GLAST Large Area Telescope:
|
|
|
- Ferdinand Rogers
- 5 years ago
- Views:
Transcription
1 GLAST Large Area Telescope: Gamma-ray Large Area Space Telescope Integration and Test Two Tower Integration Readiness Review Particle Test Elliott Bloom I&T Manager I&T Two Tower IRR 1
2 Status of Docs Doc Title In LAT Docs In Sign Off All Signed LAT-TD Particle Test Plan X X LAT-TD Calibration of the VG Photon Flux X X LAT-TD VG Accelerator Safety/Operations Handbook (includes VG operation procedure) LAT-TD VG and CR Data Runs for LAT Integration X X X X LAT-PS Procedure to Take Simultaneous BGO and LAT Data X X X LAT-TD How to Set the LAT Timing Registers X X LAT-TD How to Measure the LAT Trigger Jitter Using the Muon Telescope X X LAT-TD Muon Telescope (includes Muon Telescope operation procedure) X X LAT-TD Use of an Am241 Source for High Rate Triggering (includes source use procedure) X I&T Two Tower IRR 2
3 Status of Equipment Van de Graaff External reliability upgrades done Internal reliability upgrades next time VG must be opened 12 weeks (~30 hrs of running) since last fix (Aug 25, 2004) VG is ready to deliver 17.6 MeV gammas for 1 and 2 towers Old Muon Telescope Working and being used for EM2 timing measurements. Old telescope described in LAT-TD New Muon Telescope Meets the new requirement added by consensus to E2E/SVAC for measuring the tower trigger efficiency. Only gives an external trig when muon passes through the tower New telescope described in LAT-TD (in sign off) Smaller scintillators being fabricated. New telescope will be operational by Dec 10. I&T Two Tower IRR 3
4 VG and BGO Monitor Description Van de Graaff EM1 + VG Target + BGO Photon Monitor 2 : 1 P (440 Kev) + Li 7 Be 8 (1+)* Be 8 + γ (17.6 Mev and 14.6 Mev) I&T Two Tower IRR 4
5 Muon Telescope Description Old Muon Telescope Clean Room New Muon Telescope (Stand same as for Old Telescope) S1a,b:Two new 7.75" x 15.5" Scints placed side by side Cal Tracker 46 in 25 in 4 in 75 in S2a,b:Two new 7.75" x 15.5" Scints placed side by side 10" Pb 17 in S3: Old 24" x 24" Scint (the clear one) I&T Two Tower IRR 5
6 Use Am 241 Source as Fast Trigger for E2E Testing (In review) 7.5 mcurie Am 241 source (60 kev x-ray) at SLAC available for I&T use in Room 104 as needed. Accidental coincidences between Si layer x-ray hits make 6 in a row triggers. Source at different distances from the center of a tower front face generates the high trig rates in the E2E Nominal Rate Cosmic runs. The source is a 1 cm diameter disk. LAT-TD includes the procedure for source use. (in review) Trig rate vs. distance measured for EM2. Agrees with calculation for 7.5 mcurie source (see Figure below) Hz Tests TKR trigger Path directly by activating TKR 3-ina-row trigger primitive. External pulser trigger is a separate trigger path in the GASU, and is not used in flight cm I&T Two Tower IRR 6
7 Two Tower E2E Particle Data Runs LAT-MD Ad Committee on End-to-End Testing (E2E) LAT-TD VG and CR Data Runs for LAT Integration Individual Tests: 75 runs each with its own script (schema file) = 82 hours 1) Baseline Comic Ray (CR) Test # of 1 hour Runs Nominal (as in orbit) settings 1 2) Condition Scan CR Test Volts, temp, delays, thresholds min/max 21 3) Baseline CR Trigger Subtests Each trig (tkr, call, calh) alone 3 4) Nominal Rate CR Test Cosmics + Ext Trigs 1, 5, 10, 20 KHz 4 Cosmics + Am 241 source 1, 5, 10, 20 KHz (In Review) 4 5) Nominal Rate Condition Scan CR Test Same as (2) + Ext Trig 10 KHz 21 I&T Two Tower IRR 7
8 Two Tower E2E Data Runs 6) CAL Nominal Rate CR Test # of 1 hour of Runs Lower Cal Low thresh to give 1, 5, 10 KHz 3 Lower Cal High thresh to give 1, 5, 10 KHz 3 7) Baseline CR Data Volume Sub-Tests Same as (1) but no zero suppression 1 8) Nominal Rate CR Data Volume Sub Tests Cosmics + Ext Trigs 1, 5, 10, 20 KHz No zero suppress 4 Cosmics + Ext Trigs 1, 5, 10, 20 KHz 4 range read 4 9) Van de Graaff (VG) Tests (Target centered at EM2 front face) VG+Cosmics No zero suppress 1 VG+Cosmics Zero suppress 1 VG+Cosmics+Ext Trigs 1, 10 KHz 2 VG into side above super GLAST. Horizontal 1 A) Muon Telescope only external trig input opens trigger OR Measure fraction of events with ACD, TKR, CAL in the trigger window 1 (8 hrs) I&T Two Tower IRR 8
9 For details see LAT-TD Particle Test Runs (1) Total Time Currently is 3 weeks and 1 day at 100% efficiency. 67% efficiency is likely. Need to work on fitting required testing (E2E test report and SVAC tests) into 1 & 2 tower test schedule. I&T Two Tower IRR 9
10 Particle Test Runs (2) I&T Two Tower IRR 10
11 Particle Test Runs (3) I&T Two Tower IRR 11
12 Particle Test Run Acceptance Criteria Each E2E trigger and data flow tests will have a Pass/Fail criteria. System did not hang No parity errors No time outs i.e. no transport errors Data quality monitoring for E2E SVAC offline (see next presentation). Reconstructed angular distribution of cosmic rays I&T Two Tower IRR 12
GLAST Large Area Telescope:
Gamma-ray Large Area Space Telescope GLAST Large Area Telescope: Balloon Flight Results WBS 4.1.E Tune Kamae Stanford Linear Accelerator Center Stanford University LAT Instrument Technical Manager kamae@slac.stanford.edu
Trigger Scheduler, Engines, and Rates. Trigger Scheduler, Engines, and Rates. A proposal for flight configuration
A proposal for flight configuration Purpose Intent: Want to run LAT at SLAC with trigger config as much like flight as possible What is flight trigger config? What rate is acceptable? See Confluence page
EM Energy Spectrum from 17.6 MeV photons. Eduardo do Couto e Silva and Xin Chen Feb 13, 2002
EM Energy Spectrum from 17.6 MeV photons Eduardo do Couto e Silva and Xin Chen Feb 13, 2002 Event display of a muon passing through EM Using GLEAM V3 the official version for EM Mechanical support structure
1 Introduction STATUS OF THE GLAST LARGE AREA TELESCOPE. SLAC-PUB December Richard Dubois. Abstract
SLAC-PUB-10261 December 2003 STATUS OF THE GLAST LARGE AREA TELESCOPE Richard Dubois Stanford Linear Accelerator Center, Stanford University, PO Box 20750, Stanford, CA, USA Abstract The GLAST Large Area
GLAST Large Area Telescope
Gamma-ray Large Area Space Telescope GLAST Large Area Telescope Lowell A. Klaisner Stanford Linear Accelerator Center LAT Instrument Project Manager Klaisner@slac.stanford.edu 650-926-2726 rev. 2 1 Status
GLAST ACD Segmentation Trade Study March 6, 2001 Analysis by Alex Moiseev and J. F. Ormes
GLAST ACD Segmentation Trade Study March 6, 2001 Analysis by Alex Moiseev and J. F. Ormes ACD Subsystem ACD segmentation and the efficiency requirement at 300 GeV March 13, 2001 IDT phone call Jonathan
Preliminary results from gamma-ray observations with the CALorimeteric Electron Telescope (CALET)
Preliminary results from gamma-ray observations with the CALorimeteric Electron Telescope (CALET) Y.Asaoka for the CALET Collaboration RISE, Waseda University 2016/12/15 CTA-Japan Workshop The extreme
Gamma-ray Large Area Space Telescope (GLAST) Large Area Telescope (LAT) Integration & Test Subsystem. Particle Test Plan
Page 1 of 21 Document # LAT-TD-00440-04 Author(s) Gary Godfrey Date 14-Mar-2003 GLAST LAT SYSTEM SPECIFICATION Document Title Particle Beam Test Plan Subsystem/Office Integration and Test Gamma-ray Large
GLAST Large Area Telescope:
Gamma-ray Large Area Space Telescope GLAST Large Area Telescope: Science Requirements and Instrument Design Steven Ritz Goddard Space Flight Center LAT Instrument Scientist ritz@milkyway.gsfc.nasa.gov
GLAST Large Area Telescope:
Gamma-ray Large Area Space Telescope GLAST Large Area Telescope: Project Overview Robert P. Johnson Santa Cruz Institute for Particle Physics Physics Department University of California at Santa Cruz LAT
GLAST Large Area Telescope Monthly Mission Review
GLAST Large Area Telescope Monthly Mission Review Gamma-ray Large Area Space Telescope LAT Flight Software Status May 2, 2007 Jana Thayer Stanford Linear Accelerator Center 1 FSW Status B0-10-1 available
The Large Area Telescope on-board of the Fermi Gamma-Ray Space Telescope Mission
The Large Area Telescope on-board of the Fermi Gamma-Ray Space Telescope Mission 1 Outline Mainly from 2009 ApJ 697 1071 The Pair Conversion Telescope The Large Area Telescope Charged Background and Events
Forward Tagger Status
A. Celentano On behalf of the FT team March 6th, 2018 FT Status All three detectors fully operational Calorimeter: - Cooking circuit leak developed in December repaired early January - Calorimeter operated
The Sun and the Solar System in Gamma Rays
The Sun and the Solar System in Gamma Rays R. Desiante1 on behalf of the Fermi-LAT collaboration SciNeGHE 2016 1 INFN Torino Outline Introduction The Fermi Gamma-Ray Space Telescope The active Sun as seen
GLAST Large Area Telescope. LAT Systems Engineering. LAT Systems Engineering LAT Test Plan Update. Tom Leisgang. Gamma-ray Large Area Space Telescope
Gamma-ray Large Area Space Telescope GLAST Large Area Telescope Systems Engineering Test Plan Update Tom Leisgang Systems Engineering T. Leisgang 1 Systems Engineering Test Plan Update Additions Deletions
Gamma Ray Physics in the Fermi era. F.Longo University of Trieste and INFN
Gamma Ray Physics in the Fermi era F.Longo University of Trieste and INFN Vulcano, May 22, 2018 F.Longo et al. -- 1 Gamma-ray astrophysics above 100 MeV AGILE Fermi 2 Picture of the day, Feb. 28, 2011,
Experimental Particle
Experimental Particle Astrophysics @ Eduardo do Couto e Silva SLUO Annual Meeting July 12, 2002 OUTLINE Introduction X rays g rays Summary 1 There are two groups @ Leader: E. Bloom Leader: T. Kamae 2 Why
Justin Vandenbroucke (KIPAC, Stanford / SLAC) for the Fermi LAT collaboration
Measurement of the cosmic ray positron spectrum with the Fermi LAT using the Earth s magnetic field Justin Vandenbroucke (KIPAC, Stanford / SLAC) for the Fermi LAT collaboration International Cosmic Ray
1.5 TeV Muon Collider background rejection in ILCroot Si VXD and Tracker (summary report)
1.5 TeV Muon Collider background rejection in ILCroot Si VXD and Tracker (summary report) N. Terentiev* (Carnegie Mellon U./Fermilab) V. Di Benedetto, C. Gatto (INFN) A. Mazzacane, N. Mokhov, S. Striganov
Detector R&D in KAPAC
Detector R&D in KAPAC Hiroyasu Tajima Stanford Linear Accelerator Center Kavli Institute for Particle Astrophysics and Cosmology Outline Compton Camera SOI detector Scintillator Polarimeter Cherenkov Camera
Thermal Vacuum Test: Plans and Procedures
GLAST Large Area Telescope Gamma-ray Large Area Space Telescope Pre-Shipment Review Thermal Vacuum Test: Plans and Procedures Jesse Armiger Thermal Vacuum Test Director Thermal Vacuum Test Stanford Linear
A-Exam: e + e Cosmic Rays and the Fermi Large Array Telescope
A-Exam: e + e Cosmic Rays and the Fermi Large Array Telescope Walter Hopkins Physics Department, Cornell University. The Fermi Large Area Telescope is a particle detector in space with an effective collecting
Calibration of the AGILE Gamma Ray Imaging Detector
Calibration of the AGILE Gamma Ray Imaging Detector Andrew Chen on behalf of the AGILE Team April 11, 2011 AGILE Astrorivelatore Gamma ad Immagini LEggero Italian Space Agency (ASI) small mission Participation
Status of KEK-E391a and Future Prospects on K L π 0 νν at KEK. GeiYoub Lim IPNS, KEK
Status of KEK-E391a and Future Prospects on K L π 0 νν at KEK GeiYoub Lim IPNS, KEK E391a Collaboration Joint Institute for Nuclear Research (Dubna), Russia High Energy Accelerator Research Organization,
First results on the high energy cosmic ray electron spectrum with the Fermi-LAT
First results on the high energy cosmic ray electron spectrum with the Fermi-LAT Johan Bregeon INFN Pisa johan.bregeon@pi.infn.it on behalf of the Fermi LAT collaboration TANGO in Paris - May 4 th, 009
Studies of Hadron Calorimeter
Studies of Hadron Calorimeter Zhigang Wang Institute of High Energy Physics 2012.10.17 in IHEP Outline 1,The Dark Matter Calorimeter 2,The Hadron Calorimeter(HCAL) 3, Summary 1,Dark Matter Calorimeter
Liquid Argon TPC for Next Generation of MeV Gamma-ray Satellite
Liquid Argon TPC for Next Generation of MeV Gamma-ray Satellite Hiroyasu Tajima for LArGO team Institute for Space Earth Environmental Research Nagoya University April 22, 2017 Active medium TPC Workshop
Issues with Albedo Gammas in LAT T. Kamae September 2, 2002
Issues with Albedo Gammas in LAT T. Kamae September 2, 2002 History) The prototype tracker tray went through 2 vibration tests (one in Feb. 02 and the other in June 02). In the June test, the bottom tray
Hadronic interactions of ultra-high energy cosmic rays
Hadronic interactions of ultra-high energy cosmic rays Pierre Auger Observatory Henryk Wilczyński Instytut Fizyki Jądrowej PAN, Kraków Kraków, 31 March 2017 Ultra-high energy cosmic rays Key questions:
GLAST LAT Overview and Status
GLAST LAT Overview and Status INPAC Meeting, Berkeley May 5, 2007 Robert Johnson LAT Tracker Subsystem Manager Physics Department and Santa Cruz Institute for Particle Physics University of California
GLAST Tracker. Hiroyasu Tajima On behalf of GLAST Tracker Team. Stanford Linear Accelerator Center, Stanford, CA , USA
SLAC PUB 833 May, 26 GLAST Tracker Hiroyasu Tajima On behalf of GLAST Tracker Team Stanford Linear Accelerator Center, Stanford, CA 9439-4349, USA Abstract The Large Area Telescope (LAT) on board the Gamma-ray
A New Look at the Galactic Diffuse GeV Excess
A New Look at the Galactic Diffuse GeV Excess Brian Baughman Santa Cruz Institute for Particle Physics 1 Overview Diffuse gamma-ray emission The Galactic diffuse gamma-ray GeV excess Discussion of the
T. J. Brandt. CRISM: 27 Jun On behalf of the Fermi- LAT Collabora:on IRAP/Université Paul Saba:er.
On behalf of the Fermi- LAT Collabora:on IRAP/Université Paul Saba:er brandt@cesr.fr CRISM: 27 Jun 2011 All- par:cle CR Spectrum Cosmic rays are: charged particles from outer space (V. Hess, 1912) { ~90%
GRB observations at very high energies with the MAGIC telescopes
GRB observations at very high energies with the telescopes Markus Garczarczyk - for the collaboration - Markus GRB2012 Garczarczyk Munich GRB2012 May 2012 Munich Major Atmospheric Gamma-ray Imaging Cherenkov
Primary 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
The LHCb Experiment II Detector XXXIV SLAC Summer Institute, July, 2006
The LHCb Experiment II Detector XXXIV SLAC Summer Institute, 17-28 July, 2006 Tatsuya NAKADA CERN and Ecole Polytechnique Fédérale de Lausanne (EPFL) 1) Introduction Physics requirements for the detector
The 46g BGO bolometer
Nature, 3 The g BGO bolometer 1 Photograph of the heat [g BGO] and light [Ge; =5 mm] bolometers: see Fig. 1c for description Current events: Amplification gains: 8, (heat channel) &, (light channel). The
GLAST Mission: Status and Science Opportunities
Gamma-ray Large Area Space Telescope GLAST Mission: Status and Science Opportunities Bill Atwood SCIPP / UCSC atwood@scipp.ucsc.edu Outline GLAST: An International Science Mission Large Area Telescope
Tevatron Detector Upgrades
Tevatron Detector Upgrades Contents Upgrade History The Detectors in Run IIa Tevatron Scenarios and Running Conditions CDF and D0 Upgrades Maximizing Physics Conclusions This will not have WBS numbers/l1,2,3
Current Status of Luminosity Measurement with the CMD-3 Detector at the VEPP-2000 e + e collider
Proceedings of the CERN-BINP Workshop for Young Scientists in e + e Colliders, Geneva, Switzerland, 5 August 16, edited by V. Brancolini ans L. Linssen, CERN Proceedings, Vol. 1/17, CERN-Proceedings-17-1
Introduction. Technical and Production Status L. Klaisner. Instrument Science Operations Center Plans. Project Status, Cost and Schedule L.
Gamma-ray Large Area Space Telescope Introduction S. Ritz Technical and Production Status L. Klaisner Instrument Science Operations Center Plans R. Cameron Project Status, Cost and Schedule L. Klaisner
Anders W. Borgland. On behalf of the Fermi/LAT Collaboration. Fermi LAT ISOC/SLAC
Fermi Status And Prospects borgland@slac.stanford.edu Fermi LAT ISOC/SLAC On behalf of the Fermi/LAT Collaboration 1 A Broad Overview Of The Fermi Mission From GLAST To Fermi The Fermi Mission LAT Instrument
PoS(ICHEP2016)474. SoLid: Search for Oscillations with a Lithium-6 Detector at the SCK CEN BR2 reactor
SoLid: Search for Oscillations with a Lithium-6 Detector at the SCK CEN BR2 reactor University of Bristol E-mail: dan.saunders@bristol.ac.uk The disappearance of reactor antineutrinos into a new neutral
First Year Fermi Gamma ray Space Telescope Observations of Centaurus A
First Year Fermi Gamma ray Space Telescope Observations of Centaurus A C.C. Teddy Cheung (NASA GSFC) Yasushi Fukazawa (Hiroshima Univ) on behalf of the Fermi LAT collaboration The Many Faces of Centaurus
GLAST, a Gamma-Ray Large Area Space Telescope
GLAST, a Gamma-Ray Large Area Space Telescope Hartmut F.-W. Sadrozinski SCIPP, Univ. of California Santa Cruz, CA 95064 (Representing the GLAST Collaboration) Abstract The GLAST LAT instrument has been
Soft Gamma-ray Detector (SGD) for the NeXT mission and beyond Astro-E2 Tadayuki Takahashi
T.Takahashi, Astronomy with Radioactivies IV,2003 Soft Gamma-ray Detector (SGD) for the NeXT mission and beyond Astro-E2 Tadayuki Takahashi Institute of Space and Astronautical Science (ISAS, Japan) 2005
Can we constrain GRB shock parameters using the Gamma Ray Large Area Space Telescope? Eduardo do Couto e Silva SLAC/KIPAC SABER Workshop Mar 15, 2006
Can we constrain GRB shock parameters using the Gamma Ray Large Area Space Telescope? Eduardo do Couto e Silva SLAC/KIPAC SABER Workshop Mar 15, 2006 The Main Questions Is there any connection between
MINOS. Physics Program and Construction Status. Karol Lang The University of Texas at Austin. YITP: Neutrinos and Implications for Physics Beyond
MINOS Physics Program and Construction Status Karol Lang The University of Texas at Austin YITP: Neutrinos and Implications for Physics Beyond YITP Conference: Neutrinos and Implications The Standard for
The Silicon-Tungsten Tracker of the DAMPE Mission
The Silicon-Tungsten Tracker of the DAMPE Mission Philipp Azzarello, DPNC, University of Geneva for the DAMPE-STK collaboration 10th International Hiroshima Symposium on the Development and Application
Search for Oscillation with Lithium-6 Detector at BR2 Prototype Update and short perspectives
SoLi Search for Oscillation with Lithium-6 Detector at BR2 Prototype Update and short perspectives A. Baird, N. Ryder, P. R. Scovell, A. Vacheret, A. Weber (Oxford, UK) G. Barber, J. Nash, A. Rose (Imperial
Validation of EM Part of Geant4
Validation of EM Part of Geant4 February 22, 2002 @ Geant4 Work Shop Tsuneyoshi Kamae/Tsunefumi Mizuno 1 Purpose and Plan of this Talk We have validated EM processes in Geant4 important for gamma-ray satellite
IceCube: 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
VERITAS Design. Vladimir Vassiliev Whipple Observatory Harvard-Smithsonian CfA
VERITAS Design Vladimir Vassiliev Whipple Observatory Harvard-Smithsonian CfA VERITAS design goals VERITAS is a ground-based observatory for gamma-ray astronomy VERITAS design is derived from scientific
L esperimento di Astrofisica GLAST il Large Area Telescope
Gamma-ray Large Area Space Telescope Riccardo Rando L esperimento di Astrofisica GLAST il Large Area Telescope Scuola Nazionale "Rivelatori ed Elettronica per Fisica delle Alte Energie, Astrofisica e Applicazioni
Compton suppression spectrometry
Compton suppression spectrometry In gamma ray spectrometry performed with High-purity Germanium detectors (HpGe), the detection of low intensity gamma ray lines is complicated by the presence of Compton
High-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
The new event analysis of the Fermi Large Area Telescope
The new event analysis of the Fermi Large Area Telescope LUPM (Laboratoire Univers et Particule de Montpellier) E-mail: thibaut.desgardin@univ-montp2.fr Since its launch on June 11, 2008 the Large Area
Brief Report from the Tevatron. 1 Introduction. Manfred Paulini Lawrence Berkeley National Laboratory Berkeley, California 94720
Brief Report from the Lawrence Berkeley National Laboratory Berkeley, California 9472 1 Introduction It might appear surprising to include a report from the Fermilab, a proton-antiproton collider, in a
GLAST Silicon Tracker Vertex 98, Santorini (Greece), Sep 29-Oct The Silicon Strip Tracker for the Gamma-ray Large Area Space Telescope
Vertex 98, Santorini (Greece), Sep 29-Oct 4 1998 The Silicon Strip Tracker for the Gamma-ray Large Area Space Telescope University of California, Santa Cruz Bill Atwood (SLAC) Jose A. Hernando Masaharu
arxiv: v1 [physics.ins-det] 22 Dec 2013
![arxiv: v1 [physics.ins-det] 22 Dec 2013](/thumbs/93/111563422.jpg "arxiv: v1 [physics.ins-det] 22 Dec 2013")
arxiv:1312.6334v1 [physics.ins-det] 22 Dec 213 Test of the prototype of electron detector for LHAASO project using cosmic rays * WANG Xu 1 XU Tongye 1 DU Yanyan 1 SHAO Ruobin 1 ZHU Chengguang 1;1) for
The Gamma-ray Albedo of the Moon
[albedo] the proportion of the incident light that is reflected by a surface The Gamma-ray Albedo of the Moon Igor V. Moskalenko & Troy A. Porter Astrophys. J. 670, 1467-1472 (2007) Masaki Mori ICRR CANGAROO
Instrumentation Issues
Gamma-Ray Large Area Space Telescope GLAST Instrumentation Issues Hartmut F.-W. Sadrozinski SCIPP, Univ. of California Santa Cruz Through most of history, the cosmos has been viewed as eternally tranquil
Distillation purification and radon assay of liquid xenon
Distillation purification and radon assay of liquid xenon Yasuo Takeuchi Kamioka Observatory, ICRR, Univ. of Tokyo, Kamioka-cho, Hida-shi, Gifu 56-125, Japan Abstract. We succeeded to reduce the Kr contamination
Science of Compact X-Ray and Gamma-ray Objects: MAXI and GLAST
Science of Compact X-Ray and Gamma-ray Objects: MAXI and GLAST D. J. Thompson, 1 on behalf of the GLAST LAT Collaboration 1 NASA Goddard Space Flight Center, Greenbelt, MD 20771 USA E-mail(DJT): David.J.Thompson@nasa.gov
9/27 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:
Final Results from the MEG Experiment and the Status of MEG-II
Final Results from the MEG Experiment and the Status of MEGII Francesco Renga INFN Roma HQL 2016 Virginia Tech, May 2227 2016 1 Charged Lepton Flavor Violation (clfv) Highlights Charge Lepton Flavor conservation
PARTICLES REVELATION THROUGH SCINTILLATION COUNTER
14-25 JUNE 2004 SUMMER STAGE PARTICLES REVELATION THROUGH SCINTILLATION COUNTER by Flavio Cavalli and Marcello De Vitis Liceo Scientifico Statale Farnesina Tutor: Marco Mirazita 1) COSMIC RAYS - The Muons
On-Orbit Performance of the GLAST Burst Monitor
On-Orbit Performance of the GLAST Burst Monitor Curran D. Muhlberger (RA) Charles A. Meegan (PI) Cornell University University of Maryland August 8, 2008 What is GLAST? What is GBM? What is it Good for?
The AMIGA detector of the Pierre Auger Observatory: an overview
The AMIGA detector of the Pierre Auger Observatory: an overview Federico Sánchez 1 for the Pierre Auger Collaboration 2 1 Instituto de Tecnologías en Detección y Astropartículas (CNEA-CONICET-UNSAM), Buenos
Observation of Reactor Antineutrinos at RENO. Soo-Bong Kim for the RENO Collaboration KNRC, Seoul National University March 29, 2012
Observation of Reactor Antineutrinos at RENO Soo-Bong Kim for the RENO Collaboration KNRC, Seoul National University March 29, 2012 Outline Introduction Experimental setup & detector Data-taking & data
VERITAS Performance Gernot Maier
VERITAS Performance Gernot Maier Alliance for Astroparticle Physics What scientific impact will VERITAS have in the next 3-5 years? Galactic long-term plan Performance Operations LTP & Performance May
Risultati dell esperimento ATLAS dopo il run 1 di LHC. C. Gemme (INFN Genova), F. Parodi (INFN/University Genova) Genova, 28 Maggio 2013
Risultati dell esperimento ATLAS dopo il run 1 di LHC C. Gemme (INFN Genova), F. Parodi (INFN/University Genova) Genova, 28 Maggio 2013 1 LHC physics Standard Model is a gauge theory based on the following
Lepton Flavour Violation
Lepton Flavour Violation Search for e at Paul Scherrer Institut Satoshi Mihara ICEPP, Univ. of Tokyo http://meg.icepp icepp.s..s.u-tokyo.ac.jp, http://meg.psi psi.ch,http://meg.pi.,http://meg.pi.infn.it
Detector R&D at KIPAC. Hiro Tajima Kavli InStitute of Particle Astrophysics and Cosmology
Detector R&D at KIPAC Hiro Tajima Kavli InStitute of Particle Astrophysics and Cosmology Detector R&D Overview Si detector ASIC Integration GLAST GeV Gamma-ray Observatory ASIC DAQ Next generation X-ray
Recent Developments of the Real-Time Capabilities of IceCube
Recent Developments of the Real-Time Capabilities of IceCube Thomas Kintscher for the IceCube Collaboration TAUP 2015 Neutrinos B Torino, 2015/09/10 Multi-Messenger Observations > Combination of different
A beam line for schools
A beam line for schools Great things can happen when high schools get involved with cutting edge science, and that s exactly what CERN is proposing with its new beam line for schools competition, which
A Search for Point Sources of High Energy Neutrinos with AMANDA-B10
A Search for Point Sources of High Energy Neutrinos with AMANDA-B10 Scott Young, for the AMANDA collaboration UC-Irvine PhD Thesis: http://area51.berkeley.edu/manuscripts Goals! Perform an all-sky search
Digital Gamma-ray Spectroscopy & Imaging with Semiconductor detectors Frontiers of gamma-ray spectroscopy
Digital Gamma-ray Spectroscopy & Imaging with Semiconductor detectors Frontiers of gamma-ray spectroscopy AGATA GRETA Dr Andy Boston ajboston@liv.ac.uk And its applications The AGATA Concept Without Compton
Search for K + π + νν decay at NA62 experiment. Viacheslav Duk, University of Birmingham for the NA62 collaboration
Search for K + π + νν decay at NA62 experiment Viacheslav Duk, University of Birmingham for the NA62 collaboration Durham, 04-06.09.2017 1 Outlook 1. Motivation 2. NA62 experiment 3. Event selection 4.
PoS(TIPP2014)033. Upgrade of MEG Liquid Xenon Calorimeter. Ryu SAWADA. ICEPP, the University of Tokyo
ICEPP, the University of Tokyo E-mail: sawada@icepp.s.u-tokyo.ac.jp The MEG experiment yielded the most stringent upper limit on the branching ratio of the flavorviolating muon decay µ + e + γ. A major
The Pierre Auger Observatory
The Pierre Auger Observatory Hunting the Highest Energy Cosmic Rays I High Energy Cosmic Rays and Extensive Air Showers March 2007 E.Menichetti - Villa Gualino, March 2007 1 Discovery of Cosmic Rays Altitude
First tests of the big volume ultra low background gamma spectrometer
First tests of the big volume ultra low background gamma spectrometer N. Todorović,, D. MrđaM rđa,, I. Bikit, M. Vesković,, S. Forkapić,, J. Slivka Departman za fiziku, PMF, Novi Sad 1. Introduction Even
Undulator-Based Production of Polarized Positrons. Project Name LCRD Contact Person William Bugg, University of Tennessee
Project Name LCRD 2.37 Undulator-Based Production of Polarized Positrons Progress Report of E-166 at FFTB at Stanford Linear Accelerator Center. University of Tennessee, Knoxville FY 2004 funding 25,000
Results of the Search for Ultra High-Energy Neutrinos with ANITA-II
Results of the Search for Ultra High-Energy Neutrinos with ANITA-II Abby Goodhue Vieregg for the ANITA Collaboration University of California, Los Angeles 25 March 2010 (ANITA-II Launch Day in Antarctica)
The Mu3e PSI
The Mu3e Experiment @ PSI searching for the neutrinoless muon decay m + e + e - e + Tau 2016 Beijing, Sept. 23, 2016 Alessandro Bravar for the Mu3e Collaboration LFV in Standard Model Flavor Conservation
ABSTRACT 1. INTRODUCTION. Presented at the SPIE Astronomical Telescopes+ Instrumentation Conference Amsterdam, The Netherlands, July 1-6, 2012
SLAC-PUB-15123 Fermi Large Area Telescope Operations: Progress Over 4 Years Robert A. Cameron* a on behalf of the Fermi Large Area Telescope Collaboration a SLAC National Accelerator Laboratory, 2575 Sand
Fluorescence Measurements at ANL and the Auger Experiment
Fluorescence Measurements at ANL and the Auger Experiment Motivation for Fluorescence Calibrations AIRFLY Fluorescence Experiment at ANL Auger Experiment Update N 2 Molecule Vibrational Energy Levels 337nm
Status of ATLAS and Preparation for the Pb-Pb Run
Status of ATLAS and Preparation for the Pb-Pb Run Jiří Dolejší a for the ATLAS Collaboration a Charles University, Faculty of Mathematics and Physics, IPNP, V Holesovickach 2, CZ-180 00 Praha 8, Czech
The JUNO veto detector system. Haoqi Lu Institute of High Energy physics (On Behalf of the JUNO Collaboration) TIPP2017, May22-26,Beijing
The JUNO veto detector system Haoqi Lu Institute of High Energy physics (On Behalf of the JUNO Collaboration) TIPP2017, May22-26,Beijing 1 The Jiangmen Underground Neutrino Observatory (JUNO) Detector
AugerPrime. 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
arxiv: v1 [astro-ph.he] 2 Jul 2009
![arxiv: v1 [astro-ph.he] 2 Jul 2009](/thumbs/87/97070104.jpg "arxiv: v1 [astro-ph.he] 2 Jul 2009")
PROCEEDINGS OF THE 31 st ICRC, ŁÓDŹ 2009 1 First results on Cosmic Ray electron spectrum below 20 GeV from the Fermi LAT. M.Pesce-Rollins on behalf of the Fermi LAT Collaboration Istituto Nazionale di
CMS ECAL status and performance with the first LHC collisions
CMS ECAL status and performance with the first LHC collisions XIV International Conference on Calorimetry in High Energy Physics (Calor 2010) Konstantinos Theofilatos (ETH Zurich) on behalf of CMS ECAL
Juan Estrada Fermi National Accelerator Laboratory 1
Juan Estrada Fermi National Accelerator Laboratory estrada@fnal.gov 1 NEW PHYSICS IN THE LOW ENERGY NEUTRINO SECTOR 2 Coherent scattering is the limitation of the next generations of Dark Matter experiments.
DOUBLE BETA DECAY OF 106 Cd - EXPERIMENT TGV (Telescope Germanium Vertical) EXPERIMENT SPT (Silicon Pixel Telescope)
DOUBLE BETA DECAY OF 106 Cd - EXPERIMENT TGV (Telescope Germanium Vertical) EXPERIMENT SPT (Silicon Pixel Telescope) I. Štekl (IEAP CTU in Prague) on behalf of TGV collaboration CSNSM Orsay, France CU
AGIS (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
Year- 1 (Heavy- Ion) Physics with CMS at the LHC
Year- 1 (Heavy- Ion) Physics with CMS at the LHC Edwin Norbeck and Yasar Onel (for the CMS collaboration) University of Iowa For the 26 th Winter Workshop on Nuclear Dynamics Ocho Rios, Jamaica 8 January
Astrophysics with GLAST: dark matter, black holes and other astronomical exotica
Astrophysics with GLAST: dark matter, black holes and other astronomical exotica Greg Madejski Stanford Linear Accelerator Center and Kavli Institute for Particle Astrophysics and Cosmology (KIPAC) Outline:
Study of the HARPO TPC for a high angular resolution g-ray polarimeter in the MeV-GeV energy range. David Attié (CEA/Irfu)
Study of the HARPO TPC for a high angular resolution g-ray polarimeter in the MeV-GeV energy range David Attié (CEA/Irfu) Outline Motivation of an MeV-GeV polarimeter Scientific case and expected performance
Gamma-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
Detector R&D at KIPAC
Detector R&D at KIPAC Hiro Tajima Kavli Institute for Particle Astrophysics and Cosmology 1 Detector R&D Overview Si detector ASIC Integration GLAST GeV Gamma-ray Observatory ASIC DAQ Next generation X-ray