839 research outputs found

    Near-Infrared Band Strengths of Molecules Diluted in N2 and H20 Ice Mixtures Relevant to Interstellar and Planetary Ices

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    In order to determine the column density of a component of an ice from its infrared absorption features, the strengths of these features must be known. The peak positions, widths, profiles, and strengths of a certain ice component's infrared absorption features are affected be the overall composition of the ice. Many satellites within the solar system have surfaces that are dominated by H2O or N2 and ices in the interstellar medium (ISM) are primarily composed of H2O. The experiments presented here focus on the near-infrared absorption features of CO, CO2, CH4, and NH3 (nu=10,000-4,000/cm, lambda=1-2.5 microns) and the effects of diluting these molecules in N2 or H2O ice (mixture ratio of 5:1). This is a continuation of previous results published by our research group

    Manipulation of drugs to achieve the required dose is intrinsic to paediatric practice but is not supported by guidelines or evidence

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    Background: A lack of age-appropriate formulations can make it difficult to administer medicines to children. A manipulation of the dosage form may be required to achieve the required dose. This study aimed to describe medicines that are manipulated to achieve the required dose in paediatric practice.Method: A structured, undisguised observational study and postal survey. The observational study investigated drug manipulations occurring in clinical practice across three sites. The questionnaire, administered to a sample of paediatric nurses throughout the UK, surveyed manipulations conducted and nurses' experiences and views.Results: The observational study identified 310 manipulations, of which 62% involved tablets, 21% were intravenous drugs and 10% were sachets. Of the 54 observed manipulations 40 involved tablets with 65% of the tablets being cut and 30% dispersed to obtain a smaller dose. 188 manipulations were reported by questionnaire respondents, of these 46% involved tablets, 12% were intravenous drugs, and 12% were nebuliser solutions. Manipulations were predominantly, but not exclusively, identified in specialist clinical areas with more highly dependent patients. Questionnaire respondents were concerned about the accuracy of the dose achieved following manipulations and the lack of practice guidance.Conclusion: Manipulations to achieve the required dose occur throughout paediatric in-patient settings. The impact of manipulations on the efficacy of the drugs, the accuracy of the dose and any adverse effects on patients is not known. There is a need to develop evidence-based guidance for manipulations of medicines in children

    Cerebrovascular Dysfunction is Related to Depressive Symptom Severity in Young Adults

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    Cerebral vasodilatory responsiveness is blunted in older adults (~70 yrs) with depressive disorders and is thought to contribute to the link between depressive symptomology and increased risk for neurocognitive (e.g., dementia) and cerebral vascular (e.g., stroke) diseases. In young adults with major depressive disorder (MDD), peripheral vascular endothelial dysfunction is present and graded in relation to the severity of depressive symptoms; however, to date, limited investigations have examined cerebral vasodilatory function in young otherwise healthy adults with MDD. PURPOSE: We tested the hypothesis that cerebral vasodilatory responsiveness to a hypercapnic stimulus would be blunted in young otherwise healthy adults with MDD compared to healthy non-depressed adults (HA). Further, we hypothesized, that the magnitude of impairment in cerebrovascular function would be related to depressive symptom severity. METHODS: Ten HA (7 women; 22±2yrs) and 10 adults with MDD (8 women; 22±2yrs; n=5 tested during a major depressive episode) participated. Depressive symptom severity was evaluated with the Patient Health History Questionnaire-9 (PHQ-9) in both HA and adults with MDD. Beat-to-beat mean arterial pressure (MAP; finger photoplethysmography), middle cerebral artery blood velocity (MCAv; transcranial Doppler ultrasound), and end-tidal carbon dioxide concentration (PETCO2; capnograph) were continuously measured during baseline (i.e., normocapnia) and rebreathing-induced hypercapnia. Cerebral vascular conductance index (CVCi=MCAv•MAP-1) was calculated at baseline and at the highest common magnitude of hypercapnia achieved by all subjects during rebreathing (∆PETCO2 = 9 Torr). RESULTS: At baseline, there were no differences in MAP or CVCi between groups (both p\u3e0.05). During hypercapnia, there were no group differences in the increase in MAP (∆3±3 HA vs. ∆4±3 mmHg MDD; p=0.78). Further, neither the hypercapnia-induced increase in MCAv (∆29±7 HA vs. ∆26±8 cm•s-1 MDD; p=0.37) nor the increase in CVCi (∆39±12 HA vs. ∆30±12 %baseline MDD; p=0.13) were different between groups. However, greater severity of depressive symptoms was negatively related to cerebral vasodilatory responsiveness (R2=0.219, p=0.04). CONCLUSION: These preliminary data suggest that cerebral vasodilatory responsiveness to hypercapnia is not impaired in young adults with MDD, despite a negative relation between depressive symptom severity and the magnitude of hypercapnia-induced cerebral vasodilation

    Optical Properties of Iron Silicates in the Infrared to Millimeter as a Function of Temperatures and Wavelength

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    The Optical Properties of Astronomical Silicates with Infrared Techniques (OPASI-T) program utilizes multiple instruments to provide spectral data over a wide range of temperature and wavelengths. Experimental methods include Vector Network Analyzer (VNA) and Fourier Transform Spectroscopy (FTS) transmission, and reflection/scattering measurements. From this data, we can determine the optical parameters for the index of refraction, \textit{n}, and the absorption coefficient, \textit{k}. The analysis of the laboratory transmittance data for each sample type is based upon different mathematical models, which are applied to each data set according to their degree of coherence. Presented here are results from iron silicate dust grain analogs, in several sample preparations and at temperatures ranging from 5--300 K, across the infrared and millimeter portion of the spectrum (from 2.5--10,000 \mic\ or 4,000--1 \wvn).Comment: Revised manuscript submitted to Ap

    Current Population Statistics Do Not Favor Photoevaporation over Core-Powered Mass Loss as the Dominant Cause of the Exoplanet Radius Gap

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    We search for evidence of the cause of the exoplanet radius gap, i.e. the dearth of planets with radii near 1.8 R⊕1.8\ R_\oplus. If the cause was photoevaporation, the radius gap should trend with proxies for the early-life high-energy emission of planet-hosting stars. If, alternatively, the cause was core-powered mass loss, no such trends should exist. Critically, spurious trends between the radius gap and stellar properties arise from an underlying correlation with instellation. After accounting for this underlying correlation, we find no trends remain between the radius gap and stellar mass or present-day stellar activity as measured by near-UV emission. We dismiss the nondetection of a radius gap trend with near-UV emission because present-day near-UV emission is unlikely to trace early-life high-energy emission, but we provide a catalog of GALEX near-UV and far-UV emission measurements for general use. We interpret the nondetection of a radius gap trend with stellar mass by simulating photoevaporation with mass-dependent evolution of stellar high-energy emission. The simulation produces an undetectable trend between the radius gap and stellar mass under realistic sources of error. We conclude that no evidence, from this analysis or others in the literature, currently exists that clearly favors either photoevaporation or core powered mass loss as the primary cause of the exoplanet radius gap. However, repeating this analysis once the body of well-characterized <4 R⊕< 4\ R_\oplus planets has roughly doubled could confirm or rule out photoevaporation.Comment: 27 pages, 32 figures, accepted to Ap

    Antiferromagnetic Heisenberg model on anisotropic triangular lattice in the presence of magnetic field

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    We use Schwinger boson mean field theory to study the antiferromagnetic spin-1/2 Heisenberg model on an anisotropic triangular lattice in the presence of a uniform external magnetic field. We calculate the field dependence of the spin incommensurability in the ordered spin spiral phase, and compare the results to the recent experiments in Cs2_{2}CuCl4_{4} by Coldea et al. (Phys. Rev. Lett. 86, 1335 (2001)).Comment: 4 pages with 4 figures include
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