Composición y espesor de las decoraciones nasales de oro y plata provenientes de la tumba de la Dama de Cao determinados por la combinación del análisis EDXRF y las medidas de transmisión de rayos X

Treinta y cuatro adornos de nariz de la tumba de la Señora de Cao han sido analizados por análisis de EDXRF y medidas de transmisión. Estas decoraciones de nariz están hechas en parte en oro, y en parte en plata. Análisis EDXRF mostró que, mientras que las áreas de oro todas muestran una composición similar, las áreas de plata exhiben una composición irregular, y también un alto porcentaje inusual de oro, de hasta 35 %. Para verificar que esta composición errática no depende de los procesos de enriquecimiento en la superficie, se llevaron a cabo medidas de transmisión de rayos-X, lo que da la composición en el bulk de las muestras. Estas últimas mediciones confirman completamente los resultados de EDXRF. Por lo tanto, la conclusión podría ser que una gran cantidad de oro fue añadida intencionalmente a las aleaciones de plata, por razones no claras, se puede evitar los procesos de oxidación típica de alta concentración de plata en aleaciones de plata

Selective dynamical imaging of interferometric data

Recent developments in very long baseline interferometry (VLBI) have made it possible for the Event Horizon Telescope (EHT) to resolve the innermost accretion flows of the largest supermassive black holes on the sky. The sparse nature of the EHT’s (u, v)-coverage presents a challenge when attempting to resolve highly time-variable sources. We demonstrate that the changing (u, v)-coverage of the EHT can contain regions of time over the course of a single observation that facilitate dynamical imaging. These optimal time regions typically have projected baseline distributions that are approximately angularly isotropic and radially homogeneous. We derive a metric of coverage quality based on baseline isotropy and density that is capable of ranking array configurations by their ability to produce accurate dynamical reconstructions. We compare this metric to existing metrics in the literature and investigate their utility by performing dynamical reconstructions on synthetic data from simulated EHT observations of sources with simple orbital variability. We then use these results to make recommendations for imaging the 2017 EHT Sgr A* data sethttp://iopscience.iop.org/2041-8205Physic

Sistema Interactivo para la Enseñanza de la Lectoescritura para niños con Implante Coclear

El diseño de un sistema interactivo está orientado al usuario final, con el objetivo de estalecer una relación entre el usuario y el sistema. Un sistema interactivo para un niño con discapacidad auditiva involucra aspectos pedagógicos y tecnológicos que deben ser considerados. Por lo que, para diseñar un sistema, es necesario la participación de un equipo multidisciplinario formado de profesionales en diferentes dominios, como: educación especial, terapia ocupacional, fisioterapia, tecnología educacional, ergonomía, ciencia computacional, entre otros. Siguiendo una metodología compuesta por 3 etapas: conceptualización, ideación /estructuración y validación es diseñado un sistema interactivo llamado Fono-Mágica, el cual involucra un juego conformado por un tablero físico  con un entorno digital

A esquistossomose mansoni no contexto da política de saúde brasileira Schistosoma mansoni in the context of the Brazilian health policy

São muitos os fatores envolvidos na determinação da emergência e reemergência de doenças infecciosas. No caso da esquistossomose destacam-se os fatores biológicos como os relacionados ao habitat, às mutações e adaptações de microrganismos e hospedeiros, à resposta imunológica do hospedeiro e às adaptações bioecológicas de hospedeiros intermediários. Somam-se a esses, os não menos importantes fatores relacionados à gestão política, ocupação do ambiente e alocação de recursos financeiros. O Brasil reúne, hoje, importantes condições ecoepidemiológicas para a reemergência da esquistossomose e aumento da prevalência de algumas formas graves como mielorradiculopatia esquistossomótica, principalmente em áreas de baixa endemicidade. A expansão de suas fronteiras atinge os meios urbanos e rurais, destinados ao trabalho ou ao lazer, com comprometimento inclusive de setores de renda como o ecoturismo. Os avanços nas pesquisas acerca dos hospedeiros intermediário e definitivo do Schistosoma mansoni, para se transformarem em benefícios públicos, necessitam da sustentabilidade gerencial pública comprometida, interdisciplinar, fortalecida nas diferentes esferas de governo, vinculada ás sociedades civis tecnicamente capacitadas ao gerenciamento e comprometidas com as necessidades de saúde da população.<br>There are many factors involved in the determination of the emergence and reemergence of infectious diseases. In the case of Schistosomiasis biological factors are highlighted as related to the habitat, to the microorganisms and hosts adaptations and mutations, to the immunologic reply of the host and to the bio-ecology adaptations of intermediate hosts. These are added to the not less important factors related to the management politics, occupation of the environment and allocation of financial resources. Brazil congregates, today, an important echo-epidemiologic conditions for the reemergence of Schistosomiasis. The expansion of its borders reaches the urban and agricultural environments, destined to work or leisure, also damaging income sectors as the ecotourism. The advances in the researches concerning the intermediate and definitive hosts of the Schistosoma mansoni, to change them into public benefits, need the public sustainability, compromised, interdisciplinary, and strengthened in the government's different spheres. The organized civil society has fundamental paper in the control of the government actions

Selective Dynamical Imaging of Interferometric Data

Funding Information: We thank the National Science Foundation (awards OISE-1743747, AST-1816420, AST-1716536, AST-1440254, AST-1935980) and the Gordon and Betty Moore Foundation (GBMF-5278) for financial support of this work. This work was supported in part by the Black Hole Initiative, which is funded by grants from the John Templeton Foundation and the Gordon and Betty Moore Foundation to Harvard University. Support for this work was also provided by the NASA Hubble Fellowship grant HST-HF2-51431.001-A awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5-26555. Publisher Copyright: © 2022. The Author(s)Recent developments in very long baseline interferometry (VLBI) have made it possible for the Event Horizon Telescope (EHT) to resolve the innermost accretion flows of the largest supermassive black holes on the sky. The sparse nature of the EHT's (u, v)-coverage presents a challenge when attempting to resolve highly time-variable sources. We demonstrate that the changing (u, v)-coverage of the EHT can contain regions of time over the course of a single observation that facilitate dynamical imaging. These optimal time regions typically have projected baseline distributions that are approximately angularly isotropic and radially homogeneous. We derive a metric of coverage quality based on baseline isotropy and density that is capable of ranking array configurations by their ability to produce accurate dynamical reconstructions. We compare this metric to existing metrics in the literature and investigate their utility by performing dynamical reconstructions on synthetic data from simulated EHT observations of sources with simple orbital variability. We then use these results to make recommendations for imaging the 2017 EHT Sgr A* data set.Peer reviewe

Selective Dynamical Imaging of Interferometric Data

International audienceRecent developments in very long baseline interferometry (VLBI) have made it possible for the Event Horizon Telescope (EHT) to resolve the innermost accretion flows of the largest supermassive black holes on the sky. The sparse nature of the EHT's (u, v)-coverage presents a challenge when attempting to resolve highly time-variable sources. We demonstrate that the changing (u, v)-coverage of the EHT can contain regions of time over the course of a single observation that facilitate dynamical imaging. These optimal time regions typically have projected baseline distributions that are approximately angularly isotropic and radially homogeneous. We derive a metric of coverage quality based on baseline isotropy and density that is capable of ranking array configurations by their ability to produce accurate dynamical reconstructions. We compare this metric to existing metrics in the literature and investigate their utility by performing dynamical reconstructions on synthetic data from simulated EHT observations of sources with simple orbital variability. We then use these results to make recommendations for imaging the 2017 EHT Sgr A* data set

The Variability of the Black Hole Image in M87 at the Dynamical Timescale

Abstract: The black hole images obtained with the Event Horizon Telescope (EHT) are expected to be variable at the dynamical timescale near their horizons. For the black hole at the center of the M87 galaxy, this timescale (5–61 days) is comparable to the 6 day extent of the 2017 EHT observations. Closure phases along baseline triangles are robust interferometric observables that are sensitive to the expected structural changes of the images but are free of station-based atmospheric and instrumental errors. We explored the day-to-day variability in closure-phase measurements on all six linearly independent nontrivial baseline triangles that can be formed from the 2017 observations. We showed that three triangles exhibit very low day-to-day variability, with a dispersion of ∼3°–5°. The only triangles that exhibit substantially higher variability (∼90°–180°) are the ones with baselines that cross the visibility amplitude minima on the u–v plane, as expected from theoretical modeling. We used two sets of general relativistic magnetohydrodynamic simulations to explore the dependence of the predicted variability on various black hole and accretion-flow parameters. We found that changing the magnetic field configuration, electron temperature model, or black hole spin has a marginal effect on the model consistency with the observed level of variability. On the other hand, the most discriminating image characteristic of models is the fractional width of the bright ring of emission. Models that best reproduce the observed small level of variability are characterized by thin ring-like images with structures dominated by gravitational lensing effects and thus least affected by turbulence in the accreting plasmas

First M87 Event Horizon Telescope Results. II. Array and Instrumentation

The Event Horizon Telescope (EHT) is a very long baseline interferometry (VLBI) array that comprises millimeter- and submillimeter-wavelength telescopes separated by distances comparable to the diameter of the Earth. At a nominal operating wavelength of similar to 1.3 mm, EHT angular resolution (lambda/D) is similar to 25 mu as, which is sufficient to resolve nearby supermassive black hole candidates on spatial and temporal scales that correspond to their event horizons. With this capability, the EHT scientific goals are to probe general relativistic effects in the strong-field regime and to study accretion and relativistic jet formation near the black hole boundary. In this Letter we describe the system design of the EHT, detail the technology and instrumentation that enable observations, and provide measures of its performance. Meeting the EHT science objectives has required several key developments that have facilitated the robust extension of the VLBI technique to EHT observing wavelengths and the production of instrumentation that can be deployed on a heterogeneous array of existing telescopes and facilities. To meet sensitivity requirements, high-bandwidth digital systems were developed that process data at rates of 64. gigabit s(-1), exceeding those of currently operating cm-wavelength VLBI arrays by more than an order of magnitude. Associated improvements include the development of phasing systems at array facilities, new receiver installation at several sites, and the deployment of hydrogen maser frequency standards to ensure coherent data capture across the array. These efforts led to the coordination and execution of the first Global EHT observations in 2017 April, and to event-horizon-scale imaging of the supermassive black hole candidate in M87

Event Horizon Telescope imaging of the archetypal blazar 3C 279 at an extreme 20 microarcsecond resolution

3C 279 is an archetypal blazar with a prominent radio jet that show broadband flux density variability across the entire electromagnetic spectrum. We use an ultra-high angular resolution technique - global Very Long Baseline Interferometry (VLBI) at 1.3 mm (230 GHz) - to resolve the innermost jet of 3C 279 in order to study its fine-scale morphology close to the jet base where highly variable gamma -ray emission is thought to originate, according to various models. The source was observed during four days in April 2017 with the Event Horizon Telescope at 230 GHz, including the phased Atacama Large Millimeter/submillimeter Array (ALMA), at an angular resolution of similar to 20 mu as (at a redshift of z=0.536 this corresponds to similar to 0.13 pc similar to 1700 Schwarzschild radii with a black hole mass M-BH=8x10(8) M-circle dot). Imaging and model-fitting techniques were applied to the data to parameterize the fine-scale source structure and its variation. We find a multicomponent inner jet morphology with the northernmost component elongated perpendicular to the direction of the jet, as imaged at longer wavelengths. The elongated nuclear structure is consistent on all four observing days and across different imaging methods and model-fitting techniques, and therefore appears robust. Owing to its compactness and brightness, we associate the northern nuclear structure as the VLBI &quot;core&quot;. This morphology can be interpreted as either a broad resolved jet base or a spatially bent jet. We also find significant day-to-day variations in the closure phases, which appear most pronounced on the triangles with the longest baselines. Our analysis shows that this variation is related to a systematic change of the source structure. Two inner jet components move non-radially at apparent speeds of similar to 15 c and similar to 20 c (similar to 1.3 and similar to 1.7 mu as day(-1), respectively), which more strongly supports the scenario of traveling shocks or instabilities in a bent, possibly rotating jet. The observed apparent speeds are also coincident with the 3C 279 large-scale jet kinematics observed at longer (cm) wavelengths, suggesting no significant jet acceleration between the 1.3 mm core and the outer jet. The intrinsic brightness temperature of the jet components are less than or similar to 10(10) K, a magnitude or more lower than typical values seen at &gt;= 7 mm wavelengths. The low brightness temperature and morphological complexity suggest that the core region of 3C 279 becomes optically thin at short (mm) wavelengths

3C 279 Event Horizon Telescope imaging

VizieR online Data Catalogue associated with article published in journal Astronomy &amp; Astrophysics with title 'Event Horizon Telescope imaging of the archetypal blazar 3C 279 at an extreme 20 microarcsecond resolution.' (bibcode: 2020A&amp;A...640A..69K