10 research outputs found

    En bĂşsqueda de interfaces naturales para personas con discapacidad

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    Dentro de la población de personas en situación de discapacidad, hay un colectivo que tiene discapacidad intelectual, sensorial, motriz o una combinación de éstas. La Clasificación Internacional del Funcionamiento, de la Discapacidad y de la Salud (CIF) define la discapacidad como un término genérico que abarca deficiencias, limitaciones de la actividad y restricciones a la participación. Se calcula que más del 15% de la población mundial está aquejada por la discapacidad en alguna forma. En Argentina esta prevalencia asciende a 7,1%. Cuando estas personas quieren acceder a algún dispositivo tecnológico, generalmente se encuentran con interfaces que no son accesibles. A menudo se tiene que recurrir a adaptaciones, lo cual eleva costos y no se asegura completa accesibilidad. Las tecnologías actuales permiten interfaces “más naturales” o intuitivas, donde el feedback es inmediato. La aplicación de la tecnología adecuada, con interfaces naturales o intuitivas, permite una mayor accesibilidad que las adaptaciones comúnmente usadas para el desarrollo integral de alumnos con trastornos psicomotores. El objetivo de este trabajo es facilitar el desarrollo integral de los alumnos con trastornos sensopsicomotores que asisten a la Escuela Especial Beatriz A. Martínez Allio, a través de la incorporación e implementación de interfaces naturales para el trabajo con computadoras en el ámbito educativo, ofreciendo al docente una herramienta complementaria para el desarrollo de sus actividades diarias. Se plantea la implementación de interfaces de hardware y software para alcanzar el objetivo general. Se pretende realizar al menos una pantalla táctil y al menos una interfaz con la cámara Kinect de la consola de juegos Xbox 360.Fil: Beltramone, Diego Antonio. Universidad Nacional de Córdoba. Facultad de Ciencias Exactas, Físicas y Naturales. Ingeniería Biomédica; Argentina.Fil: Tula, Silvia Matilde. Ministerio de Educación-Provincia de Córdoba. * Escuela Especial Beatriz Angélica Martínez Ayillo; Argentina.Fil: Rivarola, Marcela Fabiana. Universidad Nacional de Córdoba. Facultad de Medicina. Escuela de Kinesiología y Fisioterapia; Argentina.Fil: Hidalgo, María Belén. Universidad Nacional de Córdoba. Facultad de Ciencias Exactas, Físicas y Naturales. Ingeniería Biomédica; Argentina.Fil: Tancredi, Pablo Daniel. Universidad Nacional de Córdoba. Facultad de Ciencias Exactas, Físicas y Naturales. Ingeniería Biomédica; Argentina.Fil: Quinteros Quintana, María Luz. Universidad Nacional de Córdoba. Facultad de Ciencias Exactas, Físicas y Naturales. Ingeniería Biomédica; Argentina.Fil: Díaz, Juan Manuel. Universidad Nacional de Córdoba. Facultad de Ciencias Exactas, Físicas y Naturales. Ingeniería Biomédica; Argentina.Fil: Marcotti, Aída. Universidad Nacional de Córdoba. Facultad de Ciencias Exactas, Físicas y Naturales. Ingeniería Biomédica; Argentina.Fil: Atea, Juan Javier. Universidad Nacional de Córdoba. Facultad de Ciencias Exactas, Físicas y Naturales. Departamento de Electrónica; Argentina.Otras Ingenierías y Tecnología

    IMPACT-Global Hip Fracture Audit: Nosocomial infection, risk prediction and prognostication, minimum reporting standards and global collaborative audit. Lessons from an international multicentre study of 7,090 patients conducted in 14 nations during the COVID-19 pandemic

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    The Forward Physics Facility at the High-Luminosity LHC

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    The stellar occultation by Makemake on 2011 April 23

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    International audienceWe have taken advantage of a stellar occultation by the dwarf planet Makemake on 2011 April 23, to determine several of its main physical properties. We present results from a multisite campaign with 8 positive occultation detections from 5 different sites, including data from the 8-m VLT and 3.5-m NTT telescopes in Chile, which have very high temporal resolution. Because the star was significantly fainter than Makemake (setting a record in the magnitude of a star whose occultation has been detected), the occultation resulted in a drop of just ~0.3 mag in the lightcurves. From the lightcurves we have been able to determine the size and shape of the body, its geometric albedo and constraints on its atmosphere

    The stellar occultation by Makemake on 2011 April 23

    No full text
    International audienceWe have taken advantage of a stellar occultation by the dwarf planet Makemake on 2011 April 23, to determine several of its main physical properties. We present results from a multisite campaign with 8 positive occultation detections from 5 different sites, including data from the 8-m VLT and 3.5-m NTT telescopes in Chile, which have very high temporal resolution. Because the star was significantly fainter than Makemake (setting a record in the magnitude of a star whose occultation has been detected), the occultation resulted in a drop of just ~0.3 mag in the lightcurves. From the lightcurves we have been able to determine the size and shape of the body, its geometric albedo and constraints on its atmosphere

    The stellar occultation by Makemake on 2011 April 23

    No full text
    International audienceWe have taken advantage of a stellar occultation by the dwarf planet Makemake on 2011 April 23, to determine several of its main physical properties. We present results from a multisite campaign with 8 positive occultation detections from 5 different sites, including data from the 8-m VLT and 3.5-m NTT telescopes in Chile, which have very high temporal resolution. Because the star was significantly fainter than Makemake (setting a record in the magnitude of a star whose occultation has been detected), the occultation resulted in a drop of just ~0.3 mag in the lightcurves. From the lightcurves we have been able to determine the size and shape of the body, its geometric albedo and constraints on its atmosphere

    The Forward Physics Facility at the High-Luminosity LHC

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    High energy collisions at the High-Luminosity Large Hadron Collider (LHC) produce a large number of particles along the beam collision axis, outside of the acceptance of existing LHC experiments. The proposed Forward Physics Facility (FPF), to be located several hundred meters from the ATLAS interaction point and shielded by concrete and rock, will host a suite of experiments to probe standard model (SM) processes and search for physics beyond the standard model (BSM). In this report, we review the status of the civil engineering plans and the experiments to explore the diverse physics signals that can be uniquely probed in the forward region. FPF experiments will be sensitive to a broad range of BSM physics through searches for new particle scattering or decay signatures and deviations from SM expectations in high statistics analyses with TeV neutrinos in this low-background environment. High statistics neutrino detection will also provide valuable data for fundamental topics in perturbative and non-perturbative QCD and in weak interactions. Experiments at the FPF will enable synergies between forward particle production at the LHC and astroparticle physics to be exploited. We report here on these physics topics, on infrastructure, detector, and simulation studies, and on future directions to realize the FPF's physics potential

    The Forward Physics Facility at the High-Luminosity LHC

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    International audienceHigh energy collisions at the High-Luminosity Large Hadron Collider (LHC) produce a large number of particles along the beam collision axis, outside of the acceptance of existing LHC experiments. The proposed Forward Physics Facility (FPF), to be located several hundred meters from the ATLAS interaction point and shielded by concrete and rock, will host a suite of experiments to probe Standard Model (SM) processes and search for physics beyond the Standard Model (BSM). In this report, we review the status of the civil engineering plans and the experiments to explore the diverse physics signals that can be uniquely probed in the forward region. FPF experiments will be sensitive to a broad range of BSM physics through searches for new particle scattering or decay signatures and deviations from SM expectations in high statistics analyses with TeV neutrinos in this low-background environment. High statistics neutrino detection will also provide valuable data for fundamental topics in perturbative and non-perturbative QCD and in weak interactions. Experiments at the FPF will enable synergies between forward particle production at the LHC and astroparticle physics to be exploited. We report here on these physics topics, on infrastructure, detector, and simulation studies, and on future directions to realize the FPF's physics potential
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