2,168 research outputs found

    Scoping review of measures of treatment burden in patients with multimorbidity: advancements and current gaps

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    Objectives: To identify, assess, and summarize the measures to assess burden of treatment in patients with multimorbidity (BoT-MMs) and their measurement properties. Study Design and Setting: MEDLINE via PubMed was searched from inception until May 2021. Independent reviewers extracted data from studies in which BoT-MMs were developed, validated, or reported as used, including an assessment of their measurement properties (e.g., validity and reliability) using the COnsensus-based Standards for the selection of health Measurement INstruments. Results: Eight BoT-MMs were identified across 72 studies. Most studies were performed in English (68%), in high-income countries (90%), without noting urban-rural settings (90%). No BoT-MMs had both sufficient content validity and internal consistency; some measurement properties were either insufficient or uncertain (e.g., responsiveness). Other frequent limitations of BoT-MMs included absent recall time, presence of floor effects, and unclear rationale for categorizing and interpreting raw scores. Conclusion: The evidence needed for use of extant BoT-MMs in patients with multimorbidity remains insufficiently developed, including that of suitability for their development, measurement properties, interpretability of scores, and use in low-resource settings. This review summarizes this evidence and identifies issues needing attention for using BoT-MMs in research and clinical practice

    Mitigating Predatory Ants Promotes Establishment of Biological Control of Arundo by Arundo Scale in the Cattle Fever Tick Quarantine Zone

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    Ant collection, identification, and control experiments were conducted to improve the establishment of the arundo scale, Rhizaspidiotus donacis, a biological control agent of Arundo donax, an invasive weed in the riparian habitats along the Rio Grande in Texas. Observational studies indicated R. donacis immatures are preyed upon by a variety of predator insects, especially ants. A survey of the principle ant species was made at sites along the Rio Grande with Arundo donax to help direct biological control strategies. We conclude that uses of ant baits can effectively control the common ant species found in these habitats and improve the establishment of R. donacis

    Satisfacao dos profissionais e da comunidade com a estrategia da saude da familia

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    OBJETIVO: Analisar as limitações e os pontos positivos da Estratégia de Saúde da Família na perspectiva dos profissionais da saúde e da comunidade. MÉTODOS: Estudo realizado entre os meses de junho e agosto de 2009, na cidade de Vespasiano, MG, localizada na região Sudeste do Brasil. Para avaliar a Estratégia de Saúde da Família (ESF), foi aplicado questionário em 77 profissionais da saúde e 293 cuidadores de crianças menores de cinco anos. Variáveis como o treinamento das equipes de saúde, acesso da comunidade aos serviços prestados pelas equipes de ESF, comunicação com os pacientes, a atenção prestada à criança e as informações de saúde passadas aos cuidadores foram alguns dos pontos de interesse da investigação. Análises de regressão logística foram utilizadas para se avaliar a significância estatística das variáveis estudadas, bem como os valores de odds ratio e intervalo de confiança. RESULTADOS: A maioria dos profissionais relatou que seus treinamentos foram insuficientes em quantidade, conteúdo e metodologia utilizada. Os cuidadores e profissionais identificaram semelhantes limitações da Estratégia de Saúde da Família (os serviços inacessíveis à comunidade, falta de treinamento e número insuficiente de profissionais) e também pontos fortes semelhantes (a comunicação entre agentes comunitários e comunidade, fornecimento de informações educacionais e foco na atenção à criança). Como recomendações para a melhoria do programa foram apontados: a necessidade de mais médicos e especialistas, treinamentos em maior quantidade e qualidade e melhoria na marcação de consultas. A satisfação dos cuidadores foi relacionada aos benefícios ofertados, como as visitas dos profissionais às casas (OR 5,8; IC95% 2,8;12,1), boa relação entre comunidade e profissionais (OR 4,8; IC95% 2,5;9,3) e foco na saúde da família (OR 4,1; IC95% 1,6;10,2). Problemas como número insuficiente de profissionais (OR 0,3; IC95% 0,2;0,6), dificuldade de acesso aos serviços prestados pela ESF (OR 0,2; IC95% 0,1;0,4) e qualidade ruim dos serviços ofertados (OR 0,3; IC95% 0,1;0,6) foram relacionados à insatisfação da comunidade com a ESF. De uma maneira geral, a maioria dos cuidadores (62%) mostraram estar satisfeitos com os serviços prestados pela ESF. CONCLUSÕES: Identificar as limitações e os pontos positivos da ESF pode gerar uma valiosa informação, que auxiliará na melhoria dessa estratégia para a atenção primária no Brasil.OBJETIVO: Analizar las limitaciones y los puntos positivos de la Estrategia de Salud de la Familia en la perspectiva de los profesionales de la salud y de la comunidad. MÉTODOS: Estudio realizado entre los meses de Junio y Agosto de 2009, en la ciudad de Vespasiano, MG, localizada en el la región sureste de Brasil. Para evaluar la Estrategia de la Salud de la Familia (ESF), se aplicó cuestionario en 77 profesionales de la salud y 293 cuidadores de niños menores de cinco años. Las Variables, entrenamiento de los grupos de salud, acceso de la comunidad a los servicios suministrados por los grupos de ESF, comunicación con los pacientes, la atención suministrada al niño y las informaciones de salud entregadas a los cuidadores, fueron algunos de los puntos de interés de la investigación. Los análisis de regresión logística se utilizaron para evaluar la significancia estadística de las variables estudiadas, así como los valores de odds ratio (OR) e intervalo de confianza (IC). RESULTADOS: La mayoría de los profesionales mencionó que sus entrenamientos fueron insuficientes en cantidad, contenido y metodología utilizada. Los cuidadores y profesionales identificaron limitaciones semejantes de la ESF (los servicios inaccesibles a la comunidad, falta de entrenamiento e insuficiente número de profesionales) y también semejantes puntos fuertes (la comunicación entre agentes comunitarios y comunidad, suministro de informaciones educativas y énfasis en la atención del niño). Como recomendaciones para mejorar el programa fueron señalados: la necesidad de más médicos y especialistas, entrenamientos en mayor cantidad y calidad y mejoría al concertar cita con médicos. La satisfacción de los cuidadores fue relacionada con los beneficios ofertados, como las visitas de los profesionales a las casas (OR 5,8; IC95% 2,8;12,1), buena relación entre comunidad y profesionales (OR 4,8; IC95% 2,5;9,3) y, énfasis en la salud de la familia (OR 4,1; IC 95% 1,6; 10,2). Problemas como insuficiente número de profesionales (OR 0,3; IC95% 0,2;0,6), dificultad en el acceso a los servicios suministrados por la ESF (OR 0,2; IC95% 0,1;0,4) y mala calidad de los servicios ofertados (OR 0,3; IC95% 0,1;0,6) se relacionaron con la insatisfacción de la comunidad con la ESF. De una forma general, la mayoría de los cuidadores (62%) mostraron estar satisfechos con los servicios suministrados por la ESF. CONCLUSIONES: Identificar las limitaciones y los puntos positivos de la ESF puede generar una información valiosa que ayudará en la mejoría de ésta estrategia de atención primaria en Brasil.OBJECTIVE: To analyze the strengths and limitations of the Family Health Strategy from the perspective of health care professionals and the community. METHODS: Between June-August 2009, in the city of Vespasiano, Minas Gerais State, Southeastern Brazil, a questionnaire was used to evaluate the Family Health Strategy (ESF) with 77 healthcare professionals and 293 caregivers of children under five. Health care professional training, community access to health care, communication with patients and delivery of health education and pediatric care were the main points of interest in the evaluation. Logistic regression analysis was used to obtain odds ratios and 95% confidence intervals as well as to assess the statistical significance of the variables studied. RESULTS: The majority of health care professionals reported their program training was insufficient in quantity, content and method of delivery. Caregivers and professionals identified similar weaknesses (services not accessible to the community, lack of healthcare professionals, poor training for professionals) and strengths (community health worker-patient communications, provision of educational information, and pediatric care). Recommendations for improvement included: more doctors and specialists, more and better training, and scheduling improvements. Caregiver satisfaction with the ESF was found to be related to perceived benefits such as community health agent household visits (OR 5.8, 95%CI 2.8;12.1), good professional-patient relationships (OR 4.8, 95%CI 2.5;9.3), and family-focused health (OR 4.1, 95%CI 1.6;10.2); and perceived problems such as lack of personnel (OR 0.3, 95%CI 0.2;0.6), difficulty with access (OR 0.2, 95%CI 0.1;0.4), and poor quality of care (OR 0.3, 95%CI 0.1;0.6). Overall, 62% of caregivers reported being generally satisfied with the ESF services. CONCLUSIONS: Identifying the limitations and strengths of the Family Health Strategy from the healthcare professional and caregiver perspective may serve to advance primary community healthcare in Brazil

    The 2HWC HAWC Observatory Gamma Ray Catalog

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    We present the first catalog of TeV gamma-ray sources realized with the recently completed High Altitude Water Cherenkov Observatory (HAWC). It is the most sensitive wide field-of-view TeV telescope currently in operation, with a 1-year survey sensitivity of ~5-10% of the flux of the Crab Nebula. With an instantaneous field of view >1.5 sr and >90% duty cycle, it continuously surveys and monitors the sky for gamma ray energies between hundreds GeV and tens of TeV. HAWC is located in Mexico at a latitude of 19 degree North and was completed in March 2015. Here, we present the 2HWC catalog, which is the result of the first source search realized with the complete HAWC detector. Realized with 507 days of data and represents the most sensitive TeV survey to date for such a large fraction of the sky. A total of 39 sources were detected, with an expected contamination of 0.5 due to background fluctuation. Out of these sources, 16 are more than one degree away from any previously reported TeV source. The source list, including the position measurement, spectrum measurement, and uncertainties, is reported. Seven of the detected sources may be associated with pulsar wind nebulae, two with supernova remnants, two with blazars, and the remaining 23 have no firm identification yet.Comment: Submitted 2017/02/09 to the Astrophysical Journa

    The Sensitivity of HAWC to High-Mass Dark Matter Annihilations

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    The High Altitude Water Cherenkov (HAWC) observatory is a wide field-of-view detector sensitive to gamma rays of 100 GeV to a few hundred TeV. Located in central Mexico at 19 degrees North latitude and 4100 m above sea level, HAWC will observe gamma rays and cosmic rays with an array of water Cherenkov detectors. The full HAWC array is scheduled to be operational in Spring 2015. In this paper, we study the HAWC sensitivity to the gamma-ray signatures of high-mass (multi- TeV) dark matter annihilation. The HAWC observatory will be sensitive to diverse searches for dark matter annihilation, including annihilation from extended dark matter sources, the diffuse gamma-ray emission from dark matter annihilation, and gamma-ray emission from non-luminous dark matter subhalos. Here we consider the HAWC sensitivity to a subset of these sources, including dwarf galaxies, the M31 galaxy, the Virgo cluster, and the Galactic center. We simulate the HAWC response to gamma rays from these sources in several well-motivated dark matter annihilation channels. If no gamma-ray excess is observed, we show the limits HAWC can place on the dark matter cross-section from these sources. In particular, in the case of dark matter annihilation into gauge bosons, HAWC will be able to detect a narrow range of dark matter masses to cross-sections below thermal. HAWC should also be sensitive to non-thermal cross-sections for masses up to nearly 1000 TeV. The constraints placed by HAWC on the dark matter cross-section from known sources should be competitive with current limits in the mass range where HAWC has similar sensitivity. HAWC can additionally explore higher dark matter masses than are currently constrained.Comment: 15 pages, 4 figures, version to be published in PR

    ALMA Observations of Asteroid 3 Juno at 60 Kilometer Resolution

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    We present Atacama Large Millimeter/submillimeter Array (ALMA) 1.3 mm continuum images of the asteroid 3 Juno obtained with an angular resolution of 0.042 arcseconds (60 km at 1.97 AU). The data were obtained over a single 4.4 hr interval, which covers 60% of the 7.2 hr rotation period, approximately centered on local transit. A sequence of ten consecutive images reveals continuous changes in the asteroid's profile and apparent shape, in good agreement with the sky projection of the three-dimensional model of the Database of Asteroid Models from Inversion Techniques. We measure a geometric mean diameter of 259pm4 km, in good agreement with past estimates from a variety of techniques and wavelengths. Due to the viewing angle and inclination of the rotational pole, the southern hemisphere dominates all of the images. The median peak brightness temperature is 215pm13 K, while the median over the whole surface is 197pm15 K. With the unprecedented resolution of ALMA, we find that the brightness temperature varies across the surface with higher values correlated to the subsolar point and afternoon areas, and lower values beyond the evening terminator. The dominance of the subsolar point is accentuated in the final four images, suggesting a reduction in the thermal inertia of the regolith at the corresponding longitudes, which are possibly correlated to the location of the putative large impact crater. These results demonstrate ALMA's potential to resolve thermal emission from the surface of main belt asteroids, and to measure accurately their position, geometric shape, rotational period, and soil characteristics.Comment: 8 pages, 3 figures, 2 tables, accepted for publication in the Astrophysical Journal Letter

    First Results from High Angular Resolution ALMA Observations Toward the HL Tau Region

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    We present Atacama Large Millimeter/submillimeter Array (ALMA) observations from the 2014 Long Baseline Campaign in dust continuum and spectral line emission from the HL Tau region. The continuum images at wavelengths of 2.9, 1.3, and 0.87 mm have unprecedented angular resolutions of 0.075 arcseconds (10 AU) to 0.025 arcseconds (3.5 AU), revealing an astonishing level of detail in the circumstellar disk surrounding the young solar analogue HL Tau, with a pattern of bright and dark rings observed at all wavelengths. By fitting ellipses to the most distinct rings, we measure precise values for the disk inclination (46.72pm0.05 degrees) and position angle (+138.02pm0.07 degrees). We obtain a high-fidelity image of the 1.0 mm spectral index (α\alpha), which ranges from α∼2.0\alpha\sim2.0 in the optically-thick central peak and two brightest rings, increasing to 2.3-3.0 in the dark rings. The dark rings are not devoid of emission, we estimate a grain emissivity index of 0.8 for the innermost dark ring and lower for subsequent dark rings, consistent with some degree of grain growth and evolution. Additional clues that the rings arise from planet formation include an increase in their central offsets with radius and the presence of numerous orbital resonances. At a resolution of 35 AU, we resolve the molecular component of the disk in HCO+ (1-0) which exhibits a pattern over LSR velocities from 2-12 km/s consistent with Keplerian motion around a ~1.3 solar mass star, although complicated by absorption at low blue-shifted velocities. We also serendipitously detect and resolve the nearby protostars XZ Tau (A/B) and LkHa358 at 2.9 mm.Comment: 11 pages, 5 figures, 2 tables, accepted for publication in the Astrophysical Journal Letter
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