8,037 research outputs found

    Medicaid's Role in the Health Benefits Exchange: A Road Map for States

    Get PDF
    Examines issues for integrating Medicaid into the administration, operation, and coverage continuum of insurance exchanges. Discusses eligibility, enrollment, and outreach; contracting, standards, and requirements; benefits design; and infrastructure

    Steerable filters generated with the hypercomplex dual-tree wavelet transform

    Get PDF
    The use of wavelets in the image processing domain is still in its infancy, and largely associated with image compression. With the advent of the dual-tree hypercomplex wavelet transform (DHWT) and its improved shift invariance and directional selectivity, applications in other areas of image processing are more conceivable. This paper discusses the problems and solutions in developing the DHWT and its inverse. It also offers a practical implementation of the algorithms involved. The aim of this work is to apply the DHWT in machine vision. Tentative work on a possible new way of feature extraction is presented. The paper shows that 2-D hypercomplex basis wavelets can be used to generate steerable filters which allow rotation as well as translation.</p

    Evidence for a non-universal stellar initial mass function in low-redshift high-density early-type galaxies

    Full text link
    We determine an absolute calibration of stellar mass-to-light ratios for the densest \simeq 3% of early-type galaxies in the local universe (redshift z\simeq 0.08) from SDSS DR7. This sample of \sim 4000 galaxies has, assuming a Chabrier IMF, effective stellar surface densities, Sigma_e > 2500 M_sun/pc^2, stellar population synthesis (SPS) stellar masses log_10(M_sps/M_sun)<10.8, and aperture velocity dispersions of sigma_ap=168^{+37}_{-34} km/s (68% range). In contrast to typical early-type galaxies, we show that these dense early-type galaxies follow the virial fundamental plane, which suggests that mass-follows-light. With the additional assumption that any dark matter does not follow the light, the dynamical masses of dense galaxies provide a direct measurement of stellar masses. Our dynamical masses (M_dyn), obtained from the spherical Jeans equations, are only weakly sensitive to the choice of anisotropy (\beta) due to the relatively large aperture of the SDSS fiber for these galaxies: R_ap \simeq 1.5 R_e. Assuming isotropic orbits (\beta=0) we find a median log_{10} (M_dyn/M_sps) = 0.233 \pm 0.003, consistent with a Salpeter IMF, while more bottom heavy IMFs and standard Milky-Way IMFs are strongly disfavored. Our results are consistent with, but do not require, a dependence of the IMF on dynamical mass or velocity dispersion. We find evidence for a color dependence to the IMF such that redder galaxies have heavier IMFs with M_dyn/M_sps \propto (g-r)^{1.13\pm0.09}. This may reflect a more fundamental dependence of the IMF on the age or metallicity of a stellar population, or the density at which the stars formed.Comment: 5 pages, 6 figures, accepted to MNRAS Letters, minor changes to previous versio

    The use of satellite data in understanding and predicting convective and large-scale dynamical processes

    Get PDF
    Mesoscale convective processes and how they affect and interact with mid-latitude cyclones were studied. The ageostrophic and associated vertical motion field was calculated using a highly accurate iterative method of solving the semigeostrophic omega equation. The tendencies for convective destabilization in the 850-750 mb layer due to differential geostrophic and ageostrophic advection and differential moist adiabatic ascent, were found. The spectral models of the index oscillation, one barotropic and the other baroclinic, were developed. Theoretical and observational studies of cloud streets were conducted

    Collisions of solitons and vortex rings in cylindrical Bose-Einstein condensates

    Full text link
    Interactions of solitary waves in a cylindrically confined Bose-Einstein condensate are investigated by simulating their head-on collisions. Slow vortex rings and fast solitons are found to collide elastically contrary to the situation in the three-dimensional homogeneous Bose gas. Strongly inelastic collisions are absent for low density condensates but occur at higher densities for intermediate velocities. The scattering behaviour is rationalised by use of dispersion diagrams. During inelastic collisions, spherical shell-like structures of low density are formed and they eventually decay into depletion droplets with solitary wave features. The relation to similar shells observed in a recent experiment [Ginsberg et al. Phys Rev. Lett. 94, 040403 (2005)] is discussed

    HHS Proposed Rules on Exchange Implementation Requirements

    Get PDF
    Highlights provisions of the new regulations and commentary on state health insurance exchanges that clarify or amplify the 2010 healthcare reform or offer insight into federal guidance or consensus on their establishment, functions, and other issues

    The Role of the Basic Health Program in the Coverage Continuum: Opportunities, Risks and Considerations for States

    Get PDF
    Outlines issues for offering subsidized coverage to those eligible for insurance exchange subsidies by using federal dollars that would otherwise go to those subsidies, including continuity of coverage, impact on exchanges, and financial feasibility
    • …
    corecore