Determining if we, or another agent, were responsible for a sensory event can require an accurate sense of timing.Our sense of appropriate timing relationships must, however, be malleable as there is a variable delay between the physical timing of an event and when sensory signals concerning that event are encoded in the brain.One dramatic demonstr
Neutron capture and total cross-section measurements on 94,95,96Mo at n_TOF and GELINA
Capture and total Bracelets cross section measurements for 94,95,96Mo have been performed at the neutron time-of-flight facilities, n_TOF at CERN and GELINA at JRC-Geel.The measurements were performed using isotopically enriched samples with an enrichment above 95% for each of the 94,95,96Mo isotopes.The capture measurements were performed at n_TOF
Statistically Optimized Near-Field Acoustic Holography Using Prolate Spheroidal Wave Functions
Near-field acoustic holography (NAH) is an effective tool for realizing accurate sound field reconstruction in three-dimensional space on the prerequisite that appropriate elementary wave functions are selected or constructed to match the characteristics of the sound sources.However, for elongated sources, common wave functions, i.e., plane, cylind
Sensitivity of physiological emotional measures to odors depends on the product and the pleasantness ranges used
Emotions are characterized by synchronized changes in several components of an organism.Among them, physiological variations provide energy support for the expression of approach/avoid action REPAIR CONCENTRATE SERUM tendencies induced by relevant stimuli, while self-reported subjective pleasantness feelings integrate all other emotional components
A low-mass galaxy cluster as a test-case study for the NIKA2 SZ Large Program
High-resolution mapping of the hot gas in galaxy clusters is a key tool for cluster-based cosmological analyses.Taking advantage of the NIKA2 millimeter camera operated at the IRAM 30-m telescope, the NIKA2 SZ Large Program seeks to get a high-resolution follow-up of 45 galaxy clusters covering a wide mass range at high redshift in order to re-cali