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UCM-ELECTRONICS. Members and EPOs with active participation

UCM-ELECTRONICS. Members and EPOs with active participation. P. Antoranz, “Ayudante de Universidad”. Physicist and Electronic Engineer. Full time dedication to the project. Long standing experience working in hardware for Cherenkov telescopes. MAGIC members since 2005

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UCM-ELECTRONICS. Members and EPOs with active participation

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  1. UCM-ELECTRONICS. Members and EPOs with active participation P. Antoranz, “Ayudante de Universidad”. Physicist and Electronic Engineer. Full time dedication to the project. • Long standing experience working in hardware for Cherenkov telescopes. • MAGIC members since 2005 • Expertise in high frequency electronics and electromagnetic compatibility. Mr. Teodoro Bernardino Santos. Manager of different projects related to satellite based timing and european navegation systems. Pursuing the PhD degree. Dr. J.M. Miranda. “Profesor Titular de Universidad”. Full time dedication to the project. Expertise in high frequency electronics. Deep knowledge on state of the art hardware for synchronization and timing. Dr. J.J. Jimenez, “Profesor Titular de Universidad”. Headmaster of the Electronics department. Full time dedication to the project. Joining efforts Expertise in quality control and reliability analysis. Close contact with industries involved in key technologies for CTA. Dr. J.C. Jimenez, “Profesor Titular de Universidad”. Full time dedication to the project. Expertise in • Solid state devices • Microelectronics • Monte Carlo simulation of different technologies involved in solid state photodetectors. Dr. M.C. Perez. “Profesor Titular de Universidad”. Full time dedication to the project. Mr. Lamberto Fresnillo. Manager of Fidias. Pursuing the PhD degree. European auditor in quality control (EOQ).

  2. Mr. Ignacio Vegas is Electronic Engineer. He is presently pursuing the PhD degree and about to defend his master thesis. He has worked in evaluation boards for MAGIC II telescope hardware testing. First author of a technical application note for the MAGIC collaboration. Mr. Ricardo Padrino will become Electronic Engineer soon. Presently preparing his degree project on signal conditioning and test of GAPD clusters. ELECTRONICS GROUP at UCM The youngest collaborators. Four of us are teachers in Electronic Engineering and Physics. We are in an excellent situation to find and recruit young and highly motivated people with important skills for CTA.

  3. UCM-ELEC GROUP have well equipped laboratories FACILITIES • 80 m2 clean room class 100,000 for high reliability litography and prototype fabrication. • GTEM cell for Electromagnetic Compatibility (EMC) Compliance tests. • Standard and advanced facilities for SMD board prototyping. • High precision soldering and rework stations. INSTRUMENTATION • Vector Network Analyzer (VNA) with high precision calibration kit. • Spectrum Analyzer for noise and nonlinear analysis. • Dynamic Signal Analyzer Agilent 35670A for reliability tests. • Specific instrumentation for phase noise and jitter measurements. • Portable Electromagnetic field meters • EMC test facilities for radiated and conducted interference monitoring. • Commercial ns-range pulse generators for testing. • Laser and pulsed LED sources for photodetector testings. 3/10

  4. Activities: Noise metrology for reliability and failure prediction Failure diagnostics of solid state devices based on noise measurements. Noise of solid state photodetectors (1995-1999) Transistors for pulse amplifiers (1997-2002)

  5. Activities: Fabrication and test of high frequency low noise amplifiers 1998-2000. 2000-2004. Monolithic Microwave integrated circuit amplifiers. GaAs foundry. Low noise measurements and design of criogenically cooled amplifier for the Square Kilometer Array (SKA) facility. Measured and modeled noise vs frequency at temperatures of 300 K, 77 K, and 4.2 K. 1.2 mm Ultra low noise Monolithic Microwave Integrated Circuit (MMIC) amplifier. Noise figure of 3 dB and G=20 dB Quantum noise limit Grounded-gate low power consumption amplifier (60 mW) 5/10

  6. UCM-ELEC. Previous fund and corresponding results Astrofísica de altas energías con MAGIC FPA2006-12383-C02-01 (2006-2009) EDP of 8 (1.5 from UCM-ELEC) MV Fonseca 608 k€ See presentation of MV Fonseca for further details: FPA2009-08938 ASTROFISICA DE ALTAS ENERGIAS CON MAGIC 1 peer reviewed paper (high frequency modelling of LEDs) 2 MAGIC internal notes 2 peer reviewed papers (testbenches and central pixel) 6 peer reviewed conference presentations. 4 Electronic engineering projects 2 Msc thesis 1 PhD thesis (to be read in September) • Pulse amplifiers for MAGIC II camera and receiver boards. • Software tools. • Multichannel eval boards with ns pulse generators. • MAGIC shifts according to the MAGIC CB policies. • MAGIC I central pixel design and test (in collaboration with UCM-GAE, IFAE and other researchers). • Test benches for single photoelectron counting, noise and pulse distortion measurements of PMT, HPD and GAPD-based pixels (in collaboration with UCM-GAE, IFAE and other researchers).

  7. UCM-ELEC. Previous fund and corresponding results (only 2 EDP) “Participación Española en la puesta en marcha del Estudio de Diseño del Cherenkov Telescope Array (CTA)” Manel Martínez – IFAE FPA2007-30012-E 10 k€ FPA2007-31120-E 74 K€ • Development of test bench for GAPD based on new pulsed LED head. • Barcelona, March 2009.Presentation of the amplifiers designed by UCM-ELEC in a meeting with HESS researchers, including the main responsible of the WP ELEC (Pascal Vincent) • May 2009, Cracow. Attendance to the CTA meeting, with two important decisions: • Manel Martinez and Werner Hofmann elected as spoke-persons. • CB board and CTA groups configured by consensus. All the PIs of the subprojects presented in this application are members of it.

  8. Objectives and requested budget • Our objectives were chosen considering: • Needs of CTA collaboration • CTA schedule • Our previous work • Our expertise • Our links with industry 8/10

  9. Identifying CTA needs with UCM-ELEC objectives (I) PMTs are likely to be the first option, but today there is only ONE company able to provide suitable PMTs to CTA. Solid state photodetectors (mainly GAPD) evolve very fast, and have been identified as a backup option. W. Hofmann • Task 2 is coming in the right moment, with the right objectives and with well prepared and coordinated people. • Furthermore, • There is a strong interest within the particle physicist community in GAPDs and other solid state photodetectors. • There are many opportunities of quality research and technology transfer within this field LATEST NEWS (Cracow meeting)

  10. Identifying CTA needs with UCM-ELEC objectives (II) We are about to obtain ENAC qualification for our lab. This will enable us to offer certificates of CEM and reliability compliance. LATEST NEWS (Cracow meeting) B. Yoffo, Quality and Assurance work package M. Panter, Telescope work package 10/10

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