 2025, 19:03
1m
Auditorium Enzo Biagi (Biblioteca Salaborsa)

Auditorium Enzo Biagi

Biblioteca Salaborsa

Biblioteca Salaborsa, Piazza del Nettuno, 3, 40121 Bologna BO
Poster Electronics and Readout Poster Session

Speaker

Andrea Di Salvo (Istituto Nazionale di Fisica Nucleare)

Description

This work presents the implementation and the preliminary tests of the Multi-channel Integrated Zone-sampling Analogue-memory based Readout (MIZAR) ASIC. Developed using commercial 65 nm CMOS technology, the MIZAR ASIC is designed as part of the Cherenkov camera for the POEMMA Balloon with Radio (PBR) mission. The goal of the Cherenkov camera is to detect direct Cherenkov signals produced by Extensive Air Showers (EASs) pointing towards the detector. The broader objective of the PBR mission is the detection of Ultra-High Energy Cosmic Rays (UHECRs) and tau-induced air showers resulting from the interaction of Cosmic Neutrinos with the Earth's crust. In the MIZAR ASIC, a single channel is segmented into 256 acquisition cells and each one includes a capacitor, a Wilkinson Analog-to-Digital Converter (ADC) and a digital memory. This full waveform sampling system operates with an integration time of 5 ns and the data are converted on chip at the same frequency. MIZAR is designed to send out a 64-bit hitmap to use as first-level trigger to recognize patterns of interest. Each channel can be programmed to reduce the sampling window to 32 or 64 cells and the resolution can be set within the interval 8-12 bits. MIZAR was delivered in March 2025 and it has undergone laboratory testing in recent months.

Speaker Confirmation Yes

Authors

Andrea Di Salvo (Istituto Nazionale di Fisica Nucleare) Angelo Rivetti (Istituto Nazionale di Fisica Nucleare) Emanuele Trossarello (INFN) Federico Reynaud (Istituto Nazionale di Fisica Nucleare) Marco Mignone (TO) Mario Edoardo Bertaina (Istituto Nazionale di Fisica Nucleare) Matteo Abrate (Istituto Nazionale di Fisica Nucleare) Micol Bargelli (INFN) Richard James Wheadon (Istituto Nazionale di Fisica Nucleare) Sara Garbolino (Istituto Nazionale di Fisica Nucleare)

Presentation materials