A VLSI ASIC front end for the optical module of the NEMO underwater neutrino detector

Details A VLSI ASIC front end for the optical module of the NEMO underwater neutrino detector A VLSI ASIC front end for the optical module of the NEMO underwater neutrino detector

Nov 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006nimpa.567..548l&link_type=abstract

Nuclear Instruments and Methods in Physics Research Section A, Volume 567, Issue 2, p. 548-551.

Physics

1

Scientific paper

The work described here has been developed in the context of the NEMO Collaboration with the aim of studying and designing a front-end electronics for the Optical Modules, which contains the telescope optical sensors, as a full-custom Very Large Scale Integration (VLSI) Application Specific Integrated Circuit (ASIC). The solution has a multitude of advantages. The most important are low power consumption and the pre-analysis and suitable reduction of data to be transferred to the shore station for acquisition. A detailed description of the chosen architecture and the design principles of the blocks, that carry out the specialized function required by this architecture, will be given. The chips produced will be described and the test measurements performed will be shown.

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