Event selection algorithm

Slides:

Advertisements

Similar presentations

Antonis Leisos KM3NeT Collaboration Meeting the calibration principle using atmospheric showers the calibration principle using atmospheric showers Monte.

Advertisements

Multiplicity analysis and dN/d  reconstruction with the silicon pixel detector Terzo Convegno Nazionale sulla Fisica di ALICE Frascati (Italy) – November.

New results from the CHORUS Neutrino Oscillation Experiment Pasquale Migliozzi CERN XXIX International Conference on High Energy Physics UBC, Vancouver,

Stereo Spectrum of UHECR Showers at the HiRes Detector  The Measurement Technique  Event Reconstruction  Monte Carlo Simulation  Aperture Determination.

N. Saoulidou Fermilab 1 Update on track reconstruction in the Near Detector N. Saoulidou, Fermilab

Angular resolution of LAT Agnieszka Kowal University of Science and Technology, Cracow TESLA Workshop on Forward Calorimetry Cracow, 10 October 2003.

Detection of atmospheric muon bundles using ALICE detectors A. Fernández Tellez Universidad Autonoma de Puebla for the ALICE Collaboration VIII Simposio.

The presence of the South Pole Air Shower Experiment (SPASE) on the surface provides a set of externally tagged muon bundles that can be measured by AMANDA.

Searching for Atmospheric Neutrino Oscillations at MINOS Andy Blake Cambridge University April 2004.

A Search for Point Sources of High Energy Neutrinos with AMANDA-B10 Scott Young, for the AMANDA collaboration UC-Irvine PhD Thesis:

DSP online algorithms for the ATLAS TileCal Read Out Drivers Cristobal Cuenca Almenar IFIC (University of Valencia-CSIC)

Characterization of Orbiting Wide-angle Light-collectors (OWL) By: Rasha Usama Abbasi.

Report of the HOU contribution to KM3NeT TDR (WP2) A. G. Tsirigotis In the framework of the KM3NeT Design Study WP2 Meeting - Marseilles, 29June-3 July.

11.5 Day 2 Lines and Planes in Space. Equations of planes.

Anisotropy Studies in the Pierre Auger Observatory Beatriz Blanco Siffert for the Auger Collaboration Instituto de Física - Universidade Federal do Rio.

Report of the HOU contribution to KM3NeT TDR (WP2) A. G. Tsirigotis In the framework of the KM3NeT Design Study WP2 Meeting - Erlangen, May 2009.

Ronald Bruijn – 10 th APP Symposium Antares results and status Ronald Bruijn.

Response of AMANDA-II to Cosmic Ray Muons and study of Systematics Newt,Paolo and Teresa.

Point Source Search with 2007 & 2008 data Claudio Bogazzi AWG videconference 03 / 09 / 2010.

Gael Rospabe Lapp 15/04/08 CaloSoft Meeting 1 Ecal calibration using  0 Sabine Elles/ Marie-Noëlle Minard/ Gaël Rospabé.

V.Petracek TU Prague, UNI Heidelberg GSI Detection of D +/- hadronic 3-body decays in the CBM experiment ● D +/- K  B. R. 

Study of neutrino oscillations with ANTARES J. Brunner.

June 6, 2006 CALOR 2006 E. Hays University of Chicago / Argonne National Lab VERITAS Imaging Calorimetry at Very High Energies.

POINT SOURCE ANALYSIS WITH 5-LINE DATA SUMMARY AWG PHONE CALL Juan Pablo Gómez-Gozález 20 th April

D 0 reconstruction: 15 AGeV – 25 AGeV – 35 AGeV M.Deveaux, C.Dritsa, F.Rami IPHC Strasbourg / GSI Darmstadt Outline Motivation Simulation Tools Results.

Introduction to Irene’s talk (reminder) Coincidence window  500s  GWHEN group, Astropart. Phys. 35 (2011) 1-7 Ph. D Thesis of I. Di Palma (AEI) Ph. D.

The KASCADE-Grande Experiment: an Overview Andrea Chiavassa Universita’ di Torino for the KASCADE-Grande Collaboration.

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

Régis Lefèvre (LPC Clermont-Ferrand - France)ATLAS Physics Workshop - Lund - September 2001 In situ jet energy calibration General considerations The different.

Khaled Belkadhi (LLR-Ecole Polytechnique)1 DHCAL Test Beam Results using Full Train Reconstruction Khaled Belkadhi.

Study of Charged Hadrons in Au-Au Collisions at with the PHENIX Time Expansion Chamber Dmitri Kotchetkov for the PHENIX Collaboration Department of Physics,

Aug _5071 Top stop by charm channel analysis using D0 runI data OUTLINE physics process of top to stop Monte Carlo simulation for signal data.

The Performance of the ALICE experiment for cosmic ray physics B. Alessandro, V. Canoa, A. Fernández, M. Rodríguez, M. Subieta for the ALICE Collaboration.

MC study of TREND Ground array Feng Zhaoyang Institute of High Energy Physics,CAS

Can we detect a marble tomb with cosmic muons ? Corinne Goy, Max Chefdeville, Jean Jacquemier, Yannis Karyotakis 21 December 2015.

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.

First All-Sky Measurement of Muon Flux with IceCube IceCube REU Summer 2008 Kristin Rosenau Advisor: Teresa Montaruli.

A Search for Higgs Decaying to WW (*) at DØ presented by Amber Jenkins Imperial College London on behalf of the D  Collaboration Meeting of the Division.

Iterative local  2 alignment algorithm for the ATLAS Pixel detector Tobias Göttfert IMPRS young scientists workshop 17 th July 2006.

Time-zero evaluation using TOF, T0 and vertex detectors

R.W. Assmann, V. Boccone, F. Cerutti, M. Huhtinen, A. Mereghetti

Update on the analysis of muon angular distributions in equatorial coordinates F.Riggi Dept. of Physics and INFN, Catania.

Detection of atmospheric muons using ALICE detectors

Muons in IceCube PRELIMINARY

Using IP Chi-Square Probability

Darius Bellamy Powerpoint.

ATLAS Upgrade Program Sarah Demers, US ATLAS Fellow with BNL

STT pattern recognition improvements since last December meeting and

11.5 Day 2 Lines and Planes in Space

Newt Ganugapati and Teresa Montaruli

Neutrinos from BBfit J. Brunner.

A novel gaseous X-ray polarimeter: data analysis and simulation

GAMMA-400 performance a,bLeonov A., a,bGalper A., bKheymits M., aSuchkov S., aTopchiev N., bYurkin Y. & bZverev V. aLebedev Physical Institute of the Russian.

Systematic uncertainties in MonteCarlo simulations of the atmospheric muon flux in the 5-lines ANTARES detector VLVnT08 - Toulon April 2008 Annarita.

Performance of the AMANDA-II Detector

Michele Pioppi* on behalf of PRIN _005 group

Status of the Offline Pattern Recognition Code Goa, March 12th 2013

Response of AMANDA-II to Cosmic Ray Muons and study of Systematics

Litao Zhao Liaoning University&IHEP

OPERETTE TEST BEAM EXPERIMENT :

Quarkonium production in ALICE

Anisotropy of Primary Cosmic Rays

Comparisons of data/mc using down-going muons

Preliminary Comparison of Monte Carlo and 9-string IceCube Data

Claudio Bogazzi * - NIKHEF Amsterdam ICRC 2011 – Beijing 13/08/2011

Event Monitor and Display for Muon Tomography Station

Progress in angular acceptance study

The Aperture and Precision of the Auger Observatory

WARP: fitting gamma signals

Status report on CATA-01/POLA-01 coincidence measurements

Presentation transcript:

Event selection algorithm Almaz Fazliakhmetov MIPT

Outline Statistics after primary processing of data Event selection algorithm Reconstruction of muon track Result histograms 09.08.16

Event selection algorithm Number of detector Number of pixel '77_1', '81_15', '91_13' - event Pixels on top and bottom level are chosen Cycle 1500 iterations Two points inside these pixels are acted out and direct line is created Intersection with pixel on middle level is checked If the number of intersections < 5 the event will be rejected Experimental data: 109083 After cut: 95634 09.08.16

Reconstruction of muon track Task: to reconstruct direction of muon using positions of triggered pixels. Solution: use LSM Algorithm: REGRESSIONS et TRAJECTOIRES en 3D. Jean Jacquelin https://www.scribd.com/doc/31477970/Regressions-et-trajectoires-3D The best direct line L is parametrized by plane z=ax+by and point (u, w, v) on this plane. 09.08.16

Results histograms Experimental data: 109083 After cut: 95634 09.08.16

Results histograms Experimental data: 109083 After cut: 95634 09.08.16

Results histograms 09.08.16

Muon angular distribution map 09.08.16

Conclusion The method for selection of muon events was created A way for reconstruction of the track of muon was created The histograms for distribution of zenith and azimuth angle were obtained 09.08.16