White paper sobre Open Source, Open Access, open Standards e o futuro da catalogação

The discussions on the future of cataloging has received increased attention in the last ten years, mainly due to the impact of rapid development of information and communication technologies in the same period, which has provided access to the Web anytime, anywhere. These discussions revolve around the need for a new bibliographic framework to meet the demand of this new reality in the digital environment, ie how libraries can process, store, deliver, share and integrate their collections (physical, digital or scanned), in current post-PC era? Faced with this question, Open Access, Open Source and Open Standards are three concepts that need to receive greater attention in the field of Library and Information Science, as it is believed to be fundamental elements for the change of paradigm of descriptive representation, currently based conceptually on physical item rather than intellectual work. This paper aims to raise and discuss such issues and instigate information professionals, especially librarians, to think, discuss and propose initiatives for such problems, contributing and sharing ideas and possible solutions, in multidisciplinary teams. At the end is suggested the effective creation of multidisciplinary and inter-institutional study groups on the future of cataloging and its impact on national collections, in order to contribute to the area of descriptive representation in national and international level

A arquitetura patrimonial através dos jogos digitais

O presente artigo pretende ressaltar o potencial dos jogos digitais como instrumento de assimilação do conhecimento em arquitetura patrimonial, através da pesquisa Patrimônio arquitetônico, design e educação: desenvolvimento de Sistemas Interativos Lúdicos (jogos educativos em meio digital). Nesta pesquisa foram desenvolvidos jogos digitais a partir do levantamento das características arquitetônicas dos edifícios de relevância histórica e cultural da cidade de São Carlos. Através da interação e exploração da interface digital pelo usuário, a apropriação do conhecimento ocorre de uma forma lúdica e criativa. Por meio da manipulação desses jogos, os alunos, cidadãos e visitantes podem aproximar-se da educação patrimonial adquirindo consciência histórica e aprendendo a valorizar as origens da cidade e a arquitetura do município. Ressalta-se a importância das metodologias que permitem viabilizar o desenvolvimento dos jogos eletrônicos (desenho e linguagem de programação) e que se apresentam como importantes ferramentas de representação da arquitetura. Por fim, destaca-se a importância da educação patrimonial para a formação do cidadão e preservação do patrimônio cultural.

Galaxy triplets in Sloan Digital Sky Survey Data Release 7-I. Catalogue

We present a new catalogue of galaxy triplets derived from the Sloan Digital Sky Survey (SDSS) Data Release 7. The identification of systems was performed considering galaxies brighter than Mr=-20.5 and imposing constraints over the projected distances, radial velocity differences of neighbouring galaxies and isolation. To improve the identification of triplets, we employed a data pixelization scheme, which allows us to handle large amounts of data as in the SDSS photometric survey. Using spectroscopic and photometric data in the redshift range 0.01 =z= 0.40, we obtain 5901 triplet candidates. We have used a mock catalogue to analyse the completeness and contamination of our methods. The results show a high level of completeness ( 80 per cent) and low contamination ( 5 per cent). By using photometric and spectroscopic data, we have also addressed the effects of fibre collisions in the spectroscopic sample. We have defined an isolation criterion considering the distance of the triplet brightest galaxy to the closest neighbour cluster, to describe a global environment, as well as the galaxies within a fixed aperture, around the triplet brightest galaxy, to measure the local environment. The final catalogue comprises 1092 isolated triplets of galaxies in the redshift range 0.01 =z= 0.40. Our results show that photometric redshifts provide very useful information, allowing us to complete the sample of nearby systems whose detection is affected by fibre collisions, as well as extending the detection of triplets to large distances, where spectroscopic redshifts are not available.