1,449 research outputs found

    Neutrophil gelatinase-associated lipocalin: its response to hypoxia and association with acute mountain sickness.

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    Acute Mountain Sickness (AMS) is a common clinical challenge at high altitude (HA). A point-of-care biochemical marker for AMS could have widespread utility. Neutrophil gelatinase-associated lipocalin (NGAL) rises in response to renal injury, inflammation and oxidative stress. We investigated whether NGAL rises with HA and if this rise was related to AMS, hypoxia or exercise. NGAL was assayed in a cohort (n = 22) undertaking 6 hours exercise at near sea-level (SL); a cohort (n = 14) during 3 hours of normobaric hypoxia (FiO2 11.6%) and on two trekking expeditions (n = 52) to over 5000 m. NGAL did not change with exercise at SL or following normobaric hypoxia. During the trekking expeditions NGAL levels (ng/ml, mean ± sd, range) rose significantly (P < 0.001) from 68 ± 14 (60-102) at 1300 m to 183 ± 107 (65-519); 143 ± 66 (60-315) and 150 ± 71 (60-357) at 3400 m, 4270 m and 5150 m respectively. At 5150 m there was a significant difference in NGAL between those with severe AMS (n = 7), mild AMS (n = 16) or no AMS (n = 23): 201 ± 34 versus 171 ± 19 versus 124 ± 12 respectively (P = 0.009 for severe versus no AMS; P = 0.026 for mild versus no AMS). In summary, NGAL rises in response to prolonged hypobaric hypoxia and demonstrates a relationship to the presence and severity of AMS

    PSS32 Impact of dry eye on everyday life (Ideel) - Symptom bother: Estimating cut-off scores for dry eye severity groups

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    The aims of the study were to estimate score ranges associated with dry eye severity based on the Impact of Dry Eye on Everyday Life (IDEEL) Symptom Bother (SB) domain, and to evaluate the overall performance of the SB domain

    The connection between stellar mass, age and quenching timescale in massive quiescent galaxies at z1z \simeq 1

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    We present a spectro-photometric study of a mass-complete sample of quiescent galaxies at 1.0<z<1.31.0 < z < 1.3 with log10(M/M)10.3\mathrm{log_{10}}(M_{\star}/\mathrm{M_{\odot}}) \geq 10.3 drawn from the VANDELS survey, exploring the relationship between stellar mass, age and star-formation history. Within our sample of 114 galaxies, we derive a stellar-mass vs stellar-age relation with a slope of 1.200.27+0.281.20^{+0.28}_{-0.27} Gyr per decade in stellar mass. When combined with recent literature results, we find evidence that the slope of this relation remains consistent over the redshift interval 0<z<40<z<4. The galaxies within the VANDELS quiescent display a wide range of star-formation histories, with a mean star-formation timescale of 1.5±0.11.5\pm{0.1} Gyr and a mean quenching timescale of 1.4±0.11.4\pm{0.1} Gyr. We also find a large scatter in the quenching timescales of the VANDELS quiescent galaxies, in agreement with previous evidence that galaxies at z1z \sim 1 cease star formation via multiple mechanisms. We then focus on the oldest galaxies in our sample, finding that the number density of galaxies that quenched before z=3z = 3 with stellar masses log10(M/M)10.6\mathrm{log_{10}}(M_{\star}/\mathrm{M_{\odot}}) \geq 10.6 is 1.120.72+1.47×105 Mpc3 1.12_{-0.72}^{+1.47} \times 10^{-5} \ \mathrm{Mpc}^{-3}. Although uncertain, this estimate is in good agreement with the latest observational results at 3<z<43<z<4, tentatively suggesting that neither rejuvenation nor merger events are playing a major role in the evolution of the oldest massive quiescent galaxies within the redshift interval 1<z<31<z<3.Comment: Accepted for publication in MNRAS, 11 pages, 6 figure

    Dopamine D_2-receptor activation elicits akinesia, rigidity, catalepsy, and tremor in mice expressing hypersensitive 4 nicotinic receptors via a cholinergic-dependent mechanism

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    Recent studies suggest that high-affinity neuronal nicotinic acetylcholine receptors (nAChRs) containing α4 and β2 subunits (α4β2*) functionally interact with G-protein-coupled dopamine (DA) D_2 receptors in basal ganglia. We hypothesized that if a functional interaction between these receptors exists, then mice expressing an M2 point mutation (Leu9'Ala) rendering 4 nAChRs hypersensitive to ACh may exhibit altered sensitivity to a D_2-receptor agonist. When challenged with the D_(2)R agonist, quinpirole (0.5–10 mg/kg), Leu9'Ala mice, but not wild-type (WT) littermates, developed severe, reversible motor impairment characterized by rigidity, catalepsy, akinesia, and tremor. While striatal DA tissue content, baseline release, and quinpirole-induced DA depletion did not differ between Leu9'Ala and WT mice, quinpirole dramatically increased activity of cholinergic striatal interneurons only in mutant animals, as measured by increased c-Fos expression in choline acetyltransferase (ChAT)-positive interneurons. Highlighting the importance of the cholinergic system in this mouse model, inhibiting the effects of ACh by blocking muscarinic receptors, or by selectively activating hypersensitive nAChRs with nicotine, rescued motor symptoms. This novel mouse model mimics the imbalance between striatal DA/ACh function associated with severe motor impairment in disorders such as Parkinson’s disease, and the data suggest that a D_(2)R–α4*-nAChR functional interaction regulates cholinergic interneuron activity.—Zhao-Shea, R., Cohen, B. N., Just, H., McClure-Begley, T., Whiteaker, P., Grady, S. R., Salminen, O., Gardner, P. D., Lester, H. A., Tapper, A. R. Dopamine D2-receptor activation elicits akinesia, rigidity, catalepsy, and tremor in mice expressing hypersensitive α4 nicotinic receptors via a cholinergic-dependent mechanism

    Surface relaxation and ferromagnetism of Rh(001)

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    The significant discrepancy between first-principles calculations and experimental analyses for the relaxation of the (001) surface of rhodium has been a puzzle for some years. In this paper we present density functional theory calculations using the local-density approximation and the generalized gradient approximation of the exchange-correlation functional. We investigate the thermal expansion of the surface and the possibility of surface magnetism. The results throw light on several, hitherto overlooked, aspects of metal surfaces. We find, that, when the free energy is considered, density-functional theory provides results in good agreement with experiments.Comment: 6 pages, 4 figures, submitted to Phys. Rev. Lett. (April 28, 1996

    Strained tetragonal states and Bain paths in metals

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    Paths of tetragonal states between two phases of a material, such as bcc and fcc, are called Bain paths. Two simple Bain paths can be defined in terms of special imposed stresses, one of which applies directly to strained epitaxial films. Each path goes far into the range of nonlinear elasticity and reaches a range of structural parameters in which the structure is inherently unstable. In this paper we identify and analyze the general properties of these paths by density functional theory. Special examples include vanadium, cobalt and copper, and the epitaxial path is used to identify an epitaxial film as related uniquely to a bulk phase.Comment: RevTeX, 4 pages, 4 figures, submitted to Phys. Rev. Let

    Meanings of epilepsy in its sociocultural context and implications for stigma: Findings from ethnographic studies in local communities in China and Vietnam

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    We investigated beliefs about the causes, course, and treatment of epilepsy and its impact on quality of life (QOL) in key target groups, using “mini-ethnographies” involving 141 in-depth interviews and 12 focus groups in China, and 84 in-depth interviews and 16 focus groups in Vietnam. Data were analyzed thematically, using a qualitative data analysis package. In both countries, beliefs about causes and triggers of epilepsy and seizures were a complex interweaving of Western, traditional, and folk medicine concepts. Epilepsy was understood to be chronic, not curable, but controllable, and was seen as enormously socially disruptive, with wide-ranging impact on QOL. Our findings suggest a more “embodied” and benign set of theories about epilepsy than in some other cultural contexts; nonetheless, people with epilepsy are still seen as having low social value and face social rejection. By exploring meanings attached to epilepsy in these two cultural contexts, we have clarified reasons behind previously documented negative attitudes and foci for future intervention studies

    Evidence for the emergence of dust-free stellar populations at z > 10

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    We present an analysis of the UV continuum slopes for a sample of 176176 galaxy candidates at 8<zphot<168 < z_{\mathrm{phot}} < 16. Focusing primarily on a new sample of 125125 galaxies at z11\langle z \rangle \simeq 11 selected from 320\simeq 320 arcmin2^2 of public JWST imaging data across 1515 independent datasets, we investigate the evolution of β\beta in the galaxy population at z>8z > 8. In the redshift range 8<z<108 < z < 10, we find evidence for a relationship between β\beta and MUVM_{\rm UV}, such that galaxies with brighter UV luminosities display redder UV slopes, with dβ/dMUV=0.17±0.03\rm{d}\beta/ \rm{d} M_{\rm UV} = -0.17 \pm 0.03. A comparison with literature studies down to z2z\simeq2 suggests that a βMUV\beta-M_{\rm UV} relation has been in place from at least z10z\simeq10, with a slope that does not evolve strongly with redshift, but with an evolving normalisation such that galaxies at higher redshifts become bluer at fixed MUVM_{\rm UV}. We find a significant trend between β\beta and redshift, with the inverse-variance weighted mean value evolving from β=2.17±0.05\langle \beta \rangle = -2.17 \pm 0.05 at z=9.5z = 9.5 to β=2.56±0.05\langle \beta \rangle = -2.56 \pm 0.05 at z=11.5z = 11.5. Based on a comparison with stellar population models, we find that at z>10.5z>10.5 the average UV continuum slope is consistent with the intrinsic blue limit of `dust-free' stellar populations (βint2.6)(\beta_{\mathrm{int}} \simeq -2.6). These results suggest that the moderately dust-reddened galaxy population at z<10z < 10 was essentially dust free at z11z \simeq 11. The extremely blue galaxies being uncovered at z>10z>10 place important constraints on the dust content of early galaxies, and imply that the already observed galaxy population is likely supplying an ionizing photon budget capable of maintaining ionized IGM fractions of 5\gtrsim 5 per cent at z11z\simeq11.Comment: 16 pages, 12 figures, submitted to MNRA
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