18 research outputs found
Testes de envelhecimento acelerado e deterioração controlada na avaliação do vigor de aquênios de girassol
Sistema silvipastoril na Amazônia: ferramenta para elevar o desempenho produtivo de búfalos
Value of SP1-beta, alfa- Fetoprotein, unconjugated Estriol and hCG immunoassays for the risk calculation of fetal Down's syndrome in middle second trimester of pregnancy
Influence of insulin resistance status on the development of gallstones following roux-en-Y gastric bypass: a prospective cohort study
The occurrence of gallstones following Roux-en-Y gastric bypass (RYGB) has been extensively reported. As RYGB promotes improvement in insulin resistance (IR), which is one of the factors enrolled in the pathophysiology of gallstones, this study aims to determine the influence of IR and its post-RYGB course on the development of gallstones. This is a prospective cohort study that enrolled 108 morbidly obese subjects free of gallstones which underwent RYGB and were followed up for 24 months, through clinical, laboratory, and ultrasound examinations. IR was assessed through the surrogate marker homeostasis model assessment (HOMA). Of the individuals evaluated, 29 (26.8 %) developed gallstones following RYGB. In the univariate analysis, postsurgical gallstones were associated with preoperative HOMA (p < 0.0001), preoperative fasting glucose (p = 0.0019), preoperative fasting insulin (p = 0.0001), and preoperative triglycerides (p = 0.0001). Multivariate analysis revealed that preoperative HOMA was the only factor independently associated with gallstones (p < 0.0001). The incidence of gallstones among individuals with IR was 46.8 %; in the non-IR subjects, the incidence was 7.4 % (p < 0.0001). Preoperative IR led to a relative risk of 6.02 (95 % CI = 2.1-17.3; p = 0.0009) of gallstones. As gallstones often occur following RYGB, there is controversy regarding their management. Some authors propose systematic cholecystectomy along with RYGB, while others suggest that the aggregate risk of the concomitant approach is significantly higher. As IR was a significant risk factor in this study, an individualized approach for this population may be proposed. Further research is needed to confirm these findings.The occurrence of gallstones following Roux-en-Y gastric bypass (RYGB) has been extensively reported. As RYGB promotes improvement in insulin resistance (IR), which is one of the factors enrolled in the pathophysiology of gallstones, this study to determ264769775sem informaçãosem informaçã
Toxicidade de óleos essenciais de alho e casca de canela contra fungos do grupo Aspergillus flavus Evaluation of essential oils from Allium sativum and Cinnamomum zeilanicum and their toxicity against fungi of the Aspergillus flavus group
Diante da propriedade inibitória de óleos essenciais vegetais sobre o desenvolvimento micelial de fungos e da importância das espécies do grupo Aspergillus flavus, que apresentam potencial para síntese de aflatoxina, este trabalho teve como objetivo avaliar in vitro a toxicidade de óleos essenciais vegetais contra fungos do grupo A. flavus, isolados a partir da cultura do amendoim. Inicialmente, foi avaliada a toxicidade de oito óleos essenciais vegetais no desenvolvimento micelial de dois isolados do grupo A. flavus, em comparação ao fungicida sintético benomyl. Em seguida, foi avaliada a toxicidade dos óleos de casca de canela (Cinnamomum zeilanicum Breym.) e de bulbilho de alho (Allium sativum L.) contra 37 isolados do grupo A. flavus, durante 12 meses. A maior inibição do desenvolvimento micelial de A. flavus foi obtida com o emprego dos óleos essenciais de casca de canela e de bulbilho de alho, e o efeito inibitório variou com o isolado testado.<br>Considering the inhibitory property of essential plant oils on the mycelial development of fungi, and the importance of Aspergillus flavus-like fungi which may produce aflatoxins, this research was designed to evaluate the toxicity of essential oils against fungi belonging to the group A. flavus isolated from peanut crops. The toxicity of eight essential oils against two isolates of A. Flavuslike fungi was evaluated in comparison to the synthetic fungicide benomyl. The toxicity of Cinnamomum zeilanicum Breym. and Allium sativum L. essential oils was also evaluated against 37 fungal isolates for a period of 12 months. The highest inhibition of the mycelial development of A. flavus was obtained with cinnamon and garlic essential oils. The inhibitory effect on growth was variable according to the fungal isolate
Influência da calagem, da época de colheita e da secagem na incidência de fungos e aflatoxinas em grãos de amendoim armazenados Storage peanut kernels fungal contamination and aflatoxin as affected by liming, harvest time and drying
O objetivo deste trabalho foi avaliar a contaminação e o potencial para síntese de aflatoxinas pelos isolados do grupo Aspergillus flavus em grãos armazenados de amendoim (Arachis hypogaea L.), que foram produzidos com distintos procedimentos de calagem, de colheita e de secagem. Para isto, foram avaliadas doze amostras de grãos de amendoim, cv. Botutatu, provenientes de plantas cultivadas em área que recebeu ou não a aplicação de calcário, colhidas aos 104, 114 e 124 dias após a semeadura e secas em condições ambientais e em estufa. Aos 12 e 18 meses de armazenamento, os grãos foram tratados com hipoclorito de sódio e incubados em BDA, a 20°C, por cinco dias. As espécies do grupo Aspergillus flavus foram identificadas após incubação em meio ADM. Posteriormente, o potencial toxígeno foi avaliado pelo método da cromatografia de camada delgada. A análise da freqüência de fungos revelou que os grãos de amendoim armazenados estavam contaminados por Aspergillus spp., Penicillium spp. e Fusarium spp. Os grãos de amendoim, provenientes da colheita antecipada, apresentaram maior contaminação pelo grupo Aspergillus flavus, sendo menor a proporção destes com potencial toxígeno.<br>The objective of this work was to evaluate the effect of the storage on the potential of aflatoxin production by isolates from Aspergillus flavus group in peanut (Arachis hypogaea L.). These kernels were obtained from a field experiment with two areas (with or without lime), three times of harvest (104, 114 and 124 days after planting) and two types of dryer conditions (ambient and chamber with forced air). After 12 and 18 months of storage, the kernels were treated with sodium hypochloride and incubated in a PDA at 20°C during five days. The isolates from Aspergillus flavus group were identified after incubation in ADM culture medium. The toxigenic potential was analyzed by thin layer chromatography. The genera detected were Aspergillus, Penicillium and Fusarium. The kernels from the first harvest, showed higher contamination by the Aspergillus flavus group, but the small proportion with toxigen potential
Contaminação fúngica do amendoim em função das doses de calcário e épocas de amostragem Fungus contamination on peanut as affected by liming and sampling time
A população de fungos no solo varia de acordo com os fatores abióticos e bióticos, e, no caso do amendoim, podem contaminar as sementes, comprometendo sua qualidade. O objetivo do trabalho foi o de avaliar o efeito da calagem e da época de amostragem do solo e das vagens do amendoim na população de fungos, visando analisar a contaminação por Aspergillus spp., Rhizopus spp. e Penicillium spp. O experimento foi efetuado em Planassolo, no período das águas (outubro de 2001 a fevereiro de 2002), empregando o amendoim, cv. Botutatu. O delineamento experimental utilizado foi o de blocos ao acaso em parcela subdividida, com quatro repetições. As doses de calcário dolomítico (0,0 e 1,8 t.ha-1) foram aplicadas nas parcelas, em dezembro de 2000 e, as subparcelas, em quatro épocas de amostragem, com intervalos de 10 dias, a partir de 104.º dia após a semeadura (DAS). Nas amostras, foram realizadas a avaliação da população de fungos no solo e sua incidência nos pericarpos das vagens e nas sementes. Os resultados permitiram concluir que nas condições deste experimento, a época de amostragem e a aplicação de calcário não interferiram na população de Aspergillus spp. nas amostras de solo e sua incidência nos pericarpos das vagens. Nas amostras efetuadas aos 104 e 114 DAS, período com menores teores de água no solo, houve maior número de isolados pertencentes ao grupo Aspergillus flavus no solo e maiores incidências desses fungos nas vagens e sementes.<br>Diversity of fungus populations in soil could vary according to abiotic and biotic factors. On peanut cultivated soils, these can contaminate seeds, affecting their quality. This experiment was carried out to evaluate the effects of liming and sampling time, both of soil and peanut pods, fungus populations in the soil, specially in respect to possible contamination with Aspergillus , Rhizopus and Penicillium species. The experiment was installed in Planassol that was cultivated with peanut cv. Botutatu, during the raining season (October of 2001 to February of 2002). The experimental design was a subplot with four replications, in completely randomized blocks. Lime levels (0,0 and 1,8 t.ha-1) were applied to the plots in December of 2000, and the subplots were harvested during four intervals of 10 days, starting at 104 days after planting (DAP). Samples were evaluated regarding fungus population in the soil and their incidence in pods and seeds. The results allowed to conclude at these experimental conditions, the sampling time and application of lime do not interfere in the soil population of Aspergillus species. In samples collected at 104 and 114 DAP, period with lower water contents in the soil, there was an increase of Aspergillus flavus group isolates in the soil and more intense incidence of this fungus in pods and seeds
Reports of new wing color polymorphism and taxonomic information to cercopids (Auchenorrhyncha: Cercopidae) from upland rice crop, Pará State, Brazil
SDSS-III : massive spectroscopic surveys of the distant universe, the Milk Way, and extra-solar planetary systems
Building on the legacy of the Sloan Digital Sky Survey (SDSS-I and II), SDSS-III is a program of four spectroscopic surveys on three scientific themes: dark energy and cosmological parameters, the history and structure of the Milky Way, and the population of giant planets around other stars. In keeping with SDSS tradition, SDSS-III will provide regular public releases of all its data, beginning with SDSS Data Release 8 (DR8), which was made public in 2011 January and includes SDSS-I and SDSS-II images and spectra reprocessed with the latest pipelines and calibrations produced for the SDSS-III investigations. This paper presents an overview of the four surveys that comprise SDSS-III. The Baryon Oscillation Spectroscopic Survey will measure redshifts of 1.5 million massive galaxies and Lyα forest spectra of 150,000 quasars, using the baryon acoustic oscillation feature of large-scale structure to obtain percent-level determinations of the distance scale and Hubble expansion rate at z < 0.7 and at z ≈ 2.5. SEGUE- 2, an already completed SDSS-III survey that is the continuation of the SDSS-II Sloan Extension for Galactic Understanding and Exploration (SEGUE), measured medium-resolution (R = λ/Δλ ≈ 1800) optical spectra of 118,000 stars in a variety of target categories, probing chemical evolution, stellar kinematics and substructure, and the mass profile of the dark matter halo from the solar neighborhood to distances of 100 kpc. APOGEE, the Apache Point Observatory Galactic Evolution Experiment, will obtain high-resolution (R ≈ 30,000), high signal-to-noise ratio (S/N 100 per resolution element), H-band (1.51μm < λ < 1.70μm) spectra of 105 evolved, late-type stars, measuring separate abundances for ∼15 elements per star and creating the first high-precision spectroscopic survey of all Galactic stellar populations (bulge, bar, disks, halo) with a uniform set of stellar tracers and spectral diagnostics. The Multi-object APO Radial Velocity Exoplanet Large-area Survey (MARVELS) will monitor radial velocities of more than 8000 FGK stars with the sensitivity and cadence (10–40ms−1, ∼24 visits per star) needed to detect giant planets with periods up to two years, providing an unprecedented data set for understanding the formation and dynamical evolution of giant planet systems. As of 2011 January, SDSS-III has obtained spectra of more than 240,000 galaxies, 29,000 z 2.2 quasars, and 140,000 stars, including 74,000 velocity measurements of 2580 stars for MARVELS