Advanced Research in VLSI: Proceedings of the 6th MIT by William J. Dally

By William J. Dally

APRIL 2, 1990, CAMBRIDGE, MASSACHUSETTS Theory or perform in VLSI structures: hugely parallel architectures, special-purpose VLSI chips and structures, sensory platforms, checking out, and fault tolerance. Design and Automation: synthesis and silicon compilation, structure and routing, research and simulation, novel layout equipment. Circuits and units: cutting edge electric circuits, technique and equipment modeling, automatic semiconductor production, wafer-scale structures.

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B. ca/cadcbin/wdbi. cgi/astrocat/stetson/query Radial Velocity Measurements Based on FORS2 and FLAMES Spectra M. Monelli1 , M. Nonino2 , G. Bono3 , P. Fran¸cois4 , F. Th´evenin5 , R. Buonanno6 , F. Caputo3 , C. E. Corsi3 , L. Pulone3 , H. A. Smith7 , P. B. Stetson8 , and A. R. es INAF–Osservatorio Astronomico di Trieste, Via Tiepolo 11, 34131 Trieste, Italy INAF–Osservatorio Astronomico di Roma, Via Frascati 33, 00040 Monte Porzio Catone, Rome, Italy GEPI–Observatoire de Paris-Meudon, 92125 Meudon Cedex, France D´ept.

The ability to detect 100% of the incident light is achieved with detectors with quantum efficiency up to 99%. 12 P. Amico et al. 2. g. Megacam at CFHT, Omegacam at ESO). 3. g. 255 kbps) On the other hand, when dealing with performance of modern detectors in detail, the astronomers are confronted with many issues that can significantly affect their science projects. For example, when looking at the signal in a detector, it is important to know the signal gain variation and stability, the QE spatial variations (intrinsic or as a result of external contamination), the effects of flux, bias voltages and temperature on linearity, the conditions under which signal persistence becomes significant, just to name a few.

G. the detector linearity algorithm. Each pipeline will call these functions from the instrument specific recipes, thus providing the flexibility required to cope with instrument-specific features, keywords, or data structures. Acknowledgement. The authors would like to thank Nicolas Haddad, Pedro Mardones, Emanuela Pompei and Martin Roth for the fruitful discussions and comments. James Brewer and Thomas Agustejin for having pioneered the work for a common algorithm for detector monitoring in La Silla.

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