857 resultados para Massive open online courses


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Diversity-based designing, or the goal of ensuring that web-based information is accessible to as many diverse users as possible, has received growing international acceptance in recent years, with many countries introducing legislation to enforce it. This paper analyses web content accessibility levels in Spanish education portals according to the international guidelines established by the World Wide Web Consortium (W3C) and the Web Accessibility Initiative (WAI). Additionally, it suggests the calculation of an inaccessibility rate as a tool for measuring the degree of non-compliance with WAI Guidelines 2.0 as well as illustrating the significant gap that separates people with disabilities from digital education environments (with a 7.77% average). A total of twenty-one educational web portals with two different web depth levels (42 sampling units) were assessed for this purpose using the automated analysis tool Web Accessibility Test 2.0 (TAW, for its initials in Spanish). The present study reveals a general trend towards non-compliance with the technical accessibility recommendations issued by the W3C-WAI group (97.62% of the websites examined present mistakes in Level A conformance). Furthermore, despite the increasingly high number of legal and regulatory measures about accessibility, their practical application still remains unsatisfactory. A greater level of involvement must be assumed in order to raise awareness and enhance training efforts towards accessibility in the context of collective Information and Communication Technologies (ICTs), since this represents not only a necessity but also an ethical, social, political and legal commitment to be assumed by society.

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Nowadays, online media represent a great choice for advertising. From de advertising media planning, new media give new ways to reach the consumers, but they also add more complexity. The communication capacity of online media and the greater use of that media by part of the users open up the debate about the necessity of rethinking the approach of the ‘traditional’ advertising media planning, which structure and work processes were developed when media were offline. So, this article gives a panoramic view about the influence of new media in advertising media planning. To do this, in first place, describes the current scenario, analyzing the penetration and advertising expenditure in Internet. Also, it shows the main online media according to their proximity to the offline advertising media planning conception. In second place, this article addresses the current challenges at measuring new media as a symptom of the impulse at the change of model. Finally, the article ends up showing some trends that are presented as drivers of change. However, after this analysis, comes up the point that those aspects would not change the essence of advertising media planning, so it is questionable if we can speak of a crisis or, instead, if new media are showing the necessity that media planning have to be involved with this new scenario.

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Context. The first soft gamma-ray repeater was discovered over three decades ago, and was subsequently identified as a magnetar, a class of highly magnetised neutron star. It has been hypothesised that these stars power some of the brightest supernovae known, and that they may form the central engines of some long duration gamma-ray bursts. However there is currently no consenus on the formation channel(s) of these objects. Aims. The presence of a magnetar in the starburst cluster Westerlund 1 implies a progenitor with a mass ≥40 M⊙, which favours its formation in a binary that was disrupted at supernova. To test this hypothesis we conducted a search for the putative pre-SN companion. Methods. This was accomplished via a radial velocity survey to identify high-velocity runaways, with subsequent non-LTE model atmosphere analysis of the resultant candidate, Wd1-5. Results. Wd1-5 closely resembles the primaries in the short-period binaries, Wd1-13 and 44, suggesting a similar evolutionary history, although it currently appears single. It is overluminous for its spectroscopic mass and we find evidence of He- and N-enrichement, O-depletion, and critically C-enrichment, a combination of properties that is difficult to explain under single star evolutionary paradigms. We infer a pre-SN history for Wd1-5 which supposes an initial close binary comprising two stars of comparable (~ 41 M⊙ + 35 M⊙) masses. Efficient mass transfer from the initially more massive component leads to the mass-gainer evolving more rapidly, initiating luminous blue variable/common envelope evolution. Reverse, wind-driven mass transfer during its subsequent WC Wolf-Rayet phase leads to the carbon pollution of Wd1-5, before a type Ibc supernova disrupts the binary system. Under the assumption of a physical association between Wd1-5 and J1647-45, the secondary is identified as the magnetar progenitor; its common envelope evolutionary phase prevents spin-down of its core prior to SN and the seed magnetic field for the magnetar forms either in this phase or during the earlier episode of mass transfer in which it was spun-up. Conclusions. Our results suggest that binarity is a key ingredient in the formation of at least a subset of magnetars by preventing spin-down via core-coupling and potentially generating a seed magnetic field. The apparent formation of a magnetar in a Type Ibc supernova is consistent with recent suggestions that superluminous Type Ibc supernovae are powered by the rapid spin-down of these objects.

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We present an analysis of a 78 ks Chandra high-energy transmission gratings observation of the B0I star QV Nor, the massive donor of the wind-accreting pulsar 4U1538−52. The neutron star (NS) orbits its companion in a very close orbit (r < 1.4R*, in units of the stellar radii), thereby allowing probing of the innermost wind regions. The flux of the Fe Kα line during eclipse reduces to only ∼30% of the flux measured out of eclipse. This indicates that the majority of Fe fluorescence must be produced in regions close to the NS, at distances smaller than 1R* from its surface. The fact that the flux of the continuum decreases to only ∼3% during eclipse allows for a high contrast of the Fe Kα line fluorescence during eclipse. The line is not resolved and centered at 1.9368 0.0018 l = 0.0032 - + Å. From the inferred plasma speed limit of v < c l < 800 l D km s−1 and range of ionization parameters of log 1, 2 x = [- ], together with the stellar density profile, we constrain the location of the cold, dense material in the stellar wind of QV Nor using simple geometrical considerations. We then use the Fe Kα line fluorescence as a tracer of wind clumps and determine that these clumps in the stellar wind of QV Nor (B0I) must already be present at radii r < 1.25R*, close to the photosphere of the star.

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Machine vision is an important subject in computer science and engineering degrees. For laboratory experimentation, it is desirable to have a complete and easy-to-use tool. In this work we present a Java library, oriented to teaching computer vision. We have designed and built the library from the scratch with enfasis on readability and understanding rather than on efficiency. However, the library can also be used for research purposes. JavaVis is an open source Java library, oriented to the teaching of Computer Vision. It consists of a framework with several features that meet its demands. It has been designed to be easy to use: the user does not have to deal with internal structures or graphical interface, and should the student need to add a new algorithm it can be done simply enough. Once we sketch the library, we focus on the experience the student gets using this library in several computer vision courses. Our main goal is to find out whether the students understand what they are doing, that is, find out how much the library helps the student in grasping the basic concepts of computer vision. In the last four years we have conducted surveys to assess how much the students have improved their skills by using this library.

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La red de investigación en docencia universitaria “De las tabletas a los MOOC en la LIJ 2.0 y la didáctica de lengua y literatura” (Modalidad II. Código 2962 http://web.ua.es/es/ice/redes/2014/proyectos-modalidad-ii-2013-2014.html) ha continuado las principales líneas de trabajo desarrolladas por las anteriores redes del área de didáctica de la lengua y la literatura de la Universidad de Alicante (Mula et alii 2011, Llorens et alii 2012, Rovira et alii, 2013 http://web.ua.es/es/ice/redes/proyectos-cursos-anteriores.html). La integración de las Tecnologías de la Información y la Comunicación (TIC) o las Tecnologías del Aprendizaje y el Conocimiento (TAC) en el aula de lengua y literatura española es una realidad que presenta múltiples formas según el nivel, los equipos y herramientas disponibles o las metodologías utilizadas. Se han planteado dos líneas principales, recogidas en el título de la red: el estudio de las posibilidades didácticas de las tabletas y aplicaciones móviles, coordinado por Pedro Mendiola y la introducción a los MOOC Massive Online Open Course (Cursos Masivos, Abiertos y En línea) dirigida por Arantxa Martín Martín. Además, se han planteado otra serie de actuaciones como el uso del Moodle o la introducción al formato de los Book-tráilers como herramienta de animación lectora para seguir analizando las posibilidades de Internet para la didáctica de la lengua y la literatura.

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Context. The young open cluster Dolidze 25, in the direction of the Galactic anticentre, has been attributed a very low metallicity, with typical abundances between −0.5 and −0.7 dex below solar. Aims. We intend to derive accurate cluster parameters and accurate stellar abundances for some of its members. Methods. We have obtained a large sample of intermediate- and high-resolution spectra for stars in and around Dolidze 25. We used the fastwind code to generate stellar atmosphere models to fit the observed spectra. We derive stellar parameters for a large number of OB stars in the area, and abundances of oxygen and silicon for a number of stars with spectral types around B0. Results. We measure low abundances in stars of Dolidze 25. For the three stars with spectral types around B0, we find 0.3 dex (Si) and 0.5 dex (O) below the values typical in the solar neighbourhood. These values, even though not as low as those given previously, confirm Dolidze 25 and the surrounding H ii region Sh2-284 as the most metal-poor star-forming environment known in the Milky Way. We derive a distance 4.5 ± 0.3 kpc to the cluster (rG ≈ 12.3 kpc). The cluster cannot be older than ~3 Myr, and likely is not much younger. One star in its immediate vicinity, sharing the same distance, has Si and O abundances at most 0.15 dex below solar. Conclusions. The low abundances measured in Dolidze 25 are compatible with currently accepted values for the slope of the Galactic metallicity gradient, if we take into account that variations of at least ±0.15 dex are observed at a given radius. The area traditionally identified as Dolidze 25 is only a small part of a much larger star-forming region that comprises the whole dust shell associated with Sh2-284 and very likely several other smaller H ii regions in its vicinity.

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The subject of Construction of Structures I studies, from a constructive point of view and taking into account current legislation, reinforced concrete structures used in buildings, through the acquisition of knowledge and construction criteria required in the profession of a Technical Architect. The contents acquired in this course are essential for further professional development of technicians and are closely related to many of the subjects taught in the same or other courses of the Degree in Technical Architecture at the University of Alicante. The aim of this paper is to present, analyze and discuss the development of a new methodology proposed in the mentioned subject, as it supposed an important change in the traditional way of teaching Construction and Structures I. In order to incorporate new teaching tools in 2013-2014, the course has been implemented by using a Moodle software tool to promote blended learning with online exercises. Our Moodle community allows collaborative work within an open-source platform where teachers and students share a new and personalized learning environment. Students are easily used to the interface and the platform, value the constant connection with teachers or other fellows and completely agree with the possibility of making questions or share documents 24 hours a day. The proposed methodology consists of lectures and practical classes. In the lectures, the basics of each topic are discussed; class attendance, daily study and conducting scheduled exercises are indispensable. Practical classes allow to consolidate the knowledge gained in theory classes by solving professional exercises and actual construction problems related to structures, that shall be compulsorily delivered online. So, after the correction of the teacher and the subsequent feedback of students, practical exercises ensure lifelong learning of the student, who can download any kind of material at any time (constructive details, practical exercises and even corrected exams). Regarding the general evaluation system, goals achievement is assessed on an ongoing basis (65% of the final mark) along the course through written and graphic evidences in person and online, as well as a individual development of a workbook. In all cases, the acquisition of skills, the ability to synthesize, the capacity of logical and critical thinking are assessed. The other 35 % of the mark is evaluated by a complementary graphic exam. Participation in the computing platform is essential and the student is required to do and present, at least 90% of the practices proposed. Those who do not comply with the practices in each specific date could not be assessed continuously and may only choose the final exam. In conclusion, the subject of Construction of Structures I is essential in the development of the regulated profession of Technical Architect as they are considered, among other professional profiles, as specialists in construction of building structures. The use of a new communication platform and online teaching allows the acquisition of knowledge and constructive approaches in a continuous way, with a more direct and personal monitoring by the teacher that has been highly appreciated by almost 100% of the students. Ultimately, it is important to say that the use of Moodle in this subject is a very interesting tool, which was really well welcome by students in one of the densest and important subjects of the Degree of Technical Architecture.

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This paper studies the use of directories of open access repositories worldwide (DOARW) to search Spanish repositories containing learning objects in the field of building engineering (BE). Results show that DOARW are powerful tools, but deficiencies (indicated in this study) have to be solved in order to obtain more accurate searches, and to facilitate repository-finding for potential users who are seeking learning objects (LOs) for reuse. Aiming to contribute to the promotion of the reuse of Spanish LOs, this study exposes to the academic community all existing Spanish repositories with LOs, and in particular, the repositories that contain LOs in the field of BE. This paper also studies the critical mass of available content (LOs) in the field of BE in Spain. It has been found to be low.

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Context. The eclipsing binary GU Mon is located in the star-forming cluster Dolidze 25, which has the lowest metallicity measured in a Milky Way young cluster. Aims. GU Mon has been identified as a short-period eclipsing binary with two early B-type components. We set out to derive its orbital and stellar parameters. Methods. We present a comprehensive analysis, including B and V light curves and 11 high-resolution spectra, to verify the orbital period and determine parameters. We used the stellar atmosphere code FASTWIND to obtain stellar parameters and create templates for cross-correlation. We obtained a model to fit the light and radial-velocity curves using the Wilson-Devinney code iteratively and simultaneously. Results. The two components of GU Mon are identical stars of spectral type B1 V with the same mass and temperature. The light curves are typical of an EW-type binary. The spectroscopic and photometric analyses agree on a period of 0.896640 ± 0.000007 d. We determine a mass of 9.0 ± 0.6 M⊙ for each component and for temperatures of 28 000 ± 2000 K. Both values are consistent with the spectral type. The two stars are overfilling their respective Roche lobes, sharing a common envelope and, therefore the orbit is synchronised and circularised. Conclusions. The GU Mon system has a fill-out factor above 0.8, containing two dwarf B-type stars on the main sequence. The two stars are in a very advanced stage of interaction, with their extreme physical similarity likely due to the common envelope. The expected evolution of such a system very probably leads to a merger while still on the main sequence.

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El siguiente artículo hace una reflexión crítica sobre los MOOC, prestando especial atención al análisis de los nuevos sistemas de evaluación; en concreto, el método peer to peer, y cómo esto afecta al rol de docentes y estudiantes. El estudio se ha llevado a cabo tomando como referencia dos sMOOC liderados por el Proyecto Europeo ECO (Elearning, Communication and Open-data: Massive Mobile, Ubiquitous and Open Learning). Los resultados que se presentan han sido analizados desde una perspectiva cuantitativa, utilizando como muestra a los miembros de la comunidad de aprendizaje que han participado en ambos cursos. A través de la utilización de un cuestionario se ha podido conocer cómo han valorado su experiencia formativa y su grado de satisfacción. La mitad de los sujetos encuestados ha considerado adecuado y justo el nuevo sistema evaluativo, sin embargo existe otra mitad que lo considera injusto y que tiene lagunas. Se ha abordado la evaluación como una parte intrínseca del proceso educativo y por ello se ha enfatizado en aspectos como el empoderamiento del alumnado, la cultura de la participación y la interacción social, conceptos que nos acercan a nuevos modelos de aprendizaje que potencian el intelecto colectivo y dejan atrás sistemas transmisivos de conocimiento.

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O presente Relatório Detalhado de Atividade Profissional é apresentado no âmbito da obtenção do Grau de Mestre dos Oficiais do Exército licenciados pré-Bolonha pela Academia Militar na Área específica de Administração Militar. A sua redação e estruturação tem por base o definido na NEP 520 e NEP 517/1ª da AM, para esta tipologia de trabalhos, tendo o autor, optado por desenvolver um tema no âmbito da sua atividade profissional, considerado como pioneiro e inovador. O Tenente-Coronel de Administração Militar do Exército Português, Luís Miguel Gonçalves, nasceu a 25 de Novembro de 1971. Do seu percurso académico e formativo, consta frequência pré-Universitária, em estabelecimento militar de ensino, no Instituto Militar dos Pupilos do Exército, na área de Contabilidade e Administração; a Licenciatura em Ciências Militares, na especialidade de Administração Militar, pela Academia Militar, em 1995, com a Classificação final de 13,58 valores; o tirocínio para Oficiais de Administração Militar, com a nota final de 15,38 valores; o Curso de Operações Irregulares, tendo obtido a classificação de 17,67 valores; o Curso de Promoção a Capitão, com 16,63 valores; e o Curso de Promoção a Oficial Superior do Instituto de Altos Estudos Militares, com a classificação final de 14,50 valores. No âmbito da formação de pós-graduação, tem averbado créditos no módulo de Metodologia de Investigação Cientifica, pela Academia Militar, no Ano Letivo 2013/14, com a classificação final de 16,00 valores. Para além destes, o Environmental Course For Portugal – NATO School/ SHAPE; formação em Gestão de Projetos/ Exército - Microsoft Enterprise Project Management; o Curso de Formação Pedagógica Inicial de Formadores do Instituto de Emprego e Formação Profissional, com Homologação das Competências Pedagógicas; e vários certificados de formações no âmbito da Contabilidade, Administração, Finanças Públicas e Auditorias Financeiras, atribuídas pela Direção de Finanças do Exército e pelo Instituto de Gestão e Administração Pública do Porto. Ao longo dos 25 anos de serviço prestado ao Exército Português, como Oficial de Administração Militar, desempenhou diversos cargos e funções de Comando e Chefia, em várias UEO, nas áreas setoriais e funcionais, da formação, da instrução, da componente operacional, da logística, do pessoal, das finanças públicas, das inspeções e auditorias, da gestão e da Administração Militar. Atualmente o Tenente-Coronel Miguel Gonçalves, desempenha as Funções de Comandante de Batalhão na Escola dos Serviços. Para além dos cargos e funções averbadas no seu Curriculum Vitae detalhado, constituiu em 1996 o Núcleo Logístico de Projeção, Implantação, Acompanhamento e Ajuda Técnica no âmbito do emprego dos meios táticos e operacionais da Área de Responsabilidade FND/ IFOR na Bósnia-Herzegovina (Jugoslávia). Tem publicado na Revista da Administração Militar, vários artigos no âmbito da logística operacional, na função de combate Apoio de Serviços. Na área da formação, foi orientador e supervisor de vários trabalhos, individuais e de grupo aos cursos de promoção a capitão; e constitui-se como elemento primariamente responsável pelo planeamento e implementação dos primeiros cursos no Exército, com formação certificado pela Agência Nacional para a Qualificação e Ensino Profissional, I.P., do Sistema Nacional de Qualificações, certificação inserida no Catálogo Nacional de Qualificações. Na área Inspetiva, integrou várias equipas de Inspeção-Geral do Exército, como inspetor responsável pelas áreas de Logística e Finanças, bem como as de Inspetor, para a área dos recursos humanos – Despesas com Pessoal, nas equipas de inspeção do Comando do Pessoal do Exército. No desempenho das funções de Auditor Financeiro do Centro de Finanças do Comando do Pessoal, realizou diversas auditorias financeiras às UEO do Comando do Pessoal, na sua dependência, tendo desenvolvido e implementado um sistema pioneiro e inovador de monitorização e controlo interno, de auditorias “Online” com análise e reporte mensal, às contas das UEO do Comando do Pessoal, tendo em vista a validação das Demonstrações Financeiras para a Conta de Gerência Anual do Exército. A escolha do tema, “O Controlo Interno e a implementação de Auditorias Online no SAFEx em contexto de e-Governance: Tecnologias, desafios e oportunidades” surge na sequência da implementação destes procedimentos pelo autor, numa altura em que o Exército entrava em operativo com o Sistema Integrado de Gestão (SIG/DN), tendo sido à data reconhecido publicamente pelo TGEN Comandante do Pessoal do Exército, como sendo um procedimento inovador, com notáveis vantagens para a eficiência e eficácia do sistema administrativo-financeiro do Comando do Pessoal e consequentemente do Exército.

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Editor: Feb. 1887-1919, Paul Carus.