Laboratory for the Integration of Electronic Processing and Acquisition Systems (LISETA)

The Laboratory for the Integration of Electronic Processing and Acquisition Systems (LISETA) designs, produces, assembles and validates the electronic equipment and software integrated into the scientific detection instruments developed and used by the IRFU’s various departments. It is involved in the development and production of both very large research instruments (CTA, ATLAS, ALICE, ESS, etc.) and smaller-scale experiments or R&D programs (Calipso, Sphère, MicroCal-X).

The laboratory develops the electronic boards that make up the various links in the acquisition chain, from the detector to the control and acquisition systems. It also develops the test, characterization and quality control hardware and software needed to evaluate and validate systems and their components. Finally, it oversees industrial manufacturing, assembly, integration and validation of research equipment prior to on-site commissioning.

Designed as part of international collaborations, the systems developed and their interfaces are increasingly complex. Their manufacture and integration are a challenge in themselves, which LISETA takes up through methodological actions (quality control, logistics of production and integration flows, database management) and also thanks to the expertise of each individual and the generalist skills of the whole team.

LISETA’s operational resources make an effective contribution to the running of the department. The laboratory provides a wiring service to equip prototype boards designed in the department, to troubleshoot faulty boards, to adapt existing boards and to support the production of small series. The laboratory also makes available to the department the work of the printed circuit CAD group, which each year designs the printed circuits for dozens of electronic boards, from the simplest to the most complex, and the routing of detector floors using printed circuit technology (Micromegas detectors). With the miniaturization of components and the ever-increasing speed of analog and digital signals, mastering and extending wiring and CAD resources is a major challenge for LISETA.

The laboratory is also responsible for the design, development and testing of integrated circuits and electronic readout boards operating at ultra-low temperatures (50 mK to 4 K), as well as the integration of these very high-density systems in their cryogenic environment. The challenge is to combine very low noise, ultra-low power consumption, speed and thousands of readout channels, for dark matter detection (DPhP) and space astronomy (DAp) experiments.

Placement and routing of 24-layer LTDB board components for ATLAS.
ZedBoard-based test bench for Nectar ASICs

Projects

  • AGATA

    AGATA

    AGATA (Advanced Gamma-ray Tracking Array)is a new generation high-resolution γ-ray spectrometer providing unprecedented Doppler-correction capabilities thanks to a combination of fine detector…

  • ALICE

    ALICE

    The ALICE experiment is devoted to the study of nuclear matter under extreme conditions of temperature and density. It is specially designed to test the fundamental theory of the strong interaction,…

  • Antares, a high energy neutrino telescope

    Antares, a high energy neutrino telescope

    Overview Most of our current knowledge of the Universe comes from the observation of photons. Photons have many advantages as cosmic information carriers: they are copiously produced, they are…

  • ATHENA

    ATHENA

    Un satellite pour l’étude del’univers chaud et énergétique. Lancement prévu pour 2031. A satellite to study hot and energetic universe to be launched in 2031.

  • ATLAS

    ATLAS

    Atlas is one of the general purpose detectors which started operation in 2008 at the the CERN proton collider, to study the Higgs boson. Goals: Unifying the elementary constituants of matter and…

  • BABAR

    BABAR

    Goal The main goal of theexperiment was toperforma complete study of CP violation (CP is the symmetry linking particulesand antiparticules) in the systemof Bmesons. Moregenerally the experiment…

  • BAO

    BAO

    Most of the content of the Universe, about 70%, is dominated by an energetic component that is neither matter nor radiation: dark energy. This mysterious component, first observed in 1998 with…

  • CLAS12

    CLAS12

    Deeply Virtual Compton Scattering experiment at Jefferson Lab Hall B , with CLAS12, large acceptance spectrometer. Goals: Theoretical concepts asGeneralized Parton Distributions (GPD), enable to…

  • CLIC: CTF3-CALIFES

    Objectives The scientific exploitation of the LHC (Large Hadron Collider), planned to start operation in 2008 will be the higher priorityin high energy physics for the next coming years. In the…

  • CMS

    CMS

    CMS is the detector of one of the 2 multi-purpose experiments out of the 4 experiments located at the LHC at CERN near Geneva. CMS is installed at point 5 in Cessy. Main goals : During the last…

  • COAST  COmputational ASTrophysics

    COAST COmputational ASTrophysics

    Simulation numérique en astrophysique spécialisé dans l’activité de “calcul de haute performance”. Astrophysics digital simulation for “high performance computing”.

  • COAST  COmputational ASTrophysics

    COAST COmputational ASTrophysics

    Web site of the COASTproject Presentation The COAST project is a DAPNIA program of high performances computing in astrophysics. It includes developments of codes, numerical methods, visualization…

  • CTA (Cherenkov Telescope Array)

    CTA (Cherenkov Telescope Array)

    A new generation observatory to explore the high energy Universe. Une nouvelle génération d’observatoire pour explorer l’Univers à haute énergie.

  • D0

    D0

    Presentation The D0 experiment was located at the proton-antiproton Tevatron collider at the Fermilab laboratory (Chicago, USA). There was two data taking periods: Run I from 1992 to 1996 with a…

  • Detectors for linear collider

    Detectors for linear collider

    FELICE (acronym for “Future Electron LInear Collider Experiment”) is a group of physicists and engineers working for the physics and detectors at the ILC (International Linear Collider). An…

  • Edelweiss

    Edelweiss

    Objectives The goal of Edelweiss is to detect the dark matter of our Galaxy through its interactions in detectors operated in underground laboratory. The EROS experiment, searching for massive…

  • ESS: The European Spallation Source

    ESS: The European Spallation Source

    The linear accelerator includes a low-energy section (E≤ 90MeV) with a Radio Frequency Quadrupole (RFQ), a Drift Tube Linac (DTL), and a high-energy section made up of superconducting cavities that…

  • Fulis rotating Target

    Fulis rotating Target

    Objectives While the heaviest element on earth is 238-uranium (with traces of Pu and Np in natural nuclear reactors) whose lifetime is 5 billion years, the last 60 years have seen the synthesis of…

  • GBAR

    GBAR

    Aims: One of the fundamental questions of today’s physics concerns the action of gravity upon antimatter. No experimental direct measurement has ever been successfully performed with antimatter…

  • HESS

    HESS

    H.E.S.S. Exploring the High Energy gamma ray sky H.E.S.S stands for “High Energy Stereoscopic System”. This telescope system been designed and built by a large international collaboration which…

  • JWST

    JWST

    The James Webb Space Telescope (JWST) launched on 25 December 2021 isthe successor of the Hubble Space Telescope. This is a NASA led mission with the participation of Europe, under the…

  • LISA

    LISA (Laser Interferometer Space Antenna) is the large-class mission of the European Space Agency’s (ESA) long-term Cosmic Vision programme for the observation of gravitational waves. It will be the…

PhD thesis