Common projects IceCube – Antares ? Simulation Physics Analysis DAQ synchronization J. Brunner.

Slides:



Advertisements
Similar presentations
Towards joint searches of gravitational waves (GW) and high-energy neutrinos (HEN) Eric Chassande-Mottin (CNRS, APC, France) for the GW+HEN group References:
Advertisements

Trigger issues for KM3NeT the large scale underwater neutrino telescope the project objectives design aspects from the KM3NeT TDR trigger issues outlook.
Longitude Latitude A recent analysis of the Fermi-LAT data by M. Su et al. [1] revealed two large spherical structures centered by our Galactic Center.
High-energy particle acceleration in the shell of a supernova remnant F.A. Aharonian et al (the HESS Collaboration) Nature 432, 75 (2004) Nuclear Physics.
Growth of Structure Measurement from a Large Cluster Survey using Chandra and XMM-Newton John R. Peterson (Purdue), J. Garrett Jernigan (SSL, Berkeley),
A Search for Point Sources of High Energy Neutrinos with AMANDA-B10 Scott Young, for the AMANDA collaboration UC-Irvine PhD Thesis:
The National Science FoundationThe Kavli Foundation AAS 211th meeting - Austin, TX Implications of Recent UHECR Data for Multi-Messenger Studies of Cosmic.
Search for Extremely-high Energy Cosmic Neutrino with IceCube Chiba Univ. Mio Ono.
Energy Reconstruction Algorithms for the ANTARES Neutrino Telescope J.D. Zornoza 1, A. Romeyer 2, R. Bruijn 3 on Behalf of the ANTARES Collaboration 1.
Gary C. Hill, CCAPP Symposium 2009, Ohio State University, October 12th, 2009 Photograph: Forest Banks Gary C. Hill University of Wisconsin, Madison for.
Realtime follow-up analyses with IceCube / M. Kowalski / Realtime follow-up analyses with IceCube Marek Kowalski Universität Bonn High Energy.
Antares/KM3NeT M. de Jong. neutrinos  p Scientific motivation: – origin cosmic rays – birth & composition relativistic jets – mechanism of cosmic particle.
Alexander Kappes UW-Madison 4 th TeVPA Workshop, Beijing (China) Sep. 24 – 28, 2008 The Hunt for the Sources of the Galactic Cosmic Rays — A multi-messenger.
Connections IceCube – KM3NeT Christian Spiering DESY.
Neutrino telescopes in the Mediterranean sea Marco Anghinolfi INFN-Genova on behalf of the ANTARES Collaboration HEP2012 Vlaparaiso, January 2012 The ANTARES.
Moriond 2001Jordan GoodmanMilagro Collaboration The Milagro Gamma Ray Observatory The Physics of Milagro Milagrito –Mrk 501 –GRB a Milagro –Description.
SEARCHING FOR A DIFFUSE FLUX OF ULTRA HIGH-ENERGY EXTRATERRESTRIAL NEUTRINOS WITH ICECUBE Henrik Johansson, for the IceCube collaboration LLWI H.
1 Recent Results from the ANTARES Neutrino Telescope Salvatore Mangano (IFIC/CSIC-Valencia) On behalf of the ANTARES Collaboration.
March 02, Shahid Hussain for the ICECUBE collaboration University of Delaware, USA.
AMANDA. Latest Results of AMANDA Wolfgang Rhode Universität Dortmund Universität Wuppertal for the AMANDA Collaboration.
AMANDA Per Olof Hulth The Wierdest wonder Is it good or is it bad?
The IceCube Neutrino Observatory is a cubic kilometer detector at the geographic South Pole. We give an overview of searches for time-variable neutrino.
Data collected during the year 2006 by the first 9 strings of IceCube can be used to measure the energy spectrum of the atmospheric muon neutrino flux.
Search for neutrinos from gamma-ray bursts with the ANTARES telescope D. Dornic for the ANTARES Collaboration.
The Tale of IceCube and GRB080319B or the Mystic Magic of TestDAQ Alexander Kappes UW-Madison IceCube Collaboration Meeting May 3, 2008, Madison.
Study of the Atmospheric Muon and Neutrinos for the IceCube Observatory Ryan Birdsall Paolo Desiati, Patrick Berghaus,
1 Towards a common skymap based on Antares & IceCube data J. Brunner 24/09/2011.
Kirsten Münich University of Dortmund, Germany Analysis strategies and recent results from AMANDA-II.
Astroparticle physics with large neutrino detectors  Existing detectors  Physics motivation  Antares project  KM3NeT proposal M. de Jong.
Alexander Kappes Extra-Galactic sources workshop Jan. 2009, Heidelberg Gamma ray burst detection with IceCube.
Combining Gamma and Neutrino Observations Christian Spiering, DESY.
POINT SOURCE ANALYSIS WITH 5-LINE DATA SUMMARY AWG PHONE CALL Juan Pablo Gómez-Gozález 20 th April
Gamma-Ray Bursts with the ANTARES neutrino telescope S. Escoffier CNRS/CPPM, Marseille.
2005 Unbinned Point Source Analysis Update Jim Braun IceCube Fall 2006 Collaboration Meeting.
ANTARES/KM3Net Neutrino Alert System Jürgen Brunner CPPM Image credit: Heidi Sagerud (IRAP,Toulouse) 1.
A search for neutrinos from long-duration GRBs with the ANTARES underwater neutrino telescope arxiv C.W. James for the ANTARES collaboration.
Results from the ANTARES Neutrino Telescope VLVNT - Roma 14/7/2015 ANTARES Results - M. Spurio 1 Maurizio Spurio VLVnT– Roma 14/09/2015.
Search for diffuse cosmic neutrino fluxes with the ANTARES detector Vladimir Kulikovskiy The ANTARES Collaboration 3-9 August 2014ANTARES diffuse flux.
Results of Searches for Muon Neutrinos from Gamma-Ray Bursts with IC-22 Madison Collaboration Meeting 2009 Erik Strahler UW-Madison 28/4/2009.
31/03/2008Lancaster University1 Ultra-High-Energy Neutrino Astronomy From Simon Bevan University College London.
Time-Dependent Searches for Neutrino Point Sources with IceCube Mike Baker University of Wisconsin-Madison Erice, Sicily June 14, 2010.
1 Comparing Unbinned likelihood methods IceCube/Antares Common Point source analysis from IC22 & Antares 2007/2008 data sets J. Brunner.
Prospects of Identifying the Sources of the Galactic Cosmic Rays with IceCube Alexander Kappes Francis Halzen Aongus O’Murchadha University Wisconsin-Madison.
Search for time correlations in atmospheric muon arrival times in the ANTARES Telescope Laboratoire de Physique, Radiation et Matière LPRM, Oujda 1 CERN,
Imen Al Samarai CPPM France Search for neutrinos from transient sources with the ANTARES telescope and optical follow-up observations Imen Al Samarai On.
The IceCube Neutrino Observatory is a cubic kilometer detector currently under construction at the geographic South Pole. We will give an overview of searches.
Brennan Hughey MIT Kavli Institute Postdoc Symposium
Muons in IceCube PRELIMINARY
Search for neutrinos from gamma-ray bursts with the ANTARES telescope
IceCube: Multiwavelength Approach to
Searching for gravitational-wave transients with Advanced detectors
Direct Measurement of the Atmospheric Muon Spectrum with IceCube
Recent Results of Point Source Searches with the IceCube Neutrino Telescope Lake Louise Winter Institute 2009 Erik Strahler University of Wisconsin-Madison.
Theoretical status of high energy cosmic rays and neutrinos
LIGO detectors: past, present and future
Systematic uncertainties in MonteCarlo simulations of the atmospheric muon flux in the 5-lines ANTARES detector VLVnT08 - Toulon April 2008 Annarita.
IC40 Physics Run Preparations
Instrumentation and Methods in Astroparticle Physics Physics 801
Brennan Hughey for the IceCube Collaboration
science with 40 IceCube strings
Diffuse neutrino flux J. Brunner CPPM ESA/NASA/AVO/Paolo Padovani.
Alexander Kappes Francis Halzen Aongus O’Murchadha
The arrival of Gravitational Waves and the EEE network:
Brennan Hughey for the IceCube Collaboration
Claudio Bogazzi * - NIKHEF Amsterdam ICRC 2011 – Beijing 13/08/2011
Investigation of multi-messenger and rare events in EEE
IceCube Construction and Analysis Report
Time-Dependent Searches for Neutrino Point Sources with IceCube
Time-Dependent Searches for Neutrino Point Sources with IceCube
IC59+40 Point Source Analysis
Presentation transcript:

Common projects IceCube – Antares ? Simulation Physics Analysis DAQ synchronization J. Brunner

Simulation Cosmic ray spectrum –Large theoretical error on CR composition and spectrum in the knee region –Large variety of hadronic shower models to derive muon fluxes –Possible common effort on data/MC comparisons and eventually recommendation for best model Photon propagation –Light diffusion in ice and water critical point in simulation chain –CPU time consuming, approximate –Possible common effort to improve corresponding simulation techniques

Physics Analysis Use completed analyses of both collaborations after unblinding has been agreed Combine results if possible and useful Example: point source search –Complementary in sky coverage –2007 / IC22 analysis finished –Need individual neutrino list –PSF per event (or zenith/azimuth dependent) –Efficiency functions –Possible result: 4  sky map –Cluster search in overlap region (25% at any given moment, 70% of IceCube sky seen by Antares at some moment)

Physics Analysis Example GRB stacking analysis –Time and direction constraint –Single event typically significant –Combine Antares/Icecube GRB lists might increases overall sensitivity

DAQ synchronization Multi-messenger Antares –GRB alerts from Swift & Fermi Storage of unfiltered data, higher efficiency at low E –Optical follow up with Tarot –Offline analysis with Auger and Virgo Icecube –SuperNovae alert network –Optical follow up with Rotse –Gamma ray follow up with Magic –Offline analysis GRB, Ligo

Multi-messenger Try to combine both network Most direct –Send alerts from Icecube to Antares –Same selection as for optical follow up ? –Only for upward going in both devices with reduced cuts ? –Include high energy event sample ? –Blindness concern Antares does not need directional information for alert handling Icecube might send “fake” alerts