446 research outputs found

    An Examination of Frequent Emergency Department Use and Emergency Department Reliance among OIF/OEF Veterans

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    Frequent emergency department (ED) use has been studied for decades but frequent ED user subgroups have not been adequately studied, classified, and validated by the research community so designing clear, focused policies have remained problematic. This study used a cross-sectional design, using secondary data obtained from national Veteran Health Administration’s (VHA) administrative databases for fiscal years 2010- 2011 in order to inform and enhance the VHA’s understanding about frequent ED users among the Operation Iraqi Freedom (OIF) and Operation Enduring Freedom (OEF) veteran group through the classification of distinct subgroups within the frequent ED user group including examining factors that explain variation in ED utilization among OIF/OEF veterans, address whether using Department of Veterans Affairs (VA) secondary data sources can classify distinct subgroups within a frequent ED user population, and determine if prior fiscal year ED utilization and associated factors can be used to predict future ED utilization. Using counts of ED visits as the dependent variable, results indicated that 5.2% of all ED OEF/OIF veteran users could be considered frequent ED users which is in alignment with previous studies. The adapted model of Andersen’s Behavioral Model of Health Services Use was adept at selecting predisposing, enabling, and need variables for our predictive models with a Zero-inflated Negative Binomial (ZINB) regression model. Results showed that veterans over 30 years of age within the OEF/OIF cohort had significant decreased odds of having another ED visit compared to the younger under 30 group. Compared to Whites, Blacks or African Americans were the only race group found to be significantly more likely to have increased numbers of ED visits. However, the final ZINB predictive regression model was unable to accurately predict future year utilization using only one prior year’s utilization and associated factors. Three distinct subgroups within ED users were identified, classified and characterized in this study: The Low ED-use/Low EDR subgroup constituted the majority of the sample, Based on primary care use, this subgroup has a primary care physician but never use the ED except in rare circumstances when they find themselves in the ED due to a traumatic event such as a broken bone, car accident or other type of true emergency; The Low EDuse/High EDR subgroup, which consisted of veterans who based on primary care use also have a primary care physician who helps them manage a chronic illness such as Asthma or Diabetes but had an incident where their chronic illness gets out of control after business hours and requires a trip to the ED for care. The High ED-use/High EDR subgroup consisted of those veterans who based on primary care use may or may not have a primary care physician and appear to use the ED as a source of usual care or as a method to access the VA system in order to obtain pain medications, care for their physical needs, or counseling for mental health needs since all of these services are in high demand within the VA system and often difficult to gain access to these services in a timely manner

    Resolving the inner jet structure of 1924-292 with the EVENT HORIZON TELESCOPE

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    We present the first 1.3 mm (230 GHz) very long baseline interferometry model image of an AGN jet using closure phase techniques with a four-element array. The model image of the quasar 1924-292 was obtained with four telescopes at three observatories: the James Clerk Maxwell Telescope (JCMT) on Mauna Kea in Hawaii, the Arizona Radio Observatory's Submillimeter Telescope (SMT) in Arizona, and two telescopes of the Combined Array for Research in Millimeterwave Astronomy (CARMA) in California in April 2009. With the greatly improved resolution compared with previous observations and robust closure phase measurement, the inner jet structure of 1924-292 was spatially resolved. The inner jet extends to the northwest along a position angle of 53-53^\circ at a distance of 0.38\,mas from the tentatively identified core, in agreement with the inner jet structure inferred from lower frequencies, and making a position angle difference of 80\sim 80^{\circ} with respect to the cm-jet. The size of the compact core is 0.15\,pc with a brightness temperature of 1.2×10111.2\times10^{11}\,K. Compared with those measured at lower frequencies, the low brightness temperature may argue in favor of the decelerating jet model or particle-cascade models. The successful measurement of closure phase paves the way for imaging and time resolving Sgr A* and nearby AGN with the Event Horizon Telescope.Comment: 6 pages, 4 figures, accepted for publication in ApJ

    Detection of intrinsic source structure at ~3 Schwarzschild radii with Millimeter-VLBI observations of SAGITTARIUS A*

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    We report results from very long baseline interferometric (VLBI) observations of the supermassive black hole in the Galactic center, Sgr A*, at 1.3 mm (230 GHz). The observations were performed in 2013 March using six VLBI stations in Hawaii, California, Arizona, and Chile. Compared to earlier observations, the addition of the APEX telescope in Chile almost doubles the longest baseline length in the array, provides additional {\it uv} coverage in the N-S direction, and leads to a spatial resolution of \sim30 μ\muas (\sim3 Schwarzschild radii) for Sgr A*. The source is detected even at the longest baselines with visibility amplitudes of \sim4-13% of the total flux density. We argue that such flux densities cannot result from interstellar refractive scattering alone, but indicate the presence of compact intrinsic source structure on scales of \sim3 Schwarzschild radii. The measured nonzero closure phases rule out point-symmetric emission. We discuss our results in the context of simple geometric models that capture the basic characteristics and brightness distributions of disk- and jet-dominated models and show that both can reproduce the observed data. Common to these models are the brightness asymmetry, the orientation, and characteristic sizes, which are comparable to the expected size of the black hole shadow. Future 1.3 mm VLBI observations with an expanded array and better sensitivity will allow a more detailed imaging of the horizon-scale structure and bear the potential for a deep insight into the physical processes at the black hole boundary.Comment: 11 pages, 5 figures, accepted to Ap

    Reinventing grounded theory: some questions about theory, ground and discovery

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    Grounded theory’s popularity persists after three decades of broad-ranging critique. In this article three problematic notions are discussed—‘theory,’ ‘ground’ and ‘discovery’—which linger in the continuing use and development of grounded theory procedures. It is argued that far from providing the epistemic security promised by grounded theory, these notions—embodied in continuing reinventions of grounded theory—constrain and distort qualitative inquiry, and that what is contrived is not in fact theory in any meaningful sense, that ‘ground’ is a misnomer when talking about interpretation and that what ultimately materializes following grounded theory procedures is less like discovery and more akin to invention. The procedures admittedly provide signposts for qualitative inquirers, but educational researchers should be wary, for the significance of interpretation, narrative and reflection can be undermined in the procedures of grounded theory
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