“NIM” Paper Cy Hoffman.

Slides:



Advertisements
Similar presentations
Cygnus Paper Analysis & A 4 Properties Aous Abdo Michigan State University Milagro Collaboration Meeting LANL. December 18-19, 2006.
Advertisements

JNM Dec Annecy, France The High Resolution Fly’s Eye John Matthews University of Utah Department of Physics and High Energy Astrophysics Institute.
AGASA update M. Teshima ICRR, U of CfCP mini workshop Oct
Gus Sinnis HAWC Review December 2007 Milagro a TeV Gamma-Ray Observatory Gus Sinnis Los Alamos National Laboratory.
A Search for Point Sources of High Energy Neutrinos with AMANDA-B10 Scott Young, for the AMANDA collaboration UC-Irvine PhD Thesis:
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.
HAWC Gus Sinnis VHE Workshop UCLA October, 2005 HAWC: A Next Generation Wide-Field VHE Gamma-Ray Telescope.
MACRO Atmospheric Neutrinos Barry Barish 5 May 00 1.Neutrino oscillations 2.WIMPs 3.Astrophysical point sources.
Julie McEnery GLAST Science Lunch Milagro: A Wide Field of View Gamma-Ray Telescope Julie McEnery.
Atmospheric Neutrino Oscillations in Soudan 2
July 2004, Erice1 The performance of MAGIC Telescope for observation of Gamma Ray Bursts Satoko Mizobuchi for MAGIC collaboration Max-Planck-Institute.
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.
Size and Energy Spectra of incident cosmic radiation obtained by the MAKET - ANI surface array on mountain Aragats. (Final results from MAKET-ANI detector)‏
Outrigger Timing Calibration & Reconstruction Milagro – 11/17/03 Shoup – 1 Purpose: To incorporate outrigger hits in event angle fitting Additionally incorporated.
Moriond 2001Jordan GoodmanMilagro Collaboration The Milagro Gamma Ray Observatory The Physics of Milagro Milagrito –Mrk 501 –GRB a Milagro –Description.
A statistical test for point source searches - Aart Heijboer - AWG - Cern june 2002 A statistical test for point source searches Aart Heijboer contents:
Preliminary analysis of p-Pb data update n. 6 Lorenzo Bonechi LHCf Catania meeting – 19 December 2013.
Analysis chain for MAGIC Telescope data Daniel Mazin and Nadia Tonello Max-Planck-Institut für Physik München D.Mazin, N.Tonello MPI for Physics, Munich.
Latest Results from the MINOS Experiment Justin Evans, University College London for the MINOS Collaboration NOW th September 2008.
Gus Sinnis Asilomar Meeting 11/16/2003 The Next Generation All-Sky VHE Gamma-Ray Telescope.
HAWC Sensitivity Andrew Smith April 20-21,2007 Collaboration Meeting.
Investigation of different types radio sources by IPS method at 111MHz S.A.Tyul’bashev Pushchino Radio Astronomy Observatory, Astro Space Center of P.N.Lebedev.
Multi-TeV  -ray Astronomy with GRAPES-3 Pravata K Mohanty On behalf of the GRAPE-3 collaboration Tata Institute of Fundamental Research, Mumbai Workshop.
AGASA Results Masahiro Teshima for AGASA collaboration
A. Smith UMD, April 20-21, 2007 Milagro collaboration meeting The Hidden Potential of the “Gamma’’ Data. The Milagro Gamma-Hadron separation is bases on.
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 ( 
A Future All-Sky High Duty Cycle VHE Gamma Ray Detector Gus Sinnis/Los Alamos with A. Smith/UMd J. McEnery/GSFC.
DIJET STATUS Kazim Gumus 30 Aug Our signal is spread over many bins, and the background varies widely over the bins. If we were to simply sum up.
JPS 2003 in Sendai Measurement of spectral function in the decay 1. Motivation ~ Muon Anomalous Magnetic Moment ~ 2. Event selection 3. mass.
1 Constraining ME Flux Using ν + e Elastic Scattering Wenting Tan Hampton University Jaewon Park University of Rochester.
Aous Abdo Ground-based Gamma-ray Astronomy: Towards the Future. Santa Fe, NM May 11–12, 2006 Detection of Tev  -rays from the Cygnus Region with Milagro.
The KASCADE-Grande Experiment: an Overview Andrea Chiavassa Universita’ di Torino for the KASCADE-Grande Collaboration.
Cosmic Rays from to eV. Open Problem and Experimental Results. (KASCADE-Grande view) Very High Energy Phenomena in the Universe XLIV th Rencontres.
A search for neutrinos from long-duration GRBs with the ANTARES underwater neutrino telescope arxiv C.W. James for the ANTARES collaboration.
Detecting Air Showers on the Ground
Event by Event Energy Estimation Algorithm and Determination of Spectra (Update) Branden T. Allen, MILAGRO Colaboration Meeting, May 2006.
Milagro at Tibet Gus Sinnis LANL/P-23. Challenge and Opportunity Milagro will run for ~2 more years (or less) No viable candidate to replace Milagro on.
Comparison of MC and data Abelardo Moralejo Padova.
Belle General meeting Measurement of spectral function in the decay 1. Motivation 2. Event selection 3. mass spectrum (unfolding) 4. Evaluation.
AGASA Results Masahiro Teshima Max-Planck-Institut für Physik, München, Germany for AGASA collaboration.
January 21, 2005Peter Rovegno and David Williams, Milagro Collaboration Meeting 1 Background Rejection using Angle Fit Quality Source analysis has an implicit.
Gus Sinnis RICAP, Rome June 2007 The Milagro Observatory: Recent Results & Future Plans Gus Sinnis Los Alamos National Laboratory for the Milagro Collaboration.
2011, 10th AprilIII Fermi symposium , 10th AprilIII Fermi symposium2.
Comparison of reconstruction strategies in IceCube Lake Geneva, April 2007.
Analysis for Soft-Spectrum Sources Gary Walker Los Alamos National Laboratory.
32 nd ICRC –Beijing – August 11-18, 2011 Silvia Vernetto IFSI-INAF Torino, ITALY On behalf of the ARGO-YBJ collaboration Observation of MGRO J with.
IC40 Spectrum Unfolding 7/1/2016Warren Huelsnitz1 SVD Method described in A. Höcker and V. Kartvelishvili, NIM A 372 (1996) 469NIM A 372 (1996) 469 Implemented.
Xiong Zuo IHEP, CAS, for the LHAASO Collaboration
Measurement of high energy cosmic rays by the new Tibet hybrid experiment J. Huang for the Tibet ASγCollaboration a a Institute of high energy physics,
On behalf of the ARGO-YBJ collaboration
Update on Muon Flux Underground Using Geant4 Simulation
Systematic uncertainties in MonteCarlo simulations of the atmospheric muon flux in the 5-lines ANTARES detector VLVnT08 - Toulon April 2008 Annarita.
Astronomy session: a summary
A Survey of EGRET GeV Sources
Ultra High Energy Cosmic Ray Spectrum Measured by HiRes Experiment
Action Items Maryland Stuff Outriggers I will produce a budget summary
HAWC Science Survey of 2p sr up to 100 TeV energies Extended Sources
Erik Strahler UW-Madison 4/27/2008
Telescope Array Experiment Status and Prospects
Claudio Bogazzi * - NIKHEF Amsterdam ICRC 2011 – Beijing 13/08/2011
G0 Beam Polarization T. Horn, D. Gaskell Jefferson Lab
UVIS Calibration Update
UVIS Calibration Update
Estimation of Sensitivity to Gamma Ray point Sources above 30TeV
Search for coincidences and study of cosmic rays spectrum
Atmospheric muons in ANTARES
MAP 2014 Spring Workshop Fermilab May, 2014
More on Milagro Observations of TeV Diffuse Emission in Cygnus
Hellenic Open University
Presentation transcript:

“NIM” Paper Cy Hoffman

Focus on analysis methods and what has changed since Grito. This is paper is a vehicle to making analysis papers go out faster. If what we publish in this paper is not what we do in our analysis, then the this paper will not be as useful. Elements may be published elsewhere which will reduce the length, publication time.

Outline Introduction: (bla bla bla novel new detector bla bla bla) Detector Description: (Heavily reference Grito and stress differences, improvements) Reservoir -GS (not much needed) Liner/Cover -GS (not much needed) Inflation/Installation -MS/DC(?) (new to Milagro) PMTs/Baffles - DW (Baffles new and important) Outrigger Array -TS(?)/GBY (lots of stuff here. ORs new to Milagro) Water System -MS DAQ/Trigger -BD Repairs and Maintenance -BD Plots: OR diagram OR layout

Outline (cont.) Plots Historic on-time Operation of Milagro: Calibration -AJS,BD,NYU Pedestal shift -CL Alignment - Zenith Align, Pointing Accuracy, Precision -AJS Online Reconstruction -AJS Data handling -AJS Online analysis -AJS GCN -?? Plots Historic on-time Calibration Diagram (In print? ICRC?)

Outline (cont.) Detector Simulation Corsika -VV GEANT -VV PMT -VV Water Tests -MS Detailed explanation of g4sim will be relegated to a separate paper.

Outline (cont.) Event Reconstruction Plots: Core Fitting -AJS?? Angle Fitting -AJS?? Curvature Sampling Gamma/Hadron Separation: -AA Compactness A4 Plots: DelEO (???) Gamma/Hadron variables for MC gammas, MC hadrons, data

Outline (cont.) Background Estimation -GW Direct Integration ROI exclusion Anisotropy (Mention this. It is important to the limit) Ref. paper by RF/LF and Cygnus (expt. not region) Plots: Allsky signif. distribution

Outline (cont.) Significance Computation -JL/AJS Plots: Event Weighting (gamma/hadron weighting) PSF Weighting Plots: Sensitivity improvement for various spectra for given assumed spectra. (This could be separate paper, in which case this lengthy section could be replaced by a shorter section with a reference to the paper.)

Outline (cont.) Energy Spectrum Estimation BA/GBY Energy estimators Fit method Precision (Reference separate spectral analysis paper) (Does the moon belong here as a verification of the energy scale?) Plot showing dE vs E.

Outline (cont.) The Crab Nebula - A Demonstration of Milagro’s sensitivity Verification of gamma/hadron variables Verification of point spread function Measurement of flux and spectrum Plots: “sigma” map PSF plot Gamma/hadron comparison Spectrum

What’s Missing? GRB Analysis Extended source sensitivity ????