A new perspective on design thinking and design practice: beyond products and projects, toward participatory design things. Design Things offers an innovative view of design thinking and design practice, envisioning ways to combine creative design with a participatory approach encompassing aesthetic and democratic practices and values. The authors of Design Things look at design practice as a mode of inquiry that involves people, space, artifacts, materials, and aesthetic experience, following the process of transformation from a design concept to a thing. Design Things, which grew out of the Atelier (Architecture and Technology for Inspirational Living) research project, goes beyond the making of a single object to view design projects as sociomaterial assemblies of humans and artifacts—“design things.” The book offers both theoretical and practical perspectives, providing empirical support for the authors' conceptual framework with field projects, case studies, and examples from professional practice. The authors examine the dynamics of the design process; the multiple transformations of the object of design; metamorphing, performing, and taking place as design strategies; the concept of the design space as “emerging landscapes”; the relation between design and use; and the design of controversial things.

Aims.In this paper we demonstrate how Strömgren uvby photometry can be efficiently used to: 1. identify red giant branch stars that are members in a dwarf spheroidal galaxy; 2. derive age-independent metallicities for the same stars and quantify the associated errors. Methods. Strömgren uvby photometry in a 11 × 22 arcmin field centered on the Draco dwarf spheroidal galaxy was obtained using the Isaac Newton Telescope on La Palma. Members of the Draco dSph galaxy were identified using the surface gravity sensitive c 1 index which discriminates between red giant and dwarf stars. Thus enabling us to distinguish the (red giant branch) members of the dwarf spheroidal galaxy from the foreground dwarf stars in our galaxy. The method is evaluated through a comparison of our membership list with membership classifications in the literature based on radial velocities and proper motions. The metallicity sensitive m 1 index was used to derive individual and age-independent metallicities for the members of the Draco dSph galaxy. The derived metallicities are compared to studies based on high resolution spectroscopy and the agreement is found to be very good. Results. We present metallicities for 169 members of the red giant branch in the Draco dwarf spheroidal galaxy (the largest sample to date). The metallicity distribution function for the Draco dSph galaxy shows a mean [Fe/H] = -1.74 dex with a spread of 0.24 dex. The correlation between metallicity and colour for the stars on the red giant branch is consistent with a dominant old, and coeval population. There is a possible spatial population gradient over the field with the most metal-rich stars being more centrally concentrated than the metal-poor stars.

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