The Large Aperture GRB Observatory (LAGO) Humberto Salazar for the LAGO collaboration August 11, 2011.

Slides:

Advertisements

Similar presentations

Web: Contact: HAWC is a collaborative effort between institutions in the United States of America.

Advertisements

Proposal Submitted to NSF/DoE HEP Given the large increase in sensitivity for a moderate cost, we have decided to propose to build HAWC. A proposal was.

COSMIC RAY PHYSICS IN BOLIVIA 4TH School on Cosmic Rays and Astrophysics UFABC-Santo André-SP-Brasil August 2010 Alfonso Velarde Cosmic Ray Laboratory.

DAQ System to Search for GRBs using Water Cerenkov Detectors Mario Castillo*, Gonzalo Perez*, Humberto Salazar* and L. Villaseñor ** * Facultad de Ciencias.

Kay Graf University of Erlangen for the ANTARES Collaboration 13th Lomonosov Conference on Elementary Particle Physics Moscow, August 23 – 29, 2007 Acoustic.

George W.S. Hou & M.A. Huang Center for Cosmology and Particle Astrophysics Department of Physics, National Taiwan University, 1, Sec. 4, Roosevelt Rd.,Taipei,

Large Magellanic Cloud, 1987 (51.4 kparsec) SN 1987a after before 2006 Hubble.

Jun 27, 2005S. Kahn -- Ckov1 Simulation 1 Ckov1 Simulation and Performance Steve Kahn June 27, 2005 MICE Collaboration PID Meeting.

GLAST LAT Project Test Beam Meeting, June 6, 2006 S. Funk 1/6 PS Positron Simulations Stefan Funk June 6, 2006.

A Large High Altitude Air Shower Observatory LHAASO Project Zhen Cao Institute of High Energy Physics, China, Beijing TeVPA, SLAC,2009.

Design and status of the Pierre Auger Observatory J. C. Arteaga Velázquez 1, Rebeca López 2, R. Pelayo 1 and Arnulfo Zepeda 1 1 Departamento de Física,

MiniHAWC Jordan Goodman Beijing – June 2006 Jordan Goodman University of Maryland mini- High Altitude Water Cherenkov experiment  miniHAWC.

Gus Sinnis RICAP, Rome June 2007 High Altitude Water Cherenkov Telescope  Gus Sinnis Los Alamos National Laboratory for the HAWC Collaboration.

Milagro Gus Sinnis Milagro NSF Review July 18-19, 2005 Milagro: A Synoptic VHE Gamma-Ray Telescope Gus Sinnis Los Alamos National Laboratory.

SINP MSU, July 7, 2012 I.Belolaptikov behalf BAIKAL collaboration.

A High Altitude Mexican ACT Project, OMEGA J. R. Sacahui 1, F. Huidobro 2, R. Núñez 2, R. Alfaro 2, E. Belmont-Moreno 2, O. Blanch 3, A. Carramiñana 4,

X.-X. Li, H.-H. He, F.-R. Zhu, S.-Z. Chen on behalf of the ARGO-YBJ collaboration Institute of High Energy Physics Nanjing GRB Conference,Nanjing,

High Energy Particle Astrophysics PRC-US Collaboration Summary Report Gus Sinnis David Kieda Gus Sinnis Hu Hongbo Jordan Goodman Min Zha.

Moriond 2001Jordan GoodmanMilagro Collaboration The Milagro Gamma Ray Observatory The Physics of Milagro Milagrito –Mrk 501 –GRB a Milagro –Description.

Milagro Status Report - October October 1998 The Milagro Project Physics Goals Overall Design Milagrisimo - Milagrito - Milagro Comparison of Milagro.

Atmospheric shower simulation studies with CORSIKA Physics Department Atreidis George ARISTOTLE UNIVERSITY OF THESSALONIKI.

Electronics and data acquisition system of the extensive air shower detector array at the University of Puebla R. Conde 1, O. Martinez 1, T. Murrieta 1,

Gus Sinnis Asilomar Meeting 11/16/2003 The Next Generation All-Sky VHE Gamma-Ray Telescope.

Humberto Salazar (FCFM-BUAP) for the Pierre Auger Collaboration, CTEQ- Fermilab School Lima, Peru, August 2012 Ultrahigh Cosmic Rays: The highest energy.

HAWC Andrew Smith - University of Maryland TeV Astrophysics II, August 28,2006 High Altitude Water Cherenkov experiment  HAWC Andrew Smith, University.

Multi-TeV  -ray Astronomy with GRAPES-3 Pravata K Mohanty On behalf of the GRAPE-3 collaboration Tata Institute of Fundamental Research, Mumbai Workshop.

XXXI International Cosmic Ray Conference, ICRC 2009 Lodz, Poland, July 7-15, 2009 Time structure of the Extensive Air Shower front with the ARGO-YBJ experiment.

Detection of electromagnetic showers along muon tracks Salvatore Mangano (IFIC)

Search for emission from Gamma Ray Bursts with the ARGO-YBJ detector Tristano Di Girolamo Universita` “Federico II” and INFN, Napoli, Italy ECRS, September.

con i neutrini1 Showering Neutrino Astronomies at Horizons.

Hadronic interaction studies with the ARGO-YBJ experiment (5,800 m 2 ) 10 Pads (56 x 62 cm 2 ) for each RPC 8 Strips (6.5 x 62 cm 2 ) for each Pad ( 

Search for neutrinos from gamma-ray bursts with the ANTARES telescope D. Dornic for the ANTARES Collaboration.

A Complex Detector Array at the Tibet Cosmic Ray Observatory

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.

Design for Wide FOV Cherenkov telescope upgrading THE 2 nd WORKSHOP OF IHEP Shoushan Zhang Institute of High Energy Physics.

“The Cosmic Ray composition in the knee region and the hadronic interaction models” G. Navarra INFN and University, Torino, Italy For the EAS-TOP Collaboration.

Temporal and spatial structure of the Extensive Air Shower front with the ARGO- YBJ experiment 1 - INFN-CNAF, Bologna, Italy 2 - Università del Salento.

Exploring Laser Light Ruben Conceição. Pierre Auger Observatory Ultra High Energy Cosmic Rays Pierre Auger Observatory – Fluorescence Detector Longitudinal.

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.

LIGO- G D Experimental Upper Limit from LIGO on the Gravitational Waves from GRB Stan Whitcomb For the LIGO Scientific Collaboration Informal.

Prospects to Use Silicon Photomultipliers for the Astroparticle Physics Experiments EUSO and MAGIC A. Nepomuk Otte Max-Planck-Institut für Physik München.

STAR Analysis Meeting, BNL – oct 2002 Alexandre A. P. Suaide Wayne State University Slide 1 EMC update Status of EMC analysis –Calibration –Transverse.

Search for GRBs Using ARGO Data in Shower Mode Guo Y.Q. For ARGO-YBJ Collaboration BeiJing 2008/09/26.

What we do know about cosmic rays at energies above eV? A.A.Petrukhin Contents 4 th Round Table, December , Introduction. 2. How these.

AMIGA – A direct measurement of muons in Pierre Auger Observatory

Detecting Air Showers on the Ground

Performances of the KM2A prototype array J.Liu for the LHAASO Collaboration Institute of High Energy Physics, CAS 32nd International Cosmic Ray Conference,

NEVOD-DECOR experiment: results and future A.A.Petrukhin for Russian-Italian Collaboration Contents MSU, May 16, New method of EAS investigations.

Olivier Deligny for the Pierre Auger Collaboration IPN Orsay – CNRS/IN2P3 TAUP 2007, Sendai Limit to the diffuse flux of UHE ν at EeV energies from the.

CsI Veto Detector Performance Study He Dao DMRC. Tsinghua University For KIMS Collaboration.

ICRC 2011Ignacio Taboada | Georgia Tech1 Sensitivity of HAWC to Gamma Ray Bursts Ignacio Taboada Georgia Institute of Technology Aug 11, 2011 – ICRC.

1 Observation of GRBs at tens of GeV with a full-coverage air shower array at m elevation Zhaoyang Feng (Speaker), Yiqing Guo, Yi Zhang, Hong.

The end of the electromagnetic spectrum

1 Cosmic Ray Physics with IceTop and IceCube Serap Tilav University of Delaware for The IceCube Collaboration ISVHECRI2010 June 28 - July 2, 2010 Fermilab.

“Separation of cosmic-ray components in a single water Cherenkov detector" Yasser Jerónimo, Luis Villaseñor IFM-UMSNH X Mexican School of Particles and.

Measurement of the CR light component primary spectrum B. Panico on behalf of ARGO-YBJ collaboration University Rome Tor Vergata INFN, Rome Tor Vergata.

Measurement of the Response of Water Cherenkov Detectors to Secondary Cosmic-Ray Particles in the HAWC Engineering Array Using a Fast Custom-Made DAQ System.

Electronica para los detectores Cherenkov de LAGO Rubén Conde*, Humberto Salazar* and L. Villaseñor ** * Facultad de Ciencias FisicoMatematicas, BUAP,

The dynamic range extension system for the LHAASO-WCDA experiment

Xiong Zuo IHEP, CAS, for the LHAASO Collaboration

Test Beam Request for the Semi-Digital Hadronic Calorimeter

Discussion session: other (crazy

University and INFN of Naples

HAWC Science Survey of 2p sr up to 100 TeV energies Extended Sources

The Aperture and Precision of the Auger Observatory

Research algorithm of overlapping clusters in PrimEx

Xiong Zuo IHEP, CAS, for the LHAASO Collaboration

Detection of GRB with Water Cherenkov Detectors

Presentation transcript:

The Large Aperture GRB Observatory (LAGO) Humberto Salazar for the LAGO collaboration August 11, 2011

Main goal:  Search for GRBs with gammas in the range energy 1 GeV - 1 TeV. Single particle technique High altitude water cerenkov detectors

Fermi-LAT, > 10 GeV photons event (1s) (1sec !

LAG0 : Single particle technique

LAGO 2011 * 4550m asl 4470m asl 4780m asl 5250m asl 1400m asl * Bariloche, Colombia, Venezuela, Mexico and Guatemala have Universities

Chacaltaya´s LAGO WCDs array

 DAQ System (Old Auger electronics).  Rate; 5 ms (above 0.5 phe)  Calibration software

Sierra Negra Array  4550 asl.  4 Water Cherenkov Detectors (3 operating)

 DAQ System.  Rate; 5 ms

Marcapomacocha, Peru.

Some candidates But, No confirmation: Fluence limits Data analysis and results

SH poster & SH poster

Present and Future plans for LAGO… Large area, New electronics. New sites. 40m2 4m2

New Detector Sierra Negra: 4x (40m2) x1.1m height

Rate vs distance Rate/seg distance to the center (cm) 7, , , , Threshold 0.9 phe For simulations of the performance of the detectors see OG poster

New 4 Channels Sierra Negra. Baseline noise. Average rate (5seg)

New detectors and new Bolivia, Peru and Ecuador ? (>5000masl).

Conclusions An efficient dedicated experiment can be done at low cost by using WCD at high altitude.