3,223 research outputs found

    Interception and Offshore Processing of Asylum Seekers: The International Law Dimensions

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    For decades the international community has conducted a delicate and politically charged balancing act trying to reconcile the inexorable increase in refugees-and the need to find permanent homes for them with the fundamental right of all countries to have secure frontiers. While the notion of non-refoulement remains fundamental to the treatment of asylum seekers, their rights vis A vis the states in which they seek asylum are significantly circumscribed by their alien status. States have a right to control entry to their territories. In the development of asylum law and policy, the central difficulty for states, and indeed the international community, is how to construct an appropriate balance between the urgent humanitarian demands to protect those who are genuinely in need of asylum, and the exclusion of those who do not qualify for humanitarian protection

    Inspiring Music for All: next steps in innovation, improvement and integration

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    The report, funded by the Paul Hamlyn Foundation, provides an overview of schools-based music education in England. It represents the outcomes of research undertaken in January and February 2014 which included detailed literature reviews, personal interviews with thirty-five specialists involved in leading various organisations responsible for different aspects of music education, focus group discussions and an on-line survey of the music education workforce that generated 515 responses. The findings suggest that the place and status of music in schools vary widely across the country. The best music in schools is significantly more inclusive, more musically diverse and better quality that it was a decade ago. However, the quality and reach of schools-based music education is still unacceptably variable and inconsistent at both primary and secondary levels. Detailed findings and recommendations are included in the report

    Appearance-based localization for mobile robots using digital zoom and visual compass

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    This paper describes a localization system for mobile robots moving in dynamic indoor environments, which uses probabilistic integration of visual appearance and odometry information. The approach is based on a novel image matching algorithm for appearance-based place recognition that integrates digital zooming, to extend the area of application, and a visual compass. Ambiguous information used for recognizing places is resolved with multiple hypothesis tracking and a selection procedure inspired by Markov localization. This enables the system to deal with perceptual aliasing or absence of reliable sensor data. It has been implemented on a robot operating in an office scenario and the robustness of the approach demonstrated experimentally

    ROSAT and ASCA observations of the Crab-Like Supernova Remnant N157B in the Large Magellanic Cloud

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    We report the results of ROSAT and ASCA X-ray observations of the supernova remnant N157B (or 30 Dor B, SNR 0539-69.1) in the Large Magellanic Cloud. For comparison, we also briefly describe the results on SNR 0540-69.3, the only confirmed Crab-like remnant in the Cloud. The X-ray emission from N157B can be decomposed into a bright comet-shaped feature, superimposed on a diffuse emission region of a dimension 20\sim 20 pc. The flat and nearly featureless spectrum of the remnant is distinctly different from those of young shell-like remnants, suggesting a predominantly Crab-like nature of N157B. Characterized by a power law with an energy slope 1.5\sim 1.5, the spectrum of N157B above 2\sim 2 keV is, however, considerably steeper than that of SNR 0540-69.3, which has a slope of 1.0\sim 1.0. At lower energies, the spectrum of N157B presents marginal evidence for emission lines, which if real most likely arise in hot gas of the diffuse emission region. The hot gas has a characteristic thermal temperature of 0.4-0.7 keV. No significant periodic signal is detected from N157B in the period range of 3×10320003 \times 10^{-3}-2000 s. The pulsed fraction is 9\lesssim 9% (99% confidence) in the 272-7 keV range. We discuss the nature of the individual X-ray components. In particular, we suggest that the synchrotron radiation of relativistic particles from a fast-moving (103kms1\sim 10^3 km s^{-1}) pulsar explains the size, morphology, spectrum, and energetics of the comet-shaped X-ray feature. We infer the age of the remnant as 5×103\sim 5 \times 10^3 yrs. The lack of radio polarization of the remnant may be due to Faraday dispersion by foreground \ion{H}{2} gas.Comment: To be published in The Astrophysical Journal, 21 pages, plus 11 images in the PS, GIF, or jpeg format. Postscript files of images are available at http://www.astro.nwu.edu/astro/wqd/paper/n157b
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