11 research outputs found
A century of trends in adult human height
Abstract Being taller is associated with enhanced longevity, and higher education and earnings.
We reanalysed 1472 population-based studies, with measurement of height on more than 18.6
million participants to estimate mean height for people born between 1896 and 1996 in 200
countries. The largest gain in adult height over the past century has occurred in South Korean
women and Iranian men, who became 20.2 cm (95% credible interval 17.5–22.7) and 16.5 cm (13.3–
19.7) taller, respectively. In contrast, there was little change in adult height in some sub-Saharan
African countries and in South Asia over the century of analysis. The tallest people over these 100
years are men born in the Netherlands in the last quarter of 20th century, whose average heights
surpassed 182.5 cm, and the shortest were women born in Guatemala in 1896 (140.3 cm; 135.8–
144.8). The height differential between the tallest and shortest populations was 19-20 cm a century
ago, and has remained the same for women and increased for men a century later despite
substantial changes in the ranking of countries
Gold nanorods 3D-supercrystals as surface enhanced Raman scattering spectroscopy substrates for the rapid detection of scrambled prions
Highly organized supercrystals of Au nanorods with plasmonic antennae enhancement of electrical field have made possible fast direct detection of prions in complex biological media such as serum and blood. The nearly perfect three-dimensional organization of nanorods render these systems excellent surface enhanced Raman scattering spectroscopy substrates with uniform electric field enhancement, leading to reproducibly high enhancement factor in the desirable spectral range
Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layout
The Cherenkov Telescope Array (CTA) is the major next-generation observatory for ground-based very-high-energy gamma-ray astronomy. It will improve the sensitivity of current ground-based instruments by a factor of five to twenty, depending on the energy, greatly improving both their angular and energy resolutions over four decades in energy (from 20 GeV to 300 TeV). This achievement will be possible by using tens of imaging Cherenkov telescopes of three successive sizes. They will be arranged into two arrays, one per hemisphere, located on the La Palma island (Spain) and in Paranal (Chile). We present here the optimised and final telescope arrays for both CTA sites, as well as their foreseen performance, resulting from the analysis of three different large-scale Monte Carlo productions