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Cristina Galea

Researcher at Radboud University Nijmegen

Publications -  1005
Citations -  82194

Cristina Galea is an academic researcher from Radboud University Nijmegen. The author has contributed to research in topics: Large Hadron Collider & Higgs boson. The author has an hindex of 128, co-authored 1000 publications receiving 75663 citations. Previous affiliations of Cristina Galea include Paris Diderot University & West University of Timișoara.

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Erratum to: "Search for particles decaying into a Z boson and a photon in p over(p, ̄) collisions at sqrt(s) = 1.96 TeV" [Phys. Lett. B 641 (2006) 415] (DOI:10.1016/j.physletb.2006.08.079)

V. M. Abazov, +578 more
- 05 Jan 2009 - 
TL;DR: In this paper, the authors search for particles decaying into a Z boson and a photon in collisions p (p)over-bar at root s = 1.96 TeV.

Search for direct pair production of a chargino and a neutralino decaying to the 125 GeV Higgs boson in √s = 8 TeV pp collisions with the ATLAS detector

Georges Aad, +2809 more
TL;DR: In this paper, a search for the direct pair production of a chargino and a neutralino was presented, where the chargino decayed to the lightest neutralino and the W boson, and the neutralino to the 125 GeV Higgs boson.

Measurement of jet shapes in top-quark pair events at \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$\sqrt{s} = 7 \ \mbox{TeV}$\end{document} using the ATLAS detector

Georges Aad, +2898 more
TL;DR: A measurement of jet shapes in top-quark pair events using 1.8 fb−1 collision data recorded by the ATLAS detector at the LHC is presented in this article.
Posted Content

The energy spectrum of cosmic rays beyond the turn-down around $10^{17}$ eV as measured with the surface detector of the Pierre Auger Observatory

P. Abreu, +375 more
TL;DR: In this paper, the authors present a measurement of the cosmic-ray spectrum above 100 ε,PeV using the part of the surface detector of the Pierre Auger Observatory that has a spacing of 750~m.