968 resultados para The Palgrave dictionary of transnational history


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Added t.-p. engraved: Third American edition of Nicholson's British encyclopedia; or, Dictionary of arts & sciences.

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De luxe supplement. Chicago, The S.J. Clarke publishing company, 1921. 716 p. incl. ports. 32 cm.

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"Chronological tables of Greek and Roman history, civil and literary, from the first Olympiad, B.C. 776, to the fall of the Western Empire, A.D. 476. With tables of Greek and Roman measures, weights, and money. Ed. by William Smith ... ": p. [957]-1039.

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Vol. 1 has t.p.: The century dictionary and cyclopedia, an encyclopedic lexicon of the English language and a pronouncing and etymological dictionary of names in geography, biography, mythology, history, art, etc., etc. together with atlas of the world.

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The purpose of this thesis was to explore how Christian networks enable strategies of transnational alliance, whereby groups in different nations strive to strengthen one another’s leverage and credibility in order to resolve conflicts and elaborate new possibilities. This research does so by analyzing the case of the Presbyterian Church of Colombia (IPC). The project examines the historical development of the IPC from the initial missionary period of the 1850s until the present. Specifically, the purpose of the study was to consider how the historical struggle to articulate autonomy and equality vis-à-vis the U.S. Presbyterians (PCUSA) and paternalist models of ecclesial relations has affected recent political strategies pursued by the IPC. Despite the paternalism of the early missionary model, changing conceptions of social transformation during the 60s contributed to a shift in relations. Over time the IPC and PCUSA negotiated relationships in which groups both acknowledge a problematic history and insist upon an ethnic of partnership and respect. Today, PCUSA groups, in concert with the IPC, collaborate on a range of transnational political strategies aimed at strengthening the IPC’s leverage in local struggles for justice and peace. A review of this case suggests that long-established Christian networks may have an advantage over other civil society groups such as NGOs in facilitating strategies of transnational alliance. Although civil society organizations often have better access to important resources needed for international advocacy initiatives, Christian networks, such as the one established between the IPC and U.S. Presbyterian communities, rely on a history of negotiating power-disparity in order to elaborate relationships based on listening and partnership. Such findings prove important not only to how we conceptualize transnational alliance but also to the ways that we think about the history and future of Christian networks.

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The objective of this study was to estimate the regressions calibration for the dietary data that were measured using the quantitative food frequency questionnaire (QFFQ) in the Natural History of HPV Infection in Men: the HIM Study in Brazil. A sample of 98 individuals from the HIM study answered one QFFQ and three 24-hour recalls (24HR) at interviews. The calibration was performed using linear regression analysis in which the 24HR was the dependent variable and the QFFQ was the independent variable. Age, body mass index, physical activity, income and schooling were used as adjustment variables in the models. The geometric means between the 24HR and the calibration-corrected QFFQ were statistically equal. The dispersion graphs between the instruments demonstrate increased correlation after making the correction, although there is greater dispersion of the points with worse explanatory power of the models. Identification of the regressions calibration for the dietary data of the HIM study will make it possible to estimate the effect of the diet on HPV infection, corrected for the measurement error of the QFFQ.

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The VISTA near infrared survey of the Magellanic System (VMC) will provide deep YJK(s) photometry reaching stars in the oldest turn-off point throughout the Magellanic Clouds (MCs). As part of the preparation for the survey, we aim to access the accuracy in the star formation history (SFH) that can be expected from VMC data, in particular for the Large Magellanic Cloud (LMC). To this aim, we first simulate VMC images containing not only the LMC stellar populations but also the foreground Milky Way (MW) stars and background galaxies. The simulations cover the whole range of density of LMC field stars. We then perform aperture photometry over these simulated images, access the expected levels of photometric errors and incompleteness, and apply the classical technique of SFH-recovery based on the reconstruction of colour-magnitude diagrams (CMD) via the minimisation of a chi-squared-like statistics. We verify that the foreground MW stars are accurately recovered by the minimisation algorithms, whereas the background galaxies can be largely eliminated from the CMD analysis due to their particular colours and morphologies. We then evaluate the expected errors in the recovered star formation rate as a function of stellar age, SFR(t), starting from models with a known age-metallicity relation (AMR). It turns out that, for a given sky area, the random errors for ages older than similar to 0.4 Gyr seem to be independent of the crowding. This can be explained by a counterbalancing effect between the loss of stars from a decrease in the completeness and the gain of stars from an increase in the stellar density. For a spatial resolution of similar to 0.1 deg(2), the random errors in SFR(t) will be below 20% for this wide range of ages. On the other hand, due to the lower stellar statistics for stars younger than similar to 0.4 Gyr, the outer LMC regions will require larger areas to achieve the same level of accuracy in the SFR( t). If we consider the AMR as unknown, the SFH-recovery algorithm is able to accurately recover the input AMR, at the price of an increase of random errors in the SFR(t) by a factor of about 2.5. Experiments of SFH-recovery performed for varying distance modulus and reddening indicate that these parameters can be determined with (relative) accuracies of Delta(m-M)(0) similar to 0.02 mag and Delta E(B-V) similar to 0.01 mag, for each individual field over the LMC. The propagation of these errors in the SFR(t) implies systematic errors below 30%. This level of accuracy in the SFR(t) can reveal significant imprints in the dynamical evolution of this unique and nearby stellar system, as well as possible signatures of the past interaction between the MCs and the MW.

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Small mammals are subject to predation from mammalian, avian and reptilian predators. There is an obvious advantage for prey species to detect the presence of predators in their environment, enabling them to make decisions about movement and foraging behaviour based on perceived risk of predation. We examined the effect of faecal odours from marsupial and eutherian predators, and a native reptilian predator, on the behaviour of three endemic Australian rodent species (the fawn-footed melomys, Melomys cervinipes, the bush rat, Rattus fuscipes, and the giant white-tailed rat, Uromys caudimaculatus) in rainforest remnants on the Atherton Tableland, North Queensland, Australia. Infrared camera traps were used to assess visit rates of rodents to odour stations containing faecal and control odours. Rodents avoided odour stations containing predator faeces, but did not avoid herbivore or control odours. The responses of the three prey species differed: in the late wet season U. caudimaculatus avoided predator odours, whereas R. fuscipes and M. cervinipes did not. In contrast, in the late dry season all three species avoided odour stations containing predator odours. We speculate that these different responses may result from variation in life history traits between the species. (c) 2006 The Association for the Study of Animal Behaviour Published by Elsevier Ltd. All rights reserved.