Perfil de resistencia bacteriana en el Hospital de los Valles en el periodo 2017-2018

Objective: The objective of this study is to describe the antibiotic resistance profiles in the most common bacteria isolated in patients of “Hospital de los Valles” in the period of 2017-2018, providing support to the medical staff of this hospital in the decision-making process during management of different types of infections..Objetivo: Describir los perfiles de resistencia antibiótica más comunes en las bacterias aisladas en cultivos de pacientes del Hospital de los Valles en el periodo de 2017-2018, de esta manera proveer apoyo a los profesionales de salud de esta institución en la toma de decisiones sobre el manejo terapéutico más apropiado para cada tipo de infección mediante el diseño de una cartilla de resistencia antibiótica..

Um estudo da empresa de vendas diretas equatoriana e seu impacto no emprego feminino adequado

The content of this paper involves a crucial phenomenon in the analysis of the labor market: the description of adequate female employment in Ecuador. The present paper examines the relationship between the behavior of the female employment rate and the evolution of some of the most critical variables of direct selling firms in Ecuador, such as sales revenue, solvency ratio, liquidity ratio, and assets return. The panel data technique of dynamic mean groups [ARDL (1,1,1)] was used to generate empirical evidence. It was found that the liquidity ratio, solvency ratio, and income of direct selling firms show an effect statistically significant on adequate female employment. However, it is considerably small, implying that the productive linkages generated by these firms do not tend to substantially impact the generation of better-quality jobs for women in Ecuador.El contenido de este trabajo aborda un fenómeno importante dentro del análisis del mercado laboral, este es el empleo adecuado femenino en Ecuador. El análisis busca indagar si existe alguna relación entre el crecimiento de la tasa de empleo adecuado femenino y la evolución de algunas de las variables más relevantes de las firmas de venta directa en Ecuador, tales como el ingreso por ventas (IV), las ratios de solvencia (RSOLV), de liquidez (RLIQ), y el rendimiento sobre los activos (ROA). Para hacer esto, se utiliza la técnica de datos de panel de grupos medios dinámicos [ARDL (1,1,1)] para generar evidencia empírica; se encuentra que la ratio de liquidez, la ratio de solvencia y el ingreso de las empresas de venta directa muestran un efecto estadísticamente significativo sobre el empleo adecuado femenino, aunque pequeño, lo que implica que los encadenamientos productivos originados por estas empresas desde el año 2010 no tienden a crear un impacto importante en la creación de empleos de mejor calidad para las mujeres en Ecuador.O conteúdo deste trabalho aborda um fenômeno importante dentro da análise do mercado de trabalho, isto é, o emprego feminino adequado no Equador. A análise busca descobrir se existe alguma relação entre o crescimento da taxa de emprego feminino adequado e a evolução de algumas das variáveis mais importantes das empresas de vendas diretas no Equador, como a receita de vendas (RV), os índices de solvência (ISOLV), liquidez (ILIQ) e rendimento sobre ativos (ROA). Para fazer isso, usando a técnica de dados em painel de grupos médios dinâmicos [ARDL (1,1,1)] para gerar evidências empíricas, verifica-se que o índice de liquidez, o índice de solvência e o lucro das empresas de vendas diretas mostram um efeito estatisticamente significativo no emprego feminino adequado, embora pequeno, o que implica que as cadeias produtivas geradas por essas empresas desde 2010 não tendem a criar um impacto significativo na geração de empregos de melhor qualidade para as mulheres no Equador

MANEJO ONCOLÓGICO Y TERAPÉUTICO EN EL HEPATOBLASTOMA

El Hepatoblastoma es el tumor hepático maligno más frecuente en la edad pediátrica. Es una neoplasia de origen embrionario que representa el 1-2% de todos los tumores infantiles. Predomina en el sexo masculino, en edades tempranas, lactantes y niños menores de 5 años de edad. Su etiología es incierta. La tasa de supervivencia a 5 años es del 70%, con resultados comparables en los recién nacidos. Puede ser asintomático en sus inicios o presentarse con una masa abdominal palpable en el cuadrante superior derecho del abdomen, dolor abdominal localizado o difuso, pérdida de peso, anorexia, náuseas y vómitos. La ictericia es infrecuente.  Este tipo de tumor puede asociarse con determinados síndromes. La realización de biopsia de la lesión tumoral, pruebas de imágenes, y marcadores tumorales como la alfafetoproteína y gonadotropina coriónica humana beta son de gran utilidad. En el momento del diagnóstico, aproximadamente el 40% de los pacientes presentan enfermedad hepática avanzada, por lo que resulta de vital importancia sospecharlo para realizar el diagnóstico oportuno y obtener un mejor pronóstico.  El tratamiento de elección de este tipo de tumor es la combinación de quimioterapia y cirugía, por la imposibilidad de ser resecados completamente. La radioterapia se reserva para tratar las metástasis pulmonares no resecables y como tratamiento paliativo en los casos de mal pronóstico

The Fourteenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the extended Baryon Oscillation Spectroscopic Survey and from the second phase of the Apache Point Observatory Galactic Evolution Experiment

The fourth generation of the Sloan Digital Sky Survey (SDSS-IV) has been in operation since July 2014. This paper describes the second data release from this phase, and the fourteenth from SDSS overall (making this, Data Release Fourteen or DR14). This release makes public data taken by SDSS-IV in its first two years of operation (July 2014-2016). Like all previous SDSS releases, DR14 is cumulative, including the most recent reductions and calibrations of all data taken by SDSS since the first phase began operations in 2000. New in DR14 is the first public release of data from the extended Baryon Oscillation Spectroscopic Survey (eBOSS); the first data from the second phase of the Apache Point Observatory (APO) Galactic Evolution Experiment (APOGEE-2), including stellar parameter estimates from an innovative data driven machine learning algorithm known as "The Cannon"; and almost twice as many data cubes from the Mapping Nearby Galaxies at APO (MaNGA) survey as were in the previous release (N = 2812 in total). This paper describes the location and format of the publicly available data from SDSS-IV surveys. We provide references to the important technical papers describing how these data have been taken (both targeting and observation details) and processed for scientific use. The SDSS website (www.sdss.org) has been updated for this release, and provides links to data downloads, as well as tutorials and examples of data use. SDSS-IV is planning to continue to collect astronomical data until 2020, and will be followed by SDSS-V.Comment: SDSS-IV collaboration alphabetical author data release paper. DR14 happened on 31st July 2017. 19 pages, 5 figures. Accepted by ApJS on 28th Nov 2017 (this is the "post-print" and "post-proofs" version; minor corrections only from v1, and most of errors found in proofs corrected

El papel de las mujeres en el Turismo y la Gastronomía: Historia, Restos y Perspectivas.

El presente trabajo es el primero de una serie que conformarán la colección Estudios de Género de la Facultad de Turismo y Gastronomía de la Universidad Autónoma del Estado de México. Este libro es un primer esfuerzo por generar conocimiento en un tema tan relevante como es el papel de la mujer en el turismo y la gastronomía. Tradicionalmente, la mujer ha desempeñado un rol preponderante en ambas especialidades, sin embargo, éste no ha sido reconocido principalmente por el predominio masculino en todas las esferas públicas, privadas y sociales. De ahí el interés por iniciar la formación de un acervo propio que distinga aquellos aspectos históricos, rurales y sociales vinculantes entre la mujer y estas disciplinas. A lo largo de estos cincos capítulos, el lector podrá descubrir una visión un tanto de corte feminista, pero a la vez reivindicativa que busca concientizar a través de la investigación la importancia del género femenino en el turismo y la gastronomía

Sloan Digital Sky Survey IV: mapping the Milky Way, nearby galaxies, and the distant universe

We describe the Sloan Digital Sky Survey IV (SDSS-IV), a project encompassing three major spectroscopic programs. The Apache Point Observatory Galactic Evolution Experiment 2 (APOGEE-2) is observing hundreds of thousands of Milky Way stars at high resolution and high signal-to-noise ratios in the near-infrared. The Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey is obtaining spatially resolved spectroscopy for thousands of nearby galaxies (median ). The extended Baryon Oscillation Spectroscopic Survey (eBOSS) is mapping the galaxy, quasar, and neutral gas distributions between and 3.5 to constrain cosmology using baryon acoustic oscillations, redshift space distortions, and the shape of the power spectrum. Within eBOSS, we are conducting two major subprograms: the SPectroscopic IDentification of eROSITA Sources (SPIDERS), investigating X-ray AGNs and galaxies in X-ray clusters, and the Time Domain Spectroscopic Survey (TDSS), obtaining spectra of variable sources. All programs use the 2.5 m Sloan Foundation Telescope at the Apache Point Observatory; observations there began in Summer 2014. APOGEE-2 also operates a second near-infrared spectrograph at the 2.5 m du Pont Telescope at Las Campanas Observatory, with observations beginning in early 2017. Observations at both facilities are scheduled to continue through 2020. In keeping with previous SDSS policy, SDSS-IV provides regularly scheduled public data releases; the first one, Data Release 13, was made available in 2016 July

Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe

We describe the Sloan Digital Sky Survey IV (SDSS-IV), a project encompassing three major spectroscopic programs. The Apache Point Observatory Galactic Evolution Experiment 2 (APOGEE-2) is observing hundreds of thousands of Milky Way stars at high resolution and high signal-to-noise ratios in the near-infrared. The Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey is obtaining spatially resolved spectroscopy for thousands of nearby galaxies (median $z\sim 0.03$). The extended Baryon Oscillation Spectroscopic Survey (eBOSS) is mapping the galaxy, quasar, and neutral gas distributions between $z\sim 0.6$ and 3.5 to constrain cosmology using baryon acoustic oscillations, redshift space distortions, and the shape of the power spectrum. Within eBOSS, we are conducting two major subprograms: the SPectroscopic IDentification of eROSITA Sources (SPIDERS), investigating X-ray AGNs and galaxies in X-ray clusters, and the Time Domain Spectroscopic Survey (TDSS), obtaining spectra of variable sources. All programs use the 2.5 m Sloan Foundation Telescope at the Apache Point Observatory; observations there began in Summer 2014. APOGEE-2 also operates a second near-infrared spectrograph at the 2.5 m du Pont Telescope at Las Campanas Observatory, with observations beginning in early 2017. Observations at both facilities are scheduled to continue through 2020. In keeping with previous SDSS policy, SDSS-IV provides regularly scheduled public data releases; the first one, Data Release 13, was made available in 2016 July

Sloan Digital Sky Survey IV : mapping the Milky Way, nearby galaxies, and the distant universe

We describe the Sloan Digital Sky Survey IV (SDSS-IV), a project encompassing three major spectroscopic programs. The Apache Point Observatory Galactic Evolution Experiment 2 (APOGEE-2) is observing hundreds of thousands of Milky Way stars at high resolution and high signal-to-noise ratios in the near-infrared. The Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey is obtaining spatially resolved spectroscopy for thousands of nearby galaxies (median z ~ 0.03). The extended Baryon Oscillation Spectroscopic Survey (eBOSS) is mapping the galaxy, quasar, and neutral gas distributions between z ~ 0.6 and 3.5 to constrain cosmology using baryon acoustic oscillations, redshift space distortions, and the shape of the power spectrum. Within eBOSS, we are conducting two major subprograms: the SPectroscopic IDentification of eROSITA Sources (SPIDERS), investigating X-ray AGNs and galaxies in X-ray clusters, and the Time Domain Spectroscopic Survey (TDSS), obtaining spectra of variable sources. All programs use the 2.5 m Sloan Foundation Telescope at the Apache Point Observatory; observations there began in Summer 2014. APOGEE-2 also operates a second near-infrared spectrograph at the 2.5 m du Pont Telescope at Las Campanas Observatory, with observations beginning in early 2017. Observations at both facilities are scheduled to continue through 2020. In keeping with previous SDSS policy, SDSS-IV provides regularly scheduled public data releases; the first one, Data Release 13, was made available in 2016 July