2,549 research outputs found

    Twelve Tips for Using Co-creation for Value Creation and Professional Development

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    A growing body of research advocates the positive benefits of using co-creation projects to add value to existing services and practices and to enhance professional development. We present a practical guide to adopting the democratic principles of co-creation and structuring a project effectively. From identifying the initial focus, we provide advice concerning how to create a Mission Statement, identify objectives, and develop a cohesive learning community. We also outline how using measurable outcomes and an agreed timescale, it is possible to co-create activities that are both democratic and inclusive. Whilst co-creation can take place in face-to-face or virtual settings, we suggest ways that engaging with technology will enhance the creative elements, and how reflective practice underpins the career developments taking place. Finally, we explore the value associated with evaluating the project, and identifying avenues for the dissemination of its achievements

    Projections onto translation—Invariant subspaces of L1(G)

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    AbstractLet G be a locally compact abelian group. A translation-invariant subspace in L1(G) may or may not be complemented depending on the structure of its hull in Ĝ. Techniques for deciding this complementation problem in a variety of situations are developed and illustrated with examples. A complete characterization is obtained for those ideals with a discrete hull

    Exploring the Structure of Distant Galaxies with Adaptive Optics on the Keck-II Telescope

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    We report on the first observation of cosmologically distant field galaxies with an high order Adaptive Optics (AO) system on an 8-10 meter class telescope. Two galaxies were observed at 1.6 microns at an angular resolution as high as 50 milliarcsec using the AO system on the Keck-II telescope. Radial profiles of both objects are consistent with those of local spiral galaxies and are decomposed into a classic exponential disk and a central bulge. A star-forming cluster or companion galaxy as well as a compact core are detected in one of the galaxies at a redshift of 0.37+/-0.05. We discuss possible explanations for the core including a small bulge, a nuclear starburst, or an active nucleus. The same galaxy shows a peak disk surface brightness that is brighter than local disks of comparable size. These observations demonstrate the power of AO to reveal details of the morphology of distant faint galaxies and to explore galaxy evolution.Comment: 5 pages, Latex, 3 figures. Accepted for publication in P.A.S.

    Protein folding rates correlate with heterogeneity of folding mechanism

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    By observing trends in the folding kinetics of experimental 2-state proteins at their transition midpoints, and by observing trends in the barrier heights of numerous simulations of coarse grained, C-alpha model, Go proteins, we show that folding rates correlate with the degree of heterogeneity in the formation of native contacts. Statistically significant correlations are observed between folding rates and measures of heterogeneity inherent in the native topology, as well as between rates and the variance in the distribution of either experimentally measured or simulated phi-values.Comment: 11 pages, 3 figures, 1 tabl

    Using Co-creation as a Pedagogic Method for the Professional Development of Students undertaking a BA (Hons) in Education Studies

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    Using an interpretive epistemology to explore the perceived benefits of using co-creation as a pedagogic tool with undergraduate students, this research focuses on a collaborative project between some first year undergraduate Education Studies students, a university Senior Lecturer, and an Education Coordinator from a regional social enterprise organisation. The paper is timely given the introduction of the Teaching Excellence Framework, and explores how the use of co-creation and creativity enhances the professional development and employability of Graduates. Drawing on data collected from the students, this paper presents a range of perspectives and identifies how ‘meaningful’ problem-solving, co-creation, and collaboration lead to transformative learning and enhanced student engagement. By doing this, we explore how complex challenges create agency for learning and develop critical thinkin

    Characterising native plant resins from Australian Aboriginal artefacts using ATR-FTIR and GC/MS

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    Resin use by Australian Aborigines has been documented in ethnographic accounts across the continent and is also evident from archaeological and anthropological artefacts. This research assesses the use of attenuated total reflectance Fourier transform infrared spectroscopy (ATR-FTIR) and gas chromatography coupled mass spectrometry (GC/MS) for the identification of native plant resins on museum artefacts. A collection of thirteen museum artefacts were analysed using light microscopy and characterised using both ATR-FTIR and GC/MS. The resins were identified to the plant genus and one to the species level, as spinifex (. Triodia spp. R.Br.), ironwood (. Erythrophleum chlorostachys (F. Muell.) Baill.) and grass tree (. Xanthorrhoea spp. Sm.) by comparison to a reference collection of modern exudates from 34 Australian plant species. The two analytical methods used, produced a significant agreement in results but one has practical advantages. On eight of the artefacts, ATR-FTIR was able to be performed on the residue in situ, without removal, presenting a non-destructive analytical method for the identification of resins which is applicable to rare and delicate artefacts from museum collections. Permission to remove the residue off the artefact is not always granted or feasible, so ATR-FTIR has a significant advantage over GC/MS and other methods which require chemical treatment or even destruction of the archaeological sample. Both of the methods examined are demonstrated to accurately infer the botanical origin of archaeological and anthropological resins, providing insight on the use, preparation and trading of resins, with the consequent contribution to an understanding of the development and use of hafted tools and other aspects of cultural development

    PHotometry Assisted Spectral Extraction (PHASE) and identification of SNLS supernovae

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    Aim: We present new extraction and identification techniques for supernova (SN) spectra developed within the Supernova Legacy Survey (SNLS) collaboration. Method: The new spectral extraction method takes full advantage of photometric information from the Canada-France-Hawai telescope (CFHT) discovery and reference images by tracing the exact position of the supernova and the host signals on the spectrogram. When present, the host spatial profile is measured on deep multi-band reference images and is used to model the host contribution to the full (supernova + host) signal. The supernova is modelled as a Gaussian function of width equal to the seeing. A chi-square minimisation provides the flux of each component in each pixel of the 2D spectrogram. For a host-supernova separation greater than <~ 1 pixel, the two components are recovered separately and we do not use a spectral template in contrast to more standard analyses. This new procedure permits a clean extraction of the supernova separately from the host in about 70% of the 3rd year ESO/VLT spectra of the SNLS. A new supernova identification method is also proposed. It uses the SALT2 spectrophotometric template to combine the photometric and spectral data. A galaxy template is allowed for spectra for which a separate extraction of the supernova and the host was not possible. Result: These new techniques have been tested against more standard extraction and identification procedures. They permit a secure type and redshift determination in about 80% of cases. The present paper illustrates their performances on a few sample spectra.Comment: 27 pages, 18 Figures, 1 Table. Accepted for publication in A&
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