81 research outputs found

    Sexual function and quality of life of low-risk pregnant women

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    PURPOSE: To evaluate, in healthy women in the second trimester of pregnancy, a possible association between sexual function and quality of life, and between sexual function and sexual satisfaction. METHODS: This cross-sectional study involved 51 pregnant women managed at a low-risk antenatal care clinic. Sexual function was evaluated through the Sexual Quotient - Female Version (QS-F) questionnaire. Quality of life and sexual satisfaction were evaluated though the brief version of the World Health Organization Quality of Life questionnaire (WHOQOL-bref). Inclusion criteria were pregnancy between 15-26 weeks, maternal age 20 or more years, at least five years of scholling, in a relationship with a single partner for the last 6 months, having sexual intercourse with vaginal penetration in the last 15 days. We excluded women with a history of sexual violence, previous or current depression, habitual abortion or obstetric complications in the index pregnancy (premature rupture of membranes, preterm labor or hemorrhage). The χ² and Fisher exact tests were used for statistical analyses and p<0.05 was considered significant. RESULTS: Most of the participants (64.8%) obtained regular to excellent grades on the QS-F and 58.8% classified their quality of life as good. As to sexual satisfaction, 35.3 and 15.7% declared that they were satisfied and very satisfied with their sexual life, respectively. The study detected significant associations between bad to poor QS-F grades with a poor quality of life (p=0.002), and with regular to good and good to excellent QS-F grades with satisfaction or high sexual satisfaction (p<0.001). CONCLUSIONS: Sexual function is associated with quality of life and with sexual satisfaction in healthy women in the second trimester of pregnancy.OBJETIVO: Avaliar em gestantes saudáveis no segundo trimestre a associação entre função sexual e qualidade de vida, e função sexual e satisfação sexual. MÉTODOS: Estudo transversal com 51 gestantes em acompanhamento em ambulatório de pré-natal de baixo risco. A função sexual foi aferida por meio do Quociente Sexual - Versão Feminina (QS-F). A qualidade de vida e a satisfação sexual foram avaliadas pelo Instrumento Abreviado de Avaliação de Qualidade de Vida da Organização Mundial da Saúde (WHOQOL-bref). Os critérios de inclusão foram idade gestacional entre a 15ª e a 26ª semana, idade materna igual ou superior a 20 anos, mínimo de 5 anos de educação escolar, ter parceiro fixo há pelo menos 6 meses, ter tido relação sexual com penetração vaginal nos últimos 15 dias. Foram excluídas mulheres vítimas de violência sexual, com história pregressa ou atual de depressão, antecedente de aborto habitual ou complicações na gestação atual (amniorrexe prematura, trabalho de parto prematuro ou hemorragia). Para a análise dos dados foram utilizados os testes do χ² e exato de Fisher e p<0,05 foi considerado significante. A análise estatística foi realizada com o Statistical Package for the Social Sciences (SPSS). RESULTADOS: A maioria das gestantes (64,8%) obteve o QS-F de regular a excelente e 58,8% classificaram sua qualidade de vida como boa. Assinalaram que estavam satisfeitas com a vida sexual 35,3% das gestantes, e 15,7% estavam muito satisfeitas. O estudo mostrou que existe associação entre QS-F nulo a ruim com qualidade de vida ruim (p=0,002) e que QS-F regular a bom e bom a excelente estão associados com satisfação e muita satisfação sexual (p<0,001). CONCLUSÃO: A função sexual está associada à qualidade de vida e à satisfação sexual em gestantes saudáveis, no segundo trimestre da gestação.Universidade Federal de São Paulo (UNIFESP)/ Escola Paulista de Medicina Programa de Pós-graduação em ObstetríciaUniversidade Federal de São Paulo (UNIFESP) Escola Paulista de Medicina Departamento de ObstetríciaHospital Maternidade Leonor Mendes de Barros Departamento de SaúdeHospital Maternidade Leonor Mendes de BarrosUniversidade de São Paulo Faculdade de Medicina Departamento de PsiquiatriaUNIFESP/Escola Paulista de Medicina Programa de Pós-graduação em ObstetríciaUNIFESP, EPM, Depto. de ObstetríciaSciEL

    A population of gamma-ray emitting globular clusters seen with the Fermi Large Area Telescope

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    Globular clusters with their large populations of millisecond pulsars (MSPs) are believed to be potential emitters of high-energy gamma-ray emission. Our goal is to constrain the millisecond pulsar populations in globular clusters from analysis of gamma-ray observations. We use 546 days of continuous sky-survey observations obtained with the Large Area Telescope aboard the Fermi Gamma-ray Space Telescope to study the gamma-ray emission towards 13 globular clusters. Steady point-like high-energy gamma-ray emission has been significantly detected towards 8 globular clusters. Five of them (47 Tucanae, Omega Cen, NGC 6388, Terzan 5, and M 28) show hard spectral power indices (0.7<Γ<1.4)(0.7 < \Gamma <1.4) and clear evidence for an exponential cut-off in the range 1.0-2.6 GeV, which is the characteristic signature of magnetospheric emission from MSPs. Three of them (M 62, NGC 6440 and NGC 6652) also show hard spectral indices (1.0<Γ<1.7)(1.0 < \Gamma < 1.7), however the presence of an exponential cut-off can not be unambiguously established. Three of them (Omega Cen, NGC 6388, NGC 6652) have no known radio or X-ray MSPs yet still exhibit MSP spectral properties. From the observed gamma-ray luminosities, we estimate the total number of MSPs that is expected to be present in these globular clusters. We show that our estimates of the MSP population correlate with the stellar encounter rate and we estimate 2600-4700 MSPs in Galactic globular clusters, commensurate with previous estimates. The observation of high-energy gamma-ray emission from a globular cluster thus provides a reliable independent method to assess their millisecond pulsar populations that can be used to make constraints on the original neutron star X-ray binary population, essential for understanding the importance of binary systems in slowing the inevitable core collapse of globular clusters.Comment: Accepted for publication in A&A. Corresponding authors: J. Kn\"odlseder, N. Webb, B. Pancraz

    Fermi Large Area Telescope Constraints on the Gamma-ray Opacity of the Universe

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    The Extragalactic Background Light (EBL) includes photons with wavelengths from ultraviolet to infrared, which are effective at attenuating gamma rays with energy above ~10 GeV during propagation from sources at cosmological distances. This results in a redshift- and energy-dependent attenuation of the gamma-ray flux of extragalactic sources such as blazars and Gamma-Ray Bursts (GRBs). The Large Area Telescope onboard Fermi detects a sample of gamma-ray blazars with redshift up to z~3, and GRBs with redshift up to z~4.3. Using photons above 10 GeV collected by Fermi over more than one year of observations for these sources, we investigate the effect of gamma-ray flux attenuation by the EBL. We place upper limits on the gamma-ray opacity of the Universe at various energies and redshifts, and compare this with predictions from well-known EBL models. We find that an EBL intensity in the optical-ultraviolet wavelengths as great as predicted by the "baseline" model of Stecker et al. (2006) can be ruled out with high confidence.Comment: 42 pages, 12 figures, accepted version (24 Aug.2010) for publication in ApJ; Contact authors: A. Bouvier, A. Chen, S. Raino, S. Razzaque, A. Reimer, L.C. Reye

    Gamma-ray and radio properties of six pulsars detected by the fermi large area telescope

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    We report the detection of pulsed γ-rays for PSRs J0631+1036, J0659+1414, J0742-2822, J1420-6048, J1509-5850, and J1718-3825 using the Large Area Telescope on board the Fermi Gamma-ray Space Telescope (formerly known as GLAST). Although these six pulsars are diverse in terms of their spin parameters, they share an important feature: their γ-ray light curves are (at least given the current count statistics) single peaked. For two pulsars, there are hints for a double-peaked structure in the light curves. The shapes of the observed light curves of this group of pulsars are discussed in the light of models for which the emission originates from high up in the magnetosphere. The observed phases of the γ-ray light curves are, in general, consistent with those predicted by high-altitude models, although we speculate that the γ-ray emission of PSR J0659+1414, possibly featuring the softest spectrum of all Fermi pulsars coupled with a very low efficiency, arises from relatively low down in the magnetosphere. High-quality radio polarization data are available showing that all but one have a high degree of linear polarization. This allows us to place some constraints on the viewing geometry and aids the comparison of the γ-ray light curves with high-energy beam models

    Hyperoxemia and excess oxygen use in early acute respiratory distress syndrome : Insights from the LUNG SAFE study

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    Publisher Copyright: © 2020 The Author(s). Copyright: Copyright 2020 Elsevier B.V., All rights reserved.Background: Concerns exist regarding the prevalence and impact of unnecessary oxygen use in patients with acute respiratory distress syndrome (ARDS). We examined this issue in patients with ARDS enrolled in the Large observational study to UNderstand the Global impact of Severe Acute respiratory FailurE (LUNG SAFE) study. Methods: In this secondary analysis of the LUNG SAFE study, we wished to determine the prevalence and the outcomes associated with hyperoxemia on day 1, sustained hyperoxemia, and excessive oxygen use in patients with early ARDS. Patients who fulfilled criteria of ARDS on day 1 and day 2 of acute hypoxemic respiratory failure were categorized based on the presence of hyperoxemia (PaO2 > 100 mmHg) on day 1, sustained (i.e., present on day 1 and day 2) hyperoxemia, or excessive oxygen use (FIO2 ≥ 0.60 during hyperoxemia). Results: Of 2005 patients that met the inclusion criteria, 131 (6.5%) were hypoxemic (PaO2 < 55 mmHg), 607 (30%) had hyperoxemia on day 1, and 250 (12%) had sustained hyperoxemia. Excess FIO2 use occurred in 400 (66%) out of 607 patients with hyperoxemia. Excess FIO2 use decreased from day 1 to day 2 of ARDS, with most hyperoxemic patients on day 2 receiving relatively low FIO2. Multivariate analyses found no independent relationship between day 1 hyperoxemia, sustained hyperoxemia, or excess FIO2 use and adverse clinical outcomes. Mortality was 42% in patients with excess FIO2 use, compared to 39% in a propensity-matched sample of normoxemic (PaO2 55-100 mmHg) patients (P = 0.47). Conclusions: Hyperoxemia and excess oxygen use are both prevalent in early ARDS but are most often non-sustained. No relationship was found between hyperoxemia or excessive oxygen use and patient outcome in this cohort. Trial registration: LUNG-SAFE is registered with ClinicalTrials.gov, NCT02010073publishersversionPeer reviewe

    The Helicobacter pylori Genome Project : insights into H. pylori population structure from analysis of a worldwide collection of complete genomes

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    Helicobacter pylori, a dominant member of the gastric microbiota, shares co-evolutionary history with humans. This has led to the development of genetically distinct H. pylori subpopulations associated with the geographic origin of the host and with differential gastric disease risk. Here, we provide insights into H. pylori population structure as a part of the Helicobacter pylori Genome Project (HpGP), a multi-disciplinary initiative aimed at elucidating H. pylori pathogenesis and identifying new therapeutic targets. We collected 1011 well-characterized clinical strains from 50 countries and generated high-quality genome sequences. We analysed core genome diversity and population structure of the HpGP dataset and 255 worldwide reference genomes to outline the ancestral contribution to Eurasian, African, and American populations. We found evidence of substantial contribution of population hpNorthAsia and subpopulation hspUral in Northern European H. pylori. The genomes of H. pylori isolated from northern and southern Indigenous Americans differed in that bacteria isolated in northern Indigenous communities were more similar to North Asian H. pylori while the southern had higher relatedness to hpEastAsia. Notably, we also found a highly clonal yet geographically dispersed North American subpopulation, which is negative for the cag pathogenicity island, and present in 7% of sequenced US genomes. We expect the HpGP dataset and the corresponding strains to become a major asset for H. pylori genomics
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