386 research outputs found

    Signalling Through Rho GTPases in Cardiomyocytes

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    Endothelin-1 (ET-1) promotes changes in gene/protein expression in cardiomyocytes leading to hypertrophy. This results from activation of intracellular signalling pathways including small G proteins that activate protein kinases. Thus, ET-1 activates RhoA that stimulates ROCK and PKN, and Ras that promotes activation of extracellular signal-regulated kinases 1/2 (ERK1/2). Microarrays were used to dissect the roles of ERK1/2 vs RhoA in the cardiomyocyte transcriptomic response to ET-1 using PD184352 and C3 endotoxin from C. botulinum (C3T) for selective inhibition of the ERK1/2 cascade and RhoA, respectively. Microarray data were analysed using GeneSpring and data were validated by qPCR. ERK1/2 signalling positively regulated ~65% of the early gene expression response to ET-1 with a small (~2%) negative effect, whereas RhoA signalling positively regulated ~11% of the early gene expression response to ET-1 with a greater (~14%) negative contribution. Of RNAs non-responsive to ET-1, 66 or 448 were regulated by PD184352 or C3T, respectively, indicating that RhoA had a more significant effect on baseline RNA expression. mRNAs upregulated by ET-1 encoded several receptor ligands (e.g. Ereg, Areg) and transcription factors (e.g. Abra/STARS, Srf) that potentially propagate the response. Published studies suggest that PKN1 (activated by RhoA) is important in cardiomyocyte gene expression. Adenoviruses were generated to overexpress FLAG-tagged PKN1 in cardiomyocytes for protein kinase studies. Unexpectedly, PKN1 was not activated by ET-1, but was activated by oxidative stress, insulin, or hyperosmotic shock, stimuli that do not activate RhoA. Thus, PKN1 is not necessarily an effector of RhoA in cardiomyocytes. In conclusion, ERK1/2 dominates over RhoA in the early transcriptomic response to ET-1. RhoA plays a major role in maintaining baseline RNA expression but, as with upregulation of Abra/Srf by ET-1, RhoA may regulate changes in RNA expression over longer times. However, the effects of RhoA on cardiomyocyte gene expression are unlikely to be mediated through PKN1

    Improved Learning in U.S. History and Decision Competence with Decision-Focused Curriculum

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    Decision making is rarely taught in high school, even though improved decision skills could benefit young people facing life-shaping decisions. While decision competence has been shown to correlate with better life outcomes, few interventions designed to improve decision skills have been evaluated with rigorous quantitative measures. A randomized study showed that integrating decision making into U.S. history instruction improved students' history knowledge and decision-making competence, compared to traditional history instruction. Thus, integrating decision training enhanced academic performance and improved an important, general life skill associated with improved life outcomes. © 2012 Jacobson et al

    Effect of complete epithelial debridement before riboflavin–ultraviolet-A corneal collagen crosslinking therapy

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    Purpose: To evaluate the importance of complete epithelial removal before riboflavin–ultraviolet-A (UVA) corneal collagen crosslinking therapy. Setting: School of Optometry and Vision Sciences, Cardiff University, Wales, United Kingdom. Methods: Riboflavin eyedrops were applied at 5-minute intervals for 35 minutes to the anterior corneal surface of 36 porcine eyes (12 with no epithelial trauma but treated with tetracaine eyedrops, 12 with superficial epithelial trauma but with an intact basal epithelium, and 12 with a fully removed epithelium). The corneal surface of 6 tetracaine-treated eyes, 6 eyes with superficial epithelial trauma, and 6 eyes with a fully removed epithelium was exposed to UVA light for 30 minutes during riboflavin administration. The light transmission spectra of the enucleated corneas were analyzed with a spectrophotometer and compared with those of 9 untreated porcine corneas. Results: Corneas with a fully removed epithelium treated with riboflavin showed an abnormal dip in the transmission spectrum between 400 nm and 510 nm (P<.01). This was attributed to the presence of riboflavin in the corneal stroma. The spectra of riboflavin-treated corneas with no epithelial trauma but tetracaine administration and those with superficial epithelial trauma did not differ from those of the non–riboflavin-treated controls. Exposure to UVA following riboflavin administration did not alter corneal light transmission. Conclusions: Complete removal of the corneal epithelium is an essential component of riboflavin–UVA crosslinking therapy as superficial epithelial trauma and tetracaine administration alone are not sufficient to permit the penetration of riboflavin into the corneal stroma. Failure to achieve adequate stromal absorption of riboflavin may impair the efficacy of the crosslinking process

    Snowpack Relative Permittivity and Density Derived from Near-Coincident Lidar and Ground-Penetrating Radar

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    Depth-based and radar-based remote sensing methods (e.g., lidar, synthetic aperture radar) are promising approaches for remotely measuring snow water equivalent (SWE) at high spatial resolution. These approaches require snow density estimates, obtained from in-situ measurements or density models, to calculate SWE. However, in-situ measurements are operationally limited, and few density models have seen extensive evaluation. Here, we combine near-coincident, lidar-measured snow depths with ground-penetrating radar (GPR) two-way travel times (twt) of snowpack thickness to derive \u3e20 km of relative permittivity estimates from nine dry and two wet snow surveys at Grand Mesa, Cameron Pass, and Ranch Creek, Colorado. We tested three equations for converting dry snow relative permittivity to snow density and found the Kovacs et al. (1995) equation to yield the best comparison with in-situ measurements (RMSE = 54 kg m−3). Variogram analyses revealed a 19 m median correlation length for relative permittivity and snow density in dry snow, which increased to \u3e 30 m in wet conditions. We compared derived densities with estimated densities from several empirical models, the Snow Data Assimilation System (SNODAS), and the physically based iSnobal model. Estimated and derived densities were combined with snow depths and twt to evaluate density model performance within SWE remote sensing methods. The Jonas et al. (2009) empirical model yielded the most accurate SWE from lidar snow depths (RMSE = 51 mm), whereas SNODAS yielded the most accurate SWE from GPR twt (RMSE = 41 mm). Densities from both models generated SWE estimates within ±10% of derived SWE when SWE averaged \u3e 400 mm, however, model uncertainty increased to \u3e 20% when SWE averaged \u3c 300 mm. The development and refinement of density models, particularly in lower SWE conditions, is a high priority to fully realize the potential of SWE remote sensing methods

    3D collagen orientation study of the human cornea using X-ray diffraction and femtosecond laser technology

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    Purpose. To study the distribution and predominant orientations of fibrillar collagen at different depths throughout the entire thickness of the human cornea. This information will form the basis of a full three-dimensional reconstruction of the preferred orientations of corneal lamellae. Methods. Femtosecond laser technology was used to delaminate the central zones of five human corneas into three separate layers (anterior, mid, and posterior stroma), each with predetermined thicknesses. Wide-angle x-ray diffraction was used to study the gross collagen fibril orientation and distribution within each layer. Results. The middle and posterior parts of the human cornea demonstrated a preferential orthogonal arrangement of collagen fibrils, directed along the superior–inferior and nasal–temporal meridians, with an increase in the number of lamellae toward the periphery. However, the anterior cornea (33% of total corneal thickness) showed no systematic preferred lamellar orientation. Conclusions. In the posterior two thirds of the human cornea, collagen lies predominantly in the vertical and horizontal meridians (directed toward the four major rectus muscles), whereas collagen in the anterior third of the cornea is more isotropic. The predominantly orthogonal arrangement of collagen in the mid and posterior stroma may help to distribute strain in the cornea by allowing it to withstand the pull of the extraocular muscles, whereas the more isotropic arrangement in the anterior cornea may play an important role in the biomechanics of the cornea by resisting intraocular pressure while at the same time maintaining corneal curvature

    Detailed Abundances in the Ultra-faint Magellanic Satellites Carina II and III

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    We present the first detailed elemental abundances in the ultra-faint Magellanic satellite galaxies Carina II (Car II) and Carina III (Car III). With high-resolution Magellan/MIKE spectroscopy, we determined abundances of nine stars in Car II including the first abundances of an RR Lyrae star in an ultra-faint dwarf galaxy; and two stars in Car III. The chemical abundances demonstrate that both systems are clearly galaxies and not globular clusters. The stars in these galaxies mostly display abundance trends matching those of other similarly faint dwarf galaxies: enhanced but declining [alpha/Fe] ratios, iron-peak elements matching the stellar halo, and unusually low neutron-capture element abundances. One star displays a low outlying [Sc/Fe] = -1.0. We detect a large Ba scatter in Car II, likely due to inhomogeneous enrichment by low-mass AGB star winds. The most striking abundance trend is for [Mg/Ca] in Car II, which decreases from +0.4 to -0.4 and indicates clear variation in the initial progenitor masses of enriching core-collapse supernovae. So far, the only ultra-faint dwarf galaxies displaying a similar [Mg/Ca] trend are likely satellites of the Large Magellanic Cloud. We find two stars with [Fe/H] < -3.5, whose abundances likely trace the first generation of metal-free Population III stars and are well-fit by Population III core-collapse supernova yields. An appendix describes our new abundance uncertainty analysis that propagates line-by-line stellar parameter uncertainties.Comment: 21 pages + appendix, 9 figures, 6 tables, accepted to Ap
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