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Sökning: onr:"swepub:oai:lup.lub.lu.se:753ef790-1f4f-4a48-a383-fa95af44c27d" > Performance of a pr...

Performance of a proposed event-type based analysis for the Cherenkov Telescope Array

Hassan, T. (författare)
Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT)
Gueta, O. (författare)
German Electron Synchrotron (DESY)
Maier, G. (författare)
German Electron Synchrotron (DESY)
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Nöthe, M. (författare)
Technical University of Dortmund
Peresano, M. (författare)
Paris Diderot University,University of Paris-Saclay
Vovk, I. (författare)
University of Tokyo
Carlile, C. (författare)
Lund University,Lunds universitet,Astronomi - Genomgår omorganisation,Institutionen för astronomi och teoretisk fysik - Genomgår omorganisation,Naturvetenskapliga fakulteten,Lund Observatory - Undergoing reorganization,Department of Astronomy and Theoretical Physics - Undergoing reorganization,Faculty of Science
Dravins, D. (författare)
Lund University,Lunds universitet,Astronomi - Genomgår omorganisation,Institutionen för astronomi och teoretisk fysik - Genomgår omorganisation,Naturvetenskapliga fakulteten,Lund Observatory - Undergoing reorganization,Department of Astronomy and Theoretical Physics - Undergoing reorganization,Faculty of Science
Zmija, A. (författare)
Friedrich-Alexander University Erlangen-Nürnberg
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 (creator_code:org_t)
 
Trieste, Italy : Sissa Medialab, 2022
2022
Engelska.
Ingår i: 37th International Cosmic Ray Conference (ICRC2021) - GAI - Gamma Ray Indirect. - Trieste, Italy : Sissa Medialab. - 1824-8039. ; 395
  • Konferensbidrag (refereegranskat)
Abstract Ämnesord
Stäng  
  • The Cherenkov Telescope Array (CTA) will be the next-generation observatory in the field of very-high-energy (20 GeV to 300 TeV) gamma-ray astroparticle physics. Classically, data analysis in the field maximizes sensitivity by applying quality cuts on the data acquired. These cuts, optimized using Monte Carlo simulations, select higher quality events from the initial dataset. Subsequent steps of the analysis typically use the surviving events to calculate one set of instrument response functions (IRFs). An alternative approach is the use of event types, as implemented in experiments such as the Fermi-LAT. In this approach, events are divided into sub-samples based on their reconstruction quality, and a set of IRFs is calculated for each sub-sample. The sub-samples are then combined in a joint analysis, treating them as independent observations. This leads to an improvement in performance parameters such as sensitivity, angular and energy resolution. Data loss is reduced since lower quality events are included in the analysis as well, rather than discarded. In this study, machine learning methods will be used to classify events according to their expected angular reconstruction quality. We will report the impact on CTA high-level performance when applying such an event-type classification, compared to the classical procedure. © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0)

Ämnesord

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Nyckelord

Cosmology
Gamma rays
Germanium alloys
Germanium compounds
Intelligent systems
Learning systems
Quality control
Telescopes
Tellurium compounds
Astroparticle physics
Cherenkov telescope arrays
Event Types
Gamma-rays
Instrument response functions
Performance
Reconstruction quality
Sub-samples
Type-based analysis
Very high energies
Monte Carlo methods

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