Teacher training processes and teachers' competence : A sociological study in the primary school

The paper describes part of a study whose aim was to investigate the relation between modalities of teacher training and modalities of pedagogic practice implemented in the science classroom. The study is focused on primary school context and analyses the evolution of teachers performance in terms of their acquisition of recognition and realisation rules, i.e. coding orientation, to specific scientific learning contexts. Theoretically, the study is based on Bernstein’s theory of pedagogic discourse (1999, 2000)which provided the concepts to characterise the modalities of teacher training and of classroom pedagogic practices and to analyse teachers’ evolution in terms of recognition and realisation rules. The sample was made up of four teachers and their four socially heterogeneous school classes. An action-research methodology was followed.The results suggest that the teacher training implemented was favourable to the teachers’ professional development and their competence to lead all children to a high level of scientific development. The efficiency of the training process has to be mostly attributed to the strong classification of the researcher-teachers relation and to the strong framing of evaluation criteria, selection and sequence, together with weak framing of hierarchical rules and pacing.Fundação Calouste Gulbenkian, Instituto de Inovação Educacional e Fundação para a Ciência e Tecnologia (FCT)

Modelo de avaliação da usabilidade de interfaces Web

A investigação aqui descrita explora a avaliação da usabilidade de interfaces de sítios Web sustentada nos fundamentos da IHC e apresenta um novo metamodelo universal de avaliação da usabilidade, designado por UsaWeb, aplicável a qualquer interface Web, sendo uma proposta completa e coerente que representa um novo paradigma de avaliação da usabilidade de interfaces Web

The Phoenix Deep Survey: The 1.4 GHz microJansky catalogue

The initial Phoenix Deep Survey (PDS) observations with the Australia Telescope Compact Array have been supplemented by additional 1.4 GHz observations over the past few years. Here we present details of the construction of a new mosaic image covering an area of 4.56 square degrees, an investigation of the reliability of the source measurements, and the 1.4 GHz source counts for the compiled radio catalogue. The mosaic achieves a 1-sigma rms noise of 12 microJy at its most sensitive, and a homogeneous radio-selected catalogue of over 2000 sources reaching flux densities as faint as 60 microJy has been compiled. The source parameter measurements are found to be consistent with the expected uncertainties from the image noise levels and the Gaussian source fitting procedure. A radio-selected sample avoids the complications of obscuration associated with optically-selected samples, and by utilising complementary PDS observations including multicolour optical, near-infrared and spectroscopic data, this radio catalogue will be used in a detailed investigation of the evolution in star-formation spanning the redshift range 0 < z < 1. The homogeneity of the catalogue ensures a consistent picture of galaxy evolution can be developed over the full cosmologically significant redshift range of interest. The 1.4 GHz mosaic image and the source catalogue are available on the web at http://www.atnf.csiro.au/~ahopkins/phoenix/ or from the authors by request.Comment: 16 pages, 11 figures, 4 tables. Accepted for publication by A

Constraining the Location of Microlensing Objects by using the Finite Source Effect in EAGLE events

We propose a new method to constrain the location of microlensing objects using EAGLE (Extremely Amplified Gravitational LEnsing) events. We have estimated the rate of EAGLE events by taking the finite-source effect in to account. We found that the EAGLE event rate for using a 1-m class telescope w hose limiting magnitude is $V \sim 21$ is the same as or higher than that of the ordinary microlensing events which have been found to date. We have also found that the fraction of transit EAGLE events is large enough to detect: between $4 \sim 80$ depending on the lens location. Since the lens proper motion can be measured for a transit event, one can distinguish whether the lens is a MACHO (MAssive Compact Halo Object) in our hal o or one of the known stars in the Large Magellanic Cloud (LMC) from the proper motion measurement for each transit EAGLE event. Moreover, we show that the fraction of transit EAGLEs in all EAGLE events signif icantly depends on the lensing locations: the transit EAGLE fraction for the sel f-lensing case is $2 \sim 15$ times larger than that for halo MACHOs. Thus, one can constrain the location of lens objects by the statistics of the tr ansit events fraction. We show that we can reasonably expect $0 \sim 6$ transit events out of 21 EAGLE events in 3 years. We can also constrain the lens population properties at a gre ater than 99% confidence level depending on the number of transit events de tected. We also present the duration of EAGLE events, and show how an hourly ob servational mode is more suitable for an EAGLE event search program.Comment: 18 pages, 4 figures, accepted for publication in Ap

Aplicación del método Delphi para la inclusión de las externalidades en análisis de seguridad y de salud laboral

Organizations should regularly conduct an assessment of their occupational hazards in order to design and implement preventive measures that are necessary and sufficient to deal with the level of risk, the costs of prevention and the safety at levels considered acceptable by the organization. Furthermore, the selection of measures to be implemented in an organization should take into account both internal and external costs. Externalities are of great importance in terms of the costs of accidents at work; nevertheless, they are not often properly addressed by the organizations. In this paper we describe an application of the Delphi method to understand how externalities can be included in Occupational Safety and Health.Las organizaciones deben realizar periódicamente una evaluación de sus riesgos laborales con el fin de diseñar y poner en práctica medidas preventivas que sean necesarias y suficientes para mantener e l nivel de riesgo, los costos de la prevención y la seguridad en los niveles considerados aceptables por la organización. Por otra parte, la selección de las medidas a aplicar en una organización debe tener en cuenta tanto los costes internos como externos. Las externalidades son de gran importancia en términos de los costos de los accidentes de trabajo; sin embargo, a menudo no se tratan adecuadamente por las organizaciones. En este artículo se describe una aplicación del método Delphi para entender cómo los factores externos pueden ser incluidos en la Seguridad y Salud Laboral.The authors would like to acknowledge all the experts who have participated in the Delphi panel. The authors also acknowledge the anonymous reviewers who helped to improve the overall quality of the current manuscript. This study was financially supported by FCT-Fundação para a Ciência e Tecnologia of Portugal, under the project ID/CEC/00319/2013

Neutrophil swarms require LTB4 and integrins at sites of cell death in vivo

Neutrophil recruitment from blood to extravascular sites of sterile or infectious tissue damage is a hallmark of early innate immune responses, and the molecular events leading to cell exit from the bloodstream have been well defined1,2. Once outside the vessel, individual neutrophils often show extremely coordinated chemotaxis and cluster formation reminiscent of the swarming behaviour of insects3,4,5,6,7,8,9,10,11. The molecular players that direct this response at the single-cell and population levels within the complexity of an inflamed tissue are unknown. Using two-photon intravital microscopy in mouse models of sterile injury and infection, we show a critical role for intercellular signal relay among neutrophils mediated by the lipid leukotriene B4, which acutely amplifies local cell death signals to enhance the radius of highly directed interstitial neutrophil recruitment. Integrin receptors are dispensable for long-distance migration12, but have a previously unappreciated role in maintaining dense cellular clusters when congregating neutrophils rearrange the collagenous fibre network of the dermis to form a collagen-free zone at the wound centre. In this newly formed environment, integrins, in concert with neutrophil-derived leukotriene B4 and other chemoattractants, promote local neutrophil interaction while forming a tight wound seal. This wound seal has borders that cease to grow in kinetic concert with late recruitment of monocytes and macrophages at the edge of the displaced collagen fibres. Together, these data provide an initial molecular map of the factors that contribute to neutrophil swarming in the extravascular space of a damaged tissue. They reveal how local events are propagated over large-range distances, and how auto-signalling produces coordinated, self-organized neutrophil-swarming behaviour that isolates the wound or infectious site from surrounding viable tissue

Microbiological analysis of Portugal northern coastal beach sands

Poster apresentado no XIV Congresso Nacional de Bioquímica, Vilamoura, Portugal, 2004

On the Determination of Star Formation Rates in Evolving Galaxy Populations

The redshift dependence of the luminosity density in certain wavebands (e.g. UV and H-alpha) can be used to infer the history of star formation in the populations of galaxies producing this luminosity. This history is a useful datum in studies of galaxy evolution. It is therefore important to understand the errors that attend the inference of star formation rate densities from luminosity densities. This paper explores the self-consistency of star formation rate diagnostics by reproducing commonly used observational procedures in a model with known galaxy populations, evolutionary histories and spectral emission properties. The study reveals a number of potential sources of error in the diagnostic processes arising from the differential evolution of different galaxy types. We argue that multi-wavelength observations can help to reduce these errors.Comment: 13 pages (including 5 encapsulated postscript figures), aastex, accepted for publication in Ap

Stress ocupacional e afrontamento em oficiais da polícia militar portuguesa

This study describes the professional experience of military police officers from the Portuguese Republican National Guard (N = 95). We focused on the main sources and consequences of stress and the coping strategies used to deal with stress. The evaluation protocol included one closed-ended question and four open-ended questions. Data analysis of meaningful text segments was conceptually based and data categorization followed deductive content analysis. Results allowed the identification of 483 meaning units. Factors intrinsic to the job and the relationships at work were the main stressors referred by participants. The consequences of stressors were evident at an individual level, affecting family, psychological, and physical/health domains. The coping strategies used to deal with the main source of stress in the professional career were focused on problem solving (e.g., active confrontation) and emotional regulation (e.g., situation acceptance). Practical implications and future avenues of research with these professionals are discussed.Este estudio analiza la experiencia profesional de agentes de la policía militar de la Guarda Nacional Republicana portuguesa (N = 95). Se centró en las principales fuentes y consecuencias del estrés, así como en las estrategias de afrontamiento. El protocolo de evaluación incluyó una pregunta cerrada y cuatro abiertas. Se realizó una categorización de datos atendiendo a un análisis de contenido deductivo. Las respuestas permitieron establecer 483 unidades de significado, a partir de las cuales se identificaron las principales quejas, relacionadas con factores intrínsecos al trabajo y a las relaciones interpersonales. Las consecuencias de estos problemas fueron evidentes en el plano individual (psicológicas y de salud física) y también afectaban a la familia. Las habilidades utilizadas para hacer frente a las principales fuentes de estrés estaban centradas en la resolución de problemas y el control emocional. Se discuten las implicaciones prácticas y las futuras vías de investigación con estos profesionales.Este estudo analisa a experiência profissional de agentes da polícia militar da Guarda Nacional Republicana Portuguesa (N=95). Centramo-nos nas principais fontes e consequências do stress assim como nas estratégias de afrontamento. O protocolo de avaliação incluiu uma pergunta fechada e quatro abertas. Realizou-se uma categorização de dados atendendo a uma análise de conteúdo dedutivo. As respostas permitiram a identificação de 483 unidades de significado, a partir das quais se identificaram as principais queixas. Estas estavam relacionadas com fatores intrínsecos ao trabalho e relações interpessoais. As consequências destes problemas foram evidentes no nível individual (psicológicas e saúde física) afetando também à família. As habilidades utilizadas para fazer frente às principais fontes de stress estavam centradas na resolução de problemas e o controle emocional. Discutem-se as implicações práticas e as futuras vias de pesquisa com estes profissionais.This study was conducted at Psychology Research Centre, University of Minho, and supported by the Portuguese Foundation for Science and Technology and the Portuguese Ministry of Education and Science through national funds and when applicable co-financed by FEDER under the PT2020 Partnership Agreement (UID/PSI/01662/2013)

Direct Detection of Giant Close-In Planets Around the Source Stars of Caustic-Crossing Microlensing Events

We propose a direct method to detect close-in giant planets orbiting stars in the Galactic bulge. This method uses caustic-crossing binary microlensing events discovered by survey teams monitoring the bulge to measure light from a planet orbiting the source star. When the planet crosses the caustic, it is more magnified than the source star; its light is magnified by two orders of magnitude for Jupiter size planets. If the planet is a giant close to the star, it may be bright enough to make a significant deviation in the light curve of the star. Detection of this deviation requires intensive monitoring of the microlensing light curve using a 10-meter class telescope for a few hours after the caustic. This is the only method yet proposed to directly detect close-in planets around stars outside the solar neighborhood.Comment: 4 pages, 2 figures. Submitted to ApJ Letter