Abstract. We introduce a new survey of massive stars in the Galaxy and the Magellanic Clouds using the Fibre Large Array Multi-Element Spectrograph (FLAMES) instrument at the Very Large Telescope (VLT). Here we present observations of 269 Galactic stars with the FLAMES-Giraffe Spectrograph (R 25 000), in fields centered on the open clusters NGC 3293, NGC 4755 and NGC 6611. These data are supplemented by a further 50 targets observed with the Fibre-Fed Extended Range Optical Spectrograph (FEROS, R = 48 000). Following a description of our scientific motivations and target selection criteria, the data reduction methods are described; of critical importance the FLAMES reduction pipeline is found to yield spectra that are in excellent agreement with less automated methods. Spectral classifications and radial velocity measurements are presented for each star, with particular attention paid to morphological peculiarities and evidence of binarity. These observations represent a significant increase in the known spectral content of NGC 3293 and NGC 4755, and will serve as standards against which our subsequent FLAMES observations in the Magellanic Clouds will be compared.
Abstract-Recent developments have shown the possibility of leveraging silicon nanophotonic technologies for chip-scale interconnection fabrics that deliver high bandwidth and power efficient communications both on-and off-chip. Since optical devices are fundamentally different from conventional electronic interconnect technologies, new design methodologies and tools are required to exploit the potential performance benefits in a manner that accurately incorporates the physically different behavior of photonics. We introduce PhoenixSim, a simulation environment for modeling computer systems that incorporates silicon nanophotonic devices as interconnection building blocks. PhoenixSim has been developed as a cross-discipline platform for studying photonic interconnects at both the physicallayer level and at the architectural and system levels. The broad scope at which modeled systems can be analyzed with PhoenixSim provides users with detailed information into the physical feasibility of the implementation, as well as the network and system performance. Here, we describe details about the implementation and methodology of the simulator, and present two case studies of silicon nanophotonic-based networks-on-chip.
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