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most citedPlanck 2018 results. X. Constraints on inflation

2.4k citations · 12.8k across the 392 of their papers we have counts for

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Showing 2014 · hep-exShow all

6 papers · 2 filters

hep-ex2014★ 52 cited

Observation of nu_tau appearance in the CNGS beam with the OPERA experiment

OPERA Collaboration, N. Agafonova, A. Aleksandrov +145

The OPERA experiment is searching for nu_mu -> nu_tau oscillations in appearance mode i.e. via the direct detection of tau leptons in nu_tau charged current interactions. The evide…

hep-ex2014★ 1 cited

Further studies of the photoproduction of isolated photons with a jet at HERA

ZEUS Collaboration, H. Abramowicz, I. Abt +170

In this extended analysis using the ZEUS detector at HERA, the photoproduction of isolated photons together with a jet is measured for different ranges of the fractional photon ene…

hep-ex2014★ 56 cited

Measurement of beauty and charm production in deep inelastic scattering at HERA and measurement of the beauty-quark mass

ZEUS collaboration, H. Abramowicz, I. Abt +171

The production of beauty and charm quarks in ep interactions has been studied with the ZEUS detector at HERA for exchanged four-momentum squared 5 < Q^2 < 1000 GeV^2 using an integ…

hep-ex2014★ 47 cited

Deep inelastic cross-section measurements at large y with the ZEUS detector at HERA

ZEUS Collaboration, H. Abramowicz, I. Abt +170

The reduced cross sections for deep inelastic scattering have been measured with the ZEUS detector at HERA at three different centre-of-mass energies, , and $22…

hep-ex2014★ 43 cited

Procedure for short-lived particle detection in the OPERA experiment and its application to charm decays

N. Agafonova, A. Anokhina, S. Aoki +135

The OPERA experiment, designed to perform the first observation of oscillations in appearance mode through the detection of the leptons produced in c…

hep-ex2014★ 29 cited

Measurement of TeV atmospheric muon charge ratio with the full OPERA data

N. Agafonova, A. Anokhina, S. Aoki +134

The OPERA detector, designed to search for oscillations in the CNGS beam, is located in the underground Gran Sasso laboratory, a privileged location to study TeV-scal…