FARCOS is a 20-telescope modular detection system intended to extend the capacity of 4π detectors in the field of dynamics of heavy ion collisions and spectroscopy of light nuclei at the border of neutron and proton drip lines. The performance of the detection system is mainly set by the custom CMOS frontend electronics with selectable full-scale energy range from 100MeV up to 2.2GeV with 4-bit granularity and high energy resolution below 10 keV FWHM at the pulser line (100MeV full-scale energy range). Automatic test and calibration tools -based on an on-chip pulser- ease the use of telescopes in experiments. The contribution reviews the status and perspectives of the FARCOS frontend electronics.
The FARCOS frontend electronics: Status and perspectives
C. Guazzoni;V. L. Sicari
2021-01-01
Abstract
FARCOS is a 20-telescope modular detection system intended to extend the capacity of 4π detectors in the field of dynamics of heavy ion collisions and spectroscopy of light nuclei at the border of neutron and proton drip lines. The performance of the detection system is mainly set by the custom CMOS frontend electronics with selectable full-scale energy range from 100MeV up to 2.2GeV with 4-bit granularity and high energy resolution below 10 keV FWHM at the pulser line (100MeV full-scale energy range). Automatic test and calibration tools -based on an on-chip pulser- ease the use of telescopes in experiments. The contribution reviews the status and perspectives of the FARCOS frontend electronics.| File | Dimensione | Formato | |
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guazzoniSicari_sif20.pdf
Open Access dal 01/02/2023
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