180 viviendas de protección oficial en La Bolueta en Bilbao

Projecte presentat a 108 viviendas de protección oficial, 63 viviendas sociales y 190 viviendas tasadas, anejos y urbanización vinculada, en las parcelas RE-1-A-1, RE-1-A-2 Y RE-1-B, del PERI AR-421 de BOLUETA en BILBAO

Habitatges en Lloguer

Projecte presentat al concurs d'un edifici plurifamiliar d’habitatges de lloguer amb protecció oficial

Remodelació del Nou Camp del F.C. Barcelona

Proposta presentada per al Concurs de Remodelació del Nou Camp del Futbol Club Barcelona.

Sant Boi 2012

Projecte presentat per al Concurs de projectes amb intervenció de jurat per al desenvolupament a nivell d'avanprojecte del Pla de Millora Urbana del Sector FECSA-ENDESA i Casernes, a Sant Boi del Llobregat

Improving energy access in rural sub-Saharan Africa

XVII Convocatòria d’ajuts a accions de cooperació - 2009GRECDH – UPC. Improving Energy Access In Rural sub- Saharan Africa. O-006/09. Informe

High-performance payload data handling system for Gaia

Gaia is the most ambitious space astrometry mission currently envisaged and is a technological challenge in all its aspects. We describe a proposal for the payload data handling system of Gaia, as an example of a high-performance, real-time, concurrent, and pipelined data system. This proposal includes the front-end systems for the instrumentation, the data acquisition and management modules, the star data processing modules, and the payload data handling unit. We also review other payload and service module elements and we illustrate a data flux proposal.

Variable Very-High-Energy Gamma-Ray Emission from the Microquasar LS I +61 303

Microquasars are binary star systems with relativistic radio-emitting jets. They are potential sources of cosmic rays and can be used to elucidate the physics of relativistic jets. We report the detection of variable gamma-ray emission above 100 gigaelectron volts from the microquasar LS I 61 + 303. Six orbital cycles were recorded. Several detections occur at a similar orbital phase, which suggests that the emission is periodic. The strongest gamma-ray emission is not observed when the two stars are closest to one another, implying a strong orbital modulation of the emission or absorption processes.