El voluntariado de la Universidad de Sevilla en los grupos interactivos de las comunidades de aprendizaje

El objetivo de este trabajo es presentar las valoraciones que los estudiantes universitarios, que han participado como voluntarios en centros constituidos como Comunidad de Aprendizaje, hacende su experiencia en Grupos Interactivos.Para la recogida de información pedimos a los participantes que entregaran una memoria con sus valoraciones. En el análisis de dichos informes se ha utilizado una metodología cualitativa basada en análisis del contenido.Los resultados se han agrupado en cinco bloques: Para qué les ha servido colaborar en el voluntariado de grupos interactivos, cómo se han sentido durante esta colaboración, los aspectos positivos que quieren destacar de esta experiencia, los aspectos negativos de la misma y por último las propuestas de mejora que quieran formular.Finalizamos el trabajo señalando que los aspectos positivos sobrepasan con creces a los aspectos negativos y superan ampliamente sus expectativas iniciales tanto a nivel personal como profesional. Por otra parte los resultados confirman en la práctica los siete principios del aprendizaje dialógico sobre el que se sustenta este modelo de actuación educativa

una mirada desde las Ciencias de la Conducta

Este libro es el resultado de los trabajos presentados en el 1er Congreso Internacional "Convivencia y bienestar con sentido humanista para una cultura de paz"

Population-based multicase-control study in common tumors in Spain (MCC-Spain): rationale and study design

Introduction: We present the protocol of a large population-based case-control study of 5 common tumors in Spain (MCC-Spain) that evaluates environmental exposures and genetic factors. Methods: Between 2008-2013, 10,183 persons aged 20-85 years were enrolled in 23 hospitals and primary care centres in 12 Spanish provinces including 1,115 cases of a new diagnosis of prostate cancer, 1,750 of breast cancer, 2,171 of colorectal cancer, 492 of gastro-oesophageal cancer, 554 cases of chronic lymphocytic leukaemia (CLL) and 4,101 population-based controls matched by frequency to cases by age, sex and region of residence. Participation rates ranged from 57% (stomach cancer) to 87% (CLL cases) and from 30% to 77% in controls. Participants completed a face-to-face computerized interview on sociodemographic factors, environmental exposures, occupation, medication, lifestyle, and personal and family medical history. In addition, participants completed a self-administered food-frequency questionnaire and telephone interviews. Blood samples were collected from 76% of participants while saliva samples were collected in CLL cases and participants refusing blood extractions. Clinical information was recorded for cases and paraffin blocks and/or fresh tumor samples are available in most collaborating hospitals. Genotyping was done through an exome array enriched with genetic markers in specific pathways. Multiple analyses are planned to assess the association of environmental, personal and genetic risk factors for each tumor and to identify pleiotropic effects. Discussion: This study, conducted within the Spanish Consortium for Biomedical Research in Epidemiology & Public Health (CIBERESP), is a unique initiative to evaluate etiological factors for common cancers and will promote cancer research and prevention in Spain.The study was partially funded by the “Accion Transversal del Cancer”, approved on the Spanish Ministry Council on the 11th October 2007, by the Instituto de Salud Carlos III-FEDER (PI08/1770, PI08/0533, PI08/1359, PS09/00773, PS09/01286, PS09/01903, PS09/02078, PS09/01662, PI11/01403, PI11/01889, PI11/00226, PI11/01810, PI11/02213, PI12/00488, PI12/00265, PI12/01270, PI12/00715, PI12/00150), by the Fundación Marqués de Valdecilla (API 10/09), by the ICGC International Cancer Genome Consortium CLL, by the Junta de Castilla y León (LE22A10-2), by the Consejería de Salud of the Junta de Andalucía (PI-0571), by the Conselleria de Sanitat of the Generalitat Valenciana (AP 061/10), by the Recercaixa (2010ACUP 00310), by the Regional Government of the Basque Country by European Commission grants FOOD-CT- 2006-036224-HIWATE, by the Spanish Association Against Cancer (AECC) Scientific Foundation, by the The Catalan Government DURSI grant 2009SGR1489

Una perspectiva multidisciplinaria

Derivado de la necesidad de fomentar la investigación multidisciplinaria, la Facultad de Economía de la Universidad Autónoma del Estado de México llevó a cabo los días 8 y 9 de septiembre de 2016, el VIII Coloquio de Investigación intitulado “Desarrollo económico, regional y sustentable”. En este magno evento se presentaron 36 ponencias agrupadas en cinco mesas de trabajo: sectores productivos, crecimiento económico y mercado de trabajo; tecnología, innovación y organizaciones; desigualdad regional, pobreza y migración; economía financiera e internacional; y medio ambiente y sociedad. Del material expuesto en el VIII Coloquio, se eligieron 16 investigaciones, mismas que integran este libro. Los estudios presentados en cada uno de los subsiguientes capítulos fueron seleccionados de acuerdo a un proceso de rigurosidad científica, siendo sometidos a dictamen por pares ciegos a partir de la integración de un Comité Académico de expertos. Lo anterior con la finalidad de proporcionar al lector un material de investigación de calidad y solidez científica respecto a temas de trascendencia vinculados con los sectores productivos, la innovación, las organizaciones, la responsabilidad social, la desigualdad, la educación y el medioambiente.Consecuencia de la apertura de los mercados y los preceptos competitivos dictados por la globalización, se manifiesta la necesidad de vincular los diversos saberes provenientes de las ciencias naturales y sociales, con el fin de complementar el conocimiento y generar nuevas formas de visualizar el entorno. A raíz de ello, la investigación multidisciplinaria asume un papel cada vez más importante en los círculos académicos, empresariales y gubernamentales. En este marco, entra en desuso la visualización del individuo como un sujeto atomístico desvinculado del medio ambiente que le rodea. El objetivo de este libro es otorgar una visión multidisciplinaria al estudio de temas económicos incorporando visiones teóricas y empíricas procedentes de las ciencias sociales y naturales. La obra está compuesta por 16 capítulos agrupados en cuatro secciones. La primera parte, conglomera cinco capítulos en torno a los tópicos sectores productivos y crecimiento económico.Facultad de Economía. Universidad Autónoma del Estado de Méxic

Measurement of the cosmic ray spectrum above 4×10184{\times}10^{18} eV using inclined events detected with the Pierre Auger Observatory

A measurement of the cosmic-ray spectrum for energies exceeding $4{\times}10^{18}$ eV is presented, which is based on the analysis of showers with zenith angles greater than $60^{\circ}$ detected with the Pierre Auger Observatory between 1 January 2004 and 31 December 2013. The measured spectrum confirms a flux suppression at the highest energies. Above $5.3{\times}10^{18}$ eV, the "ankle", the flux can be described by a power law $E^{-\gamma}$ with index $\gamma=2.70 \pm 0.02 \,\text{(stat)} \pm 0.1\,\text{(sys)}$ followed by a smooth suppression region. For the energy ($E_\text{s}$) at which the spectral flux has fallen to one-half of its extrapolated value in the absence of suppression, we find $E_\text{s}=(5.12\pm0.25\,\text{(stat)}^{+1.0}_{-1.2}\,\text{(sys)}){\times}10^{19}$ eV.Comment: Replaced with published version. Added journal reference and DO

Energy Estimation of Cosmic Rays with the Engineering Radio Array of the Pierre Auger Observatory

The Auger Engineering Radio Array (AERA) is part of the Pierre Auger Observatory and is used to detect the radio emission of cosmic-ray air showers. These observations are compared to the data of the surface detector stations of the Observatory, which provide well-calibrated information on the cosmic-ray energies and arrival directions. The response of the radio stations in the 30 to 80 MHz regime has been thoroughly calibrated to enable the reconstruction of the incoming electric field. For the latter, the energy deposit per area is determined from the radio pulses at each observer position and is interpolated using a two-dimensional function that takes into account signal asymmetries due to interference between the geomagnetic and charge-excess emission components. The spatial integral over the signal distribution gives a direct measurement of the energy transferred from the primary cosmic ray into radio emission in the AERA frequency range. We measure 15.8 MeV of radiation energy for a 1 EeV air shower arriving perpendicularly to the geomagnetic field. This radiation energy -- corrected for geometrical effects -- is used as a cosmic-ray energy estimator. Performing an absolute energy calibration against the surface-detector information, we observe that this radio-energy estimator scales quadratically with the cosmic-ray energy as expected for coherent emission. We find an energy resolution of the radio reconstruction of 22% for the data set and 17% for a high-quality subset containing only events with at least five radio stations with signal.Comment: Replaced with published version. Added journal reference and DO

Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray Energy

We measure the energy emitted by extensive air showers in the form of radio emission in the frequency range from 30 to 80 MHz. Exploiting the accurate energy scale of the Pierre Auger Observatory, we obtain a radiation energy of 15.8 \pm 0.7 (stat) \pm 6.7 (sys) MeV for cosmic rays with an energy of 1 EeV arriving perpendicularly to a geomagnetic field of 0.24 G, scaling quadratically with the cosmic-ray energy. A comparison with predictions from state-of-the-art first-principle calculations shows agreement with our measurement. The radiation energy provides direct access to the calorimetric energy in the electromagnetic cascade of extensive air showers. Comparison with our result thus allows the direct calibration of any cosmic-ray radio detector against the well-established energy scale of the Pierre Auger Observatory.Comment: Replaced with published version. Added journal reference and DOI. Supplemental material in the ancillary file