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- European Organization for Nuclear ResearchCH861 papers
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- Rutherford Appleton LaboratoryGB845 papers
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- Istituto Nazionale di Fisica Nucleare, Sezione di BolognaIT823 papers
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130 papers · 1 filter
Proportional integral derivative booster for neural networks-based time-series prediction: Case of water demand prediction
Tony Salloom, Okyay Kaynak, Xinbo Yub +1
Multi-step time-series prediction is an essential supportive step for decision-makers in several industrial areas. Artificial intelligence techniques, which use a neural network co…
A Novel Deep Neural Network Architecture for Real-Time Water Demand Forecasting
Tony Salloom, Okyay Kaynak, Wei He
Short-term water demand forecasting (StWDF) is the foundation stone in the derivation of an optimal plan for controlling water supply systems. Deep learning (DL) approaches provide…
Characterization of the quantum state of top quark pairs produced in proton-proton collisions at = 13 TeV using the beam and helicity bases
CMS Collaboration
Measurements of the spin correlation coefficients in the beam basis are presented for top quark-antiquark () systems produced in proton-proton collisions at $\sq…
Measurements of electroweak production of a photon in association with two jets in proton-proton collisions at = 13 TeV
CMS Collaboration
The first observation of electroweak production of a photon in association with two forward jets in proton-proton collisions is presented. The measurement uses data recorded by the…
Polynomial Order Selection for Savitzky-Golay Smoothers via N-fold Cross-Validation (extended version)
Cagatay Candan
Savitzky-Golay (SG) smoothers are noise suppressing filters operating on the principle of projecting noisy input onto the subspace of polynomials. A poorly selected polynomial orde…
Massive runaway star HD 254577: the pre-supernova binary companion to the progenitor of the supernova remnant IC 443
B. Dinçel, G. Paylı, S. K. Yerli +9
The secondaries of the massive binary systems can be found as runaway stars after being ejected due to the supernova (SN) of the more massive component. We search for such stars in…