Proyecto macro: Programa de educación física orientado desde las competencias motriz, expresivo corporal, axiológica y ciudadanas.

Para el desarrollo de esta propuesta de un modelo de articulación interinstitucional se determinaron necesidades, problemas, expectativas y posibles proyectos para que en realidad fuera fructífero el desarrollo de dicha investigación. A continuación se muestran dichos aspectos que fueron base para esta tesis de grado. Necesidades: Un docente de educación física o ampliar los tiempos de práctica pedagógica de los practicantes, Hacer un énfasis desde las clases de educación física en recreación, deporte, lúdica, violencia y los valores, Unificar los procesos de evaluación. Problemas: Tradicionalismo metodológico de los docentes y practicantes, La violencia y los problemas relacionados con la convivencia. Expectativas: La universidad debe propiciar el fortalecimiento de los procesos de articulación, Participación de los practicantes en todo el horario del colegio, Procesos de retroalimentación de los procesos de los practicantes. Además, hay un creciente interés por formar ciudadanos que se puedan desarrollar dentro de la sociedad como parte activa y positiva dela misma por eso se toma una guía titulada “formar para la ciudadanía ¡si es posible! Lo que necesitamos saber y saber hacer” dando como punto central la competencia ciudadana que es una de las competencias con más elementos integradores, que entre si forman un marco de referencia para la misma siendo estos, junto los conocimientos, las habilidades cognitivas, emocionales y comunicativas, que articuladas entre si favorecen que el niño tenga a la mano una serie de herramientas para desarrollarse dentro de su propio contexto así como en otros. Cabe añadir que lo anterior parte como medio fundamental la utilización de la escuela y el hogar como puntos focales donde se cumplen las primeras etapas del niño buscando que este se vuelva un ente participativo, democrático que pueda vivir en comunidad y que actué para el bien de la sociedad en la que vive abriendo espacios donde se impulse la solidaridad generando normas de convivencia sana

Comportamiento epidemiológico de la obesidad y factores de riesgo asociados en la población rural de Cumbe, Ecuador

Introducción: La obesidad constituye actualmente una de las más importantes pandemias a nivel mundial con importantes consecuencias personales, familiares y gubernamentales. Los datos epidemiológicos de la obesidad en poblaciones rurales de Ecuador son limitados, por lo que el objetivo de esta investigación fue evaluar la prevalencia y los factores asociados a la obesidad en individuos adultos de la parroquia rural de Cumbe, Ecuador. Materiales y métodos: Se realizó un estudio de campo, analítico, transversal con muestreo aleatorio multietápico, que incluyó a 374 individuos de ambos sexos mayores a 18 años residenciados en la parroquia rural de Cumbe, a quienes se les aplicó historia clínica completa. La obesidad se definió según los criterios de la Organización Mundial de la Salud (OMS) en normopeso, sobrepeso y obesidad. Se construyó un modelo de regresión logística multivariante para la estimación de Odds Ratios (IC95%) para factores asociados a la obesidad. Resultados: La prevalencia de sobrepeso y obesidad fue del 34,7% (n=140) y 19% (n=71). Las mujeres presentaron una mayor prevalencia de obesidad (21,8%), que los hombres (13,5%). Los factores asociados a obesidad fueron: el sexo femenino (OR=3,61; IC95%:1,38-9,47; p=0,009), el antecedente personal de diabetes mellitus tipo 2 (OR=3,54; IC95%:1,10-11,39; p=0,034), ser exfumador (OR=3,48; IC95%:1,02-11,83; p=0,045), realizar actividad física baja (OR=2,17; IC95%:1,02-4,63; p=0,043), la circunferencia abdominal elevada (OR=3,23; IC95%:1,37-7,62, p=0,007) y el antecedente de hipertensión (OR=5,44, IC95%:2,04- 14,45; p=0,001). Conclusiones: Se evidenció una baja prevalencia de obesidad similar a las reportadas en el país, pero bajas en comparación de otras latitudes. Ser mujer, exfumador, realizar actividad física baja, hipertenso, diabético o con obesidad abdominal fueron los factores asociados a obesidad, por lo que deben tomarse en cuenta al momento de realizar la prevención y promoción de la salud

Tele-entomology and tele-parasitology: A citizen science-based approach for surveillance and control of Chagas disease in Venezuela.

Chagas Disease (CD), a chronic infection caused by the Trypanosoma cruzi parasite, is a Neglected Tropical Disease endemic to Latin America. With a re-emergence in Venezuela during the past two decades, the spread of CD has proved susceptible to, and inhibitable by a digital, real-time surveillance system effectuated by Citizen Scientists in communities throughout the country. The #TraeTuChipo (#BringYourKissingBug) campaign implemented in January 2020, has served as such a strategy counting on community engagement to define the current ecological distribution of CD vectors despite the absence of a functional national surveillance program. This pilot campaign collected data through online surveys, social media platforms, and/or telephone text messages. A total of 79 triatomine bugs were reported from eighteen Venezuelan states; 67 bugs were identified as Panstrongylus geniculatus, 1 as Rhodnius pictipes, 1 as Triatoma dimidiata, and 10 as Triatoma maculata. We analyzed 8 triatomine feces samples spotted from 4 Panstrongylus geniculatus which were confirmed positive by qPCR for T. cruzi. Further molecular characterization of discrete typing units (DTUs), revealed that all samples contained TcI, the most highly diverse and broadly distributed strain of T. cruzi. Moreover, analysis of the mitochondrial 12S gene revealed Myotis keaysi, Homo sapiens, and Gallus gallus as the main triatomine feeding sources. This study highlights a novel Citizen Science approach which may help improve the surveillance systems for CD in endemic countries

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 ~ 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

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 ratio 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 redshift of z = 0.03). The extended Baryon Oscillation Spectroscopic Survey (eBOSS) is mapping the galaxy, quasar, and neutral gas distributions between redshifts 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 AGN and galaxies in X-ray clusters, and the Time Domain Spectroscopic Survey (TDSS), obtaining spectra of variable sources. All programs use the 2.5-meter Sloan Foundation Telescope at Apache Point Observatory; observations there began in Summer 2014. APOGEE-2 also operates a second near-infrared spectrograph at the 2.5-meter 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 July 2016

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 ). 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

Centro pedagógico de actividad física, lúdico-deportiva y cultural de la jornada nocturna del colegio distrital Magdalena Ortega de Nariño.

La propuesta pedagógica presentada en este documento se fundamenta con el ideal de la integración social. Con la creación de ocho espacios diferentes que fueron presentados mediante ofertas, y por elección propia de cada uno los estudiantes, que de acuerdo a sus intereses escogieron para participar en las clases se educación física. Es de esta manera como también se promueven los valores, el gusto por las actividades físicas y culturales y el afianzamiento de las relaciones interpersonales.The pedagogical proposal in this document is based on the ideal of social integration. With the creation of eight different areas were presented with offers, and by choice of each of the students according to their interests chose to participate in physical education classes. It is in this way also promotes the values, the taste for physical and cultural activities and the strengthening of interpersonal relationship

Divulgación Científica No.4

En las instituciones encargadas de adelantar proyectos de investigación, como es el caso de la universidad, debemos reflexionar sobre lo que hacemos y sus implicaciones, de tal forma que encontremos claves para propiciar, desde nuestros saberes, agentes dinamizadores que animen la discusión, el debate y la comparación. Lo anterior con el enfoque de proponer caminos y soluciones para problemas actuales que nos aquejan como individuos. Las distintas búsquedas que hacemos apuntan a contribuir a la construcción de mejores sociedades, y la investigación es una valiosa herramienta con a que contamos para lograrlo. Es necesario entender la investigación como un agente que permite y propicia cambios.In the institutions in charge of carrying out research projects, such as the university, we must reflect on what we do and its implications, in such a way that we find keys to promote, from our knowledge, dynamic agents that encourage discussion, debate and the comparison. The above with the focus of proposing paths and solutions for current problems that afflict us as individuals. The different searches that we do aim to contribute to the construction of better societies, and research is a valuable tool that we have to achieve it. It is necessary to understand research as an agent that allows and promotes changes