4,268 research outputs found

    Enhancing drug safety through active surveillance of observational healthcare data

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    Drug safety continues to be a major public health concern in the United States, with adverse drug reactions ranking as the 4th to 6th leading cause of death, and resulting in health care costs of $3.6 billion annually. Recent media attention and public scrutiny of high-profile drug safety issues have increased visibility and skepticism of the effectiveness of the current post-approval safety surveillance processes. Current proposals suggest establishing a national active drug safety surveillance system that leverages observational data, including administrative claims and electronic health records, to monitor and evaluate potential safety issues of medicines. However, the development and evaluation of appropriate strategies for systematic analysis of observational data have not yet been studied. This study introduces a novel exploratory analysis approach (Comparator-Adjusted Safety Surveillance or COMPASS) to identify drug-related adverse events in automated healthcare data. The aims of the study were: 1) to characterize the performance of COMPASS in identifying known safety issues associated with ACE inhibitor exposure within an administrative claims database; 2) to evaluate consistency of COMPASS estimates across a network of disparate databases; and 3) to explore differential effects across ingredients within ACE inhibitor class. COMPASS was observed to have improved accuracy to three other methods under consideration for an active surveillance system: observational screening, disproportionality analysis, and self-controlled case series. COMPASS performance was consistently strong within 5 different databases, though important differences in outcome estimates across the sources highlighted the substantial heterogeneity which makes pooling estimates challenging. The comparative safety analysis of products within the ACE inhibitor class provided evidence of similar risk profiles across an array of different outcomes, and raised questions about the product labeling differences and how observational studies should complement existing evidence as part of a broader safety assessment strategy. The results of this study should inform decisions about the appropriateness and utility of analyzing observational data as part of an active drug safety surveillance process. An improved surveillance system would enable a more comprehensive and timelier understanding of the safety of medicines. Such information supports patients and providers in therapeutic decision-making to minimize risks and improve the quality of care

    Self-referenced continuous-variable quantum key distribution protocol

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    We introduce a new continuous-variable quantum key distribution (CV-QKD) protocol, self-referenced CV-QKD, that eliminates the need for transmission of a high-power local oscillator between the communicating parties. In this protocol, each signal pulse is accompanied by a reference pulse (or a pair of twin reference pulses), used to align Alice's and Bob's measurement bases. The method of phase estimation and compensation based on the reference pulse measurement can be viewed as a quantum analog of intradyne detection used in classical coherent communication, which extracts the phase information from the modulated signal. We present a proof-of-principle, fiber-based experimental demonstration of the protocol and quantify the expected secret key rates by expressing them in terms of experimental parameters. Our analysis of the secret key rate fully takes into account the inherent uncertainty associated with the quantum nature of the reference pulse(s) and quantifies the limit at which the theoretical key rate approaches that of the respective conventional protocol that requires local oscillator transmission. The self-referenced protocol greatly simplifies the hardware required for CV-QKD, especially for potential integrated photonics implementations of transmitters and receivers, with minimum sacrifice of performance. As such, it provides a pathway towards scalable integrated CV-QKD transceivers, a vital step towards large-scale QKD networks.Comment: 14 pages, 10 figures. Published versio

    Critical function of endogenous XIAP in regulating caspase activation during sympathetic neuronal apoptosis

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    In sympathetic neurons, unlike most nonneuronal cells, growth factor withdrawal–induced apoptosis requires the development of competence in addition to cytochrome c release to activate caspases. Thus, although most nonneuronal cells die rapidly with cytosolic cytochrome c alone, sympathetic neurons are remarkably resistant unless they develop competence. We have identified endogenous X-linked inhibitor of apoptosis protein (XIAP) as the essential postcytochrome c regulator of caspase activation in these neurons. In contrast to wild-type neurons that are resistant to injection of cytochrome c, XIAP-deficient neurons died rapidly with cytosolic cytochrome c alone. Surprisingly, the release of endogenous Smac was not sufficient to overcome the XIAP resistance in sympathetic neurons. In contrast, the neuronal competence pathway permitted cytochrome c to activate caspases by inducing a marked reduction in XIAP levels in these neurons. Thus, the removal of XIAP inhibition appears both necessary and sufficient for cytochrome c to activate caspases in sympathetic neurons. These data identify a critical function of endogenous XIAP in regulating apoptosis in mammalian cells

    Stormwater Runoff Reduction on the Worcester Polytechnic Institute Campus

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    Stormwater from Worcester Polytechnic Institute (WPI) drains directly into nearby Salisbury Pond, contributing to its chronic pollution. For our project, we worked with WPI Facilities to develop a plan to more effectively manage stormwater runoff in one area of campus. We assessed WPIs current stormwater management practices, investigated existing solutions, and detailed which solution was most feasible for WPI. We found that a combined stone swale and rain garden would best serve our campus needs by reducing or eliminating frequent flooding in the center of campus and simultaneously reducing the quantity of stormwater entering Salisbury Pond through storm sewers. In collaboration with WPIs Office of Sustainability, we submitted our proposal to the US EPAs RainWorks Challenge

    HST Grism Observations of a Gravitationally Lensed Redshift 10 Galaxy

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    We present deep spectroscopic observations of a Lyman-break galaxy candidate (hereafter MACS1149-JD) at z9.5z\sim9.5 with the Hubble\textit{Hubble} Space Telescope (HST\textit{HST}) WFC3/IR grisms. The grism observations were taken at 4 distinct position angles, totaling 34 orbits with the G141 grism, although only 19 of the orbits are relatively uncontaminated along the trace of MACS1149-JD. We fit a 3-parameter (zz, F160W mag, and Lyα\alpha equivalent width) Lyman-break galaxy template to the three least contaminated grism position angles using an MCMC approach. The grism data alone are best fit with a redshift of zgrism=9.530.60+0.39z_{\mathrm{grism}}=9.53^{+0.39}_{-0.60} (68%68\% confidence), in good agreement with our photometric estimate of zphot=9.510.12+0.06z_{\mathrm{phot}}=9.51^{+0.06}_{-0.12} (68%68\% confidence). Our analysis rules out Lyman-alpha emission from MACS1149-JD above a 3σ3\sigma equivalent width of 21 \AA{}, consistent with a highly neutral IGM. We explore a scenario where the red Spitzer\textit{Spitzer}/IRAC [3.6][4.5][3.6] - [4.5] color of the galaxy previously pointed out in the literature is due to strong rest-frame optical emission lines from a very young stellar population rather than a 4000 \AA{} break. We find that while this can provide an explanation for the observed IRAC color, it requires a lower redshift (z9.1z\lesssim9.1), which is less preferred by the HST\textit{HST} imaging data. The grism data are consistent with both scenarios, indicating that the red IRAC color can still be explained by a 4000 \AA{} break, characteristic of a relatively evolved stellar population. In this interpretation, the photometry indicate that a 34035+29340^{+29}_{-35} Myr stellar population is already present in this galaxy only 500 Myr\sim500~\mathrm{Myr} after the Big Bang.Comment: Accepted to ApJ. This is the accepted versio
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