The following email has been sent to MIYAMOTO, Hiroko:

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Dear Hiroko Miyamoto,

The submission of your abstract has been successfully processed.

Abstract submitted: https://indico.cern.ch/userAbstracts.py?confId=192695.

Status of your abstract: https://indico.cern.ch/abstractDisplay.py?abstractId=150&confId=192695.

See below a detailed summary of your submitted abstract:

Conference: Tipp 2014 - Third International Conference on Technology and Instrumentation in Particle Physics

Submitted by: MIYAMOTO, Hiroko

Submitted on: 31 January 2014 14:05

Title: Performance of the EUSO-BALLOON Front-End Electronics

Abstract content Here the performance of EUSO-BALLOON front-end electronics with dedicated detector elements will be reported. EUSO-BALLOON is a balloon-borne pathfinder of the space-borne fluorescence detector JEM-EUSO (Extreme Universe Space Observatory on board Japanese Experimental Module) on board the International Space Station. The goal of EUSO-BALOON is to perform as a technological demonstrator of JEM-EUSO, to study the background and the detection of an atmospheric shower in a series of launches starting in 2014. The EUSO-BALLOON focal surface consists of one Photo Detector Module (PDM) while the focal surface of JEM-EUSO will consist of 137 PDMs which corresponding to roughly 5,000 64-channel Multi-Anode Photomultiplier Tubes (MAPMTs). One PDM consists of 9 Elementary Cell units (EC_units). Each EC_unit contains 4 MAPMTs and a set of PCBs used to supply high voltages to the MAPMTs and to read out the output signals. These signals are transmitted to the front-end electronics, the EC-ASIC boards each of which contains 6 SPACIROC ASICs which has been developed for JEM-EUSO. To be operated in a space environment with a limited power budget, and covering a wide dynamic range for extreme energy cosmic ray (>5x10^19 eV) observation, the ASIC is designed to perform single photon counting in a dynamic range of 1 photoelectron (PE) to 300 PEs/pixel/2.5 µs, with double pulse resolution of 30 ns, and low power consumption (<1 mW/ch). During the year 2013, the flight model EC_units and EC_ASIC PCBs were produced and the performance was successfully tested and confirmed.

Summary

Primary Authors: MIYAMOTO, Hiroko (LAL/Univ. Paris-SudXI/IN2P3/CNRS) miyamoto@lal.in2p3.fr

Co-authors: Mr. BACHOLLE, Simon (Université Paris Diderot Laboratoire Astro Particule et Cosmologie 10 rue A. Domon et L. Duquet 75013 Paris, France) simon.bacholle@apc.univ-paris7.fr Dr. BARRILLON, Pierre (a LAL/IN2P3/CNRS/Université Paris-Sud 11, Laboratoire de l’Accélérateur Linéaire , Bâtiment 200, 91898 Orsay Cedex, France) barrillo@lal.in2p3.fr Dr. CARL, Blaksley (Université Paris Diderot Laboratoire Astro Particule et Cosmologie 10 rue A. Domon et L. Duquet 75013 Paris, France) blaksley@apc.univ-paris7.fr BLIN, Sylvie (CNRS) sblin@in2p3.fr Dr. DAGORET-CAMPAGNE, Sylvie (LAL/IN2P3/CNRS/Université Paris-Sud 11, Laboratoire de l’Accélérateur Linéaire , Bâtiment 200, 91898 Orsay Cedex, France) dagoret@lal.in2p3.fr DE LA TAILLE, Christophe (OMEGA (FR)) taille@in2p3.fr GORODETZKY, Philippe (College de France) philippe.gorodetzky@cern.ch Mr. MORETTO, Camille (LAL/IN2P3/CNRS/Université Paris-Sud 11, Laboratoire de l’Accélérateur Linéaire , Bâtiment 200, 91898 Orsay Cedex, France) moretto@lal.in2p3.fr Mr. RABANAL REINA, Julio Arturo (LAL/IN2P3/CNRS/Université Paris-Sud 11, Laboratoire de l’Accélérateur Linéaire , Bâtiment 200, 91898 Orsay Cedex, France) rabanal@lal.in2p3.fr

Abstract presenters: MIYAMOTO, Hiroko

Track classification: Experiments: 2b) Astrophysics and Space Instrumentation Data-processing: 3a) Front-end Electronics

Presentation type: --not specified--

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