29 research outputs found

    Body weight and risk of soft-tissue sarcoma

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    The relation between body mass (BMI) and soft-tissue sarcoma (STS) risk was evaluated in a case–control study from Northern Italy based on 217 incident STS and 1297 hospital controls. The risk of STS rose with BMI, with multivariate odds ratios of 3.49 (95% confidence interval (CI) 1.06–11.55) among men and 3.26 (95% CI 1.27–8.35) among women with a BMI >30 kg m–2 compared to those with BMI ≤ 20 kg m–2. © 1999 Cancer Research Campaig

    Euclid : I. Overview of the Euclid mission

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    The current standard model of cosmology successfully describes a variety of measurements, but the nature of its main ingredients, dark matter and dark energy, remains unknown. Euclid is a medium-class mission in the Cosmic Vision 2015–2025 programme of the European Space Agency (ESA) that will provide high-resolution optical imaging, as well as near-infrared imaging and spectroscopy, over about 14 000 deg2 of extragalactic sky. In addition to accurate weak lensing and clustering measurements that probe structure formation over half of the age of the Universe, its primary probes for cosmology, these exquisite data will enable a wide range of science. This paper provides a high-level overview of the mission, summarising the survey characteristics, the various data-processing steps, and data products. We also highlight the main science objectives and expected performance

    Euclid II. The VIS instrument

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    This paper presents the specification, design, and development of the Visible Camera (VIS) on the European Space Agency's mission. VIS is a large optical-band imager with a field of view of 0.54 deg2^2 sampled at with an array of 609 Megapixels and a spatial resolution of . It will be used to survey approximately 14 000 deg2^2 of extragalactic sky to measure the distortion of galaxies in the redshift range z=0.1z=0.1--1.5 resulting from weak gravitational lensing, one of the two principal cosmology probes leveraged by With photometric redshifts, the distribution of dark matter can be mapped in three dimensions, and the extent to which this has changed with look-back time can be used to constrain the nature of dark energy and theories of gravity. The entire VIS focal plane will be transmitted to provide the largest images of the Universe from space to date, specified to reach AB with a signal-to-noise ratio S/N in a single broad E (r+i+z)bandoverasixyearsurvey.Theparticularlychallengingaspectsoftheinstrumentarethecontrolandcalibrationofobservationalbiases,whichleadtostringentperformancerequirementsandcalibrationregimes.Withitscombinationofspatialresolution,calibrationknowledge,depth,andareacoveringmostoftheextraGalacticsky,VISwillalsoprovidealegacydatasetformanyotherfields.ThispaperdiscussestherationalebehindtheconceptionofVISanddescribestheinstrumentdesignanddevelopment,beforereportingtheprelaunchperformancederivedfromgroundcalibrationsandbriefresultsfromtheinorbitcommissioning.VISshouldreachfainterthanAB=25 band over a six-year survey. The particularly challenging aspects of the instrument are the control and calibration of observational biases, which lead to stringent performance requirements and calibration regimes. With its combination of spatial resolution, calibration knowledge, depth, and area covering most of the extra-Galactic sky, VIS will also provide a legacy data set for many other fields. This paper discusses the rationale behind the conception of VIS and describes the instrument design and development, before reporting the prelaunch performance derived from ground calibrations and brief results from the in-orbit commissioning. VIS should reach fainter than AB =25 with S/N10 S/N 10 for galaxies with a full width at half maximum of in a diameter aperture over the Wide Survey, and mABforaDeepSurveythatwillcovermorethan50degm_ AB for a Deep Survey that will cover more than 50 deg^2$. The paper also describes how the instrument works with the telescope and survey, and with the science data processing, to extract the cosmological information

    613 cases of splenic rupture without risk factors or previously diagnosed disease: a systematic review

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    Background Rupture of the spleen in the absence of trauma or previously diagnosed disease is largely ignored in the emergency literature and is often not documented as such in journals from other fields. We have conducted a systematic review of the literature to highlight the surprisingly frequent occurrence of this phenomenon and to document the diversity of diseases that can present in this fashion. Methods Systematic review of English and French language publications catalogued in Pubmed, Embase and CINAHL between 1950 and 2011. Results We found 613 cases of splenic rupture meeting the criteria above, 327 of which occurred as the presenting complaint of an underlying disease and 112 of which occurred following a medical procedure. Rupture appeared to occur spontaneously in histologically normal (but not necessarily normal size) spleens in 35 cases and after minor trauma in 23 cases. Medications were implicated in 47 cases, a splenic or adjacent anatomical abnormality in 31 cases and pregnancy or its complications in 38 cases. The most common associated diseases were infectious (n = 143), haematologic (n = 84) and non-haematologic neoplasms (n = 48). Amyloidosis (n = 24), internal trauma such as cough or vomiting (n = 17) and rheumatologic diseases (n = 10) are less frequently reported. Colonoscopy (n = 87) was the procedure reported most frequently as a cause of rupture. The anatomic abnormalities associated with rupture include splenic cysts (n = 6), infarction (n = 6) and hamartomata (n = 5). Medications associated with rupture include anticoagulants (n = 21), thrombolytics (n = 13) and recombinant G-CSF (n = 10). Other causes or associations reported very infrequently include other endoscopy, pulmonary, cardiac or abdominal surgery, hysterectomy, peliosis, empyema, remote pancreato-renal transplant, thrombosed splenic vein, hemangiomata, pancreatic pseudocysts, splenic artery aneurysm, cholesterol embolism, splenic granuloma, congenital diaphragmatic hernia, rib exostosis, pancreatitis, Gaucher's disease, Wilson's disease, pheochromocytoma, afibrinogenemia and ruptured ectopic pregnancy. Conclusions Emergency physicians should be attuned to the fact that rupture of the spleen can occur in the absence of major trauma or previously diagnosed splenic disease. The occurrence of such a rupture is likely to be the manifesting complaint of an underlying disease. Furthermore, colonoscopy should be more widely documented as a cause of splenic rupture

    Re-amputation occurrence in the diabetic population in South Wales, UK

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    The incidence of re-amputation following lower extremity amputations (LEA) among the diabetic patients referred to the Artificial Limb and Appliance Centers (ALAC) in South Wales, UK, was investigated. Manual and electronic data-gathering systems were used to extract the medical records of 473 people with various causes of LEA referred to the ALAC in South Wales during 2001–2003. The data included demographic information, causes of amputation and occurrence of various levels of re-amputation. Two hundred and five subjects with diabetes underwent 316 amputations, 44 were foot amputations and 272 major amputations on the ipsilateral and contra-lateral sides. Of the diabetic patients, 45·9% with single LEA underwent re-amputations with 22% incidence of contra-lateral LEA within 2 years. In comparison, 15% underwent re-amputations in the non diabetic dysvascular patients. Ipsilateral re-amputations occurred much earlier (average 21 weeks) compared with the contra-lateral amputations which took an average of 82 weeks following the first amputation. Nearly half of the diabetic patients with single LEA referred for rehabilitation underwent re-amputations within 2 years; out of which 22% of the patients underwent contra-lateral LEA. Although the progression of level of amputations does not follow a particular pattern, re-amputation on the contra-lateral side occurred almost four times later than that on the ipsilateral side
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