298 research outputs found

    Communication Network Design: Balancing Modularity and Mixing via Optimal Graph Spectra

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    By leveraging information technologies, organizations now have the ability to design their communication networks and crowdsourcing platforms to pursue various performance goals, but existing research on network design does not account for the specific features of social networks, such as the notion of teams. We fill this gap by demonstrating how desirable aspects of organizational structure can be mapped parsimoniously onto the spectrum of the graph Laplacian allowing the specification of structural objectives and build on recent advances in non-convex programming to optimize them. This design framework is general, but we focus here on the problem of creating graphs that balance high modularity and low mixing time, and show how "liaisons" rather than brokers maximize this objective

    RCS2 J232727.6-020437: An Efficient Cosmic Telescope at z=0.6986z=0.6986

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    We present a detailed gravitational lens model of the galaxy cluster RCS2 J232727.6-020437. Due to cosmological dimming of cluster members and ICL, its high redshift (z=0.6986z=0.6986) makes it ideal for studying background galaxies. Using new ACS and WFC3/IR HST data, we identify 16 multiple images. From MOSFIRE follow up, we identify a strong emission line in the spectrum of one multiple image, likely confirming the redshift of that system to z=2.083z=2.083. With a highly magnified (μ2\mu\gtrsim2) source plane area of 0.7\sim0.7 arcmin2^2 at z=7z=7, RCS2 J232727.6-020437 has a lensing efficiency comparable to the Hubble Frontier Fields clusters. We discover four highly magnified z7z\sim7 candidate Lyman-break galaxies behind the cluster, one of which may be multiply-imaged. Correcting for magnification, we find that all four galaxies are fainter than 0.5L0.5 L_{\star}. One candidate is detected at >10σ{>10\sigma} in both Spitzer/IRAC [3.6] and [4.5] channels. A spectroscopic follow-up with MOSFIRE does not result in the detection of the Lyman-alpha emission line from any of the four candidates. From the MOSFIRE spectra we place median upper limits on the Lyman-alpha flux of 514×1019ergs1cm25-14 \times 10^{-19}\, \mathrm{erg \,\, s^{-1} cm^{-2}} (5σ5\sigma).Comment: 14 pages, 9 figures, submitted to ApJ on 3/06/201
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