The energy spectrum of cosmic rays beyond the turn-down around 10^17 eV as measured with the surface detector of the Pierre Auger Observatory

We present a measurement of the cosmic-ray spectrum above 100 PeV using the part of the surface detector of the Pierre Auger Observatory that has a spacing of 750 m. An inflection of the spectrum is observed, confirming the presence of the so-called second-knee feature. The spectrum is then combined with that of the 1500 m array to produce a single measurement of the flux, linking this spectral feature with the three additional breaks at the highest energies. The combined spectrum, with an energy scale set calorimetrically via fluorescence telescopes and using a single detector type, results in the most statistically and systematically precise measurement of spectral breaks yet obtained. These measurements are critical for furthering our understanding of the highest energy cosmic rays

Measurements of differential production cross sections for a Z boson in association with jets in pp collisions at root s=8 TeV

Peer reviewe

Charged-particle nuclear modification factors in PbPb and pPb collisions at √=sNN=5.02 TeV

The spectra of charged particles produced within the pseudorapidity window |η| < 1 at √ sNN = 5.02 TeV are measured using 404 µb −1 of PbPb and 27.4 pb−1 of pp data collected by the CMS detector at the LHC in 2015. The spectra are presented over the transverse momentum ranges spanning 0.5 < pT < 400 GeV in pp and 0.7 < pT < 400 GeV in PbPb collisions. The corresponding nuclear modification factor, RAA, is measured in bins of collision centrality. The RAA in the 5% most central collisions shows a maximal suppression by a factor of 7–8 in the pT region of 6–9 GeV. This dip is followed by an increase, which continues up to the highest pT measured, and approaches unity in the vicinity of pT = 200 GeV. The RAA is compared to theoretical predictions and earlier experimental results at lower collision energies. The newly measured pp spectrum is combined with the pPb spectrum previously published by the CMS collaboration to construct the pPb nuclear modification factor, RpA, up to 120 GeV. For pT > 20 GeV, RpA exhibits weak momentum dependence and shows a moderate enhancement above unity

Controle genético do teor proteico nos grãos e de caracteres agronômicos em milho cultivado com diferentes níveis de adubação nitrogenada Genetic control of grain protein content and of agronomic traits in maize cultivated at different levels of nitrogen fertilization

O objetivo deste trabalho foi determinar o controle genético do teor de proteína em grãos e caracteres agronômicos milho (Zea mays) cultivado com diferentes níveis de adubação nitrogenada. Foram avaliados nove genitores de milho e seus híbridos, em dialelo completo, com dois níveis de adubação nitrogenada. Os caracteres avaliados foram: índice relativo de clorofila, altura de plantas, altura de espigas, produção de espigas, produção de grãos, coloração de grãos, massa de cem grãos, densidade de grãos, teor de nitrogênio nas folhas e teor de proteína nos grãos. A elevação da adubação nitrogenada promoveu aumento nos caracteres índice relativo de clorofila, altura de espigas e teor de proteínas nos grãos. Apenas a variável produção de grãos apresentou controle genético distinto nos diferentes níveis de nitrogênio. A análise dialélica mostrou significância dos efeitos dos genótipos sobre todos os caracteres, com exceção da produção de espigas e de grãos, e foi possível observar significância da heterose na maioria das variáveis. Para o teor de proteínas nos grãos, não houve significância da capacidade específica de combinação, e a capacidade geral de combinação dos genótipos teve efeito mais importante na manifestação desse caráter.<br>The objective of this work was to determine the genetic control grain protein content and of the agronomic traits of corn (Zea mays) at different levels of nitrogen fertilization. Nine parent populations and their hybrids were evaluated in a complete diallel mating design, with two levels of nitrogen fertilization. The variables evaluated were: relative chlorophyll index, plant height, ear height, ear production, grain yield, grain color, mass of 100 grains, density of grains, nitrogen content in the leaves and grain protein content. Increasing levels of nitrogen fertilization increased the relative chlorophyll index, ear height and grain protein content. However, only grain production had distinct genetic control at different levels of nitrogen. Diallel analysis showed significant genotype effect in all traits, except for grain and ear production. For most of the variables, there was significance of heterosis effect. For grain protein content, there was no significance for specific combining ability, and genotypes general combining ability had more important effects in the expression of this character

The FRAM robotic telescope for atmospheric monitoring at the Pierre Auger Observatory

FRAM (F/Photometric Robotic Atmospheric Monitor) is a robotic telescope operated at the Pierre Auger Observatory in Argentina for the purposes of atmospheric monitoring using stellar photometry. As a passive system which does not produce any light that could interfere with the observations of the fluorescence telescopes of the observatory, it complements the active monitoring systems that use lasers. We discuss the applications of stellar photometry for atmospheric monitoring at optical observatories in general and the particular modes of operation employed by the Auger FRAM. We describe in detail the technical aspects of FRAM, the hardware and software requirements for a successful operation of a robotic telescope for such a purpose and their implementation within the FRAM system

Search for heavy neutrinos or third-generation leptoquarks in final states with two hadronically decaying tau leptons and two jets in proton-proton collisions at root s=13 TeV

Peer reviewe