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Institution

IFAE

OtherBarcelona, Spain
About: IFAE is a other organization based out in Barcelona, Spain. It is known for research contribution in the topics: Large Hadron Collider & Galaxy. The organization has 664 authors who have published 1270 publications receiving 51097 citations. The organization is also known as: Instituto de Fisica de Altas Energias & IFAE.


Papers
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Journal ArticleDOI
K. Abe1, J. Adam2, Hiroaki Aihara1, C. Andreopoulos3  +361 moreInstitutions (52)
TL;DR: In this paper, a measurement of the charged current quasi-elastic cross-sections on carbon in the T2K on-axis neutrino beam at mean neutrinos energies of 1.94 GeV and 0.93 GeV are reported.
Abstract: We report a measurement of the $ u_\mu$ charged current quasi-elastic cross-sections on carbon in the T2K on-axis neutrino beam. The measured charged current quasi-elastic cross-sections on carbon at mean neutrino energies of 1.94 GeV and 0.93 GeV are $(11.95\pm 0.19(stat.)_{-1.47}^{+1.82} (syst.))\times 10^{-39}\mathrm{cm}^2/\mathrm{neutron}$ and $(10.64\pm 0.37(stat.)_{-1.65}^{+2.03} (syst.))\times 10^{-39}\mathrm{cm}^2/\mathrm{neutron}$, respectively. These results agree well with the predictions of neutrino interaction models. In addition, we investigated the effects of the nuclear model and the multi-nucleon interaction.

39 citations

Journal ArticleDOI
K. Abe1, C. Andreopoulos2, C. Andreopoulos3, M. Antonova  +353 moreInstitutions (53)
TL;DR: T2K reports its first measurements of the parameters governing the disappearance of ν[over ¯]_{μ] in an off-axis beam due to flavor change induced by neutrino oscillations, in agreement with existing antineutrino parameter measurements and also with the ν_{μ} disappearance parameters measured by T2K.
Abstract: We thank the J-PARC staff for superb accelerator performance and the CERN NA61 Collaboration for providing valuable particle production data. We acknowledge the support of MEXT, Japan; NSERC (Grant No. SAPPJ-2014-00031), NRC and CFI, Canada; CEA and CNRS/IN2P3, France; DFG, Germany; INFN, Italy; National Science Centre (NCN), Poland; RSF, RFBR, and MES, Russia; MINECO and ERDF funds, Spain; SNSF and SERI, Switzerland; STFC, UK; and DOE, USA. We also thank CERN for the UA1/NOMAD magnet, DESY for the HERA-B magnet mover system, NII for SINET4, the WestGrid and SciNet consortia in Compute Canada, and GridPP and the Emerald High Performance Computing facility in the United Kingdom. In addition, participation of individual researchers and institutions has been further supported by funds from ERC (FP7), H2020 Grant No. RISE-GA644294-JENNIFER, EU; JSPS, Japan; Royal Society, UK; and the DOE Early Career program, USA.

39 citations

Journal ArticleDOI
Morad Aaboud, Alexander Kupco1, Peter Davison2, Samuel Webb3  +2936 moreInstitutions (220)
TL;DR: In this paper, a search for flavour-changing neutral current processes in top-quark decays is presented, with one top quark decaying through the t → qZ (q = u, c) flavourchanging neutral-current channel, and the other through the dominant Standard Model mode t → bW.
Abstract: A search for flavour-changing neutral-current processes in top-quark decays is presented. Data collected with the ATLAS detector from proton-proton collisions at the Large Hadron Collider at a centre-of-mass energy of $ \sqrt{s}=13 $ TeV, corresponding to an integrated luminosity of 36.1 fb$^{−1}$, are analysed. The search is performed using top-quark pair events, with one top quark decaying through the t → qZ (q = u, c) flavour-changing neutral-current channel, and the other through the dominant Standard Model mode t → bW. Only Z boson decays into charged leptons and leptonic W boson decays are considered as signal. Consequently, the final-state topology is characterized by the presence of three isolated charged leptons (electrons or muons), at least two jets, one of the jets originating from a b-quark, and missing transverse momentum from the undetected neutrino. The data are consistent with Standard Model background contributions, and at 95% confidence level the search sets observed (expected) upper limits of 1.7 × 10$^{−4}$ (2.4 × 10$^{−4}$) on the t → uZ branching ratio and 2.4 × 10$^{−4}$ (3.2 × 10$^{−4}$) on the t → cZ branching ratio, constituting the most stringent limits to date.

39 citations

Journal ArticleDOI
Matt J. Jarvis1, Gary Bernstein1, Alexandra Amon2, C. Davis2, P. F. Léget3, Keith Bechtol4, Ian Harrison5, M. Gatti6, A. Roodman2, A. Roodman7, Chihway Chang8, R. Chen9, A. Choi10, S. Desai11, Alex Drlica-Wagner12, Alex Drlica-Wagner8, Daniel Gruen7, Daniel Gruen2, Robert A. Gruendl13, Robert A. Gruendl14, A. Hernandez2, Niall MacCrann10, J. Meyers15, A. Navarro-Alsina16, S. Pandey1, A. A. Plazas17, L. F. Secco1, Erin Sheldon18, Michael Troxel9, S. Vorperian, K. Wei8, Joe Zuntz19, T. M. C. Abbott, Michel Aguena20, S. Allam12, Santiago Avila21, Sunayana Bhargava22, Sarah Bridle5, David J. Brooks23, A. Carnero Rosell24, A. Carnero Rosell25, M. Carrasco Kind14, M. Carrasco Kind13, J. Carretero6, M. Costanzi26, L. N. da Costa, J. De Vicente, H. T. Diehl12, Peter Doel23, S. Everett27, B. Flaugher12, Pablo Fosalba25, Josh Frieman8, Josh Frieman12, Juan Garcia-Bellido21, Enrique Gaztanaga25, D. W. Gerdes28, G. Gutierrez12, Samuel Hinton29, D. L. Hollowood27, K. Honscheid10, David J. James30, S. Kent12, S. Kent8, Kyler Kuehn31, Kyler Kuehn32, N. Kuropatkin12, Ofer Lahav23, M. A. G. Maia, M. March1, Jennifer L. Marshall33, Peter Melchior17, Felipe Menanteau13, Felipe Menanteau14, Ramon Miquel6, Ramon Miquel34, R. L. C. Ogando, F. Paz-Chinchón35, F. Paz-Chinchón14, Eli S. Rykoff2, Eli S. Rykoff7, E. J. Sanchez, V. Scarpine12, Michael Schubnell28, S. Serrano25, I. Sevilla-Noarbe, M. Smith36, E. Suchyta37, M. E. C. Swanson14, G. Tarle28, T. N. Varga38, T. N. Varga39, A. R. Walker, W. C. Wester12, R. D. Wilkinson22 
TL;DR: A new software package for modeling the point-spread function (PSF) of astronomical images, called Piff (PSFs In the Full FOV), is introduced, which is applied to the first three years of the Dark Energy Survey data.
Abstract: We introduce a new software package for modelling the point spread function (PSF) of astronomical images, called PIFF (PSFs In the Full FOV), which we apply to the first three years (known as Y3) of the Dark Energy Survey (DES) data. We describe the relevant details about the algorithms used by PIFF to model the PSF, including how the PSF model varies across the field of view (FOV). Diagnostic results show that the systematic errors from the PSF modelling are very small over the range of scales that are important for the DES Y3 weak lensing analysis. In particular, the systematic errors from the PSF modelling are significantly smaller than the corresponding results from the DES year one (Y1) analysis. We also briefly describe some planned improvements to PIFF that we expect to further reduce the modelling errors in future analyses.

39 citations

Journal ArticleDOI
Morad Aaboud, Georges Aad1, Brad Abbott2, Ovsat Abdinov3  +2902 moreInstitutions (198)
TL;DR: Results are interpreted using simplified models, and exclude gluinos and squarks with masses as large as 1.85 and 1.3 $$\text {Te}\text {V}$$Te at 95% confidence level, respectively.
Abstract: A search for new phenomena in final states containing an e(+)e(-) or m(+)m(-) pair, jets, and large missing transverse momentum is presented. This analysis makes use of proton-proton collision data ...

39 citations


Authors

Showing all 672 results

NameH-indexPapersCitations
J. S. Lange1602083145919
Diego F. Torres13794872180
M. I. Martínez134125179885
Jose Flix133125790626
Matteo Cavalli-Sforza129127389442
Ilya Korolkov12888475312
Martine Bosman12894273848
Maria Pilar Casado12898178550
Clement Helsens12887074899
Imma Riu12895473842
Sebastian Grinstein128122279158
Remi Zaidan12674471647
Arely Cortes-Gonzalez12477468755
Trisha Farooque12484169620
Martin Tripiana12471669652
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Performance
Metrics
No. of papers from the Institution in previous years
YearPapers
20232
202210
2021119
2020150
2019133
2018154