scholarly journals Commissioning of the muon track reconstruction in the ATLAS experiment

2010 ◽  
Vol 219 (3) ◽  
pp. 032026
Author(s):  
M J Woudstra ◽  
the Atlas Muon collaboration
2005 ◽  
Vol 20 (16) ◽  
pp. 3886-3888 ◽  
Author(s):  
◽  
D. POMAREDE

The Muon Spectrometer of the ATLAS experiment is a large and complex system relying on several detector technologies. The simulation and reconstruction of muon events require a very careful description of these detectors, some of which provide a muon trigger while the others make precision measurements of tracks. A precise description of the passive materials, toroidal magnet systems and shield is also needed to account for Coulomb scattering and energy losses. Finally, the spectrometer performance is enhanced by the alignment of its precision chambers, so the detector description model must fully implement misalignments and deformations. We present the Detector Description chain employed in the Muon system and its integration in the ATLAS software framework. It relies on a database technology and a standard set of geometrical primitives common to all ATLAS subsystems. The Muon Detector Description has been used successfully in the context of the ATLAS Data Challenges, where it provides a unique and coherent geometry source for the simulation and reconstruction algorithms. It has also been validated in the context of the experimental program of the ATLAS testbeams, where analyses of the treatment of chamber alignment in track reconstruction relies crucially upon the detector description model.


2019 ◽  
Vol 207 ◽  
pp. 05002 ◽  
Author(s):  
Federica Bradascio ◽  
Thorsten Glüsenkamp

IceCube is a cubic-kilometer Cherenkov telescope operating at the South Pole. Its goal is to detect astrophysical neutrinos and identify their sources. High-energy muon neutrinos are identified through the secondary muons produced via charge current interactions with the ice. The present bestperforming directional reconstruction of the muon track is a maximum likelihood method which uses the arrival time distribution of Cherenkov photons registered by the experiment’s photomultipliers. Known systematic shortcomings of this method are to assume continuous energy loss along the muon track, and to neglect photomultiplier-related effects such as prepulses and afterpulses. This work discusses an improvement of about 20% to the muon angular resolution of IceCube and its planned extension, IceCube-Gen2. In the reconstruction scheme presented here, the expected arrival time distribution is now parametrized by a predetermined stochastic muon energy loss pattern. The inclusion of pre- and afterpulses modelling in the PDF has also been studied, but no noticeable improvement was found, in particular in comparison to the modification of the energy loss profile.


2011 ◽  
Vol 34 (9) ◽  
pp. 652-662 ◽  
Author(s):  
J.A. Aguilar ◽  
I. Al Samarai ◽  
A. Albert ◽  
M. André ◽  
M. Anghinolfi ◽  
...  

2019 ◽  
Author(s):  
Federica Bradascio ◽  
Thorsten Gluesenkamp ◽  

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