Software alignment for tracking detectors

By V. Blobel. 2006

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Search for the lepton flavour violating decay μ+→e+γ\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\mu ^+ \rightarrow (2016, unknown): “Millepede algorithm [29] and uses cosmic-rays reconstructed without magnetic field.”
Identification of b-quark jets with the CMS experiment (2012, background): “minimum bias collisions [35, 36], and is regularly monitored.”
Performance of the EUDET-type beam telescopes (2016, methodology): “In addition, precise offline detector alignment can be performed by minimising track residuals using the EUTelescope alignment processor which utilises the Millepede-II algorithm [25].”
Identification of b-quark jets with the CMS experiment (2013, methodology): “The alignment of the CMS tracker is performed using a mixture of tracks from cosmic rays and minimum bias collisions [33, 34], and is regularly monitored.”
Technical design of the phase I Mu3e experiment (2020, methodology): “There are efficient algorithms for the inversion of such gigantic sparse matrices, one of which is implemented in the Millepede II programme [123], which we are using.”