Titlebook: Innovations in Multi-Agent Systems and Application – 1; Dipti Srinivasan,Lakhmi C. Jain Book 2010 Springer-Verlag Berlin Heidelberg 2010 a

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fferent scenes. The method described in this chapter was designed for non-parametric, “example-based” depth estimation of objects appearing in single photos. It consults a database of example 3D geometries and associated appearances, searching for those which look similar to the object in the photo.

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P. G. Balaji,D. Srinivasanarning by doing" approach.Written in a style suitable as eitThe purpose and motivation of these lectures can be summarized in the following two questions: • What is the ground state (and its properties) of dense matter? • What is the matter composition of a compact star? The two questions are, of co

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Howard Li,Fakhri Karray,Otman Basirars. There is also convincing evidence for relations between the properties of supermassive black holes in the nuclei of galaxies and those of their host galaxies. It is much less clear, however, how stellar starburstt) and non-stellar (AGN) activity in the nuclear regions can be initiated and fuell

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Toshiyuki Sueyoshir resolution and high sensitivity carried out with the IRAM Plateau de Bure interferometer (PdBI). The observations cover galaxies in a redshift range of ∼0.03–1.4. We have so far observed five different active galaxies: NGC3718, NGC1068, HE1029-1831, 3C48 and Q0957 + 561. The first two objects belo

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