2,632 research outputs found

    Fostering college and career readiness: how career development activities in schools impact on graduation rates and students' life success

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    This paper sets out the recent evidence around career development. This evidence is examined within the context of the college and career readiness agenda. The argument is made that in order for young people to be genuinely “ready” for both college and career they need to have attended to their academic achievement, their aspirations and plans for the future, their ability to make transitions and their ability to direct their own careers. It is argued that career development offers schools a body of practice that has been shown to have a positive impact on young people’s readiness for college and career. The report acknowledges that the provision of career development has been in decline in many North American schools despite evidence of its effectiveness. Given the current instability of the labor market, the increasing complexity of the education system and the need to grow the skills base of the workforce in a competitive global market, failing to attend to young people’s careers seems shortsighted. As this paper shows, there is a strong body of evidence which demonstrates that career development activity in schools can help young people to experience academic achievement, successfully transition to the labor market and live happier and more productive lives. It is hoped that setting out the evidence in this area of research will provide policy makers and school leaders with the resources required to make informed decisions and to support the development of the future generations of talent. The paper explores the impacts of career development in relation to four main questions: ‱ Does career development engage young people in their schooling and help keep them attending school? ‱ Does career development positively impact on young people’s academic achievement? ‱ Does career development assist young people in making successful transitions to college or the labor market? ‱ Does career development have a positive effect on people’s career and life success?Career Cruisin

    Embedded AGN and star formation in the central 80 pc of IC 3639

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    [Abridged] Methods: We use interferometric observations in the NN-band with VLTI/MIDI to resolve the mid-IR nucleus of IC 3639. The origin of the nuclear infrared emission is determined from: 1) the comparison of the correlated fluxes from VLTI/MIDI with the fluxes measured at subarcsec resolution (VLT/VISIR, VLT/ISAAC); 2) diagnostics based on IR fine-structure line ratios, the IR continuum emission, IR bands produced by polycyclic aromatic hydrocarbons (PAH) and silicates; and 3) the high-angular resolution spectral energy distribution. Results: The unresolved flux of IC 3639 is 90±20 mJy90 \pm 20\, \rm{mJy} at 10.5 Όm10.5\, \rm{\mu m}, measured with three different baselines in VLTI (UT1-UT2, UT3-UT4, and UT2-UT3; 4646-58 m58\, \rm{m}), making this the faintest measurement so far achieved with mid-IR interferometry. The correlated flux is a factor of 33-44 times fainter than the VLT/VISIR total flux measurement. The observations suggest that most of the mid-IR emission has its origin on spatial scales between 1010 and 80 pc80\, \rm{pc} (4040-340 mas340\, \rm{mas}). A composite scenario where the star formation component dominates over the AGN is favoured by the diagnostics based on ratios of IR fine-structure emission lines, the shape of the IR continuum, and the PAH and silicate bands. Conclusions: A composite AGN-starburst scenario is able to explain both the mid-IR brightness distribution and the IR spectral properties observed in the nucleus of IC 3639. The nuclear starburst would dominate the mid-IR emission and the ionisation of low-excitation lines (e.g. [NeII]12.8ÎŒm_{12.8 \rm{\mu m}}) with a net contribution of ∌70%\sim 70\%. The AGN accounts for the remaining ∌30%\sim 30\% of the mid-IR flux, ascribed to the unresolved component in the MIDI observations, and the ionisation of high-excitation lines (e.g. [NeV]14.3ÎŒm_{14.3 \rm{\mu m}} and [OIV]25.9ÎŒm_{25.9 \rm{\mu m}}).Comment: Accepted for publication in A&

    Polarization measurements analysis II. Best estimators of polarization fraction and angle

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    With the forthcoming release of high precision polarization measurements, such as from the Planck satellite, it becomes critical to evaluate the performance of estimators for the polarization fraction and angle. These two physical quantities suffer from a well-known bias in the presence of measurement noise, as has been described in part I of this series. In this paper, part II of the series, we explore the extent to which various estimators may correct the bias. Traditional frequentist estimators of the polarization fraction are compared with two recent estimators: one inspired by a Bayesian analysis and a second following an asymptotic method. We investigate the sensitivity of these estimators to the asymmetry of the covariance matrix which may vary over large datasets. We present for the first time a comparison among polarization angle estimators, and evaluate the statistical bias on the angle that appears when the covariance matrix exhibits effective ellipticity. We also address the question of the accuracy of the polarization fraction and angle uncertainty estimators. The methods linked to the credible intervals and to the variance estimates are tested against the robust confidence interval method. From this pool of estimators, we build recipes adapted to different use-cases: build a mask, compute large maps, and deal with low S/N data. More generally, we show that the traditional estimators suffer from discontinuous distributions at low S/N, while the asymptotic and Bayesian methods do not. Attention is given to the shape of the output distribution of the estimators, and is compared with a Gaussian. In this regard, the new asymptotic method presents the best performance, while the Bayesian output distribution is shown to be strongly asymmetric with a sharp cut at low S/N.Finally, we present an optimization of the estimator derived from the Bayesian analysis using adapted priors

    Three-dimensional matter-wave vortices in optical lattices

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    We predict the existence of spatially localized nontrivial vortex states of a Bose-Einstein condensate with repulsive atomic interaction confined by a three-dimensional optical lattice. Such vortex-like structures include planar vortices, their co- and counter-rotating bound states, and distinctly three-dimensional non-planar vortex states. We demonstrate numerically that many of these vortex structures are remarkably robust, and therefore can be generated and observed in experiment.Comment: 4 pages, 6 figure

    Career guidance in communities

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    Career guidance in communities, by Rie Thomsen, Aarhus, Denmark, Aarhus University Press, 2012, 256 pp., ÂŁ34.78 (paperback), ISBN 9788771240122 Reviewed by Tristram Hooley, Reader in Career Development, University of Derby, UK. Email: [email protected]/

    Vortices in atomic-molecular Bose-Einstein condensates

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    The structure and stability of vortices in hybrid atomic-molecular Bose-Einstein condensates is analyzed in the framework of a two-component Gross-Pitaevskii-type model that describes the stimulated Raman-induced photoassociation process. New types of topological vortex states are predicted to exist in the coherently coupled two-component condensates even without a trap, and their nontrivial dynamics in the presence of losses is demonstrated.Comment: 7 pages, 6 figure

    Coast Calendar

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    https://digitalmaine.com/books/1167/thumbnail.jp

    Data Encoding in Lossless Prediction-Based Compression Algorithms

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