11,581 research outputs found

    'I just want a job' : what do we really know about young people in jobs without training?

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    Over recent years, a central concern of policy has been to drive up post-16 participation rates in full-time education and address the needs of young people not in education, employment or training (NEET). As a result, young people who enter work which is classified as 'without training' at 16/17 have largely been ignored. However, the decision to Raise the Participation Age (RPA) for continuing in learning for all 17-year olds from 2013 and for all 18-year olds from 2015 in England, together with a growing unease about the impact of the current recession on youth unemployment rates, have revived interest in the 'jobs without training' (JWT) group. This paper draws on the findings from two studies: first, a qualitative study in two contrasting local labour markets, of young people in JWT, together with their employers and parents; and second, an evaluation of the Learning Agreement Pilots (LAP), which was the first policy initiative in England targeted at the JWT group. Both studies reveal a dearth of understanding about early labour market entrants and a lack of policy intervention and infrastructure to support the needs of the JWT group throughout the UK. From this, it is concluded that questionable assumptions have been made about the composition and the aspirations of young people in JWT, and their employers, on the basis of little or no evidence. As a consequence, a policy 'quick fix' to satisfy the RPA agenda will not easily be achieved. If the decision to raise the participation age is adopted also by the Welsh and Scottish parliaments, similar challenges may have to be faced

    The Price Premium for Organic Babyfood: A Hedonic Analysis

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    The price premium associated with organic babyfood is estimated by applying a hedonic model to price and characteristic data for babyfood products collected in two cities: Raleigh, North Carolina, and San Jose, California. The price per ounce of babyfood is modeled as a function of a number of babyfood and store characteristics. The estimated organic price premium is generally equal to 3 cents to 4 cents per ounce. To the extent this premium reflects consumer willingness to pay to reduce pesticide exposures, it could be used to infer values for reduced dietary exposures to pesticide residues for babies.babyfood, hedonic analysis, organic foods, Demand and Price Analysis,

    Two on-line tools for feedback on grammar and style in academic writing

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    This paper introduces two online academic writing tools which should help address two common feedback problems at ECU. Undergraduate students often consider that they receive little appraisal of the style (including grammar), rather than the content, of their academic writing. In contrast, many research students frustrate their supervisors by failing to learn from detailed corrections of their writing style. I independently developed a coding system for specific types of style errors, as have other academics and editors. The more significant innovation is the much more expansive interactive web tool which matches the numbered fault types to multi-layered explanations of each fault, complete with corrected examples. Feedback can involve highlighting the problem text and providing the fault number with or without further editing for style; the latter approach is time-efficient while also fostering self-reliance. In writing workshops I also promote independent learning by only teaching a few of these faults intensively and challenging students to master the rest by exploring the interactive web tool. While feedback on these tools from academic writing clients has been encouraging, convincing more academics to trial these tools with their students could help provide valuable appraisal of their usefulness

    Model Theory, Hume's Dictum, and the Priority of Ethical Theory

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    It is regrettably common for theorists to attempt to characterize the Humean dictum that one can’t get an ‘ought’ from an ‘is’ just in broadly logical terms. We here address an important new class of such approaches which appeal to model-theoretic machinery. Our complaint about these recent attempts is that they interfere with substantive debates about the nature of the ethical. This problem, developed in detail for Daniel Singer’s and Gillian Russell and Greg Restall’s accounts of Hume’s dictum, is of a general type arising for the use of model-theoretic structures in cashing out substantive philosophical claims: the question of whether an abstract model-theoretic structure successfully interprets something often involves taking a stand on non-trivial issues surrounding the thing. In the particular case of Hume’s dictum, given reasonable conceptual or metaphysical claims about the ethical, Singer’s and Russell and Restall’s accounts treat obviously ethical claims as descriptive and vice versa. Consequently, their model-theoretic characterizations of Hume’s dictum are not metaethically neutral. This encourages skepticism about whether model-theoretic machinery suffices to provide an illuminating distinction between the ethical and the descriptive

    The Curious Conundrum Regarding Sulfur Abundances In Planetary Nebulae

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    Sulfur abundances derived from optical emission line measurements and ionization correction factors in planetary nebulae are systematically lower than expected for the objects' metallicities. We have carefully considered a large range of explanations for this "sulfur anomaly", including: (1) correlations between the size of the sulfur deficit and numerous nebular and central star properties; (2) ionization correction factors which under-correct for unobserved ions; (3) effects of dielectronic recombination on the sulfur ionization balance; (4) sequestering of S into dust and/or molecules; and (5) excessive destruction of S or production of O by AGB stars. It appears that all but the second scenario can be ruled out. However, we find evidence that the sulfur deficit is generally reduced but not eliminated when S^+3 abundances determined directly from IR measurements are used in place of the customary sulfur ionization correction factor. We tentatively conclude that the sulfur anomaly is caused by the inability of commonly used ICFs to properly correct for populations of ionization stages higher than S^+2.Comment: 40 pages, 14 figures, 3 tables. Accepted for publication in the Astrophysical Journa

    Literature review of human microbes' interaction with plants

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    Human carried microorganisms, which cannot practically be excluded from human supporting agricultural systems of extra terrestrial stations, are considered. These microorganisms damage the plants on which the people depend for oxygen and food. The inclusion of carefully screened or constructed, but more or less normal, phylloplane and rhizosphere microbial communities is studied

    A study of the social and physical environment in catering kitchens and the role of the chef in promoting positive health and safety behaviour

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    This is the account of a mixed method study of chefs and their kitchens in order to identify the nature of their workplace and how this affects their ability to manage health and safety in the kitchen. It included extended periods of observation, monitoring of physical parameters, analysis of records of reported accidents, and a series of reflexive interviews. The findings were integrated and then fed back in a smaller number of second interviews in order to test whether the findings fitted in with the chefs' understanding of their world. Major factors identified included survival in a market environment, the status of the chef (and the kitchen) within organisations, marked autocracy of chefs, and an increasing tempo building up to service time with commensurate heat, noise, and activity. In particular during the crescendo, a threshold shift in risk tolerance was identified. The factors, their interplay, and their implications for health and safety in the catering kitchen are discussed

    Nebular spectroscopy of SN 2014J: Detection of stable nickel in near infrared spectra

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    We present near infrared (NIR) spectroscopy of the nearby supernova 2014J obtained ∌\sim450 d after explosion. We detect the [Ni II] 1.939 ÎŒ\mum line in the spectra indicating the presence of stable 58^{58}Ni in the ejecta. The stable nickel is not centrally concentrated but rather distributed as the iron. The spectra are dominated by forbidden [Fe II] and [Co II] lines. We use lines, in the NIR spectra, arising from the same upper energy levels to place constraints on the extinction from host galaxy dust. We find that that our data are in agreement with the high AVA_V and low RVR_V found in earlier studies from data near maximum light. Using a 56^{56}Ni mass prior from near maximum light Îł\gamma-ray observations, we find ∌\sim0.05 M⊙_\odot of stable nickel to be present in the ejecta. We find that the iron group features are redshifted from the host galaxy rest frame by ∌\sim600 km s−1^{-1}.Comment: 6 pages, 4 figures, submitted to A&
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