Properties of the Higgs boson are measured in the H → ZZ → 4ℓ (ℓ = e, μ) decay channel. A data sample of proton-proton collisions at √{s}=13 TeV, collected with the CMS detector at the LHC and corresponding to an integrated luminosity of 35.9 fb-1 is used. The signal strength modifier μ, defined as the ratio of the observed Higgs boson rate in the
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Measurements of properties of the Higgs boson decaying into the four-lepton final state in pp collisions at √{s}=13 TeVSirunyan, A. M. et al.112017
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Measurements of the associated production of a Z boson and b jets in pp collisions at {√{s}} = 8 {TeV}
Measurements of the associated production of a Z boson with at least one jet originating from a b quark in proton-proton collisions at √{s} = 8 {TeV} are presented. Differential cross sections are measured with data collected by the CMS experiment corresponding to an integrated luminosity of 19.8 {fb}^{-1}. Z bosons are reconstructed through their
Khachatryan, V. et al.Fecha de publicación:
112017 -
Measurements of the solar aureole at the Teide Observatory
Daily measurements of the solar aureole were made at the Vacuum Newton Telescope (/D=40 cm) at the Teide Observatory (Tenerife) for various airmasses. We use these measurements to understand how the aureole is produced and to extrapolate visible measurements to the infrared range (1.6 /μm). This information will be used to correct sunspot
González Jorge, H. et al.Fecha de publicación:
111998 -
Measures of star formation rates from infrared (Herschel) and UV (GALEX) emissions of galaxies in the HerMES fields
The reliability of infrared (IR) and ultraviolet (UV) emissions to measure star formation rates (SFRs) in galaxies is investigated for a large sample of galaxies observed with the Spectral and Photometric Imaging Receiver (SPIRE) and the Photodetector Array Camera and Spectrometer (PACS) instruments on Herschel as part of the Herschel Multi-Tiered
Buat, V. et al.Fecha de publicación:
112010 -
Measuring masses in low mass X-ray binaries via X-ray spectroscopy: the case of MXB 1659-298
The determination of fundamental parameters in low-mass X-ray binaries (LMXBs) typically relies on measuring the radial velocity curve of the companion star through optical or near-infrared spectroscopy. It was recently suggested that high resolution X-ray spectroscopy might enable a measurement of the radial velocity curve of the compact object by
Ponti, G. et al.Fecha de publicación:
112018 -
Megalithic astronomy of Easter Island: a reassessment
Not Available
Edwards, Edmundo R. et al.Fecha de publicación:
112004