Post-detection analysis for grating-based ultra-small angle X-ray scattering.

Until recently, the hard X-ray, phase-sensitive imaging technique called grating interferometry was thought to provide information only in real space. However, by utilizing an alternative approach to data analysis we demonstrated that the angular resolved ultra-small angle X-ray scattering distribution can be retrieved from experimental data. Thus, reciprocal space information is accessible by grating interferometry in addition to real space. Naturally, the quality of the retrieved data strongly depends on the performance of the employed analysis procedure, which involves deconvolution of periodic and noisy data in this context. The aim of this article is to compare several deconvolution algorithms to retrieve the ultra-small angle X-ray scattering distribution in grating interferometry. We quantitatively compare the performance of three deconvolution procedures (i.e., Wiener, iterative Wiener and Lucy-Richardson) in case of realistically modeled, noisy and periodic input data. The simulations showed that the algorithm of Lucy-Richardson is the more reliable and more efficient as a function of the characteristics of the signals in the given context. The availability of a reliable data analysis procedure is essential for future developments in grating interferometry.

Avaliação da macroporosidade e da densidade de partículas do solo através da microtomografia de raios-x

A Ciência do Solo procura compreender e modelar os fenômenos ocorridos no solo, principalmente na zona não saturada. Como o entendimento de muitos desses fenômenos exige determinações em escalas que permitam incorporar aos modelos a variabilidade de poros e agregados, desenvolveu-se, na Embrapa Instrumentação Agropecuária, um tomógrafo de raios-X, de resolução micrométrica, com o objetivo de se obterem imagens, de forma não-destrutiva, de amostras de solo, com resolução espacial igual ou inferior a 100 μm. Foi possível projetar e construir um equipamento, de alta resolução, com baixo custo, comparativamente aos equipamentos comerciais disponíveis, cujos preços são proibitivos para aplicações em solo. Obtiveram-se imagens de amostras de solos com estrutura deformada, compostos por agregados de 212 a 250 μm, nos quais foram identificados poros medindo 100 μm ou menos. Poros dessas dimensões foram visualizados, também, em tomografias de amostras compostas de grãos de areia de 1 mm e capilares de vidro com diâmetros internos de 100, 200 e 300 μm. Tomografias de amostras não deformadas de solos evidenciaram, além de poros de 200 a 800 μm, partículas de alta densidade não-detectáveis com a tomografia de resolução milimétrica.

Pharmacogenetic Study on Risperidone Long-Acting Injection: Influence of Cytochrome P450 2D6 and Pregnane X Receptor on Risperidone Exposure and Drug-Induced Side-Effects.

Risperidone is metabolized by polymorphic enzymes, and a large variability in plasma concentration and therapeutic response is observed. Risperidone long-acting injection (RLAI) avoids the first-pass effect, and little is known about the influence of gene polymorphisms involved in its pharmacokinetics. The influence on plasma concentrations of risperidone (RIS), its metabolite 9-hydroxy-risperidone, and on adverse effects were investigated for polymorphisms of cytochrome P450 2D6 (CYP2D6) (*3, *4, *5, *6), CYP3A (CYP3A4*1B, CYP3A4 rs4646437, CYP3A5*3, CYP3A7*1C), ABCB1 (1236C>T, 2677G>T, 3435C>T), NR1/2 coding for pregnane X receptor (rs1523130, rs2472677, rs7643645), and for CYP3A activity measured by a phenotyping test. Forty-two patients with at least 4 consecutive unchanged doses of RLAI were included in a multicenter cross-sectional study. A 55% lower dose-adjusted plasma levels of RIS were observed for CYP2D6 ultrarapid metabolizers (n = 5) as compared with CYP2D6 intermediate metabolizers (P < 0.007). NR1/2 polymorphism (rs7643645A>G) influenced RIS exposure with a 2.8-fold lower active moiety (P = 0.031) in GG compared with the AA genotype. This was confirmed in a second independent cohort (n = 16). Furthermore, high-density lipoprotein cholesterol was positively correlated with CYP3A activity (P = 0.01), and the NR1/2 (rs2472677) polymorphism was associated with different adverse effects including prolactin plasma levels adjusted for age and sex. In conclusion, our results confirmed the influence of CYP2D6 genotype on plasma levels of RIS. This is the first report on the influence of NR1/2 polymorphisms on RLAI exposure and on drug-induced adverse effects. These results should be validated in larger cohorts.

Influência de diferentes manejos agrícolas na distribuição de metais pesados no solo e em plantas de tomate

Paty do Alferes (RJ) é um município com tradição agrícola, sendo a olericultura a sua principal atividade econômica. A região apresenta uma topografia e regime de chuvas que favorecem a erosão. A falta de um manejo adequado do solo e o uso excessivo de agroquímicos favorecem os processos de degradação física e química do solo, acarretando sérios impactos ao ambiente. Com o objetivo de avaliar o acúmulo de metais pesados no solo e em plantas de tomate (Lycopersicon esculentum Mill), cultivadas sob diferentes sistemas de preparo do solo, foi realizado um trabalho no município de Paty do Alferes (RJ), entre os meses de agosto e dezembro de 1999. Foram instaladas parcelas do tipo Wischmeier (com coletores de enxurrada e sedimentos), com dimensões de 22,0 x 4,0 m, em um Latossolo Vermelho-Amarelo com 30 % de declividade. Cada tratamento consistiu de um tipo de sistema de preparo do solo: (a) preparo convencional: aração no sentido morro abaixo e queima dos restos vegetais (PC); (b) preparo em curvas de nível: aração com tração animal em nível com faixas de capim-colonião a cada 7,0 m (PN); (c) cultivo mínimo: apenas abertura de covas para plantio e conservação dos restos vegetais (CM). Foram coletadas amostras de solo e plantas de tomate, sendo analisados os teores de metais pesados nas amostras coletadas, a produtividade das plantas e a fertilidade do solo. A produtividade no cultivo mínimo foi significativamente inferior à de outros manejos, apesar de tal sistema favorecer a maior fertilidade do solo. Esse manejo também proporcionou maior acúmulo de metais pesados no solo, principalmente quando comparado ao plantio convencional. Com relação às plantas, a aplicação foliar de defensivos agrícolas favoreceu o maior acúmulo de metais pesados na parte aérea das plantas, e os teores de Cu e Zn estiveram acima dos limites permitidos para metais pesados em plantas. Os frutos produzidos nos três sistemas de preparo do solo apresentaram concentrações de Pb próximas ao limites permitidos para alimentos frescos.

Exploring the high frequency emission of radio loud X-ray binaries

We report millimetre-wave continuum observations of the X-ray binaries Cygnus X-3, SS 433, LSI+61 303, Cygnus X-1 and GRS 1915+105. The observations were carried out with the IRAM 30 m-antenna at 250 GHz (1.25 mm) from 1998 March 14 to March 20. These millimetre measurements are complemented with centimetre observations from the Ryle Telescope, at 15 GHz (2.0 cm) and from the Green Bank Interferometer at 2.25 and 8.3 GHz (13 and 3.6 cm). Both Cygnus X-3 and SS 433 underwent moderate flaring events during our observations, whose main spectral evolution properties are described and interpreted. A significant spectral steepening was observed in both sources during the flare decay, that is likely to be caused by adiabatic expansion, inverse Compton and synchrotron losses. Finally, we also report 250 GHz upper limits for three additional undetected X-ray binary stars: LSI+65 010, LSI+61 235 and X Per.

Faint arc-minute extended radio emission around Cygnus X-3

Aims.We revisit the vicinity of the microquasar Cygnus X-3 at radio wavelengths. We aim to improve our previous search for possible associated extended radio features/hot spots in the position angle of the Cygnus X-3 relativistic jets focusing on shorter angular scales than previously explored. Methods.Our work is mostly based on analyzing modern survey and archive radio data, mainly including observations carried out with the Very Large Array and the Ryle Telescopes. We also used deep near-infrared images that we obtained in 2005. Results.We present new radio maps of the Cygnus X-3 field computed after combining multi-configuration Very Large Array archive data at 6 cm and different observing runs at 2 cm with the Ryle Telescope. These are probably among the deepest radio images of Cygnus X-3 reported to date at cm wavelengths. Both interferometers reveal an extended radio feature within a few arc-minutes of the microquasar position, thus making our detection more credible. Moreover, this extended emission is possibly non-thermal, although this point still needs confirmation. Its physical connection with the microquasar is tentatively considered under different physical scenarios. We also report on the serendipitous discovery of a likely Fanaroff-Riley type II radio galaxy only away from Cygnus X-3.

Possible hot spots excited by the relativistic jets of Cygnus X-3

We present the results of a deep search for associated radio features in the vicinity of the microquasar Cygnus X-3. The motivation behind is to find out evidence for interaction between its relativistic jets and the surrounding interstellar medium, which could eventually allow us to perform calorimetry of the total energy released by this microquasar during its flaring lifetime. Remarkably, two radio sources with mJy emission level at centimeter wavelengths have been detected in excellent alignment with the position angle of the inner radio jets. We propose that these objects could be the hot spots where the relativitic outflow collides with the ambient gas in analogy with Fanaroff-Riley II radio galaxies. These candidate hot spots are within a few arc-minutes of Cygnus X-3 and, if physically related, the full linear extent of the jet would reach tens of parsecs. We discuss here the evidence currently available to support this hypothesis based on both archival data and our own observations.