Cosmic Rays physics, Gamma-Ray Astronomy. Expert on gaseous detectors (MWPC and RPC), front end electronics, DAQ, data analysis and MC simulations.
|
|
- Morgan Rodgers
- 5 years ago
- Views:
Transcription
1 Dr. Giovanni MARSELLA Via F. Milizia, 677 Lecce 338/ CURRICULUM VITAE Giovanni Marsella born on 12-feb-1966 in La Chaux-de-Fonds (Switzerland), married, 2 daughters. Double Nationality: Italian and Swiss h-index: 17 (isi web of knowledge) [ ] Liceo Scientifico "C. De Giorgi", Lecce. Maturity evaluation: 58/60. [ ] Graduate in Physics at University of Pisa. 100/110. Experimental thesis: "Cerenkov ultraviolet light detection in atmospheric showers by multistep photosensitive chambers ", tutor Doct.. A.Menzione. [1994] Corso di perfezionamento in Physics at Physics Department, University of Pisa [ ] 2 years post-graduate grant by INFN (National Institute of Nuclear Physics). Mainly the job has been done at IAC (Instituto de Astrofisica de Canarias) In La Palma, Canary Islands, (Spain). [ ] Ph.D. in Physics at University of Lecce. Discussed the thesis on February the 22nd The title: " High altitude atmospheric shower detection techniques for gamma-ray Astronomy". [ ] Three trimestral contracts with University of Lecce by ARGO-YBJ collaboration. [2000] 4 year post-doc grant by INFN to realize FRONT-END electronics and relative ON- LINE control in the ARGO-YBJ collaboration. [2001] Assistant Professor position in Physics at Lecce University. RESEARCH ACTIVITIES: Cosmic Rays physics, Gamma-Ray Astronomy. Expert on gaseous detectors (MWPC and RPC), front end electronics, DAQ, data analysis and MC simulations. [1992] Started an experimental thesis in the CLUE collaboration. The activity concerned the detection of UV Cherenkov Light. The idea was to extend the sensibility and duty cycle of a Cosmic Ray Cherenkov Detector using a photocathode sensitive in UV. My principal activity was to build and test a MultiWire Proportional Chamber sensitive to UV photons. [ ] Within the CLUE collaboration I participated to the installation of a matrix of 9 UV Cherenkov telescopes at the Observatory of Roque de Los Muchachos in La Palma Canary Islands, to data taking and analysis The activity is well documented in the following publications: Alexandreas, D. et al. "Status report on CLUE", Nuclear Inst. and Methods in Physics Research, A 360 (1-2), pp (1995) Alexandreas, D. et al., "The CLUE experiment operating with 4 telescopes in La Palma", Nuclear Instruments and Methods in Physics Research, Section A: 409 (1-3), pp (1998)
2 Alexandreas, D. et al.,"the CLUE trigger: A VME based two level trigger for VHE experiments" Nuclear Instruments and Methods in Physics Research, Section A: 409 (1-3), pp (1998) Alexandreas, D. et al., "Reconstruction of showers at TeV energy by the CLUE experiment and its application to recent data", Nuclear Physics B - Proceedings Supplements 75 (1-2), pp (1999) [ ] In this period I get my PhD at Lecce University. The work was a MC study on a combined technique of a Cherenkov Telescope Array and a full coverage carpet made by RPCs to. The previous experience with the CLUE collaboration was combined with the new experience with ARGO-YBJ, an Italian-chinese collaboration for the realization of an high altitude (Tibet, 4300 m asl) and full coverage detector made by RPC to detect VHE cosmic rays (100 GeV TeV) and suitable for TeV Gamma ray Astronomy. The Combination of the two techniques allows to improve the sensitivity to TeV Gamma Ray Sources. This study was useful to both collaborations. The results are published in the following works: G. Marsella PhD thesis: " High altitude atmospheric shower detection techniques for gamma-ray Astronomy". Bartoli, B. et al., "Shower reconstruction in the CLUE experiment", Nuclear Instruments and Methods in Physics Research, Section A: 461 (1-3), pp (2001) Bartoli, B. et al., "Observation of γ-sources using a new reconstruction technique in the CLUE experiment", Nuclear Physics B - Proceedings Supplements 97 (1-3), pp (2001) G. Marsella on behalf of CLUE coll. "Preliminary results from the CLUE Cherenkov UV experiment" Vulcano Workshop on Frontier Objects in Astrophysics and Particle Physics, Vulcano, Italy, May C. Bacci et al. "Results from the analysis of data collected with a 50-m**2 RPC carpet at YangBaJing" NIM A456: ,2000 [ ] In this three years I get various grants from University of Salento and INFN to continue the activity with the ARGO-YBJ collaboration. I developed a System to test the 600 TDCs that were needed for the timing measurement of the pads of the detector with 1 ns time resolution. I developed a system based on a VME, controlled first by Labview and later by a Linux CPU, like the final DAQ system of ARGO- YBJ, in oder to develop in the same time some important routines for DAQ Online Control and data taking. I also developed the routines for the data decoding of the official Analysis program of the collaboration. This work is well documented in many internal notes and manuals of the ARGO-YBJ collaboration [ ] In 2001 I have been engaged as Professor Assistant at the University of Salento. I essentially devoted my research activity in ARGO-YBJ collaboration. I continued developing the Online routines for the monitoring of the front-end electronic and for the data decoding. I also contributed to the detector and DAQ installation at YangBaijing (Tibet). Since 2004 till the end of data taking (February 2013) I have been the Runn Coordinator. I contributed to many analysis items. In particular I
3 worked on algorithms for Gamma-Hadron separation to enhance our sensitivity to gamma sources, on the time structure of the Cosmic Ray Shower fronts, and on the Proton-Air and Proton- Proton cross section with ARGO-YBJ detector (ARGO Collaboration, "Proton-air cross section measurement with the ARGO-YBJ cosmic ray experiment PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY, vol. 80; p ). Since 2012 I m the local coordinator for the ARGO-YBJ collaboration. The work of all these years is documented in many publications and in the following conferences: "ARGO-YBJ: A high altitude detector for cosmic ray physics." G. Marsella for the ARGO-YB collaboration, Jan st Rencontres de Moriond Workshop on Very High-Energy Phenomena in the Universe, Les Arcs, France, Jan Published in *Les Arcs 2001, Very high energy phenomena in the universe* HEG-T18 "Multiscale image analysis applied to gamma/hadron discrimination for vhe gamma-ray astronomy with argo-ybj" I. De Mitri, G. Marsella, F. Salamida. Jul pp. Published in Nucl.Instrum.Meth.A525: ,2004. e-print: astro-ph/ "The Trigger system of the ARGO-YBJ detector" By the ARGO-YBJ Collaboration (S. Mastroianni et al.) Published in IEEE Trans.Nucl.Sci.51: ,2004 Also in *Tsukuba 2003, Cosmic Ray* e-print: hep-ex/ "Algorithms for the determination of the primary particle direction with ARGO-YBJ detector" By ARGO-YBJ Collaboration Jul th International Cosmic Ray Conferences (ICRC 2003), Tsukuba, Japan, 31 Jul - 7 Aug "Local Station: The data read-out basic unit for the ARGO-YBJ experiment" By ARGO-YBJ Collaboration (R. Assiro et al.) pp. 9th Pisa Meeting on Advanced Detectors: Frontier Detectors for Frontier Physics, La Biodola, Isola d'elba, Italy, May Published in Nucl.Instrum.Meth.A518: ,2004 "ARGO-YBJ: A unique device for the EAS study" G. Marsella for the ARGO-YBJ collaboration th International Conference on Astroparticle and Underground Physics (TAUP 2005), Zaragoza, Spain, Sep 2005 Published in J.Phys.Conf.Ser.39: ,2006. "The ARGO-YBJ Daq System and the GRID Based Data Transfer" A. Aloisio, P. Branchini, A. Budano, S. Catalanotti, P. Celio, P. Creti, F. Galeazzi, R.Gargana, G. Marsella, S. Mastroianni, F. Ruggieri, C. Stanescu pp. Published in IEE transactions on nuclear science vol 55, N.1, Febbruary "Study of cosmic ray showers front with ARGO-YBJ, data compared to simulation" A.K. Calabrese Melcarne, I. De Mitri, G. Marsella, L. Perrone, G. Petronelli, A. Surdo, G. Zizzi 30th International Cosmic Ray Conference (ICRC) Merida, Mexico, July 2007 "The architecture of DAQ system for the ARGO-YBJ experiment" F. Galeazzi, R. Gargana, G. Marsella, S. Mastroianni, F. Ruggieri for the ARGO-YBJ Collaboration 30th International Cosmic Ray Conference (ICRC) Merida, Mexico, July 2007 "Event selection to improve ARGO-YBJ sensitivity to gamma sources using Crab as a standard candle" G. Marsella, C. Bleve, D. Martello, S. Vernetto, J.L. Zhang on behalf of the ARGO-YBJ Collaboration 31th International Cosmic Ray Conference (ICRC) Lodz, Poland, July 2009 "Gamma Astronomy with the ARGO-YBJ experiment" G. Marsella on behalf of the ARGO-YBJ collaboration 44th Rencontres de Moriond Very High Energy phenomena in the Universe La Thuile, Valle d Aosta, Italy 1-8 February 2009 "Physics and astronomy results with the ARGO-YBJ experiment" G. Marsella on behalf of the ARGO-YBJ collaboration Nuclear Physics B (Proc. Suppl.) 188 (2009)
4 "Astroparticle Physics with ARGO-YBJ experiment" G. Marsella for the ARGO-YBJ Collaboration ICHEP 2010 Paris, france, July 22-28, 2010: Published on PoS "Recent results from the ARGO-YBJ Experiment",G. Marsella, for the ARGO-YBJ Collaboration, XIIIth ICATPP Conference, Villa Olmo, 3-7 October 2011 "Hadronic interaction studies with the ARGO-YBJ experiment", I. De Mitri, G. Marsella, L. Perrone, A. Surdo, G. Zizzi for ARGO-YBJ coll. XXXIInd ICRC, Beijing 2011 "Temporal and spatial structure of the extensive air shower front with the ARGO-YBJ experiment", A.K. Calabrese Melcarne, G. Marsella, D. Martello, L. Perrone, S. Sbano for ARGO- YBJ coll., XXXIInd ICRC, Beijing 2011 "EAS Time Structures with ARGO-YBJ experiment", A. K. Calabrese Melcarne and G. Marsella on behalf of ARGO-YBJ collaboration, 23rd European Cosmic Ray Symposium (ECRS 2012) Moscow, Russia "Study of the time structure of EAS particles with ARGO-YBJ", A.K. Calabrese Melcarne, G. Marsella, D. Martello, L. Perrone, S.N. Sbano for the ATGO-YBJ coll., XXXIII ICRC, Brasil 2013 "Study of the shower front structure at few meters from the core with ARGO-YBJ", P. Bernardini, A. D'Amone, I. De Mitri, G. Marsella, A. Surdo for the ATGO-YBJ coll., XXXIII ICRC, Brasil 2013 [ ] In this period I dedicated part of my research activity to a Medical Physics project, MAGIC5, to design a mammographic CAD in collaboration with V. Fazzi Hospital in Lecce. The activity was devoted to develop algorithm to identificate nodules. [ ] In 2008 I became member of the AUGER collaboration. I started taking the responsibility of the PMTs test station in Malargue. The test station was built to test the 1600 PMTs of the AUGER array. My duty was to recover the old system to make it suitable for the detector maintenance. I changed the old CAMAC system and substituted it by a new VME System. Actually we are working to new possible task of the station for the AUGER upgrade beyond I m also responsible for the Work Package 1, front end package (including the ADC), of the electronic upgrade of the collaboration to be installed in OTHER EXPERIENCES: Many years working in technology transfer context and University Governement. [1990] 3 months summer student contract at FERMILAB, USA National Laboratory. During the stay he worked on the development of a prototype of electromagnetic calorimeter based on scintillating tales. [1996] "IX National Seminary on nuclear and subnuclear physics" at Otranto. [1998] "Fifth school on non-accelerator Particle Physics" at ICTP, Trieste. [1999] Coordinator of ADI-aziende at Lecce, working group in Italian PhD association (ADI), to promote PhD degree out of University and to help relationship between academia and industry. [2000] National Coordinator of ADI-aziende [ ] Lecce delegate of INFN technology transfer Commission. [2004] Nominated member of INFN patent commission, made by 5 members, whose main task is to valuate the patent proposal of INFN researcher. [2004] Member, as expert, of the new INFN Technology Transfer Commission [2005] Elected member of the Academic Senate of the Lecce University. [2005] Nominated by Regione Puglia as referee for projects related to the 3.13 action of P.O.R (UE projects) [2005] Nominated member of the University construction board
5 [2006] Organized the participation of INFN together with CERN to the fair Innovaction at Udine, to illustrate the Technology Transfer projects from elementary particle physics. [2006] Nominated by Regione Puglia as referee for projects related to APQ SJ 008 ICT [2006] Nominated by Regione Puglia as member of the Evaluation Nucleus for the action 4.1 Help to the industrial system - action a) real services to industry [2006] Nominated by Regione Puglia as member of the technical-scientific committee for the environment. [2006] Organized the conference FRONTIER TECHNOLOGIES IN HEALTH from the elementary particle physics to the medical diagnosis: the experience of INFN and research and innovation in Puglia. [2007] Organized the participation of INFN together with CERN to the fair Innovaction at Udine, to illustrate the Technology Transfer projects from elementary particle physics. [2007] Nominated technical referent for the Salento University to organize the 2007 researcher night. [2007] Nominated member of the University planning board [2008] Reelected member of the Academic Senate of the Salento University. [2008] Nominated member for the Academic Senate of the Salento University budget commission. [2008] Technical coordinator of the project INTERREGIII IT PORT- Innovative Communication Technologies for harbor services for local development [2009] Nominated technical referent for the University of Salento to organize the 2007 researcher night [2013] Nominated member of INFN National Committee for Technological Transfer and to evaluate patent query TEACHING EXPERIENCES Very good experience in teaching Mechanics and Electromagnetism to Physicists, Engineers and Medical Assistants. Very good experience in teaching Electronics and Mechanic Laboratory to Physicists. [ ] Seminars on particle detection in the course of Physics for medicine, exercises for the Physics course for medical assistant at University of Siena. [ ] Exercises for the course of Electromagnetism for engineers of materials, laboratory assistance of electronics for engineers of the University of Lecce. [ ] Expert in Electromagnetism for Engineers of materials, member of examination commissions. [ ] Exercises for the course of experiment of electronics for the student in physics, member of examination commission at University of Lecce. [ ] Course of experiment of Electronics for students in physics, member of examination commissions, exercises of Electromagnetism for student of mathematics, teacher of the course of Mechanics for students in informatics engineering of University of Lecce. [ ] Course of computational laboratory for students in physics, exercises for the courses of laboratory of Mechanics, member of the examination commissions, for student of physics at University of Lecce. [ ] Course of computational laboratory for students in physics, exercises
6 for the courses of laboratory of Mechanics, member of the examination commissions, for student of physics at University of Lecce. [ ] Laboratory of electronics for students in physics, exercises for the courses of laboratory of Mechanics and Optics. Teacher of the course of applied physics for hospital nurse laurea of the University of Bari. [2013] Course of electromagnetism for students in Optic and Optometry LANGUAGES: - Very good knowledge of French and English. Good knowledge of Spanish and Portuguese. INFORMATICS KNOWLEDGES: Good knowledge of the operative systems MS-DOS, VMS, UNIX and LINUX. Good knowledge of FORTRAN, C, C++,MATLAB, LABVIEW, WORD and EXCEL. Lecce, , Giovanni Marsella
Very High Energy Gamma Ray Astronomy and Cosmic Ray Physics with ARGO-YBJ
Very High Energy Gamma Ray Astronomy and Cosmic Ray Physics with ARGO-YBJ Ivan DE MITRI Dipartimento di Fisica Università di Lecce and Istituto Nazionale di Fisica Nucleare Lecce,, ITALY On behalf of the
More informationHighlights from the ARGO-YBJ Experiment
Highlights from the ARGO-YBJ Experiment Ivan De Mitri University of Salento and Istituto Nazionale di Fisica Nucleare Lecce, Italy On behalf of the ARGO-YBJ Collaboration 12th International Conference
More informationPoS(RPC2012)011. Results from the ARGO-YBJ experiment. Roberto Iuppa for the ARGO-YBJ collaboration
Results from the ARGO-YBJ experiment University of Rome Tor Vergata INFN Sez.ne di Roma Tor Vergata E-mail: roberto.iuppa@roma2.infn.it The ARGO-YBJ experiment consists of a 5000 m 2 single layer of Resistive
More informationCosmic Ray Physics with ARGO-YBJ
Cosmic Ray Physics with ARGO-YBJ Ivan De Mitri University of Salento and Istituto Nazionale di Fisica Nucleare Lecce, Italy On behalf of the ARGO-YBJ Collaboration 4th Workshop on Air Shower Detection
More informationStatus of ARGO-YBJ: an overview
Status of ARGO-YBJ: an overview M. Iacovacci a for the ARGO-YBJ Collaboration a INFN and University of Napoli, Complesso Universitario MSA, Via Cintia, 80126 Napoli, Italy Within a Collaboration Agreement
More informationCosmic Ray Physics with ARGO-YBJ
Cosmic Ray Physics with ARGO-YBJ Ivan De Mitri University of Salento and Istituto Nazionale di Fisica Nucleare Lecce, Italy On behalf of the ARGO-YBJ Collaboration RICAP-13 Roma International Conference
More informationCURRICULUM VITAE (June 2011) Mehdi Khakian Ghomi
CURRICULUM VITAE (June 2011) Mehdi Khakian Ghomi Assist. Prof., Faculty of Nuclear Engineering and Physics Dept., Amirkabir Univ. of Tech. (Tehran Polytechnic), 15875-4413,Tehran, Iran. Office: +9821 64545235,
More informationPrimary cosmic ray mass composition above 1 PeV as measured by the PRISMA-YBJ array
as measured by the PRISMA-YBJ array Stenkin Yu.V. 1, 2, Alekseenko V.V. 1, Cui S.W. 4, He Ya.Yu. 4, Li B.B. 4, Ma X.H. 3, Shchegolev O.B. 1, Stepanov V.I. 1, Yanin Ya. 1,2, Zhao J. 3 1 - Institute for
More informationMeasurement of the angular resolution of the ARGO-YBJ detector
Measurement of the angular resolution of the ARGO-YBJ detector G. Di Sciascio and E. Rossi for the ARGO-YBJ Collaboration INFN, sez. di Napoli and Dip. di Scienze Fisiche dell Universitá, Napoli, Italy
More informationThe Gamma Large Area Space Telescope: GLAST
Chin. J. Astron. Astrophys. Vol.3 (2003), Suppl., 523 530 (http:/www.chjaa.org) Chinese Journal of Astronomy and Astrophysics The Gamma Large Area Space Telescope: GLAST Aldo Morselli 1 INFN Roma2 and
More informationPoS(ICRC2015)641. Cloud Monitoring using Nitrogen Laser for LHAASO Experiment. Z.D. Sun 1,Y. Zhang 2,F.R. Zhu 1 for the LHAASO Collaboration
Cloud Monitoring using Nitrogen Laser for LHAASO Experiment Z.D. Sun 1,Y. Zhang 2,F.R. Zhu 1 for the LHAASO Collaboration [1]School of Physical Science and Technology, Southwest Jiaotong University, Chengdu
More informationPublications of Francesco Arneodo: journal articles
Publications of Francesco Arneodo: journal articles Figure 1: Citation report from ISI Web of Science (IF=31.0) [1] E. Aprile et al., First Axion Results from the XENON100 Experiment, arxiv.org (submitted
More informationMeasurement of the Cosmic Ray Energy Spectrum with ARGO-YBJ
Measurement of the Cosmic Ray Energy Spectrum with ARGO-YBJ Ivan De Mitri ( on behalf of the ARGO-YBJ collaboration ) Dipartimento di Matematica e Fisica " E. De Giorgi", Universita del Salento, Lecce,
More informationCosmic Ray Physics with the ARGO-YBJ experiment
Cosmic Ray Physics with the ARGO-YBJ experiment Ivan De Mitri University of Salento and Istituto Nazionale di Fisica Nucleare Lecce, Italy On behalf of the ARGO-YBJ Collaboration Second Roma International
More informationThe early days of ground-based gamma-ray astronomy in France. Gerard Fontaine - Hillas symposium Heidelberg December
The early days of ground-based gamma-ray astronomy in France Gerard Fontaine - Hillas symposium Heidelberg December 10-12 2018 Timeline from 1986 to 2004 86 87 88 89 90 91 92 93 94 95 96 97 98 99 00 01
More informationPerformance of the RPCs for the ARGO detector operated at the YangBaJing laboratory (4300 m a.s.l.)
Nuclear Instruments and Methods in Physics Research A 508 (2003) 110 115 Performance of the RPCs for the ARGO detector operated at the YangBaJing laboratory (4300 m a.s.l.) C. Bacci a, K.Z. Bao b, F. Barone
More informationAugerPrime. Primary cosmic ray identification for the next 10 years. Radomír Šmída.
AugerPrime Primary cosmic ray identification for the next 10 years Radomír Šmída radomir.smida@kit.edu The Pierre Auger Observatory The primary goal is to study the most energetic cosmic rays Southern
More informationHadronic Interaction Studies with ARGO-YBJ
Hadronic Interaction Studies with ARGO-YBJ Ivan De Mitri University of Salento and Istituto Nazionale di Fisica Nucleare Lecce, Italy On behalf of the ARGO-YBJ Collaboration Hadron-Hadron & Cosmic Ray
More informationCalibration of large water-cherenkov Detector at the Sierra Negra site of LAGO
Calibration of large water-cherenkov Detector at the Sierra Negra site of LAGO A. Galindo a, E. Moreno b, E. Carrasco a, I. Torres a, a, for the LAGO Collaboration c a Instituto Nacional de Astrofísica,
More informationPoS(Extremesky 2011)036
Univ. Complutense of Madrid E-mail: marcos@gae.ucm.es The MAGIC (Major Atmospheric Gamma-ray Imaging Cherenkov) telescopes were designed to reach the lowest possible energy threshold using the ground-based
More informationEAS lateral distribution measured by analog readout and digital readout of ARGO-YBJ experiment
EAS lateral distribution measured by analog readout and digital readout of ARGO-YBJ experiment Jing Zhao Institute of High Energy Physics, Chinese Academy of Sciences Beijing China E-mail: jzhao@ihep.ac.cn
More informationNuclear Instruments and Methods in Physics Research A
Nuclear Instruments and Methods in Physics Research A 630 (20) 22 27 Contents lists available at ScienceDirect Nuclear Instruments and Methods in Physics Research A journal homepage: www.elsevier.com/locate/nima
More informationTiming calibration of the LHAASO-KM2A electromagnetic particle detectors
Timing calibration of the LHAASO-KMA electromagnetic particle detectors Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 149, China E-mail: lvhk@ihep.ac.cn Huihai He Institute of
More informationGAMMA-RAY ASTRONOMY: IMAGING ATMOSPHERIC CHERENKOV TECHNIQUE FABIO ZANDANEL - SESIONES CCD
GAMMA-RAY ASTRONOMY: IMAGING ATMOSPHERIC CHERENKOV TECHNIQUE COSMIC RAYS Discovered in 1912 by Victor Hess (Nobel Prize) Messengers from the non-thermal part of the Universe E < 15 ev: galactic E > 17
More informationResults from the analysis of data collected with a 50 m RPC carpet at YangBaJing
Nuclear Instruments and Methods in Physics Research A 456 (2000) 121}125 Results from the analysis of data collected with a 50 m RPC carpet at YangBaJing C. Bacci, K.Z. Bao, F. Barone, B. Bartoli, P. Bernardini,
More informationCurriculum Vitae. Reader-F: Institute of Physics, Bhubaneswar (Oct till date)
Curriculum Vitae Employment Reader-F: Institute of Physics, Bhubaneswar (Oct 2015 - till date) Fellow: Deutsches Elektronen-Synchrotron - DESY, Hamburg, Germany (Feb 2014 - Oct 2015) Post-doc: Institute
More informationThe MAGIC gamma detector
The MAGIC gamma detector Alessandro De Angelis Trieste, 1 july 2003 1 Outline The observational scenario Techniques to detect cosmic gammas Imaging Cherenkov and MAGIC Physics goals The role of INFN Udine/Trieste
More informationMeasurement of the CR e+/e- ratio with ground-based instruments
Measurement of the CR e+/e- ratio with ground-based instruments Pierre Colin Max-Planck-Institut für Physik CR Moon shadow MPP retreat - 21 January 2014 Cosmic ray electrons Observation: Above the atmosphere:
More informationCurriculum Vitae. Personal Data. Larissa Carlos de Oliveira Santos. Place, date Brasília-Brazil, June 26 th of 1984 of birth
Curriculum Vitae Personal Data Full Name Larissa Carlos de Oliveira Santos Place, date Brasília-Brazil, June 26 th of 1984 of birth Nationality Sex, Marital Stattus e-mail Online Lattes CV Brazilian Female,
More informationEnergy spectrum of cosmic protons and helium nuclei by a hybrid measurement at 4300 m a.s.l.*
Energy spectrum of cosmic protons and helium nuclei by a hybrid measurement at 4300 m a.s.l.* B. Bartoli 2,3 P. Bernardini 4,5 X. J. Bi( ) 1 I. Bolognino 6,7 P. Branchini 8 A. Budano 8 A. K. Calabrese
More informationGamma-Ray Astronomy with a Wide Field of View detector operated at Extreme Altitude in the Southern Hemisphere.
Gamma-Ray Astronomy with a Wide Field of View detector operated at Extreme Altitude in the Southern Hemisphere., S. Miozzi, R. Santonico INFN - Rome Tor Vergata, Italy E-mail: disciascio@roma.infn.it P.
More informationPress release. The engine of the Crab Nebula
Press release The engine of the Crab Nebula MAGIC telescopes observe a pulsar at the highest energies yet achieved and strongly challenge current theories for the emission. The pulsar at the heart of the
More informationAccurate Measurement of the Cosmic Ray Proton Spectrum from 100TeV to 10PeV with LHAASO
Accurate Measurement of the Cosmic Ray Proton Spectrum from 1TeV to 1PeV with LHAASO L.Q. Yin ab,, Z.Cao a, S.S.Zhang a, B.Y. Bi ab for the LHAASO Collaboration a Key Laboratory of Particle Astrophysics,
More informationMeasurement of the cosmic ray all-particle and light-component energy spectra with the ARGO- YBJ experiment
Journal of Physics: Conference Series PAPER OPEN ACCESS Measurement of the cosmic ray all-particle and light-component energy spectra with the ARGO- YBJ experiment To cite this article: Ivan De Mitri and
More informationPrimary CR Energy Spectrum and Mass Composition by the Data of Tunka-133 Array. by the Tunka-133 Collaboration
Primary CR Energy Spectrum and Mass Composition by the Data of Tunka-133 Array by the Tunka-133 Collaboration Tunka-HiSCORE: First results on all-particle spectrum by the Tunka-HiSCORE Collaboration combined
More informationThe TAIGA experiment - a hybrid detector for very high energy gamma-ray astronomy and cosmic ray physics in the Tunka valley
The TAIGA experiment - a hybrid detector for very high energy gamma-ray astronomy and cosmic ray physics in the Tunka valley N. Budnev, Irkutsk State University For the TAIGA collaboration The TAIGA experiment
More informationTHE MAGIC TELESCOPES. Major Atmospheric Gamma Imaging Cherenkov Telescopes
THE MAGIC TELESCOPES Observatorio del Roque de los Muchachos, La Palma (2200 m a.s.l.) System of two 17 m Cherenkov Telescopes for VHE γ-ray astronomy MAGIC-I operational since 2004, Stereo system since
More informationStatus and results from the Pierre Auger Observatory
April 15-19, 2007 Aspen, Colorado Status and results from the Pierre Auger Observatory Lorenzo Perrone for the Auger Collaboration Università del Salento and INFN Lecce Italy The Physics Case: highest
More informationThe Extreme Energy Events experiment: The future
The Extreme Energy Events experiment: The future for the Extreme Energy Events collaboration Present status 50 telescopes at High Schools + 2 telescopes at CERN + 4 at INFN Units Total: 56 telescopes +
More informationCurriculum Vitae Manfred KRAMMER
Curriculum Vitae Manfred KRAMMER Date of birth: Birthplace: Citizenship: orcid.org/0000-0003-2257-7751 June 7, 1961 Vienna Austria 1981-1987 Study of Physics at the University of Technology in Vienna.
More informationCurriculum Vitae Duncan L. Carlsmith
February 2012 Curriculum Vitae Duncan L. Carlsmith Contact information Dept. of Physics, 1150 University Ave, Madison, WI 53706 (608) 262-2485 (WI office), (608) 263-0800 (WI FAX), +41 79 233 34 98 (Swiss
More informationCherenkov Telescope Array Status Report. Salvatore Mangano (CIEMAT) On behalf of the CTA consortium
Cherenkov Telescope Array Status Report Salvatore Mangano (CIEMAT) On behalf of the CTA consortium Outline Very-High-Energy Gamma-Ray Astronomy Cherenkov Telescope Array (CTA) Expected Performance of CTA
More informationTeV energy physics at LHC and in cosmic rays
Vulcano 2016 TeV energy physics at LHC and in cosmic rays Anatoly Petrukhin National Research Nuclear University MEPhI (Moscow Engineering Physics Institute), Russia Many physicists dream and hope to find
More informationStudy of Performance Improvement for Air Shower Array with Surface Water Cherenkov Detectors
Study of Performance Improvement for Air Shower Array with Surface Water Cherenkov Detectors, a K. Hibino, b T. K. Sako, cd T. Asaba, e Y. Katayose e and M. Ohnishi c a College of Industrial Technology,
More informationarxiv: v1 [astro-ph.im] 19 Aug 2015
arxiv:158.575v1 [astro-ph.im] 19 Aug 15 Performance of the MAGIC telescopes after the major upgrade University of Łódź, PL-96 Lodz, Poland, IFAE, Campus UAB, E-819 Bellaterra, Spain E-mail: jsitarek@uni.lodz.pl
More informationAntifreeze design for Muon Detector of LHAASO
Antifreeze design for Muon Detector of LHAASO Shaohui Feng,(Institute of High Energy Physics, Chinese Academy of Sciences), for the LHAASO Collaboration E-mail: fengsh@ihep.ac.cn Gang Xiao E-mail: xiaog@ihep.ac.cn
More informationParameters Sensitive to the Mass Composition of Cosmic Rays and Their Application at the Pierre Auger Observatory
WDS'12 Proceedings of Contributed Papers, Part III, 137 141, 2012. ISBN 978-80-7378-226-9 MATFYZPRESS Parameters Sensitive to the Mass Composition of Cosmic Rays and Their Application at the Pierre Auger
More informationLATTES Large Array Telescope to Tracking Energetic Sources
LATTES Large Array Telescope to Tracking Energetic Sources Ronald Cintra Shellard CBPF 1 Lattes LATTES Ochiallini 2 LATTES Lattes started as a name and a project submitted to CNPq at least in 2009: Very
More informationPoS(ICRC2015)1237. Using UV-pass filters for bright Moon observations with MAGIC
Using UV-pass filters for bright Moon observations with MAGIC a, J. Cortina a, R. García a, J.Herrera b, M. Manganaro b, A. Moralejo a, J. Rico a and M. Will b for the MAGIC collaboration a Institut de
More informationCosmic Rays - in Poland
Cosmic Rays - in Poland Maria Giller - University of Łódź Institutions: 1. Institute of Nuclear Physics Kraków, 2. University of Łódź, 3. Andrzej Sołtan Institute for Nuclear Studies - - Cosmic Ray group
More information9/27 JUNE 2003 SUMMER STAGE PARTICLES REVELATION THROUGH CERENKOV AND SCINTILLATION COUNTER AND THE CEBAF EXPERIMENT
9/27 JUNE 2003 SUMMER STAGE PARTICLES REVELATION THROUGH CERENKOV AND SCINTILLATION COUNTER AND THE CEBAF EXPERIMENT Students: Riccardo Falcione, Elisa Paris Liceo Scientifico Statale Farnesina Tutor:
More informationAldo Morselli, INFN & Università di Roma Tor Vergata, 1. Scineghe07. Aldo Morselli
Aldo Morselli, INFN & Università di Roma Tor Vergata, aldo.morselli@roma2.infn.it 1 Scineghe07 Aldo Morselli Proceedings in Frascati Physics series Deadline 25 of July 8 pages (4 pages for posters ) in
More informationHAWC Observation of Supernova Remnants and Pulsar Wind Nebulae
HAWC Observation of Supernova Remnants and Pulsar Wind Nebulae a, and H. Zhou a for the HAWC Collaboration b a Department of Physics, Michigan Technological University 1400 Townsend Drive, Houghton, MI,
More informationCurriculum Vitae. Grazia Luparello
Curriculum Vitae Grazia Luparello Personal Data: Surname Luparello Name Grazia Address via Portofino 30/42, 10135 Torino Telephone +39 0113910032 Mobile +39 3920182152 E-mail luparell@to.infn.it Nationality
More informationLatest news from the High Altitude Water Cherenkov Observatory
Journal of Physics: Conference Series PAPER OPEN ACCESS Latest news from the High Altitude Water Cherenkov Observatory To cite this article: A González Muñoz and HAWC Collaboration 2016 J. Phys.: Conf.
More information(Future) Experiments for gamma-ray detection
(Future) Experiments for gamma-ray detection K. Ragan McGill University ISSS (GSSI) June 2017 Cosmic Ray Physics in Space K. Ragan ISSS Jun 2017 1 Menu Antipasti Introduction & motivation: why study GeV/TeV
More informationDetectors for astroparticle physics
Detectors for astroparticle physics Teresa Marrodán Undagoitia marrodan@physik.uzh.ch Universität Zürich Kern und Teilchenphysik II, Zürich 07.05.2010 Teresa Marrodán Undagoitia (UZH) Detectors for astroparticle
More informationAn introduction to AERA. An Introduction to the Auger Engineering Radio Array (AERA)
An Introduction to the Auger Engineering Radio Array (AERA) Amin Aminaei 1 for the Pierre Auger Collaboration 2,3 Abstract The new generation of radio-telescope arrays with digital interferometry is able
More informationVasily Prosin (Skobeltsyn Institute of Nuclear Physics MSU, MOSCOW) From TAIGA Collaboration
The Results and Perspectives of Cosmic Rays Mass Composition Study with EAS Arrays in the Tunka Valley Vasily Prosin (Skobeltsyn Institute of Nuclear Physics MSU, MOSCOW) From TAIGA Collaboration TAUP-2015,
More informationHigh-energy Gamma Rays detection with the AMS-02 electromagnetic calorimeter. F. Pilo for the AMS-02 ECAL Group INFN Sezione di Pisa, Italy
Frascati Physics Series Vol. 58 (2014) Frontier Objects in Astrophysics and Particle Physics May 18-24, 2014 High-energy Gamma Rays detection with the AMS-02 electromagnetic calorimeter F. Pilo for the
More informationPerformance of the MAGIC telescopes under moonlight
Performance of the MAGIC telescopes under moonlight and P. Colin for the MAGIC collaboration Institut de Fisica d Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, 089
More informationMass Composition Study at the Pierre Auger Observatory
OBSERVATORY Mass Composition Study at the Pierre Auger Observatory Laura Collica for the Auger Milano Group 4.04.2013, Astrosiesta INAF Milano 1 Outline The physics: The UHECR spectrum Extensive Air Showers
More informationMicromegas detectors & the Great Pyramid. S. Procureur
Micromegas detectors & the Great Pyramid S. Procureur Tech Transfer Workshop January 12 th, 2018 CONTENT Introduction Micromegas and CLAS12 First muon instruments @ Saclay ScanPyramids: preparation and
More informationGamma-Ray Astronomy With Ground Based Arrays: Results and Future Perspectives
Gamma-Ray Astronomy With Ground Based Arrays: Results and Future Perspectives Eckart Lorenz (MPI-Munich) OVERVIEW INTRODUCTION THE GENERAL CONCEPT CURRENT EXPERIMENTS AND RESULTS COMPARISON WITH OTHER
More informationTHE AMS RICH COUNTER
THE AMS RICH COUNTER G. BOUDOUL ISN Grenoble ISN-GRENOBLE 1 The AMS RICH collaboration: Bologna, Grenoble, Lisbon, Madrid, Maryland, Mexico 2 The AMS collaboration UNAM S.C.C. TING (MIT), PI 3 AMS Scientific
More informationResults from the Pierre Auger Observatory
Thirteenth Marcel Grossmann Meeting - MG13 Stockholm, July 1-7, 2012 Results from the Pierre Auger Observatory Ivan De Mitri Università del Salento and INFN - Lecce, Italy for the Pierre Auger Collaboration
More informationTHE PATH TOWARDS THE CHERENKOV TELESCOPE ARRAY OBSERVATORY. Patrizia Caraveo
THE PATH TOWARDS THE CHERENKOV TELESCOPE ARRAY OBSERVATORY Patrizia Caraveo 5 y integration of the gamma-ray sky Optical +TeV The TeV sky > 40, Active Galactic Nuclei (Blazars) AGN TeV by electrons (strong
More informationWater Cherenkov Detector installation by the Vertical Muon Equivalent technique
Water Cherenkov Detector installation by the Vertical Muon Equivalent technique UNIVERSIDAD CENTRAL DE VENEZUELA and UNIVERSIDAD SIMÓN BOLÍVAR, VENEZUELA E-mail: giskya@gmail.com Haydn Barros UNIVERSIDAD
More informationUHE Cosmic Rays and Neutrinos with the Pierre Auger Observatory
UHE Cosmic Rays and Neutrinos with the Pierre Auger Observatory Gonzalo Parente Bermúdez Universidade de Santiago de Compostela & IGFAE for the Pierre Auger Collaboration Particle Physics and Cosmology
More informationWelcome to CERN! Dr. Yannis PAPAPHILIPPOU ACCELERATOR AND BEAMS Department. 05 Novembre
Welcome to CERN! Dr. Yannis PAPAPHILIPPOU ACCELERATOR AND BEAMS Department 05 Novembre 2003 1 1949-1950: First ideas for creating a European laboratory in physics 1952: Foundation of the European Council
More informationPoS(ICRC2017)168. PSD performance and charge reconstruction with DAMPE
PSD performance and charge reconstruction with DAMPE 1 Yongjie Zhang 1,2, Tiekuang Dong 3, Pengxiong Ma 2,3, Yuhong Yu 1, Paolo Bernardini 4,5, for the DAMPE collaboration 1 Institute of Modern Physics,
More informationTAIGA-HiSCORE results from the first two operation seasons
TAIGA-HiSCORE results from the first two operation seasons http://taiga experiment.info/ Presenter: Igor Yashin GA 299: M. Tluczykont et al. for the TAIGA Collaboration TAIGA collaboration see N. Budnev,
More informationFeasibility of VHE gamma ray detection by an array of imaging atmospheric Cherenkov telescopes using the fluorescence technique
Feasibility of VHE gamma ray detection by an array of imaging atmospheric Cherenkov telescopes using the fluorescence technique J.L. Contreras, J. Rosado, F. Arqueros,, J.A. Barrio and M. Nievas Departamento
More informationJob Announcement for an Assistant Professor at the Institute of Space and Astronautical Science, the Japan Aerospace Exploration Agency
Job Announcement for an Assistant Professor at the Institute of Space and Astronautical Science, the Japan Aerospace Exploration Agency The Japan Aerospace Space Exploration Agency (JAXA) is seeking to
More informationStatus and Perspectives of the LAGO Project
Status and Perspectives of the LAGO Project 5 th Workshop on Air Shower Detection at High Altitude Paris, France Édgar F. Carrera ecarrera@usfq.edu.ec (for the LAGO Collaboration) Universidad San Francisco
More informationDetermination of parameters of cascade showers in the water calorimeter using 3D-distribution of Cherenkov light
in the water calorimeter using 3D-distribution of Cherenkov light 1, A.G. Bogdanov, S.S. Khokhlov, V.A. Khomyakov, V.V. Kindin, A.A. Petrukhin, V.V. Shutenko, I.I. Yashin National Research Nuclear University
More informationTHE PATH TOWARDS THE CHERENKOV TELESCOPE ARRAY OBSERVATORY. Patrizia Caraveo
THE PATH TOWARDS THE CHERENKOV TELESCOPE ARRAY OBSERVATORY Patrizia Caraveo 1 st Interaction: X 0 40 g/cm 2 pair = 9/7 X 0 50 g/cm 2 X = X A e h/h0 and X A 10 3 g/cm 2 h pair = h 0 ln(x A / pair ) 20 km
More informationMeasurement of the cosmic ray spectrum and chemical composition in the ev energy range
Measurement of the cosmic ray spectrum and chemical composition in the - 18 ev energy range Andrea Chiavassa 1, 1 Dipartimento di Fisica dell Universitá degli Studi di Torino & INFN Via Pietro Giuria 1,
More informationThe AUGER Experiment. D. Martello Department of Physics University of Salento & INFN Lecce. D. Martello Dep. of Physics Univ. of Salento & INFN LECCE
The AUGER Experiment D. Martello Department of Physics University of Salento & INFN Lecce The Pierre Auger Collaboration Argentina Australia Bolivia Brazil Croatia Czech Rep. France Germany Italy Mexico
More informationMeasurement of the Solar Magnetic Field effect on cosmic rays using the Sun shadow observed by the ARGO-YBJ experiment
Measurement of the Solar Magnetic Field effect on cosmic rays using the Sun shadow observed by the ARGO-YBJ experiment Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, CAS, Beijing
More informationThe DISP analysis method for point-like or extended γ source searches/studies with the MAGIC Telescope
9th International Cosmic Ray Conference Pune (5), 11 16 The DISP analysis method for point-like or extended γ source searches/studies with the MAGIC Telescope E. Domingo-Santamaría a, J. Flix a, V. Scalzotto
More informationSearch for Astrophysical Neutrino Point Sources at Super-Kamiokande
Search for Astrophysical Neutrino Point Sources at Super-Kamiokande Yusuke Koshio for Super-K collaboration Kamioka, ICRR, Univ. of Tokyo LNGS, INFN Super-Kamiokande detector Recent results of search for
More informationThe influence of the global atmospheric properties on the detection of UHECR by EUSO on board of the ISS
The influence of the global atmospheric properties on the detection of UHECR by EUSO on board of the ISS C. Berat, D. Lebrun, A. Stutz, E. Plagnol To cite this version: C. Berat, D. Lebrun, A. Stutz, E.
More informationHigh energy neutrino astronomy with the ANTARES Cherenkov telescope
High energy neutrino astronomy with the ANTARES Cherenkov telescope P.Vernin CEA/Irfu/SPP On behalf of the ANTARES collaboration IWARA 2009 Conference Maresias, Sao Paulo, Brazil, 4-8/10/2009 i r f u saclay
More informationPoS(ICRC2015)1001. Gamma Hadron Separation using Pairwise Compactness Method with HAWC
Gamma Hadron Separation using Pairwise Compactness Method with HAWC a and Stefan Westerhoff a for the HAWC Collaboration b a Department of Physics and WIPAC, University of Wisconsin-Madison, Madison, WI,
More informationUC Irvine UC Irvine Previously Published Works
UC Irvine UC Irvine Previously Published Works Title Study of the Shadows of the Moon and the Sun with VHE Cosmic Rays Permalink https://escholarship.org/uc/item/7xp0j97v Authors Atkins, R Benbow, W Berley,
More informationNeutral particles energy spectra for 900 GeV and 7 TeV p-p collisions, measured by the LHCf experiment
Neutral particles energy spectra for 900 GeV and 7 TeV p-p collisions, measured by the LHCf experiment Raffaello D Alessandro 1 Department of Physics Università di Firenze and INFN-Firenze I-50019 Sesto
More informationHAWC and the cosmic ray quest
HAWC and the cosmic ray quest J.C. Arteaga-Velázquez for the HAWC Collaboration Instituto de Física y Matemáticas, Universidad Michoacana, Mexico Structure of the talk: 1) The HAWC gamma-ray observatory
More informationGamma/Proton separation study for the LHAASO-WCDA detector
Gamma/ separation study for the LHAASO-WCDA detector Wenying Liao [1], Min Zha [2], Wande Fan [1], Chunxu Yu [1] and Minjun Chen [2] on behalf of LHAASO collaboration [1]University of Nankai, Tianjin 371,
More informationGamma-ray Astrophysics
Gamma-ray Astrophysics AGN Pulsar SNR GRB Radio Galaxy The very high energy -ray sky NEPPSR 25 Aug. 2004 Many thanks to Rene Ong at UCLA Guy Blaylock U. of Massachusetts Why gamma rays? Extragalactic Background
More information(High-Energy) Cosmic Rays
APPEC Town Meeting Roadmap ( Considerations ) Discussion (High-Energy) Cosmic Rays Paris, 6-7 April 2016 Andreas Haungs Karlsruhe Institute of Technology Petr Tinyakov Université Libre de Bruxelles petr.tiniakov@ulb.ac.be
More informationRECENT RESULTS FROM CANGAROO
RECENT RESULTS FROM CANGAROO MASAKI MORI FOR THE CANGAROO TEAM Institute for Cosmic Ray Research, University of Tokyo 5-1-5 Kashiwanoha, Kashiwa, 277-8582 Chiba, Japan E-mail: morim@icrr.u-tokyo.ac.jp
More informationTEV GAMMA RAY ASTRONOMY WITH VERITAS
1 TEV GAMMA RAY ASTRONOMY WITH VERITAS Tülün Ergin (U. of Massachusetts Amherst, MA) on behalf of the VERITAS Collaboration 2 Contents The VERITAS Experiment Results and the Performance Galactic Sources
More informationThe Cosmic Ray Mass Composition in the Energy Range ev measured with the Tunka Array: Results and Perspectives
Nuclear Physics B (Proc. Suppl.) 190 (2009) 247 252 www.elsevierphysics.com The Cosmic Ray Mass Composition in the Energy Range 10 15 10 18 ev measured with the Tunka Array: Results and Perspectives V.V.
More informationPhysics Results with the ARGO-YBJ Experiment. Tristano Di Girolamo Università di Napoli Federico II INFN Sezione di Napoli
Physics Results with the ARGO-YBJ Experiment Tristano Di Girolamo Università di Napoli Federico II INFN Sezione di Napoli Napoli, 21 Febbraio 2013 Collaboration between: The ARGO-YBJ experiment Istituto
More informationVariable atmospheric transparency studies for the MAGIC telescopes
technische universität dortmund Variable atmospheric transparency studies for the MAGIC telescopes Nikola Strah (1), Dario Hrupec (2) for the MAGIC collaboration (1) Astroparticle physics group, Technische
More informationPhilip von Doetinchem
Philip von Doetinchem Institution: Physics & Astronomy Department, University of Hawaii at Manoa Address: 2505 Correa Rd, Honolulu, HI 98622, USA Phone: +1-808-956-3719 Email: philipvd@hawaii.edu Homepage:
More informationDr. David Michael South
Dr. David Michael South ATLAS, H1, LHeC and DPHEP Collaborations July 2017 Date of Birth: 18.01.1977 Marital Status: Married Languages: English, German david.south@desy.de www.desy.de/ southd Employment
More informationUltra- high energy cosmic rays
Ultra- high energy cosmic rays Tiina Suomijärvi Institut de Physique Nucléaire Université Paris Sud, Orsay, IN2P3/CNRS, France Atélier CTA, IAP, Paris, 30-31 June 2014 Outline Pierre Auger Observatory:
More informationAGIS (Advanced Gamma-ray Imaging System)
AGIS (Advanced Gamma-ray Imaging System) Seth Digel, Stefan Funk and Hiro Tajima SLAC National Accelerator Laboratory Kavli Institute for Particle Astrophysics and Cosmology Outline AGIS project and status
More information