Caracterización epidemiológica de los beneficiarios del programa nacional de asistencia ventilatoria no invasiva domiciliaria en usuarios menores de 20 años durante el período 2006-2010 en Chile.

Tesis (Licenciado en Kinesiología)RESUMEN: Chile ha tenido un gran desarrollo en el área de la pediatría en cuanto a programas de salud se trata, lo que ha permitido aumentar la sobrevida de una gran cantidad de niños, sin embargo, a su vez, esto dio paso al desarrollo de otras patologías y/o secuelas que antes no se tenían en cuenta, las que, en su mayoría, concluían en hospitalizaciones prolongadas producto de la necesidad de un soporte ventilatorio. El programa de Asistencia Ventilatoria No Invasiva AVNI, implementado en el 2006, nace al amparo de dichas necesidades, obteniendo grandes logros dentro del área de la salud tanto a nivel nacional como internacional. Para decir esto con propiedad, se necesitaba de un respaldo que avalara los resultados obtenidos por el programa, por consiguiente se analizó una base de datos facilitada por grandes autoridades de la salud de nuestro país, dicha base de datos fue construida de forma prospectiva con respecto al formulario de ingreso establecido para el programa vía online (www.avni.cl) durante el periodo 2006-2010. Desde la puesta en marcha del programa en el año 2006, hasta marzo del 2010, se registró un total de 249 usuarios, con un leve predominio del género masculino (57,8%). La mayor concentración de usuarios se encontró en la Región Metropolitana (53,41%). Las Enfermedades Neuromusculares (ENM) fueron el principal diagnóstico detectado (58,23%), y como principal comorbilidad asociada a ésta fueron las Enfermedades de la Caja Torácica (23,45% del total de ENM). Dentro de las prestaciones consideradas por el programa, el soporte BIPAP constituyó el 79,12% y se observó que la mayoría de los usuarios se encontraba en tratamiento (88,36%). Estos resultados ratifican la importancia que ha tenido el desarrollo de este programa dentro de la salud pública de nuestro país, mejorando la calidad de vida de niños y sus familias, que de otra forma no habría sido posible dado por los elevados costos de los tratamientos y la escasa accesibilidad que se tenía antes de la implementación de AVNI

The 16th data release of the sloan digital sky surveys: first release from the APOGEE-2 southern survey and full release of eBOSS spectra

Artículo escrito por un elevado número de autores, sólo se referencian el que aparece en primer lugar, los autores pertenecientes a la UAM y el nombre del grupo de colaboración, si lo hubiereThis paper documents the 16th data release (DR16) from the Sloan Digital Sky Surveys (SDSS), the fourth and penultimate from the fourth phase (SDSS-IV). This is the first release of data from the Southern Hemisphere survey of the Apache Point Observatory Galactic Evolution Experiment 2 (APOGEE-2); new data from APOGEE-2 North are also included. DR16 is also notable as the final data release for the main cosmological program of the Extended Baryon Oscillation Spectroscopic Survey (eBOSS), and all raw and reduced spectra from that project are released here. DR16 also includes all the data from the Time Domain Spectroscopic Survey and new data from the SPectroscopic IDentification of ERosita Survey programs, both of which were co-observed on eBOSS plates. DR16 has no new data from the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey (or the MaNGA Stellar Library "MaStar"). We also preview future SDSS-V operations (due to start in 2020), and summarize plans for the final SDSS-IV data release (DR17)Funding for the Sloan Digital Sky Survey IV has been provided by the Alfred P. Sloan Foundation, the U.S. Department of Energy Office of Science, and the Participating Institutions. SDSS-IV acknowledges support and resources from the Center for High-Performance Computing at the University of Uta

The 16th data release of the sloan digital sky surveys : first release from the APOGEE-2 Southern Survey and full release of eBOSS spectra

Twenty years have passed since first light for the Sloan Digital Sky Survey (SDSS). Here, we release data taken by the fourth phase of SDSS (SDSS-IV) across its first three years of operation (2014 July–2017 July). This is the third data release for SDSS-IV, and the 15th from SDSS (Data Release Fifteen; DR15). New data come from MaNGA—we release 4824 data cubes, as well as the first stellar spectra in the MaNGA Stellar Library (MaStar), the first set of survey-supported analysis products (e.g., stellar and gas kinematics, emission-line and other maps) from the MaNGA Data Analysis Pipeline, and a new data visualization and access tool we call “Marvin.” The next data release, DR16, will include new data from both APOGEE-2 and eBOSS; those surveys release no new data here, but we document updates and corrections to their data processing pipelines. The release is cumulative; it also includes the most recent reductions and calibrations of all data taken by SDSS since first light. In this paper, we describe the location and format of the data and tools and cite technical references describing how it was obtained and processed. The SDSS website (www.sdss.org) has also been updated, providing links to data downloads, tutorials, and examples of data use. Although SDSS-IV will continue to collect astronomical data until 2020, and will be followed by SDSS-V (2020–2025), we end this paper by describing plans to ensure the sustainability of the SDSS data archive for many years beyond the collection of data

Inteligencia emocional y rendimiento académico en estudiantes de nivel primaria de una institución educativa, 2023

El objetivo de la investigación fue conocer la correlación entre inteligencia emocional y rendimiento académico en estudiantes de nivel primaria de una Institución Educativa, la investigación fue de tipo fundamental, no experimental, descriptivo y no correlacional, con una muestra de 272 estudiantes. Se aplicó el cuestionario de Inteligencia Emocional Bar On Ice – NA de Ugarriza y Pajares (2005) y los registros académicos correspondientes a cada área a evaluar. Los resultados mostraron que existe relación positiva y directa entre las variables inteligencia emocional y 84 rendimiento académico (**p<0.050), del mismo modo se muestra un 88.2% de estudiantes que presentan un nivel medio de inteligencia emocional y un 54.0% presentan un nivel de logro destacado de rendimiento académico, además, también existe correlación con el componente interpersonal (**p<0.028) y con el componente manejo de estrés (**p<0.043), sin embargo, no se mostró correlación con el componente intrapersonal (**p>0.536), el componente de adaptabilidad (**p>0.369) y con el componente impresión positiva (**p>0-369). La investigación pudo concluir que existe relación entre inteligencia emocional y rendimiento académico en estudiantes de nivel primaria de una Institución Educativa, significando que, a mayor inteligencia emocional, mayor rendimiento académic

La Zona Franca de Iquique y su impacto en el trabajo informal de mujeres migrantes fronterizas

La Zona Franca de Iquique ha sido un motor sostenido de desarrollo económico en la región de Tarapacá, al norte de Chile. Desde su creación, es un espacio de tránsito de bienes y personas que conecta a Tarapacá con el Centro Oeste Sudamericano. En términos geográficos este espacio resulta ser clave para la circulación debido a su posición fronteriza. Por ello es un atractivo nicho de empleo. ¿Cuáles son las condiciones de empleo que brinda a las mujeres migrantes? A partir de entrevistas realizadas a mujeres migrantes que trabajan en el barrio industrial de la Zona Franca se concluye que la oferta de empleo en este es de tipo precario y ofrece dificultades para realizar trámites administrativos que permitan a las mujeres regularizar su condición migratoria.The Free Trade Zone of Iquique has been a sustained engine of economic development in the Tarapacá region, in northern Chile. Since its creation, it has been a transit space for goods and people that connects Tarapacá with the West Central South America. In geographic terms, this space turns out to be key for circulation due to its border position. Therefore, it is an attractive niche for employment. What are the employment conditions that it provides to migrant women? From interviews conducted with migrant women working in the industrial zone of the Free Trade Zone, it is concluded that the job offer in this area is precarious and offers difficulties to perform administrative procedures that allow women to regularize their migratory status.A Zona Franca de Iquique tem sido um motor sustentado de desenvolvimento econômico na região de Tarapacá, no norte do Chile. Desde sua criação, é um espaço de trânsito de mercadorias e pessoas que liga Tarapacá ao Centro Oeste Sul-Americano. Em termos geográficos, este espaço acaba por ser fundamental para a circulação devido à sua posição de fronteira. Portanto, é um nicho atraente para o emprego. Quais são as condições de emprego que proporciona às mulheres migrantes? A partir de entrevistas realizadas com mulheres migrantes que trabalham na zona industrial da Zona Franca, conclui-se que a oferta de trabalho nessa área é precária e oferece dificuldades para a realização de procedimentos administrativos que permitam às mulheres regularizar seu status migratório

Bioactive compounds of loquat (Eriobotrya japonica Lindl.) cv. Golden Nugget and analysis of in vitro functionality for hyperglycemia management

The loquat cultivar Golden Nugget (leaves, flowers and fruits), which has potential commercial importance in Chile, was analyzed for targeted bioactive composition (total phenolic contents: TPC, phenolic profiles and triterpenic acids) and in vitro bioactivity such as antioxidant capacity (AC) and inhibitory activity against enzymes relevant for hyperglycemia (&alpha;-amylase and &alpha;-glucosidase) and hypertension (angiotensin I-converting enzyme, ACE-I) management. Leaves and flowers had higher TPC and AC than fruits and hydroxycinnamic acid derivatives were found in all structures by HPLC. Chlorogenic acid and quercetin derivatives were detected only in leaves and flowers, which also inhibited the &alpha;-amylase and &alpha;-glucosidase enzymes, but flowers showed the highest anti-hyperglycemia activity. No inhibition of ACE-I and hyperglycemiarelevant enzymes were found in loquat fruits; additionally, TPC and AC were high at the green stage. Loquat leaves and flowers are sources of phenolic bioactives with potential for diet-based hyperglycemia management. No triterpenic acids were found in any of the loquat parts

The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data

This paper documents the seventeenth data release (DR17) from the Sloan Digital Sky Surveys; the fifth and final release from the fourth phase (SDSS-IV). DR17 contains the complete release of the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey, which reached its goal of surveying over 10,000 nearby galaxies. The complete release of the MaNGA Stellar Library accompanies this data, providing observations of almost 30,000 stars through the MaNGA instrument during bright time. DR17 also contains the complete release of the Apache Point Observatory Galactic Evolution Experiment 2 survey that publicly releases infrared spectra of over 650,000 stars. The main sample from the Extended Baryon Oscillation Spectroscopic Survey (eBOSS), as well as the subsurvey Time Domain Spectroscopic Survey data were fully released in DR16. New single-fiber optical spectroscopy released in DR17 is from the SPectroscipic IDentification of ERosita Survey subsurvey and the eBOSS-RM program. Along with the primary data sets, DR17 includes 25 new or updated value-added catalogs. This paper concludes the release of SDSS-IV survey data. SDSS continues into its fifth phase with observations already underway for the Milky Way Mapper, Local Volume Mapper, and Black Hole Mapper surveys.Fil: Abdurro'Uf, null. Academia Sinica, Institute Of Astronomy And Astrophysics; ChinaFil: Accetta, Katherine. Prynceton University, ; Estados UnidosFil: Aerts, Conny. Katholikie Universiteit Leuven; BélgicaFil: Silva Aguirre, Víctor. Aarhus University. Department of Bioscience; DinamarcaFil: Ahumada, Romina. Universidad Católica del Norte; ChileFil: Ajgaonkar, Nikhil. University of Kentucky; Estados UnidosFil: Filiz Ak, N.. Erciyes University; TurquíaFil: Alam, Shadab. University of Edinburgh; Reino UnidoFil: Allende Prieto, Carlos. Instituto de Astrofísica de Canarias, Tenerife; EspañaFil: Almeida, Andrés. University of Virginia; Estados UnidosFil: Anders, Friedrich. Leibniz-Institut fur Astrophysik Potsdam; AlemaniaFil: Anderson, Scott F.. University of Washington; Estados UnidosFil: Andrews, Brett H.. University of Pittsburgh; Estados UnidosFil: Anguiano, Borja. University of Virginia; Estados UnidosFil: Aquino Ortiz, Erik. Universidad Nacional Autónoma de México; MéxicoFil: Aragón Salamanca, Alfonso. University of Nottingham; Estados UnidosFil: Argudo Fernández, Maria. Pontificia Universidad Católica de Valparaíso; ChileFil: Ata, Metin. University of Tokyo; JapónFil: Aubert, Marie. Aix Marseille Université; FranciaFil: Avila Reese, Vladimir. Universidad Nacional Autónoma de México; MéxicoFil: Badenes, Carles. University of Pittsburgh; Estados UnidosFil: Barbá, Rodolfo. Universidad de La Serena; ChileFil: Barger, Kat. Texas Christian University; Estados UnidosFil: Barrera Ballesteros, Jorge K,. Universidad Nacional Autónoma de México; MéxicoFil: Beaton, Rachael L.. Princeton University; Estados UnidosFil: Beers, Timothy C.. University of Notre Dame; Estados UnidosFil: Belfiore, Francesco. Istituto Nazionale di Astrofisica; ItaliaFil: Bender, Chad F.. University of Arizona; Estados UnidosFil: Bernardi, Mariangela. State University of Pennsylvania; Estados UnidosFil: Bershady, Matthew A.. University of Wisconsin; Estados UnidosFil: Monachesi, Antonela. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina. Universidad de La Serena; ChileFil: Padilla, Nelson David. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentin

The Fifteenth Data Release of the Sloan Digital Sky Surveys: First Release of MaNGA-derived Quantities, Data Visualization Tools, and Stellar Library

Twenty years have passed since first light for the Sloan Digital Sky Survey (SDSS). Here, we release data taken by the fourth phase of SDSS (SDSS-IV) across its first three years of operation (2014 July–2017 July). This is the third data release for SDSS-IV, and the 15th from SDSS (Data Release Fifteen; DR15). New data come from MaNGA—we release 4824 data cubes, as well as the first stellar spectra in the MaNGA Stellar Library (MaStar), the first set of survey-supported analysis products (e.g., stellar and gas kinematics, emission-line and other maps) from the MaNGA Data Analysis Pipeline, and a new data visualization and access tool we call "Marvin." The next data release, DR16, will include new data from both APOGEE-2 and eBOSS; those surveys release no new data here, but we document updates and corrections to their data processing pipelines. The release is cumulative; it also includes the most recent reductions and calibrations of all data taken by SDSS since first light. In this paper, we describe the location and format of the data and tools and cite technical references describing how it was obtained and processed. The SDSS website (www.sdss.org) has also been updated, providing links to data downloads, tutorials, and examples of data use. Although SDSS-IV will continue to collect astronomical data until 2020, and will be followed by SDSS-V (2020–2025), we end this paper by describing plans to ensure the sustainability of the SDSS data archive for many years beyond the collection of data

The 16th Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra

This paper documents the 16th data release (DR16) from the Sloan Digital Sky Surveys (SDSS), the fourth and penultimate from the fourth phase (SDSS-IV). This is the first release of data from the Southern Hemisphere survey of the Apache Point Observatory Galactic Evolution Experiment 2 (APOGEE-2); new data from APOGEE-2 North are also included. DR16 is also notable as the final data release for the main cosmological program of the Extended Baryon Oscillation Spectroscopic Survey (eBOSS), and all raw and reduced spectra from that project are released here. DR16 also includes all the data from the Time Domain Spectroscopic Survey and new data from the SPectroscopic IDentification of ERosita Survey programs, both of which were co-observed on eBOSS plates. DR16 has no new data from the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey (or the MaNGA Stellar Library "MaStar"). We also preview future SDSS-V operations (due to start in 2020), and summarize plans for the final SDSS-IV data release (DR17)