29 research outputs found

    Relationship between aortic root size and glomerular filtration rate in hypertensive patients

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    OBJECTIVE: Recent studies suggest that enlarged aortic root diameter (ARD) may predict cardiovascular events in absence of aneurysmatic alterations. Little is known about the influence of renal function on ARD. Our study was aimed to assess the relationships between glomerular filtration rate (GFR) and ARD in hypertensive subjects. METHODS: We enrolled 611 hypertensive individuals (mean age: 52 ± 15 years; men 63%). ARD was measured by echocardiography at the level of Valsalva's sinuses using M-mode tracings. It was considered as absolute measure, normalized to body surface area (ARD/BSA) and indexed to height (ARD/H). GFR was estimated by the Chronic Kidney Disease Epidemiology Collaboration equation. The study population was categorized into seven groups: subjects without chronic kidney disease (no CKD) and subjects with increasing severity of CKD (1, 2, 3a, 3b, 4, 5), as proposed by the 2012 Kidney Disease: Improving Global Outcomes guidelines. RESULTS: ARD/BSA and ARD/H showed a stepwise increase from the group with normal renal function to the groups with increasing severity of CKD. GFR correlated significantly with ARD (r = -0.17), ARD/BSA (r = -0.43) and ARD/H (r = -0.35; all P < 0.001). The associations of GFR with ARD/BSA (β = -0.26; P < 0.001) and ARD/H (β = -0.13; P = 0.01) held in linear multiple regression analyses, after adjustment for various confounding factors. CONCLUSION: Our study seems to suggest that a reduced renal function may adversely influence ARD. This may contribute to explain the enhanced cardiovascular risk associated with renal insufficiency

    High dose esomeprazole as an anti-inflammatory agent in sepsis: Protocol for a randomized controlled trial

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    Background: Sepsis is caused by dysregulated immune responses due to infection and still presents high mortality rate and limited efficacious therapies, apart from antibiotics. Recent evidence suggests that very high dose proton pump inhibitors might regulate major sepsis mediators' secretion by monocytes, which might attenuate excessive host reactions and improve clinical outcomes. This effect is obtained with doses which are approximately 50 times higher than prophylactic esomeprazole single daily administration and 17 times higher than the cumulative dose of a three day prophylaxis. We aim to perform a randomized trial to investigate if high dose esomeprazole reduces organ dysfunction in patients with sepsis or septic shock. Methods: This study, called PPI-SEPSIS, is a multicenter, randomized, double blind, placebo-controlled clinical trial on critically ill septic patients admitted to the emergency department or intensive care unit. A total of 300 patients will be randomized to receive high dose esomeprazole (80 mg bolus followed by 12 mg/h for 72 h and a second 80 mg bolus 12 h after the first one) or equivolume placebo (sodium chloride 0.9%), with 1:1 allocation. The primary endpoint of the study will be mean daily Sequential Organ Failure Assessment (SOFA) score over 10 days. Secondary outcomes will include antibiotic-free days, single organ failure severity, intensive care unit-free days at day 28, and mortality. Discussion: This trial aims to test the efficacy of high dose esomeprazole to reduce acute organ dysfunction in patients with septic shock. Trial registration: This trial was registered on ClinicalTrials.gov with the trial identification NCT03452865 in March 2018

    RIvaroxaban and VAscular Surgery (RIVAS): insights from a multicenter, worldwide web-based survey

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    Search for photons with energies above 1018 eV using the hybrid detector of the Pierre Auger Observatory

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    Erratum: Combined fit of spectrum and composition data as measured by the Pierre Auger Observatory

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    We present a combined fit of a simple astrophysical model of UHECR sources to both the energy spectrum and mass composition data measured by the Pierre Auger Observatory. The fit has been performed for energies above 5 ⋅ 10(18) eV, i.e. the region of the all-particle spectrum above the so-called ankle feature. The astrophysical model we adopted consists of identical sources uniformly distributed in a comoving volume, where nuclei are accelerated through a rigidity-dependent mechanism. The fit results suggest sources characterized by relatively low maximum injection energies, hard spectra and heavy chemical composition. We also show that uncertainties about physical quantities relevant to UHECR propagation and shower development have a non-negligible impact on the fit results

    Combined fit of spectrum and composition data as measured by the Pierre Auger Observatory

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    The Pierre Auger Observatory: Contributions to the 35th International Cosmic Ray Conference (ICRC 2017)

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    Observation of inclined EeV air showers with the radio detector of the Pierre Auger Observatory

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    International audienceWith the Auger Engineering Radio Array (AERA) of the Pierre Auger Observatory, we have observed the radio emission from 561 extensive air showers with zenith angles between 60o and 84o. In contrast to air showers with more vertical incidence, these inclined air showers illuminate large ground areas of several km2 with radio signals detectable in the 30 to 80 MHz band. A comparison of the measured radio-signal amplitudes with Monte Carlo simulations of a subset of 50 events for which we reconstruct the energy using the Auger surface detector shows agreement within the uncertainties of the current analysis. As expected for forward-beamed radio emission undergoing no significant absorption or scattering in the atmosphere, the area illuminated by radio signals grows with the zenith angle of the air shower. Inclined air showers with EeV energies are thus measurable with sparse radio-antenna arrays with grid sizes of a km or more. This is particularly attractive as radio detection provides direct access to the energy in the electromagnetic cascade of an air shower, which in case of inclined air showers is not accessible by arrays of particle detectors on the ground

    A targeted search for point sources of EeV photons with the Pierre Auger Observatory

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    A targeted search for point sources of EeV photons with the Pierre Auger Observatory

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