VERITAS status Stephan LeBohec and Brian Humensky for the VERITAS collaboration Adelaide, December 2006.

Slides:



Advertisements
Similar presentations
1 Observation of the Crab Nebula with the MAGIC Telescope M. López-Moya Univ. Complutense de Madrid, on behalf of the MAGIC Collaboration.
Advertisements

Exploiting VERITAS Timing Information J. Holder a for the VERITAS Collaboration b a) School of Physics and Astronomy, University of Leeds, UK b) For full.
Calibration for LHAASO_WFCTA Yong Zhang, LL Ma on behalf of the LHAASO collaboration 32 nd International Cosmic Ray Conference, Beijing 2011.
H.E.S.S. Phases I and II Paula Chadwick, Dept. of Physics University of Durham.
WP-Technology Working Group Future of Ground Based Gamma-ray Astronomy Feb 8, Technology & Cost WP Working Group GOALS With the Current Generation.
TileCal Electronics A Status Report J. Pilcher 17-Sept-1998.
 Jim Hinton 2006 High Energy Stereoscopic System (H.E.S.S.)  Array of four 107 m 2 telescopes in Namibia, 120 m spacing  5° FOV  Threshold 100 GeV.
Jamie Holder School of Physics and Astronomy, University of Leeds, U.K Increasing the Collection Area for IACTs at High Energies Future of Gamma Ray Astronomy.
Gus Sinnis HAWC Review December 2007 Milagro a TeV Gamma-Ray Observatory Gus Sinnis Los Alamos National Laboratory.
Jamie Holder School of Physics and Astronomy, University of Leeds, U.K Optical SETI at Leeds Using Cherenkov Light Buckets as Optical SETI Detectors RAS.
1 VERY ENERGETIC RADIATION IMAGING TELESCOPE ARRAY SYSTEM VERITAS Mark Lang, National University of Ireland, Galway.
On A Large Array Of Midsized Telescopes Stephen Fegan Vladimir Vassiliev UCLA.
The ANTARES Neutrino Telescope Mieke Bouwhuis 27/03/2006.
Julie McEnery GLAST Science Lunch Milagro: A Wide Field of View Gamma-Ray Telescope Julie McEnery.
A crude (lower limit) estimation of resolution and event rate Development and Construction of an Extensive Air Shower Array in HOU Antonis Leisos, Hellenic.
Hanoi, Aug. 6-12, 2006 Pascal Vernin 1 Antares Status report P.Vernin CEA Saclay, Dapnia On behalf of the Antares collaboration P.Vernin
Coincidence analysis in ANTARES: Potassium-40 and muons  Brief overview of ANTARES experiment  Potassium-40 calibration technique  Adjacent floor coincidences.
P.Vincent LPNHE-Paris for H.E.S.S. collaboraton28 th ICRC - Tsukuba - Japan - 5, August 2003 Performance of the H.E.S.S. cameras Pascal Vincent (LPNHE.
Gus Sinnis RICAP, Rome June 2007 High Altitude Water Cherenkov Telescope  Gus Sinnis Los Alamos National Laboratory for the HAWC Collaboration.
Long-term monitor on Mrk 421 using ARGO-YBJ experiment S.Z Chen (IHEP/CAS/China, On behalf of the ARGO-YBJ collaboration  1. Introduction.
28 th ICRC Tsukuba Conor Masterson, H.E.S.S. Observations of Galactic Sources with H.E.S.S. Conor Masterson, MPI-K, for the H.E.S.S. Collaboration.
Moriond 2001Jordan GoodmanMilagro Collaboration The Milagro Gamma Ray Observatory The Physics of Milagro Milagrito –Mrk 501 –GRB a Milagro –Description.
Dieter Horns – University of Tübingen August 2006, Madison Wisconsin HESS: Status and future plans Dieter Horns (Univ. Tübingen) on behalf of German.
Recent TeV Observations of Blazars & Connections to GLAST Frank Krennrich Iowa State University VERITAS Collaboration GSFC, October 24, 2002 AGN.
The TeV Gamma-ray Universe Trevor C. Weekes Harvard-Smithsonian Center for Astrophysics Motivation/Techniques The TeV Sky Future Prospects.
Performance of CRTNT for Sub-EeV Cosmoc Ray Measurement Zhen Cao IHEP, Beijing & Univ. of Utah, SLC Aspen, CO, 04/2005.
Cosmology with Ground-Based Cherenkov Telescopes Wei Cui (Purdue University)
Frank Krennrich*, for the VERITAS Collaboration (*Iowa State University) Results from VERITAS Results from VERITAS New Opportunities at the interface.
Argonne / U. Chicago Initiative on R & D for Next Generation Ground Based Gamma-ray Particle Astrophysics/Astronomy Karen Byrum Jun 7, 2010 Argonne National.
5.1 Optical Observatories 5.1 a: Observatory Sites: One limitation: the time needed for optics to reach equilibrium shape when exposed to severe temperatures.
Development of Ideas in Ground-based Gamma-ray Astronomy, Status of Field and Scientific Expectations from HESS, VERITAS, MAGIC and CANGAROO Trevor C.
Fermi Symposium, Washington, DCVERITAS Observations of SNRs and PWNe B. Humensky, U. of Chicago Brian Humensky for the VERITAS Collaboration November 4,
School of something FACULTY OF OTHER Opportunities in future ground-based gamma-ray experiments Joachim Rose School of Physics and Astronomy University.
Jamie Holder University of Leeds August 2005 Status and Performance of the First VERITAS Telescope.
May 4th 2006R.Mirzoyan: CTA meeting, Berlin The MAGIC Project: Performance of the 1st telescope Razmick Mirzoyan On behalf of the MAGIC Collaboration Max-Planck-Institute.
M.Teshima MPI für Physik, München (Werner-Heisenberg-Institut) for MAGIC collaboration MAGIC.
44th Rencontres de Moriond, 7th February Luísa Arruda on behalf of the GAW collaboration LIP – Laboratório de Instrumentação e Física Experimental.
Gus Sinnis Asilomar Meeting 11/16/2003 The Next Generation All-Sky VHE Gamma-Ray Telescope.
First Results from VERITAS David Hanna McGill University Montreal, Canada.
Lead Fluoride Calorimeter for Deeply Virtual Compton Scattering in Hall A Alexandre Camsonne Hall A Jefferson Laboratory October 31 st 2008.
1 Optical observations of asteroids – and the same for space debris… Dr. D. Koschny European Space Agency Chair of Astronautics, TU Munich Stardust school.
PSROC, February 2, 2005 Sun Yat-San University Ching-Cheng Hsu National Taiwan University On behalf of NuTel Group Outline :  Overview of NuTel Experiment.
1 Status of the CANGAROO-III Project Masaki Mori ICRR, University of Tokyo International Symposium on High Energy Gamma-Ray Astronomy, June 26-30, Heidelberg.
Extending the Sensitivity Of Air-Cerenkov Telescopes Steve Biller, Oxford University (de la Calle & Biller – astro-ph/ )
HAWC Science  Survey of 2  sr (half the sky) up to 100 TeV energies Probe knee in cosmic ray spectrum Identify sources of Galactic cosmic rays  Extended.
The Auger Observatory for High-Energy Cosmic Rays G.Matthiae University of Roma II and INFN For the Pierre Auger Collaboration The physics case Pierre.
Timing Studies of Hamamatsu MPPCs and MEPhI SiPM Samples Bob Wagner, Gary Drake, Patrick DeLurgio Argonne National Laboratory Qingguo Xie Department of.
VERITAS Observations Of M 31 and some results about my recent work
Production PMT Testing and Work on Site with Prototype Tank University of California, Los Angles Department of Physics and Astronomy
A Future All-Sky High Duty Cycle VHE Gamma Ray Detector Gus Sinnis/Los Alamos with A. Smith/UMd J. McEnery/GSFC.
June 6, 2006 CALOR 2006 E. Hays University of Chicago / Argonne National Lab VERITAS Imaging Calorimetry at Very High Energies.
Optical Astronomy with Cerenkov telescopes E. Oña-Wilhelmi 1,2, O.C. de Jager 1, J. Cortina 3, V. Fonseca 2 1 NWU, Potchefstroom, South Africa. 2 UCM,
05/02/031 Next Generation Ground- based  -ray Telescopes Frank Krennrich April,
Next Generation Particle Astrophysics with GeV/TeV  -Rays D. Kieda University of Utah.
UPGRADE PLANS FOR VERITAS Ben Zitzer* for the VERITAS Collaboration *Argonne National Laboratory.
MAGIC Telescopes - Status and Results 2009/ Isabel Braun Institute for Particle Physics, ETH Zürich for the MAGIC collaboration CHIPP Plenary Meeting.
Dave Kieda* for the VERITAS Collaboration *University of Utah Department of Physics & Astronomy.
The Large High Altitude Air Shower Observatory LHAASO.
Jamie Holder Bartol Research Institute/Department of Physics and Astronomy University of Delaware VERITAS Contributions to CF6 Cosmic rays, Gamma-rays.
Abstract: In distinguishing between the atmospheric Cerenkov light initiated by the primary cosmic ray and its associated air shower, the Track Imaging.
CTA-LST Large Size Telescope M. Teshima for the CTA Consortium Institute for Cosmic Ray Research, University of Tokyo Max-Planck-Institute for Physics.
The VERITAS Trigger System A. Weinstein 1 for the VERITAS Collaboration 2 CFD x 499 (1 per pixel ) Pattern Trigger Shower Delay ( 1 PDM channel per trigger.
A. Weinstein, UCLA 2009 Fermi SymposiumVERITAS Survey of the Cygnus Region of the Galactic Plane The VERITAS Survey of the Cygnus Region of the Galactic.
MAGIC M.Teshima MPI für Physik, München (Werner-Heisenberg-Institut)
LHAASO-WCDA: Design & Performance
HAWC Science Survey of 2p sr up to 100 TeV energies Extended Sources
M.Teshima MPI für Physik, München (Werner-Heisenberg-Institut)
VERITAS: Very High Energy γ-ray Astronomy
Department of Energy/National Science Foundation
VERITAS Upgrade Overview Jamie Holder (Delaware)
Presentation transcript:

VERITAS status Stephan LeBohec and Brian Humensky for the VERITAS collaboration Adelaide, December 2006

Smithsonian Astrophysical Observatory * Smithsonian Astrophysical Observatory * Adler Planetarium Adler Planetarium Purdue University * Purdue University * Barnard College, NY Barnard College, NY Iowa State University * Iowa State University * DePauw University, IN DePauw University, IN Washington University, St. Louis * Washington University, St. Louis * Grinnell College, IA Grinnell College, IA University of Chicago * University of Chicago * University of California, Santa Cruz University of California, Santa Cruz University of Utah * University of Massachussetts University of Massachussetts University of California, Los Angeles * University of California, Los Angeles * Cork Institute of Technology Cork Institute of Technology McGill University, Montreal * McGill University, Montreal * Galway-Mayo Institute of Technology Galway-Mayo Institute of Technology National University of Ireland, Dublin * National University of Ireland, Dublin * National University of Ireland, Galway National University of Ireland, Galway University of Leeds * University of Leeds * Associate Members Associate Members Project office: Whipple observatory SAO VERITAS Collaboration ~65 members in more than 20 institutions Funding from NSF/DOE/Smithsonian/PPARC/SFI/NSERC

85 m 109 m 85 m 35 m T2 T1 T3 T4 Fall 2006 Since January 2006 January 2007

0.5 o 0.15 o pixel 340 Hexagonal Facets 0.60m across Davies-Cotton Diameter = 12m Focal Length = 12m Time dispersion < 5ns Bias alignment PSF FWHM 0.06 o

Light collecting cones to Increase light collection & shield from stray light 499 pixel camera 3.5 O FOV 0.15 O pixels Photonis XP2970 2x10 5 Gain Custom preamplifier installed in Base: 6.66 Effective Gain AC DC output for current monitoring Programmable test pulse input

Camera PMT Current monitor Charge Injection Telescope Electronics 500MHz Digitization 8(+3) bits 8  s deep memory x CFD Pattern Sensitive Trigger Readout 140ft 75  RG59 ~200m fiber Array Control Building Delays Array Trigger VERITAS ELECTRONICS

Telescope and Array Triggers Telescope: any 3 adjacent pixels within 10 ns Array: multiple telescope triggers within 100ns geometry telescope-delay (a tradition since March 2006). Trigger rate ~ 100 Hz Deadtime ~ 5 %

20ns/event 6ns frame every 2ns 85m 3.5 o

VERITAS OPtical Telescope Injection and Calibration System Pedestal Single photo-electron Raw data Time and gain corrected data

Rayleigh attenuation Rayleigh Scattering Rayleigh scattering based Absolute Calibration

7  /min 16.5  /hr 1/2 Two telescope stereo observation of the Crab Nebula

Mrk421: 5.6 gamma/minute over 7.2 hours Mrk501: 0.8 gamma/minute over 11.4 hours

Conclusions: * VERITAS FULLY OPERATIONAL IN 2007: Four 12m telescopes with 500 pixel cameras (3.5°) in southern Az (1800m) *SPECIFICATIONS: Energy threshold ~ 100GeV Angular resolution ~ 4'-6' Energy resolution~ 10-15% Collecting area~ 4×10 4 m 2 Crab rate~ 40/min

1996 First Proposal to Smithsonian (Buckley, Catanese, Weekes & Krennrich) 1998 VERITAS selected for internal support at SAO 1999 PPARC/EI approve funding for VERITAS 2000 Lehman review --> passed 2000 DOE funds VERITAS R&D 2000 VERITAS proposal to NSF/DOE --> NSF lacks funds 2001 Dec. 3 agencies appear ready to fund VERITAS --> OMB disapproves 2002 Decadel Survey by Nat. Academy --> endorses VERITAS 2003 Montosa canyon approved! --> lawsuit by environmental group decision to go to Kitt Peak instead! 2003 March VERITAS funded for 4 telescopes in U.S. by DoE & NSF! 2004 Feb. Prototype Telescope at testsite operational 2005 Feb. telescope 1 operational 2004 July site at Kitt Peak approved! 2005 Feb. infrastructure for VERITAS in place at Kitt Peak 2005 Tohono O’odham Nation files complaint --> site shutdown --> NSF volunteers to do a new EA --> resolution expected by Dec Fall Telescope 1 & 2 start FLWO basecamp 2006 Decision to built VERITAS-4 at basecamp + operate Dec. Kitt Peak site issue still unresolved …

1996 First Proposal to Smithsonian (Buckley, Catanese, Weekes & Krennrich) 1998 VERITAS selected for internal support at SAO 1999 PPARC/EI approve funding for VERITAS 2000 Lehman review --> passed 2000 DOE funds VERITAS R&D 2000 VERITAS proposal to NSF/DOE --> NSF lacks funds 2001 Dec. 3 agencies appear ready to fund VERITAS --> OMB disapproves 2002 Decadel Survey by Nat. Academy --> endorses VERITAS 2003 Montosa canyon approved! --> lawsuit by environmental group decision to go to Kitt Peak instead! 2003 March VERITAS funded for 4 telescopes in U.S. by DoE & NSF! 2004 Feb. Prototype Telescope at testsite operational 2005 Feb. telescope 1 operational 2004 July site at Kitt Peak approved! 2005 Feb. infrastructure for VERITAS in place at Kitt Peak 2005 Tohono O’odham Nation files complaint --> site shutdown --> NSF volunteers to do a new EA --> resolution expected by Dec Fall Telescope 1 & 2 start FLWO basecamp 2006 Decision to built VERITAS-4 at basecamp + operate Dec. Kitt Peak site issue still unresolved …

1996 First Proposal to Smithsonian (Buckley, Catanese, Weekes & Krennrich) 1998 VERITAS selected for internal support at SAO 1999 PPARC/EI approve funding for VERITAS 2000 Lehman review --> passed 2000 DOE funds VERITAS R&D 2000 VERITAS proposal to NSF/DOE --> NSF lacks funds 2001 Dec. 3 agencies appear ready to fund VERITAS --> OMB disapproves 2002 Decadel Survey by Nat. Academy --> endorses VERITAS 2003 Montosa canyon approved! --> lawsuit by environmental group decision to go to Kitt Peak instead! 2003 March VERITAS funded for 4 telescopes in U.S. by DoE & NSF! 2004 Feb. Prototype Telescope at testsite operational 2004 July site at Kitt Peak approved! 2005 Feb. telescope 1 operational 2005 Feb. infrastructure for VERITAS in place at Kitt Peak 2005 Tohono O’odham Nation files complaint --> site shutdown --> NSF volunteers to do a new EA --> resolution expected by Dec Fall Telescope 1 & 2 start FLWO basecamp 2006 Decision to built VERITAS-4 at basecamp + operate Dec. Kitt Peak site issue still unresolved …

1996 First Proposal to Smithsonian (Buckley, Catanese, Weekes & Krennrich) 1998 VERITAS selected for internal support at SAO 1999 PPARC/EI approve funding for VERITAS 2000 Lehman review --> passed 2000 DOE funds VERITAS R&D 2000 VERITAS proposal to NSF/DOE --> NSF lacks funds 2001 Dec. 3 agencies appear ready to fund VERITAS --> OMB disapproves 2002 Decadel Survey by Nat. Academy --> endorses VERITAS 2003 Montosa canyon approved! --> lawsuit by environmental group decision to go to Kitt Peak instead! 2003 March VERITAS funded for 4 telescopes in U.S. by DoE & NSF! 2004 Feb. Prototype Telescope at testsite operational 2004 July site at Kitt Peak approved! 2005 Feb. telescope 1 operational 2005 Feb. infrastructure for VERITAS in place at Kitt Peak 2005 Tohono O’odham Nation files complaint --> site shutdown --> NSF volunteers to do a new EA --> resolution expected by Dec Fall Telescope 1 & 2 start FLWO basecamp 2006 Decision to built VERITAS-4 at basecamp + operate Dec. Kitt Peak site issue still unresolved …

1996 First Proposal to Smithsonian (Buckley, Catanese, Weekes & Krennrich) 1998 VERITAS selected for internal support at SAO 1999 PPARC/EI approve funding for VERITAS 2000 Lehman review --> passed 2000 DOE funds VERITAS R&D 2000 VERITAS proposal to NSF/DOE --> NSF lacks funds 2001 Dec. 3 agencies appear ready to fund VERITAS --> OMB disapproves 2002 Decadel Survey by Nat. Academy --> endorses VERITAS 2003 Montosa canyon approved! --> lawsuit by environmental group decision to go to Kitt Peak instead! 2003 March VERITAS funded for 4 telescopes in U.S. by DoE & NSF! 2004 Feb. Prototype Telescope at testsite operational 2004 July site at Kitt Peak approved! 2005 Feb. telescope 1 operational 2005 Feb. infrastructure for VERITAS in place at Kitt Peak 2005 Tohono O’odham Nation files complaint --> site shutdown --> NSF volunteers to do a new EA --> resolution expected by Dec Fall Telescope 1 & 2 start FLWO basecamp 2006 Decision to built VERITAS-4 at basecamp + operate Dec. Kitt Peak site issue still unresolved …

NEAR FUTURE PLANS: Two year program at FLWO: 2007 & 2008 * Galactic plane sky survey * AGN search & monitoring, EBL studies * SNR, PWN searches and studies * Dark matter search * GRB follow-up Move in 2009 to permanent site at Kitt Peak