233 research outputs found

    The epidemiology of AIDS-associated non-Hodgkin's lymphoma in the World Health Organization European Region

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    This paper describes the epidemiology of AIDS-associated non-Hodgkin's lymphoma (NHL) in the World Health Organization (WHO) European Region. Data, collected by the WHO Collaborating Centre on AIDS in Paris, France, were derived from the national AIDS surveillance systems of 21 countries. Among 53,042 cases reported as of the end of June 1991, 1,617 (3.0%) had NHL as the presenting clinical manifestation of AIDS. The proportion of cases presenting with NHL ranged from 1.1% in children infected perinatally to 3.9% among haemophiliacs. In comparison with intravenous drug users (IVDUs) (2.6% of whom had NHL), a moderate excess was found among homosexual or bisexual men (odds ratio - OR -:1.2, 95% confidence interval - CI -:1.0-1.3). Over time, the proportion of NHL was constant, but whereas among homosexual or bisexual men the frequency of NHL as AIDS-indicator disease significantly increased (9.7% per year), among IVDUs a significant downward trend emerged (17.1% per year). In respect to age, two peaks of NHL were seen at the age groups 10-19 (3.8%) and 50-59 (4.3%). The proportion of AIDS-associated NHL significantly increased with increasing age among homosexual and bisexual men and heterosexuals whereas it decreased among IVDUs. All these differences, however, have to be interpreted cautiously on account of the limitations of the reporting systems

    Constraints on Dark Matter Annihilation in Clusters of Galaxies with the Fermi Large Area Telescope

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    Nearby clusters and groups of galaxies are potentially bright sources of high-energy gamma-ray emission resulting from the pair-annihilation of dark matter particles. However, no significant gamma-ray emission has been detected so far from clusters in the first 11 months of observations with the Fermi Large Area Telescope. We interpret this non-detection in terms of constraints on dark matter particle properties. In particular for leptonic annihilation final states and particle masses greater than ~200 GeV, gamma-ray emission from inverse Compton scattering of CMB photons is expected to dominate the dark matter annihilation signal from clusters, and our gamma-ray limits exclude large regions of the parameter space that would give a good fit to the recent anomalous Pamela and Fermi-LAT electron-positron measurements. We also present constraints on the annihilation of more standard dark matter candidates, such as the lightest neutralino of supersymmetric models. The constraints are particularly strong when including the fact that clusters are known to contain substructure at least on galaxy scales, increasing the expected gamma-ray flux by a factor of ~5 over a smooth-halo assumption. We also explore the effect of uncertainties in cluster dark matter density profiles, finding a systematic uncertainty in the constraints of roughly a factor of two, but similar overall conclusions. In this work, we focus on deriving limits on dark matter models; a more general consideration of the Fermi-LAT data on clusters and clusters as gamma-ray sources is forthcoming.Comment: accepted to JCAP, Corresponding authors: T.E. Jeltema and S. Profumo, minor revisions to be consistent with accepted versio

    LSST: from Science Drivers to Reference Design and Anticipated Data Products

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    (Abridged) We describe here the most ambitious survey currently planned in the optical, the Large Synoptic Survey Telescope (LSST). A vast array of science will be enabled by a single wide-deep-fast sky survey, and LSST will have unique survey capability in the faint time domain. The LSST design is driven by four main science themes: probing dark energy and dark matter, taking an inventory of the Solar System, exploring the transient optical sky, and mapping the Milky Way. LSST will be a wide-field ground-based system sited at Cerro Pach\'{o}n in northern Chile. The telescope will have an 8.4 m (6.5 m effective) primary mirror, a 9.6 deg2^2 field of view, and a 3.2 Gigapixel camera. The standard observing sequence will consist of pairs of 15-second exposures in a given field, with two such visits in each pointing in a given night. With these repeats, the LSST system is capable of imaging about 10,000 square degrees of sky in a single filter in three nights. The typical 5σ\sigma point-source depth in a single visit in rr will be ∌24.5\sim 24.5 (AB). The project is in the construction phase and will begin regular survey operations by 2022. The survey area will be contained within 30,000 deg2^2 with ÎŽ<+34.5∘\delta<+34.5^\circ, and will be imaged multiple times in six bands, ugrizyugrizy, covering the wavelength range 320--1050 nm. About 90\% of the observing time will be devoted to a deep-wide-fast survey mode which will uniformly observe a 18,000 deg2^2 region about 800 times (summed over all six bands) during the anticipated 10 years of operations, and yield a coadded map to r∌27.5r\sim27.5. The remaining 10\% of the observing time will be allocated to projects such as a Very Deep and Fast time domain survey. The goal is to make LSST data products, including a relational database of about 32 trillion observations of 40 billion objects, available to the public and scientists around the world.Comment: 57 pages, 32 color figures, version with high-resolution figures available from https://www.lsst.org/overvie

    Research of working area development parameters in conditions of deep steep deposit finalizing

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    ĐžŃ‚Ń€ĐžĐŒĐ°ĐœĐŸ Ń„ĐŸŃ€ĐŒŃƒĐ»Đž Ń€ĐŸĐ·Ń€Đ°Ń…ŃƒĐœĐșу ĐŸĐ±â€™Ń”ĐŒŃƒ запасіĐČ ĐșĐŸŃ€ĐžŃĐœĐžŃ… ĐșĐŸĐżĐ°Đ»ĐžĐœ ĐČ ĐżŃ€ĐžĐșĐŸĐœŃ‚ŃƒŃ€ĐœŃ–Đč та ĐłĐ»ĐžĐ±ĐžĐœĐœŃ–Đč Đ·ĐŸĐœŃ–. Đ’ŃŃ‚Đ°ĐœĐŸĐČĐ»Đ”ĐœĐŸ хараĐșтДр ĐČплОĐČу ĐżĐ°Ń€Đ°ĐŒĐ”Ń‚Ń€Ń–ĐČ ĐŽĐŸŃ€ĐŸĐ±ĐșĐž ĐłĐ»ĐžĐ±ĐŸĐșох ĐșŃ€ŃƒŃ‚ĐŸŃĐżĐ°ĐŽĐœĐžŃ… Ń€ĐŸĐŽĐŸĐČощ ĐČіЮĐșŃ€ĐžŃ‚ĐžĐŒ ŃĐżĐŸŃĐŸĐ±ĐŸĐŒ ĐœĐ° ĐŽĐŸŃ†Ń–Đ»ŃŒĐœĐ” ĐżĐŸĐ»ĐŸĐ¶Đ”ĐœĐœŃ ĐżĐŸŃ‚ĐŸŃ‡ĐœĐžŃ… та ĐżŃ€ĐŸĐ”ĐșŃ‚ĐœĐžŃ… ĐșĐŸĐœŃ‚ŃƒŃ€Ń–ĐČ Đșар’єру. Đ’ŃŃ‚Đ°ĐœĐŸĐČĐ»Đ”ĐœĐŸ, Ń‰ĐŸ ĐœĐ°ĐčĐŒĐ”ĐœŃˆĐžĐč ŃĐ”Ń€Đ”ĐŽĐœŃ–Đč ĐșĐŸĐ”Ń„Ń–Ń†Ń–Ń”ĐœŃ‚ Ń€ĐŸĐ·ĐșроĐČу ĐŽĐŸŃŃĐłĐ°Ń”Ń‚ŃŒŃŃ про ĐŒŃ–ĐœŃ–ĐŒĐ°Đ»ŃŒĐœĐŸĐŒŃƒ Đ·ĐœĐ°Ń‡Đ”ĐœĐœŃ– ŃŃƒĐŒĐž ĐŸĐ±ŃŃĐłŃ–ĐČ ĐșĐŸŃ€ĐžŃĐœĐŸŃ— ĐșĐŸĐżĐ°Đ»ĐžĐœĐž проĐșĐŸĐœŃ‚ŃƒŃ€ĐœĐŸŃ— Đ·ĐŸĐœĐž Đ»Đ”Đ¶Đ°Ń‡ĐŸĐłĐŸ і ĐČĐžŃŃŃ‡ĐŸĐłĐŸ Đ±ĐŸĐșіĐČ ĐżĐŸĐșлаЎу ĐČ ĐżŃ€ĐŸĐ”ĐșŃ‚ĐœĐŸĐŒŃƒ ĐżĐŸĐ»ĐŸĐ¶Đ”ĐœĐœŃ–. НаĐčĐŒĐ”ĐœŃˆĐžĐč ĐżĐŸŃ‚ĐŸŃ‡ĐœĐžĐč ĐșĐŸĐ”Ń„Ń–Ń†Ń–Ń”ĐœŃ‚ Ń€ĐŸĐ·ĐșроĐČу ĐŽĐŸŃŃĐłĐ°Ń”Ń‚ŃŒŃŃ про ĐŒŃ–ĐœŃ–ĐŒĐ°Đ»ŃŒĐœĐŸĐŒŃƒ Đ·ĐœĐ°Ń‡Đ”ĐœĐœŃ– ŃŃƒĐŒĐž ĐŸĐ±ŃŃĐłŃ–ĐČ ĐșĐŸŃ€ĐžŃĐœĐŸŃ— ĐșĐŸĐżĐ°Đ»ĐžĐœĐž проĐșĐŸĐœŃ‚ŃƒŃ€ĐœĐŸŃ— Đ·ĐŸĐœĐž Đ»Đ”Đ¶Đ°Ń‡ĐŸĐłĐŸ і ĐČĐžŃŃŃ‡ĐŸĐłĐŸ Đ±ĐŸĐșіĐČ ĐżĐŸĐșлаЎу, Đ° таĐșĐŸĐ¶ Ń€ĐŸĐ±ĐŸŃ‡ĐŸĐłĐŸ Đ±ĐŸŃ€Ń‚Ńƒ Đșар'єру ĐČ ĐżĐŸŃ‚ĐŸŃ‡ĐœĐŸĐŒŃƒ ĐżĐŸĐ»ĐŸĐ¶Đ”ĐœĐœŃ–

    The On-orbit Calibrations for the Fermi Large Area Telescope

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    The Large Area Telescope (LAT) on--board the Fermi Gamma ray Space Telescope began its on--orbit operations on June 23, 2008. Calibrations, defined in a generic sense, correspond to synchronization of trigger signals, optimization of delays for latching data, determination of detector thresholds, gains and responses, evaluation of the perimeter of the South Atlantic Anomaly (SAA), measurements of live time, of absolute time, and internal and spacecraft boresight alignments. Here we describe on orbit calibration results obtained using known astrophysical sources, galactic cosmic rays, and charge injection into the front-end electronics of each detector. Instrument response functions will be described in a separate publication. This paper demonstrates the stability of calibrations and describes minor changes observed since launch. These results have been used to calibrate the LAT datasets to be publicly released in August 2009.Comment: 60 pages, 34 figures, submitted to Astroparticle Physic

    New insights into the genetic etiology of Alzheimer's disease and related dementias

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    Characterization of the genetic landscape of Alzheimer's disease (AD) and related dementias (ADD) provides a unique opportunity for a better understanding of the associated pathophysiological processes. We performed a two-stage genome-wide association study totaling 111,326 clinically diagnosed/'proxy' AD cases and 677,663 controls. We found 75 risk loci, of which 42 were new at the time of analysis. Pathway enrichment analyses confirmed the involvement of amyloid/tau pathways and highlighted microglia implication. Gene prioritization in the new loci identified 31 genes that were suggestive of new genetically associated processes, including the tumor necrosis factor alpha pathway through the linear ubiquitin chain assembly complex. We also built a new genetic risk score associated with the risk of future AD/dementia or progression from mild cognitive impairment to AD/dementia. The improvement in prediction led to a 1.6- to 1.9-fold increase in AD risk from the lowest to the highest decile, in addition to effects of age and the APOE Δ4 allele

    Risk profiles and one-year outcomes of patients with newly diagnosed atrial fibrillation in India: Insights from the GARFIELD-AF Registry.

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    BACKGROUND: The Global Anticoagulant Registry in the FIELD-Atrial Fibrillation (GARFIELD-AF) is an ongoing prospective noninterventional registry, which is providing important information on the baseline characteristics, treatment patterns, and 1-year outcomes in patients with newly diagnosed non-valvular atrial fibrillation (NVAF). This report describes data from Indian patients recruited in this registry. METHODS AND RESULTS: A total of 52,014 patients with newly diagnosed AF were enrolled globally; of these, 1388 patients were recruited from 26 sites within India (2012-2016). In India, the mean age was 65.8 years at diagnosis of NVAF. Hypertension was the most prevalent risk factor for AF, present in 68.5% of patients from India and in 76.3% of patients globally (P < 0.001). Diabetes and coronary artery disease (CAD) were prevalent in 36.2% and 28.1% of patients as compared with global prevalence of 22.2% and 21.6%, respectively (P < 0.001 for both). Antiplatelet therapy was the most common antithrombotic treatment in India. With increasing stroke risk, however, patients were more likely to receive oral anticoagulant therapy [mainly vitamin K antagonist (VKA)], but average international normalized ratio (INR) was lower among Indian patients [median INR value 1.6 (interquartile range {IQR}: 1.3-2.3) versus 2.3 (IQR 1.8-2.8) (P < 0.001)]. Compared with other countries, patients from India had markedly higher rates of all-cause mortality [7.68 per 100 person-years (95% confidence interval 6.32-9.35) vs 4.34 (4.16-4.53), P < 0.0001], while rates of stroke/systemic embolism and major bleeding were lower after 1 year of follow-up. CONCLUSION: Compared to previously published registries from India, the GARFIELD-AF registry describes clinical profiles and outcomes in Indian patients with AF of a different etiology. The registry data show that compared to the rest of the world, Indian AF patients are younger in age and have more diabetes and CAD. Patients with a higher stroke risk are more likely to receive anticoagulation therapy with VKA but are underdosed compared with the global average in the GARFIELD-AF. CLINICAL TRIAL REGISTRATION-URL: http://www.clinicaltrials.gov. Unique identifier: NCT01090362
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