58 research outputs found

    Disparities in Access to Healthcare: The Case of a Drug and Alcohol Abuse Detoxification Treatment Program among Minority Groups in a Texas Hospital

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    The authors analyzed ethnic/racial disparities in healthcare access and length of stay from a defined population of individuals seeking medical detoxification services at a hospital in Texas. Results indicated Blacks were more likely to be insured compared with Whites, mostly by public insurance, but this did not hold for Hispanics, who were about three times more likely to be uninsured compared with Blacks. In addition, the authors observed lower median of length of stay in the Medicaid category among Hispanics. These results can be explained by aggressive case management, sociocultural barriers, or discriminatory practices, both intentional and unintentional

    Latino Access to Health Care: The Role of Insurance, Managed Care, and Institutional Barriers

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    The health care system in the United States is the most expensive and yet arguably among the least cost effective in the developed world (Anderson, 1998). Despite the highest per person health care spending among the Organization for Economic Cooperation and Development (OECD) nations, the United States still ranks below many along a variety of health indicators (Woolhandler & Himmelstein, 1991). In a complicated health care system where the rules are many and economic forces drive both structure and function, the needs of vulnerable populations inevitably suffer. This chapter explores the consequences of these market forces on a vulnerable population--Latinos in the United States. First, the health insurance status of Latinos is reviewed in the context of employment trends and participation in various government-sponsored programs. Next, the chapter explores the impact of managed care on Latinos, as well as that of other institutional, organizational, and structural barriers that stand between this population and full access to health care

    Mapping Drug Physico-Chemical Features to Pathway Activity Reveals Molecular Networks Linked to Toxicity Outcome

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    The identification of predictive biomarkers is at the core of modern toxicology. So far, a number of approaches have been proposed. These rely on statistical inference of toxicity response from either compound features (i.e., QSAR), in vitro cell based assays or molecular profiling of target tissues (i.e., expression profiling). Although these approaches have already shown the potential of predictive toxicology, we still do not have a systematic approach to model the interaction between chemical features, molecular networks and toxicity outcome. Here, we describe a computational strategy designed to address this important need. Its application to a model of renal tubular degeneration has revealed a link between physico-chemical features and signalling components controlling cell communication pathways, which in turn are differentially modulated in response to toxic chemicals. Overall, our findings are consistent with the existence of a general toxicity mechanism operating in synergy with more specific single-target based mode of actions (MOAs) and provide a general framework for the development of an integrative approach to predictive toxicology

    Finishing the euchromatic sequence of the human genome

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    The sequence of the human genome encodes the genetic instructions for human physiology, as well as rich information about human evolution. In 2001, the International Human Genome Sequencing Consortium reported a draft sequence of the euchromatic portion of the human genome. Since then, the international collaboration has worked to convert this draft into a genome sequence with high accuracy and nearly complete coverage. Here, we report the result of this finishing process. The current genome sequence (Build 35) contains 2.85 billion nucleotides interrupted by only 341 gaps. It covers ∼99% of the euchromatic genome and is accurate to an error rate of ∼1 event per 100,000 bases. Many of the remaining euchromatic gaps are associated with segmental duplications and will require focused work with new methods. The near-complete sequence, the first for a vertebrate, greatly improves the precision of biological analyses of the human genome including studies of gene number, birth and death. Notably, the human enome seems to encode only 20,000-25,000 protein-coding genes. The genome sequence reported here should serve as a firm foundation for biomedical research in the decades ahead

    Gas phase Elemental abundances in Molecular cloudS (GEMS) I : The prototypical dark cloud TMC 1

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    GEMS is an IRAM 30 m Large Program whose aim is determining the elemental depletions and the ionization fraction in a set of prototypical star-forming regions. This paper presents the first results from the prototypical dark cloud Taurus molecular cloud (TMC) 1. Extensive millimeter observations have been carried out with the IRAM 30 m telescope (3 and 2mm) and the 40 m Yebes telescope (1.3 cm and 7 mm) to determine the fractional abundances of CO, HCO+, HCN, CS, SO, HCS+, and N2H+ in three cuts which intersect the dense filament at the well-known positions TMC 1-CP, TMC 1-NH3, and TMC 1-C, covering a visual extinction range from A(v) similar to 3 to similar to 20 mag. Two phases with differentiated chemistry can be distinguished: (i) the translucent envelope with molecular hydrogen densities of 1-5 x 10(3) cm(-3); and (ii) the dense phase, located at A(v) > 10 mag, with molecular hydrogen densities >10(4) cm(-3). Observations and modeling show that the gas phase abundances of C and O progressively decrease along the C+/C/CO transition zone (A(v) similar to 3 mag) where C/H similar to 8 x 10(-5) and C/O similar to 0.8-1, until the beginning of the dense phase at A(v) similar to 10 mag. This is consistent with the grain temperatures being below the CO evaporation temperature in this region. In the case of sulfur, a strong depletion should occur before the translucent phase where we estimate an S/H similar to (0.4-2.2) x 10(-6), an abundance similar to 7-40 times lower than the solar value. A second strong depletion must be present during the formation of the thick icy mantles to achieve the values of S/H measured in the dense cold cores (S/H similar to 8 x 10(-8)). Based on our chemical modeling, we constrain the value of zeta(H2) to similar to(0.5-1.8) x 10(-16) s(-1) in the translucent cloud.Peer reviewe
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