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Last modified by Ricardo Julio Rodríguez Fernández on 2026/06/16 12:23
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edited by Ricardo Julio Rodríguez Fernández
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1 -Camille Normand
1 +Juan Antonio Garzón Heydt
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1 -=== A first look into 2026 LHCb data ===
2 -==== Titor: [[Camille>>https://igfae.usc.es/igfae/persoa/normand-camille-ann/676/||target="_blank"]] Normand ====
3 -==== Supervisor: [[Camille>>https://igfae.usc.es/igfae/persoa/normand-camille-ann/676/||target="_blank"]] Normand
1 +=== Characterization and Initial Analysis of a miniTrasgo Detector ===
2 +==== Titor: [[Juan Antonio>>https://igfae.usc.es/igfae/persoa/garzon-heydt-juan-antonio/145/||target="_blank"]] Garzón Heydt ====
3 +==== Supervisor: [[Juan Antonio>>https://igfae.usc.es/igfae/persoa/garzon-heydt-juan-antonio/145/||target="_blank"]] Garzón Heydt
4 4  ====
5 5  
6 -With the acquisition of new data at a faster pace than ever, maintaining and verifying its quality is of paramount importance for greater precision measurements and improved searches for physics beyond the Standard Model at LHCb. In this project, the student will give the very first look at the newly-acquired 2026 data, i.e. only a few months old, through the study of the decay B→KS J/ψ. This high-statistics channel allows for a very clear study of, on the one hand, reconstruction effects, providing results of great impact for the whole collaboration, and on the other hand, detailed aspects of signal selection tools such as ML algorithms and particle identification, directly contributing to a world-leading search for New Physics. In both aspects, the student will have the opportunity to develop their knowledge of standard Particle Physics techniques, as well as develop their own tools and measurables for data and simulation quality evaluations.
6 +A miniTrasgo detector with very high angular resolution has recently been installed at IGFAE for cosmic ray measurement.
7 +We propose to participate in the study of the performances of the detector and analyzing the relationship between variations in the angular distribution of cosmic rays and the atmospheric temperature profile above the detector.