Optimization of microesclerotia production by Trichoderma asperellum.

The Trichoderma genus, despite its widespread use for decades as a biological control in agriculture, has only recently been gaining a share in the biopesticide market, thanks to its versatility in controlling diseases and acting as a plant growth enhancer. Most Trichoderma's commercial products have aerial conidia as active ingredient, but recent studies report the production of another propagule, more robust for formulation and application under field conditions - the microsclerotia (MS). Thus, our objective was to evaluate the nutritional conditions that favor the greater production of MS, using two cultures of T. asperellum with known antagonistic activity. For this, we used the fractional factorial design approach in which we evaluated 5 variables: Carbon source, Carbon concentration, C:N ratio, Strain, Nitrogen source, all influencing the production of MS. The results indicated that all variables were statistically significant to MS production. In the best condition tested, we obtained values higher than 104 MS mL-1. In conclusion that the conditions found for the production of MS, using sucrose and lyscell, with carbon concentration 20 g L-1 and C:N ratio (10:1) and isolate TR 356, are inexpensive carbon and nitrogen sources may allow us to scale-up this biofungicide

Stability and Clinical Efficacy of Moisturizing Cosmetic Formulations Containing Vitamins C and E

The addition of different active substances in cosmetics, e.g. vitamins and their derivatives, has been quite frequent. In this way, it is fundamental to evaluate the stability and efficacy of cosmetic formulations containing these ingredients. The objective of this work was to evaluate the physical stability and the clinical efficacy of moisturizing cosmetic formulations based on panthenol, and containing ascorbyl tetraisopalmitate and α-tocopherol acetate. Formulations were developed with panthenol (FA), panthenol and ascorbyl tetraisopalmitate and α-tocopherol acetate (FBC). The latter was submitted to rheological behavior analysis and all were characterized as stable. Next, they were subjectively and objectively analyzed for clinical efficacy in 25 volunteers. Sensory evaluation and biophysical and skin imaging techniques were used to measure stratum corneum water content, transepidermal water loss (TEWL), and skin microrelief. These were carried out before application of the formulations and then after 3 hours. The formulations studied showed acceptable stability according to the physical aspects under consideration. In the clinical efficacy studies, both formulations significantly improved skin hydration and reduced TEWL. There was also improvement in skin microrelief but these results were not statistically significant. FBC received higher scores than FAin the sensory analysis as there was a significant improvement in the skin's smoothness, besides being preferred in purchase intent

ASSESSING THE NUTRITIONAL CONDITION OF PREGNANT WOMEN IN THE CITY OF SANTO ANDRÉ THROUGH ROSSO’S GRAPH

A falta de vigilancia da condição nutricional da gestante durante o exame pré-natal tem dificultado intervenções adequadas no sentido de prevenir a ocorrência do baixo peso ao nascimento (BP). Foram avaliadas, prospectivamente, 95 gestantes de baixo nível sócio-econômico do Município de Santo André, para realização de exame pré-natal, utilizando-se a curva de Rosso para sua classificação nutricional. O percentual de mãe com baixo peso foi de 36,8%. As mães com mais de duas gestações apresentaram maior ocorrência de sobrepeso ou obesidade e as com menos de duas gestações, percentual significativamente maior de baixo peso. A anemia também se associou de maneira significativa às gestantes de baixo peso. O presente trabalho ressalta a importancia da implantação de instrumento na rede básica de saúde para controlar o ganho de peso da gestante, bem como da vigilancia de outros fatores de risco no intuito de reduzir os elevados percentuais de recém-nascidos com BP.The lack of monitoring ofthenutritional condition of pregnamtwomen during theprenatal exammat^lon has made it difficult for interventions aimir g at the prevention of low weight at birth (BP). 45 pregnmt women of low socio-economic levei registered m the posts of the FOUNDATION for ASSISTANCE to INFANCY (FAISA - Santo André, São Paulo) were evaluated, for accomplishment of prenatal exammation, using Rosso’s Graph for its nutritional classification. The achieved percentage of pregnantwomenwi^th low weightwas 36,8%. Mo^therswi^thmore thamtwo ges^tations and wi^th less than two presented greater occurrence of overweight obesi^ty amd low weight, respectively. Higher percentage of amemia in the pregmant women with low weight was verified. Therefore, it is evident that this instrument should be implemented as routine in ^the prenatal examinabon

Highlights from the Pierre Auger Observatory

The Pierre Auger Observatory is the world's largest cosmic ray observatory. Our current exposure reaches nearly 40,000 km$^2$ str and provides us with an unprecedented quality data set. The performance and stability of the detectors and their enhancements are described. Data analyses have led to a number of major breakthroughs. Among these we discuss the energy spectrum and the searches for large-scale anisotropies. We present analyses of our X$_{max}$ data and show how it can be interpreted in terms of mass composition. We also describe some new analyses that extract mass sensitive parameters from the 100% duty cycle SD data. A coherent interpretation of all these recent results opens new directions. The consequences regarding the cosmic ray composition and the properties of UHECR sources are briefly discussed.Comment: 9 pages, 12 figures, talk given at the 33rd International Cosmic Ray Conference, Rio de Janeiro 201

Operations of and Future Plans for the Pierre Auger Observatory

Technical reports on operations and features of the Pierre Auger Observatory, including ongoing and planned enhancements and the status of the future northern hemisphere portion of the Observatory. Contributions to the 31st International Cosmic Ray Conference, Lodz, Poland, July 2009.Comment: Contributions to the 31st ICRC, Lodz, Poland, July 200

Anisotropy and chemical composition of ultra-high energy cosmic rays using arrival directions measured by the Pierre Auger Observatory

The Pierre Auger Collaboration has reported evidence for anisotropy in the distribution of arrival directions of the cosmic rays with energies $E>E_{th}=5.5\times 10^{19}$ eV. These show a correlation with the distribution of nearby extragalactic objects, including an apparent excess around the direction of Centaurus A. If the particles responsible for these excesses at $E>E_{th}$ are heavy nuclei with charge $Z$, the proton component of the sources should lead to excesses in the same regions at energies $E/Z$. We here report the lack of anisotropies in these directions at energies above $E_{th}/Z$ (for illustrative values of $Z=6,\ 13,\ 26$). If the anisotropies above $E_{th}$ are due to nuclei with charge $Z$, and under reasonable assumptions about the acceleration process, these observations imply stringent constraints on the allowed proton fraction at the lower energies

Measurement of the Depth of Maximum of Extensive Air Showers above 10^18 eV

We describe the measurement of the depth of maximum, Xmax, of the longitudinal development of air showers induced by cosmic rays. Almost four thousand events above 10^18 eV observed by the fluorescence detector of the Pierre Auger Observatory in coincidence with at least one surface detector station are selected for the analysis. The average shower maximum was found to evolve with energy at a rate of (106 +35/-21) g/cm^2/decade below 10^(18.24 +/- 0.05) eV and (24 +/- 3) g/cm^2/decade above this energy. The measured shower-to-shower fluctuations decrease from about 55 to 26 g/cm^2. The interpretation of these results in terms of the cosmic ray mass composition is briefly discussed.Comment: Accepted for publication by PR

The Pierre Auger Observatory III: Other Astrophysical Observations

Astrophysical observations of ultra-high-energy cosmic rays with the Pierre Auger ObservatoryComment: Contributions to the 32nd International Cosmic Ray Conference, Beijing, China, August 201

Update on the correlation of the highest energy cosmic rays with nearby extragalactic matter

Data collected by the Pierre Auger Observatory through 31 August 2007 showed evidence for anisotropy in the arrival directions of cosmic rays above the Greisen-Zatsepin-Kuz'min energy threshold, \nobreak{$6\times 10^{19}$eV}. The anisotropy was measured by the fraction of arrival directions that are less than $3.1^\circ$ from the position of an active galactic nucleus within 75 Mpc (using the V\'eron-Cetty and V\'eron $12^{\rm th}$ catalog). An updated measurement of this fraction is reported here using the arrival directions of cosmic rays recorded above the same energy threshold through 31 December 2009. The number of arrival directions has increased from 27 to 69, allowing a more precise measurement. The correlating fraction is $(38^{+7}_{-6})$, compared with $21$ expected for isotropic cosmic rays. This is down from the early estimate of $(69^{+11}_{-13})$. The enlarged set of arrival directions is examined also in relation to other populations of nearby extragalactic objects: galaxies in the 2 Microns All Sky Survey and active galactic nuclei detected in hard X-rays by the Swift Burst Alert Telescope. A celestial region around the position of the radiogalaxy Cen A has the largest excess of arrival directions relative to isotropic expectations. The 2-point autocorrelation function is shown for the enlarged set of arrival directions and compared to the isotropic expectation.Comment: Accepted for publication in Astroparticle Physics on 31 August 201