2,272 research outputs found

    LA TUTORÍA COMO HERRAMIENTA PARA EL SEGUIMIENTO ACADÉMICO DE LOS ALUMNOS

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    En los últimos tiempos se han producido múltiples transformaciones en la Educación Superior, una de ellas lo constituyen el esfuerzo para la inclusión y la democratización del acceso a la misma, la permanencia y el término. Uno de los desafíos es la retención de los alumnos en los primeros tramos de sus estudios. Las carreras de ingeniería enfrentan hoy esta problemática y es uno de los principales temas en su agenda de trabajo. En la Universidad Tecnológica Nacional - Facultad Regional Resistencia se viene desarrollando desde el año 2006, un Sistema de Acción Tutorial cuyo objetivo apunta a consolidarse como una estrategia educativa de apoyo a los alumnos y como una acción orientada a diagnosticar y asesorar en aquellas problemáticas relacionadas al desempeño académico. Desde sus inicios hasta hoy el sistema se ha desarrollado y avanzado en etapas. Una de las instancias que influye positivamente fue la implementación del Proyecto de Apoyo para el mejoramiento de la enseñanza en primer año de las carreras de grado de ciencias exactas y naturales, ciencias económicas e informáticas (PACENI). Este programa considera necesario generar estrategias institucionales específicas para promover la motivación continua de los alumnos, apoyándolos en la adquisición de habilidades cognitivas, colaborar en la conformación del autocontrol de su propio proyecto académico y el logro de sus metas personales. En esta oportunidad se presentarán los resultados del trabajo de seguimiento realizado en la carrera de Ingeniería en Sistemas de Información y en la carrera de Ingeniería Química, en la que se ha intervenido desde el seminario nivelador de ingreso. Con la información obtenida se elaboró un diagnóstico situacional de los alumnos permitiendo una clasificación según su desempeño académico; el objetivo es trabajar en la prevención y detección temprana de las dificultades de los alumnos para poder brindarle un apoyo adecuado

    Changes in Protein, Nonnutritional Factors, and Antioxidant Capacity during Germination of L. campestris

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    The changes in SDS-PAGE proteins patterns, oligosaccharides and phenolic compounds of L. campestris seeds, were evaluated during nine germination days. SDS-PAGE pattern showed 12 bands in the original protein seeds, while in the samples after 1–9 germination days, the proteins located in the range of 28–49 and 49–80 kDa indicated an important reduction, and there was an increase in bands about 27 kDa. On the other hand, oligosaccharides showed more than 50% of decrease in its total concentration after 4 germination days; nevertheless after the fifth day, the oligosaccharides concentration increases and rises more than 30% of the original concentration. Phenolic compounds increased their concentration since the first germination day reaching until 450% more than the original seed level. The obtained results are related with liberation or increase of phenolic compounds with antioxidant properties, allowing us to suggest that the germination would be used to produce legume foods for human consumption with better nutraceutical properties

    Investigación médico-antropológica documental: prescripciones enfocadas al manejo del dolor

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    Introducción: Las recetas médicas o prescripciones históricas en el territorio de la Nueva Granada (hoy Colombia) revelan la evolución del manejo de la enfermedad en función de los efectos benéficos de administrar algún tipo de agente medicinal de origen vegetal, animal o mineral. Objetivo: Describir el tratamiento del reumatismo en los siglos XVIII y XIX, con base en dos recetas médicas de la época con base en la fundamentación contemporánea de su interacción fisiológica. Materiales y métodos: Búsqueda documental en el archivo Histórico de la Biblioteca Octavio Arizmendi Posada de la Universidad de La Sabana, donde se encontraron las recetas tituladas “Reumatismo” y “Rehumas”. Resultados: Se describen cuatro clases de tratamientos para las enfermedades reumáticas utilizados en los siglos XVIII y XIX y orientados principal-mente a la disminución del dolor. Este artículo presenta las bases fisiológicas de estos tratamientos, y cómo pudieron o no haber tenido algún efecto calmante al examinar su fisiología. Conclusiones: Estos medicamentos coloniales neogranadinos no ameritan su uso en el contexto actual de la medicina, pero pudieron representar una ayuda terapéutica en su momento

    The Organizational Account of Function is an Etiological Account of Function

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    The debate on the notion of function has been historically dominated by dispositional and etiological accounts, but recently a third contender has gained prominence: the organizational account. This original theory of function is intended to offer an alternative account based on the notion of self-maintaining system. However, there is a set of cases where organizational accounts seem to generate counterintuitive results. These cases involve cross-generational traits, that is, traits that do not contribute in any relevant way to the self-maintenance of the organism carrying them, but instead have very important effects on organisms that belong to the next generation. We argue that any plausible solution to the problem of cross-generational traits shows that the organizational account just is a version of the etiological theory and, furthermore, that it does not provide any substantive advantage over standard etiological theories of function

    VAMOS: a Pathfinder for the HAWC Gamma-Ray Observatory

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    VAMOS was a prototype detector built in 2011 at an altitude of 4100m a.s.l. in the state of Puebla, Mexico. The aim of VAMOS was to finalize the design, construction techniques and data acquisition system of the HAWC observatory. HAWC is an air-shower array currently under construction at the same site of VAMOS with the purpose to study the TeV sky. The VAMOS setup included six water Cherenkov detectors and two different data acquisition systems. It was in operation between October 2011 and May 2012 with an average live time of 30%. Besides the scientific verification purposes, the eight months of data were used to obtain the results presented in this paper: the detector response to the Forbush decrease of March 2012, and the analysis of possible emission, at energies above 30 GeV, for long gamma-ray bursts GRB111016B and GRB120328B.Comment: Accepted for pubblication in Astroparticle Physics Journal (20 pages, 10 figures). Corresponding authors: A.Marinelli and D.Zaboro

    EPDR1 up-regulation in human colorectal cancer is related to staging and favours cell proliferation and invasiveness

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    The finding of novel molecular markers for prediction or prognosis of invasiveness in colorectal cancer (CRC) constitutes an appealing challenge. Here we show the up-regulation of EPDR1 in a prospective cohort of 101 CRC patients, in a cDNA array of 43 patients and in in silico analyses. EPDR1 encodes a protein related to ependymins, a family of glycoproteins involved in intercellular contacts. A thorough statistical model allowed us to conclude that the gene is significantly up-regulated in tumour tissues when compared with normal mucosa. These results agree with those obtained by the analysis of three publicly available databases. EPDR1 up-regulation correlates with the TNM staging parameters, especially T and M. Studies with CRC cell lines revealed that the methylation of a CpG island controls EPDR1 expression. siRNA knocking-down and overexpression of the gene following transient plasmid transfection, showed that EPDR1 favours cell proliferation, migration, invasiveness and adhesion to type I collagen fibres, suggesting a role in epithelial to mesenchymal transition. Both statistical and functional analysis correlated EPDR1 overexpression with invasiveness and dissemination of tumour cells, supporting the inclusion of EPDR1 in panels of genes used to improve molecular subtyping of CRC. Eventually, EPDR1 may be an actionable target.Fil: Gimeno Valiente, F.. No especifíca;Fil: Riffo Campos, Á. L.. Universidad de La Frontera; ChileFil: Ayala, G.. Universidad de Valencia; EspañaFil: Tarazona, N.. Universidad de Valencia; EspañaFil: Gambardella, V.. Universidad de Valencia; EspañaFil: Rodríguez, Fernanda Mariel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Santa Fe. Instituto de Ciencias Veterinarias del Litoral. Universidad Nacional del Litoral. Facultad de Ciencias Veterinarias. Instituto de Ciencias Veterinarias del Litoral; ArgentinaFil: Huerta, M.. Universidad de Valencia; EspañaFil: Martínez-Ciarpaglini, C.. Universidad de Valencia; EspañaFil: Montón Bueno, J.. Universidad de Valencia; EspañaFil: Roselló, S.. Universidad de Valencia; EspañaFil: Roda, D.. Universidad de Valencia; EspañaFil: Cervantes, A.. Universidad de Valencia; EspañaFil: Franco, L.. Universidad de Valencia; EspañaFil: López Rodas, G.. Universidad de Valencia; EspañaFil: Castillo, J.. Universidad de Valencia; Españ

    All-particle cosmic ray energy spectrum measured by the HAWC experiment from 10 to 500 TeV

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    We report on the measurement of the all-particle cosmic ray energy spectrum with the High Altitude Water Cherenkov (HAWC) Observatory in the energy range 10 to 500 TeV. HAWC is a ground based air-shower array deployed on the slopes of Volcan Sierra Negra in the state of Puebla, Mexico, and is sensitive to gamma rays and cosmic rays at TeV energies. The data used in this work were taken from 234 days between June 2016 to February 2017. The primary cosmic-ray energy is determined with a maximum likelihood approach using the particle density as a function of distance to the shower core. Introducing quality cuts to isolate events with shower cores landing on the array, the reconstructed energy distribution is unfolded iteratively. The measured all-particle spectrum is consistent with a broken power law with an index of 2.49±0.01-2.49\pm0.01 prior to a break at (45.7±0.1(45.7\pm0.1) TeV, followed by an index of 2.71±0.01-2.71\pm0.01. The spectrum also respresents a single measurement that spans the energy range between direct detection and ground based experiments. As a verification of the detector response, the energy scale and angular resolution are validated by observation of the cosmic ray Moon shadow's dependence on energy.Comment: 16 pages, 11 figures, 4 tables, submission to Physical Review

    Measurement of the Crab Nebula Spectrum Past 100 TeV with HAWC

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    We present TeV gamma-ray observations of the Crab Nebula, the standard reference source in ground-based gamma-ray astronomy, using data from the High Altitude Water Cherenkov (HAWC) Gamma-Ray Observatory. In this analysis we use two independent energy-estimation methods that utilize extensive air shower variables such as the core position, shower angle, and shower lateral energy distribution. In contrast, the previously published HAWC energy spectrum roughly estimated the shower energy with only the number of photomultipliers triggered. This new methodology yields a much improved energy resolution over the previous analysis and extends HAWC's ability to accurately measure gamma-ray energies well beyond 100 TeV. The energy spectrum of the Crab Nebula is well fit to a log parabola shape (dNdE=ϕ0(E/7 TeV)αβln(E/7 TeV))\left(\frac{dN}{dE} = \phi_0 \left(E/\textrm{7 TeV}\right)^{-\alpha-\beta\ln\left(E/\textrm{7 TeV}\right)}\right) with emission up to at least 100 TeV. For the first estimator, a ground parameter that utilizes fits to the lateral distribution function to measure the charge density 40 meters from the shower axis, the best-fit values are ϕo\phi_o=(2.35±\pm0.040.21+0.20^{+0.20}_{-0.21})×\times1013^{-13} (TeV cm2^2 s)1^{-1}, α\alpha=2.79±\pm0.020.03+0.01^{+0.01}_{-0.03}, and β\beta=0.10±\pm0.010.03+0.01^{+0.01}_{-0.03}. For the second estimator, a neural network which uses the charge distribution in annuli around the core and other variables, these values are ϕo\phi_o=(2.31±\pm0.020.17+0.32^{+0.32}_{-0.17})×\times1013^{-13} (TeV cm2^2 s)1^{-1}, α\alpha=2.73±\pm0.020.02+0.03^{+0.03}_{-0.02}, and β\beta=0.06±\pm0.01±\pm0.02. The first set of uncertainties are statistical; the second set are systematic. Both methods yield compatible results. These measurements are the highest-energy observation of a gamma-ray source to date.Comment: published in Ap
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