The HiSCORE Detector. HAP Topic 4 Workshop Jan th Rayk Nachtigall. Karlsruhe January 25th
|
|
- Egbert Miles
- 5 years ago
- Views:
Transcription
1 The HiSCORE Detector HAP Topic 4 Workshop Jan th 2013 Rayk Nachtigall Karlsruhe January 25th
2 Overview - Physics motivation - The HiSCORE detector - Signal processing - Physics potentials in γ-ray astronomy - Current state and plans 2
3 HiSCORE The Hundred*i Square-km Cosmic ORigin Explorer Cosmic-rays: 100 TeV < EC R < 1 EeV Gamma-rays: Eγ > 10 TeV, up to PeV, ultra-high energy regime Particle physics: beyond LHC range Concept: non-imaging air Cherenkov technique Large area: up to few 100 km² 2011AdSpR T, astro-ph/ Large Field of view: ~ 0.6 sr
4 Physics motivations 4
5 ara ys Physics motivations spectroscopy Anisotropies G am m Gamma-ray spectra Highest and morphology acceleration energies Diffuse Gamma-ray Diffuse emission Emission (Galaxy, local supercluster) C os m Cosmic-ray Origin of cosmic Origin of rays cosmic rays Nonstandard Propagation Propagation Cosmic-ray Anisotropy Sub-knee pre-ankle Spectral fine-structure NucleonNucleon interaction Particle acceleration Dark matter Particle physics 5 ic -r ay s
6 Cosmic rays HiSCORE Adapted from Donato & Medina-Tanco 2008 Spectrum&composition in transition range Galactic / extragalactic origin 6
7 Tevatron sky TeV Gammarays: E > 100 GeV 7
8 Pevatron sky? Where are the cosmic ray pevatrons? 8
9 Accessing the pevatron sky: large area The HiSCORE detector 9
10 The HiSCORE detector How to achieve large effective area? Imaging air Cherenkov telescopes: O(1000) channels / km² Non-imaging air Cherenkov technique: O(100) channels / km² 10 Picture: Serge Brunier
11 The HiSCORE detector How to achieve large effective area? Imaging air Cherenkov telescopes: O(1000) channels / km² Non-imaging air Cherenkov technique: O(100) channels / km² Air shower Cherenkov light cone 11 Picture: Serge Brunier
12 The HiSCORE detector Picture: Serge Brunier m
13 The HiSCORE detector Picture: Serge Brunier m
14 The HiSCORE detector 0.5 m² station area: E thr Readout: GHz sampling 1ns time synch. Picture: Serge Brunier m
15 The HiSCORE detector 15
16 The HiSCORE detector WinstonControl Cone Station 10 segments of slow control with ALANODMEGA 4300 UP Arduino 2562 increase light collecting DAQ interface & station areaguruplug PC 4x 16
17 The HiSCORE detector 17
18 The HiSCORE detector Winston Cone 10 segments of ALANOD 4300 UP increase light collecting area 4x 18
19 The HiSCORE detector 19
20 The HiSCORE detector Winston ET 9352KB Cone 8 PMT with 6 stages 10 segments of 4 nominal gain kV 4300 UP PHQ9352 divider base increase lightwith collecting on area 4xHV generation board readout of anode & 5th dynode 20
21 The HiSCORE detector 21
22 The HiSCORE detector Winston Cone Readout trigger board with clipped-sum-trigger 10 segments of ALANOD 4300 UP DRS4 based sampling increase light collecting 1 GS/s area sampling 4x currently Evaluation Board V3 22
23 Further component alternatives & developments MSU trigger boards (DRS4 based in prep.) PMT & divider bases ISU box mechanics 23
24 Signal Processing 24
25 Signal Processing 25
26 Signal Processing 26
27 Signal Processing D. Hampf, PhD thesis 27
28 Signal Processing 28
29 Signal Processing 29
30 Signal Processing 30
31 Physics potential of HiSCORE (gamma-ray astronomy) 31
32 Opening the Pevatron range 32
33 Opening the Pevatron range IceCube HAWC CTA 33 LHAASO
34 Opening the Pevatron range 34
35 HiSCORE current status and plans 35
36 Helmholtz Russia Joint Research Group HRJRG U. Hamburg KIT Desy Zeuthen Hamburg Tunka Cosmic ray experiment INR Moscow MSU Moscow ISU Irkutsk 36
37 First HiSCORE prototype deployed HiSCORE prototype Tunka Tunka-133 detector station First HiSCORE Prototype April 2012 FIRST LIGHT 37
38 Helmholtz Alliance for Astroparticle Physics PAO letter of intent written, waiting for decision small array (5 stations) synergy with infill SD and FD expected 10 cross events per day from arxiv:
39 Summary & outlook HiSCORE goals: Ultra-high energy gamma-ray observation window Cosmic ray physics from 100 TeV to 1 EeV Particle physics beyond LHC energy range Activities: 3 stations since April 2012 small PAO 2013/14 Engineering array (1 km²), HiSCORE-EA: Start 2013 st Potential for 1 physics results 39
40 Thank you! 40
41 Backup slides 41
42 Tunka site exposure map Tunka site exposure map Field of view: π steradian 42
43 Tunka site exposure map H.E.S.S. SCAN HiSCORE scan normal mode Tunka site exposure map First H.E.S.S. Galactic plane scan 43 Field of view: π steradian
44 Tunka site exposure map 44 Det ect or axi st iltin g HiSCORE scan normal mode
45 Tunka site exposure map 45 Det ect or axi st iltin g H.E.S.S. SCAN HiSCORE scan normal mode
46 Reconstruction Extract PMT signal parameters Preliminary shower core position (cog) Preliminary direction (time plane fit) 46 Improved core position: light distribution function (LDF) fitting Improved direction: arrival time model Fit of signal widths Simulated Cherenkov signal
47 Direction reconstruction >3 stations: model fit adapted from Stamatescu et al. 2008, Parametrization of time-delay dt at detector position 47
48 Direction reconstruction >3 stations: model fit adapted from Stamatescu et al. 2008, Parametrization of time-delay dt at detector position r: Distance from shower core to detector Shower height in km Slope of atmospheric refractive index Zenith angle 48
49 Direction reconstruction 49
50 Energy reconstruction Particle energy: Q220 = Value of LDF at 220m Q220 50
51 Energy reconstruction 51 Particle energy: Q220 = Value of LDF at 220m
52 Cosmic rays Adapted from Donato & Medina-Tanco 2008 Gammas from Galactic Cosmic rays: Eγ ~ ECR/10 52
53 Shower depth reconstruction Time model method: one free parameter in arrival time model LDF method: Depth from LDF slope, Q50/Q220 Width method: Depth from signal width 53
54 Shower depth 54 Depth of shower maximum
55 Shower depth bias Systematic bias LDF & widths : sensitive to whole shower Large overestimation for heavy particles (long tails) Timing : sensitive to specific point (edge time) Small overestimation for heavy particles 55
56 Particle separation 56
57 Particle separation (1) Lighter particles develop Higher up in atmosphere 57
58 Particle separation (2) Systematic difference Between width and timing Depths 58
59 Particle separation (3) Systematic difference Cherenkov signal rise times 59
60 The HiSCORE detector Lateral Cherenkov Photon Distribution How to achieve large effective area? Imaging air Cherenkov telescopes: O(1000) channels / km² Non-imaging air Cherenkov technique: O(100) channels / km² Air shower Cherenkov light cone 60 Picture: Serge Brunier
61 Lateral Cherenkov Photon Distribution 61
62 Lateral Cherenkov Photon Distribution Want large area Want a few stations In inner light pool ~ m spacing 62
63 Lateral Cherenkov Photon Distribution Want large area Want a few stations In inner light pool ~ m spacing Low photon density: Need large collector area 0.5 m² per station 63
64 HRJRG-303 Helmholtz Russia Joint Research Group Measurements of Gamma Rays and Charged Cosmic Rays in the Tunka-Valley in Siberia by Innovative New Technologies 04/ /2015 G. Rubtsov, I. Tkatchev (INR) A. Konstantinov, L. Kuzmichev (MSU) R. Vasilyev, N. Budnev (ISU) R. Wischnewski, C. Spiering (DESY) F. Schröder, A. Haungs (KIT) M. Tluczykont, D. Horns (U. Hamburg) 64 HiSCORE and Radio Tunka Innovation Proof-of-principle Synergies
65 Helmholtz Russia Joint Research Group HRJRG Hamburg Tunka Cosmic ray experiment 1 km² dense array Energy threshold 1015 ev core position resolution ~ 10 m energy resolution ~ 15% Xmax resolution< 25 g cm-2 65
66 References [HS1] [HS2] [HS3] [HS4] [HS5] [HS6] M. Tluczykont, D. Hampf, D. Horns, et al. (2011), Adv. Sp. Res. 48, 1935 D. Hampf (2012), PhD thesis, University of Hamburg M. Tluczykont, T. Kneiske, D. Hampf & D. Horns (2009), Proc. of the ICRC 2009, arxiv e-print (arxiv: v1) D. Hampf, M. Tluczykont & D. Horns (2009), Proc. of the ICRC 2009, arxiv e-print (arxiv: v1) M. Tluczykont, D. Hampf, D. Horns, et al., HiSCORE, in prep. D. Hampf, M. Tluczykont, D. Horns, HiSCORE reco, in prep. [Tunka133] Berezhnev S F, Besson D, Korobchenko A V et al The Tunka-133 EAS Cherenkov light array: status of 2011 NIM A DOI : /j.nima Preprint astro-ph.he/ [Hec1998] [Ber2008] [Hen1994] [Hör2003] [Abd2007] 66 D. Heck, J. Knapp, J.N. Capdevielle, G. Schatz, and T. Thouw, Report FZKA 6019 (1998), K. Bernlöhr (2008), astrop-ph preprint, arxiv: V. Henke (1994), Diploma thesis, University of Hamburg J.R. Hörandel, Astropart. Phys., 19, 193 (2003) Abdo A A, Allen B, Berley D et al Astrophys. J. 658 L33 L36
HiSCORE. M. Tluczykont for the HiSCORE Collaboration. Astroteilchenphysik in Deutschland Zeuthen, 09/2012. Sky above Tunka valley. HiSCORE.
Measurements of Gamma Rays and Charged Cosmic Rays in the Tunka-Valley in Siberia by Innovative New Technologies HRJRG 303 Sky above Tunka valley HiSCORE Detector Taiga Frozen Irkut river Irkut river HiSCORE
More informationHiSCORE. M. Tluczykont for the HiSCORE Collaboration
Measurements of Gamma Rays and Charged Cosmic Rays in the Tunka-Valley in Siberia by Innovative New Technologies HRJRG 303 Sky above Tunka valley HiSCORE Detector Taiga Frozen Irkut river Irkut river HiSCORE
More informationStatus of the HiSCORE Project
Status of the HiSCORE Project M. Tluczykont, D. Horns Tunka-HiSCORE, TAIGA HiSCORE Detector 26.05.2014 martin.tluczykont@physik.uni-hamburg.de Physics motivations & The HiSCORE concept Status of the 9-station
More informationAstroparticle and particle physics with HiSCORE
Astroparticle and particle physics with HiSCORE Martin Tluczykont for the HiSCORE group D. Horns, D. Hampf, R. Nachtigall, U. Einhaus, M. Kunnas, T. Kneiske Institut für Experimentalphysik, University
More informationMulti-TeV to PeV Gamma Ray Astronomy
Multi-TeV to PeV Gamma Ray Astronomy Motivation and Strategies Martin Tluczykont The Future of Research on Cosmic Gamma Rays, La Palma, August 2015 VHE-UHE Gamma-ray astronomy Multi-TeV to PeV Gamma rays
More informationTeV to PeV Gamma-ray Astronomy with TAIGA
TeV to PeV Gamma-ray Astronomy with TAIGA http://taiga-experiment.info/ M. Tluczykont for the TAIGA Collaboration Marcel-Grossmann-Meeting 2018, Roma TAIGA collaboration Skobeltsyn Institute of Nuclear
More informationThe Tunka-Rex Experiment for the Detection of the Air- Shower Radio Emission
The Tunka-Rex Experiment for the Detection of the Air- Shower Radio Emission a) Y. Kazarina 1, P.A. Bezyazeekov 1, N.M. Budnev 1, O.A. Gress 1, A. Haungs 2, R.Hiller 2, T. Huege 2, M. Kleifges 3, E.N.
More informationThe ground-based wide-angle gammaray and cosmic-ray experiment. HiSCORE
The ground-based wide-angle gammaray and cosmic-ray experiment HiSCORE Martin Tluczykont @ COSPAR 2010, Bremen The ground-based wide-angle gammaray and cosmic-ray experiment HiSCORE Martin Tluczykont,
More informationThe TAIGA experiment: from cosmic ray to gamma-ray astronomy in the Tunka valley. N.Budnev, Irkutsk State University for the TAIGA - collaboration
The TAIGA experiment: from cosmic ray to gamma-ray astronomy in the Tunka valley. N.Budnev, Irkutsk State University for the TAIGA - collaboration TAIGA collaboration S.F. Berezhnev 1, N.M. Budnev 2, M.
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 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 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 informationThe Pierre Auger Observatory Status - First Results - Plans
The Pierre Auger Observatory Status - First Results - Plans Andreas Haungs for the Pierre Auger Collaboration Forschungszentrum Karlsruhe Germany haungs@ik.fzk.de Andreas Haungs Pierre Auger Observatory
More informationarxiv: v1 [astro-ph.he] 8 Apr 2015
Physics Procedia 00 (2015) 1 Physics Procedia www.elsevier.com/locate/procedia 13th International Conference on Topics in Astroparticle and Underground Physics Cosmic Rays from the Knee to the Ankle arxiv:1504.01859v1
More informationarxiv: v1 [astro-ph.he] 28 Jan 2013
Measurements of the cosmic ray spectrum and average mass with IceCube Shahid Hussain arxiv:1301.6619v1 [astro-ph.he] 28 Jan 2013 Abstract Department of Physics and Astronomy, University of Delaware for
More informationLatest results and perspectives of the KASCADE-Grande EAS facility
Latest results and perspectives of the KASCADE-Grande EAS facility 29/6-2/7/2010, Nantes, France Andreas Haungs 1 Motivation KASCADE-Grande Knee EeV PeV g-eg? Radio?! KASCADE 10 15-10 17 ev: Origin of
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 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 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 informationAir Shower Measurements from PeV to EeV
Air Shower Measurements from PeV to EeV Andreas Haungs haungs@ik.fzk.de James L. Pinfold August 2006 TeV workshop Madison, US Andreas Haungs 1 Cosmic Rays around the knee(s) EeV PeV Knee 2 nd Knee? Ralph
More informationStatus KASCADE-Grande. April 2007 Aspen workshop on cosmic ray physics Andreas Haungs 1
Status KASCADE-Grande April 2007 Aspen workshop on cosmic ray physics Andreas Haungs 1 Cosmic Rays around the knee(s) Astrophysical questions for this energy range: (1 st ) knee Knee position Composition
More informationPoS(ICRC2017)756. Commissioning the joint operation of the wide angle timing HiSCORE Cherenkov array with the first IACT of the TAIGA experiment
Commissioning the joint operation of the wide angle timing HiSCORE Cherenkov array with the first IACT of the TAIGA experiment,1, I. Astapov 9, P. Bezyazeekov 2, V. Boreyko 10, A. Borodin 10, M. Brueckner
More informationUltra High Energy Cosmic Rays What we have learnt from. HiRes and Auger. Andreas Zech Observatoire de Paris (Meudon) / LUTh
Ultra High Energy Cosmic Rays What we have learnt from HiRes and Auger Andreas Zech Observatoire de Paris (Meudon) / LUTh École de Chalonge, Paris, Outline The physics of Ultra-High Energy Cosmic Rays
More informationPoS(ICRC2017)768. The TAIGA experiment - a hybrid detector for very high energy gamma-ray astronomy and cosmic ray physics in the Tunka valley
- a hybrid detector for very high energy gamma-ray astronomy and cosmic ray physics in the Tunka valley,2, I. Astapov 9, P. Bezyazeekov 2, V. Boreyko 10, A. Borodin 10, M. Brueckner 8, A. Chiavassa 4,
More informationMass composition studies around the knee with the Tunka-133 array. Epimakhov Sergey for the Tunka-133 collaboration
Mass composition studies around the knee with the Tunka-133 array Epimakhov Sergey for the Tunka-133 collaboration The Tunka-133 array non-imaging wide-angle Cherenkov array the knee energy range Tunka
More informationShort review and prospects of radio detection of high-energy cosmic rays. Andreas Haungs
Short review and prospects of radio detection of high-energy cosmic rays 1 To understand the sources of cosmic rays we need to know their arrival direction energy and mass we need large statistics large
More informationThe TAIGA - a hybrid array for high energy gamma astronomy and cosmic ray physics.
The TAIGA - a hybrid array for high energy gamma astronomy and cosmic ray physics. N. Budnev, Irkutsk State University For the TAIGA collaboration 106 years after discovery by Victor Hess "penetrating
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 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 informationP. Tinyakov 1 TELESCOPE ARRAY: LATEST RESULTS. P. Tinyakov. for the Telescope Array Collaboration. Telescope Array detector. Spectrum.
1 1 Université Libre de Bruxelles, Bruxelles, Belgium Telescope Outline Telescope Global distributions Hot spot Correlation with LSS Other searches Telescope UHECR experiments Telescope ARRAY COLLABORATION
More informationDATA ACQUISITION SYSTEM FOR THE TUNKA-133 ARRAY
DATA ACQUISITION SYSTEM FOR THE TUNKA-133 ARRAY N.M. BUDNEV 2, O.B. CHVALAEV 2, O.A. GRESS 2, N.N. KALMYKOV 1, V.A. KOZHIN 1, E.E. KOROSTELEVA 1, L.A. KUZMICHEV 1, B.K. LUBSANDORZHIEV 3, R.R. MIRGAZOV
More informationTunka Radio Extension: Overview and Recent Results
CRI 034 Tunka Radio Extension: Overview and Recent Results Frank G. Schröder for the Tunka-Rex Collaboration Karlsruhe Institute of Technology (KIT), Institut für Kernphysik, Karlsruhe, Germany KIT The
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 informationFrom the Knee to the toes: The challenge of cosmic-ray composition
New Views of the Universe December 8 th 13 th, 2005, Chicago From the Knee to the toes: The challenge of cosmic-ray composition Jörg R. Hörandel University of Karlsruhe www-ik.fzk.de/~joerg New Views of
More informationThe air-shower experiment KASCADE-Grande
The air-shower experiment KASCADE-Grande Andreas Haungs KASCADE-Grande 1 Cosmic Rays around the knee(s) galactic origin of CR EeV PeV Knee 2 nd Knee? Ralph Engel, 2004 KASCADE 1995-2009 -Grande 2003-2009
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 informationGamma-Ray Astronomy from the Ground
Gamma-Ray Astronomy from the Ground Dieter Horns University of Hamburg Introduction - summary Many new Results from ICRC 2015 No we haven't discovered dark matter, yet Yes we have discovered sources of
More informationThe KASCADE-Grande Experiment
The KASCADE-Grande Experiment O. Sima 1 for the KASCADE-Grande Collaboration 2 1 University of Bucharest, Romania 2 https://web.ikp.kit.edu/kascade/ CSSP14 Sinaia 2014 Overview 1. KASCADE-Grande experimental
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 informationThe Cherenkov Telescope Array
The Cherenkov Telescope Array Gamma-ray particle astrophysics Dark Matter Space time Cosmic rays...? Gamma-ray particle astrophysics Dark Matter Space time Cosmic rays...? Particle Dark Matter Direct Detection
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 informationThe Galactic diffuse gamma ray emission in the energy range 30 TeV 3 PeV
The Galactic diffuse gamma ray emission in the energy range 30 TeV 3 PeV Mount Rainier by Will Christiansen Silvia Vernetto & Paolo Lipari 35th ICRC 12-20 July 2017 - Busan - South Korea Gamma ray astronomy
More informationTHE PIERRE AUGER OBSERVATORY: STATUS AND RECENT RESULTS
SF2A 2006 D. Barret, F. Casoli, T. Contini, G. Lagache, A. Lecavelier, and L. Pagani (eds) THE PIERRE AUGER OBSERVATORY: STATUS AND RECENT RESULTS Serguei Vorobiov (for the Pierre Auger Collaboration)
More informationFirst Results from the HiSCORE/Siberia WR setup. Plans for CTA. and. Martin Brückner (Humboldt-Univ. Berlin) Ralf Wischnewski (DESY)
First Results from the HiSCORE/Siberia WR setup and Plans for CTA Martin Brückner (Humboldt-Univ. Berlin) Ralf Wischnewski (DESY) 7th White Rabbit workshop Madrid / Spain 28.11.2012 Outline > HiSCORE -
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 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 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 informationUHE Cosmic Rays in the Auger Era
Vulcano Workshop 2010 - May, 23-29, 2010 UHE Cosmic Rays in the Auger Era Sergio Petrera, L'Aquila University email: sergio.petrera@aquila.infn.it Vulcano Workshop 2010 - May, 23-29, 2010 UHE Cosmic Rays
More informationRecent Results from the KASCADE-Grande Data Analysis
Recent Results from the KASCADE-Grande Data Analysis Donghwa Kang for the KASCADE-Grande Collaboration Karlsruhe Institute of Technology 20 th ISVHECRI 21 25 May 2018, Nagoya, Japan Status & Prospect KASCADE
More informationUltra-High Energy Cosmic Rays and Astrophysics. Hang Bae Kim Hanyang University Hangdang Workshop,
Ultra-High Energy Cosmic Rays and Astrophysics Hang Bae Kim Hanyang University Hangdang Workshop, 2012. 08. 22 Ultra High Energy Cosmic Rays Ultra High Energy Cosmic Ray (UHECR)» E 3 E & 10 18 ev Energy
More informationCalibration of photo sensors for the space-based cosmic ray telescope JEM-EUSO
Calibration of photo sensors for the space-based cosmic ray telescope JEM-EUSO Michael Karus for the JEM-EUSO Collaboration Carpathian Summer School of Physics 2014 Sinaia Romania July 2014 Michael Karus
More informationIceCube. francis halzen. why would you want to build a a kilometer scale neutrino detector? IceCube: a cubic kilometer detector
IceCube francis halzen why would you want to build a a kilometer scale neutrino detector? IceCube: a cubic kilometer detector the discovery (and confirmation) of cosmic neutrinos from discovery to astronomy
More informationCombination of shower-front sampling and imaging in the Tunka Advanced International Gamma-ray and Cosmic ray Astrophysics (TAIGA) project
Combination of shower-front sampling and imaging in the Tunka Advanced International Gamma-ray and Cosmic ray Astrophysics (TAIGA) project a, I. Astapov j, N. Barbashina j, S. Beregnev c, A. Bogdanov g,
More informationThe LHAASO-KM2A detector array and physical expectations. Reporter:Sha Wu Mentor: Huihai He and Songzhan Chen
The LHAASO-KM2A detector array and physical expectations Reporter:Sha Wu Mentor: Huihai He and Songzhan Chen Outline 1. Introduction 2. The KM2A Detector Array 3. Physical Expectations 3.1 Sensitivity
More informationCatching Neutrinos with an IceCube
Catching Neutrinos with an IceCube Mathieu Labare (for the IceCube Collaboration) Vrije Universiteit Brussel - IIHE mlabare@icecube.wisc.edu 04 04 2011, Neutrino-Gamma Workshop @ Marseille IceCube Collaboration
More informationStudies of Ultra High Energy Cosmic Rays with the Pierre Auger Observatory
Studies of Ultra High Energy Cosmic Rays with the Pierre Auger Observatory Universidade Federal do Rio de Janeiro, Brazil E-mail: haris@if.ufrj.br Aquiring data continuously from 004, the Pierre Auger
More informationTenTen: A new IACT Array for Multi-TeV Gamma-Ray Astronomy
TenTen: A new IACT Array for Multi-TeV Gamma-Ray Astronomy Gavin Rowell, Roger Clay, Greg Thornton, Victor Stamatescu (University of Adelaide) Searching for PeV CR Accelerators Adelaide Dec 2006 The H.E.S.S.
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 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 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 informationRecent Observations of Supernova Remnants
1 Recent Observations of Supernova Remnants with VERITAS Tülün Ergin (U. of Massachusetts Amherst, MA) on behalf of the VERITAS Collaboration (http://veritas.sao.arizona.edu) 2 Contents Supernova Remnants
More informationStudy of muon bundles from extensive air showers with the ALICE detector at CERN LHC
doi:.88/174-6596/718/5/0509 Study of muon bundles from extensive air showers with the ALICE detector at CERN LHC K Shtejer 1, 1 Dipartimento di Fisica dell'università and Sezione INFN, Turin, Italy Centro
More informationA method of observing Cherenkov light at the Yakutsk EAS array
A method of observing Cherenkov light at the Yakutsk EAS array Lev Timofeev a and Anatoly Ivanov b The Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy, Russia Abstract. A proposed new method
More informationHigh-energy cosmic rays
High-energy cosmic rays And their acceleration Tom Gaisser 1 Outline Sources and acceleration mechanism End of the galactic cosmic-ray spectrum Transition to extra-galactic population Key questions Tom
More informationPoS(ICRC2015)635. The NICHE Array: Status and Plans. Douglas R Bergman
The NICHE Array: Status and Plans The University of Utah E-mail: bergman@physics.utah.edu John F Krizmanic Universities Space Research Association E-mail: jkrizmanic@usra.edu Yoshiki Tsunesada Tokyo Institute
More informationMeasuring the neutrino mass hierarchy with atmospheric neutrinos in IceCube(-Gen2)
Measuring the neutrino mass hierarchy with atmospheric neutrinos in IceCube(-Gen2) Beyond the Standard Model with Neutrinos and Nuclear Physics Solvay Workshop November 30, 2017 Darren R Grant The atmospheric
More informationArrival directions of the highest-energy cosmic rays detected by the Pierre Auger Observatory
Arrival directions of the highest-energy cosmic rays detected by the Pierre Auger Observatory a for the Pierre Auger Collaboration b a Instituto de Física, Universidade Federal do Rio de Janeiro, Brazil
More informationExperimental High-Energy Astroparticle Physics
KIT University of the State of Baden-Württemberg and National Research Center of the Helmholtz Association Experimental High-Energy Astroparticle Physics Andreas Haungs haungs@kit.edu 3 Content: 1. Introduction
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 informationCosmic Ray Composition and Spectra : Progress since Aspen 05. Gaurang B. Yodh UC Irvine
Cosmic Ray Composition and Spectra : Progress since Aspen 05 Gaurang B. Yodh UC Irvine In this talk I outline my take on the question of composition from about 1 TeV to the highest energies. Important
More informationAnisotropy studies with the Pierre Auger Observatory
Anisotropy studies with the Pierre Auger Observatory Carla Macolino 1 for the Pierre Auger Collaboration 2 Full author list: http://www.auger.org/archive/authors_2011_05.html 1 Lab. de Physique Nucleaire
More informationH.E.S.S. High Energy Stereoscopic System
H.E.S.S. High Energy Stereoscopic System MPI Kernphysik, Heidelberg Humboldt Univ. Berlin Ruhr-Univ. Bochum Univ. Hamburg Landessternwarte Heidelberg Univ. Kiel Ecole Polytechnique, Palaiseau College de
More informationSimulation of the hybrid Tunka Advanced International Gamma-ray and Cosmic ray Astrophysics (TAIGA)
Journal of Physics: Conference Series PAPER OPEN ACCESS Simulation of the hybrid Tunka Advanced International Gamma-ray and Cosmic ray Astrophysics (TAIGA) To cite this article: M Kunnas et al 2015 J.
More informationIceCube Results & PINGU Perspectives
1 IceCube Results & PINGU Perspectives D. Jason Koskinen for the IceCube-PINGU Collaboration koskinen@nbi.ku.dk September 2014 Neutrino Oscillation Workshop Otranto, Lecce, Italy 2 IceCube Detector ~1km
More informationThe Pierre Auger Observatory in 2007
The Pierre Auger Observatory in 2007 Henryk Wilczyński 1 for the Pierre Auger Collaboration 2 1 Institute of Nuclear Physics PAN, Kraków, Poland 2 Pierre Auger Observatory, Malargüe, Mendoza, Argentina
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 informationPoS(NOW2016)041. IceCube and High Energy Neutrinos. J. Kiryluk (for the IceCube Collaboration)
IceCube and High Energy Neutrinos Stony Brook University, Stony Brook, NY 11794-3800, USA E-mail: Joanna.Kiryluk@stonybrook.edu IceCube is a 1km 3 neutrino telescope that was designed to discover astrophysical
More informationCOSMIC RAY COMPOSITION.
COSMIC RAY COMPOSITION. Towards a measurement of cosmic ray composition in the TeV range with IACTs Henrike Fleischhack for the VERITAS-Collaboration HAP Composition workshop 22.09.2015 Alliance for Astroparticle
More informationIceCube: Ultra-high Energy Neutrinos
IceCube: Ultra-high Energy Neutrinos Aya Ishihara JSPS Research Fellow at Chiba University for the IceCube collaboration Neutrino2012 at Kyoto June 8 th 2012 1 Ultra-high Energy Neutrinos: PeV and above
More informationExtensive Air Shower and cosmic ray physics above ev. M. Bertaina Univ. Torino & INFN
Extensive Air Shower and cosmic ray physics above 10 17 ev M. Bertaina Univ. Torino & INFN ISMD 2015, Wildbad Kreuth 5-9 October 2015 Outline:» Part I: A general overview of cosmic ray science.» Part II:
More informationPoS(ICRC2015)432. Simulation Study On High Energy Electron and Gamma-ray Detection With the Newly Upgraded Tibet ASgamma Experiment
Simulation Study On High Energy Electron and Gamma-ray Detection With the Newly Upgraded Tibet ASgamma Experiment Xu Chen a, D. Chen b, J. Huang a, H. B. Jin b, L. M. Zhai a,b, M. Shibata c, Y. Katayose
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 informationCosmic rays in the knee energy range
Astrophys. Space Sci. Trans., 7, 295 301, 2011 doi:.5194/astra-7-295-2011 Author(s) 2011. CC Attribution 3.0 License. Astrophysics and Space Sciences Transactions Cosmic rays in the knee energy range A.
More information7 th International Workshop on New Worlds in Astroparticle Physics São Tomé, September 2009 THE AMIGA PROJECT
7 th International Workshop on New Worlds in Astroparticle Physics São Tomé, 08 10 September 2009 THE AMIGA PROJECT P. GONÇALVES, M. PIMENTA, E. DOS SANTOS, B. TOMÉ LIP S. Tomé, 8 th September 2009 OUTLINE
More informationAstroparticle Physics with IceCube
Astroparticle Physics with IceCube Nick van Eijndhoven nickve.nl@gmail.com http://w3.iihe.ac.be f or the IceCube collaboration Vrije Universiteit Brussel - IIHE(ULB-VUB) Pleinlaan 2, B-1050 Brussel, Belgium
More informationNeutrinos with a cosmic ray detector. Cosmic rays with a neutrino detector
Instead of Neutrinos with a cosmic ray detector Cosmic rays with a neutrino detector Anna Nelles University of California Radio emission of showers High energy particles interacting in dense medium (or
More informationUltra-High Energy Cosmic Rays & Neutrinos above the Terascale
Ultra-High Energy Cosmic Rays & Neutrinos above the Terascale Angela V. Olinto A&A, KICP, EFI The University of Chicago Nature sends 10 20 ev particles QuickTime and a YUV420 codec decompressor are needed
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 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 informationCosmic Ray Astronomy. Qingling Ni
Cosmic Ray Astronomy Qingling Ni What is Cosmic Ray? Mainly charged particles: protons (hydrogen nuclei)+helium nuclei+heavier nuclei What s the origin of them? What happened during their propagation?
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 informationPARTICLE IDENTIFICATION IN GROUND-BASED GAMMA-RAY ASTRONOMY USING CONVOLUTIONAL NEURAL NETWORKS
PARTICLE IDENTIFICATION IN GROUND-BASED GAMMA-RAY ASTRONOMY USING CONVOLUTIONAL NEURAL NETWORKS E.B. Postnikov 1,a, I.V. Bychkov 2,3, J.Y. Dubenskaya 1, O.L. Fedorov 4, Y.A. Kazarina 4, E.E. Korosteleva
More informationInterpretation of cosmic ray spectrum above the knee measured by the Tunka-133 experiment
Interpretation of cosmic ray spectrum above the knee measured by the Tunka-133 experiment L.G. Sveshnikova, L.A. Kuzmichev, E.E. Korosteleva, V.A. Prosin, V.S. Ptuskin et al Moscow State University Skobeltsyn
More informationSearch for a diffuse cosmic neutrino flux with ANTARES using track and cascade events
Search for a diffuse cosmic neutrino flux with ANTARES using track and cascade events Jutta Schnabel on behalf of the ANTARES collaboration Erlangen Centre for Astroparticle Physics, Erwin-Rommel Str.
More informationA CORSIKA study on the influence of muon detector thresholds on the separability of primary cosmic rays at highest energies
A CORSIKA study on the influence of muon detector thresholds on the separability of primary cosmic rays at highest energies and Markus Roth Institut für Kernphysik, Karlsruhe Institute of Technology (KIT),
More informationMonte Carlo studies of CTA: an overview. Victor Stamatescu (University of Adelaide)
Monte Carlo studies of CTA: an overview Victor Stamatescu (University of Adelaide) Outline 1) The Cherenkov Telescope Array concept 2) Imaging Air Cherenkov Technique & simulation 3) Previous and current
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 informationEeV Neutrinos in UHECR Surface Detector Arrays:
EeV Neutrinos in UHECR Surface Detector Arrays: OBSERVATORY Challenges & Opportunities Karl-Heinz Kampert Bergische Universität Wuppertal High-Energy neutrino and cosmic ray astrophysics - The way forward
More informationCosmic ray indirect detection. Valerio Vagelli I.N.F.N. Perugia, Università degli Studi di Perugia Corso di Fisica dei Raggi Cosmici A.A.
Cosmic ray indirect detection Valerio Vagelli I.N.F.N. Perugia, Università degli Studi di Perugia Corso di Fisica dei Raggi Cosmici A.A. 2016/2017 Cosmic Rays Cosmic ray flux at Earth! 1 particle per m
More informationRecent Results of the Telescope Array Experiment. Gordon Thomson University of Utah
Recent Results of the Telescope Array Experiment Gordon Thomson University of Utah 1 Outline Telescope Array Experiment TA Results Spectrum Anisotropy Future Plans Conclusions See John Belz talk for: TA
More information