Suchergebnisse

[ES]Partiendo de una inquietud sobre la actualidad de las comunidades evangélicas, primero en Salamanca y provincia, y también en la totalidad de Castilla y León; y de su vertiginoso crecimiento tras dos décadas de inmigración, particularmente latinoamericana, propuse profundizar en conocimientos de este colectivo y de la confluencia de sus distintas culturas cristianas. Las tensiones y conflictos creados por la oleada de inmigración latina en dichas comunidades era evidente, pero sin analizar en la literatura en profundidad. Basada en claves elementos de teoría y práctica antropológica, creamos con la asistencia de los directores de la tesis, unos instrumentos para explorar los detalles de las dinámicas vividas en el seno de las iglesias. Nuestra metodología se cimentó sobre estas columnas investigadoras, además de investigar documentalmente los pertenecientes datos estadísticos sobre la inmigración latina en CyL y su carácter religiosa, y un extenso período de observación participante con los actores del escenario, por medio de asistencia en sus cultos y rigurosas entrevistas de los responsables/pastores/ancianos/vicarios y de los mismos feligreses iberoamericanos (abarcando tanto hispano como porto-hablantes). Seguimos la recaudación de datos e información sobre experiencias de todos los sujetos con un exhaustivo análisis de los datos girando en torno a los cánones fundamentales de la ciencia antropológica. Esperábamos además crear un nuevo mapa de todas las localidades de dichas comunidades evangélico-protestantes en la comunidad autónoma, con un mínimo de datos geo-político y demográficos sobre su situación actual, y así aportando a la comunidad académica y al público en general una fotografía sincrónica del pueblo protestante en la región (Nota: utilizamos los términos "evangélico" y "protestante" intercambiablemente a pesar de entender bien las matices de su diferenciación). Antes de explorar la realidad presente de las iglesias, trazamos un esbozo histórico de la presencia protestante en la región, pasando por la Reforma luterana del siglo XVI, hasta la "Segunda Reforma" del siglo XIX, y las distintas leyes que paulatinamente brindaban amparo judicial al colectivo hasta la fecha. Luego, por medio de dos cuestionarios creamos 73 preguntas/variables que examinaron 10 áreas de pesquisas siguiendo las sub-hipótesis del proyecto, a los que 43 responsables/pastores respondieron y 58 latinoamericanos. Tras un capítulo de conclusiones antropológicas, agregamos a la tesis un directorio de las 228 iglesias de la región por provincia, también clasificadas entre las 16 distintas confesiones evangélico-protestantes existentes durante el período de investigación (unos cuatro años, 2007-11). Finalmente aportamos 70 páginas de "galería" ilustrando los lugares de culto, varios líderes y pastores y tomas de muchas de las mismas congregaciones celebrando distintas actividades. ; [EN]Based on a concern about current evangelical first communities in Salamanca , and also in the whole of Castilla y León, and its rapid growth after two decades of immigration, particularly Latin America , proposed deepening knowledge of this group and the confluence of the various Christian cultures. The tensions and conflicts created by the wave of Latino immigration in these communities was evident, but without analyzing the literature in depth. Based on key elements of anthropological theory and practice, created with the assistance of the directors of the thesis, some instruments to explore the details of the dynamics experienced within the churches. Our methodology was cemented on investigating these columns besides those belonging to investigate documented statistics on Latino immigration in CyL and religious character , and an extended period of participant observation stage with the actors , through assistance in their worship and rigorous interviews of responsible / pastors / elders / vicars and parishioners thereof Latin American ( including both Hispanic and porto- speakers). Continue collecting data and information on experiences of all subjects with a thorough analysis of the data revolve around the fundamental canons of anthropological science . Also hoped to create a new map of all locations of these evangelical Protestant communities in the autonomous community , with a minimum of geo - political and demographic data on your current situation, and thus contributing to the academic community and the general public a photograph synchronous Protestant village in the region (Note : use the " evangelical" and " Protestant " interchangeably despite fully understand the nuances of their differentiation terms). Before exploring the present reality of the churches , trace a historical sketch of the Protestant presence in the region , through the Lutheran Reformation of the sixteenth century to the " Second Reformation " of the nineteenth century , and the various laws that gradually afforded legal aid the group to date. Then , by means of two questionnaires created 73 questions / variables that examined 10 areas of investigation following the sub - project scenario , which charge 43 / 58 pastors responded and Latin . After a chapter of anthropological findings add to the view a directory of the 228 churches in the region by county , also rank among the 16 different existing evangelical Protestant denominations during the investigation period ( four years , 2007-11 ) . Finally we provide 70 pages of " gallery " illustrating places of worship leaders and pastors and several shots of many of the same congregations celebrating various activities.

ABSTRACTForecasting the outputs of dynamic systems develops a richer understanding of relevant inputs and their interrelationships than merely observing them ex post. Academic business simulations foster students' development of this critical competency, but learning outcomes can be significantly augmented with relatively simple, complementary exercises in forecasting. We introduce an in‐class forecasting exercise that is easily added to simulations or in any course where students gain from untangling the determinants of quantitative outcomes. The exercise also enhances opportunities for team‐building and spirited competition. Implementation details, evidence of effectiveness, and implications are discussed.

After reviewing the speculative and empirical literature of human interest, this study shows that the concept is multi-dimensional: Flesch's 'personalism' is only one factor among four.

We present the catalog of ∼31,500 extragalactic H i line sources detected by the completed Arecibo Legacy Fast ALFA (ALFALFA) survey out to z 6.5) detections and ones of lower quality that coincide in both position and recessional velocity with galaxies of known redshift. We review the observing technique, data reduction pipeline, and catalog construction process, focusing on details of particular relevance to understanding the catalog's compiled parameters. We further describe and make available the digital H i line spectra associated with the cataloged sources. In addition to the extragalactic H i line detections, we report nine confirmed OH megamasers (OHMs) and 10 OHM candidates at 0.16 < z < 0.22 whose OH line signals are redshifted into the ALFALFA frequency band. Because of complexities in data collection and processing associated with the use of a feed-horn array on a complex single-dish antenna in the terrestrial radio frequency interference environment, we also present a list of suggestions and caveats for consideration by users of the ALFALFA extragalactic catalog for future scientific investigations.© 2018. The American Astronomical Society. All rights reserved. ; The authors acknowledge the work of the entire ALFALFA collaboration who have contributed to the many aspects of the survey over the years. The ALFALFA team at Cornell has been supported by NSF grants AST-0607007, AST-1107390, and AST-1714828 and grants from the Brinson Foundation. Participation of the Undergraduate ALFALFA Team has been made possible by NSF grants AST-0724918, AST-0725267, AST-0725380, AST-0902211, AST-0903394, AST-1211005, AST-1637339, AST-1637271, AST-1637299, AST-1637262, and AST-1637276. EAKA is supported by the WISE research program, which is financed by the Netherlands Organisation for Scientific Research (NWO). BRK acknowledges the National Radio Astronomy Observatory (NRAO). The NRAO is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. MGJ acknowledges support from grant AYA2015-65973-C3-1-R (MINECO/FEDER, UE). We thank Dmitry Makarov for comments and suggestions on cross-identifications. This work is based on observations made with the Arecibo Observatory. The Arecibo Observatory has been operated by SRI International under a cooperative agreement with the National Science Foundation (AST-1100968) and in alliance with Ana G. Mendez-Universidad Metropolitana and the Universities Space Research Association. We thank the staff of the Arecibo Observatory, especially Phil Perillat, Ganesh Rajagopalan, Arun Venkataraman, Hector Hernandez, and the telescope operations group for their outstanding support of the ALFALFA survey program. We acknowledge the use of NASA's SkyView facility (http://skyview.gsfc.nasa.gov), located at NASA Goddard Space Flight Center, and the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. The Digitized Sky Surveys were produced at the Space Telescope Science Institute under U.S. Government grant NAG W-2166. The images of these surveys are based on photographic data obtained using the Oschin Schmidt Telescope on Palomar Mountain and the UK Schmidt Telescope. The plates were processed into the present compressed digital form with the permission of these institutions. The Second Palomar Observatory Sky Survey (POSS-II) was made by the California Institute of Technology with funds from the National Science Foundation, the National Geographic Society, the Sloan Foundation, the Samuel Oschin Foundation, and the Eastman Kodak Corporation. This research used data from the Sloan Digital Sky Survey. Funding for the SDSS and SDSS-II has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, the U.S. Department of Energy, the National Aeronautics and Space Administration, the Japanese Monbukagakusho, the Max Planck Society, and the Higher Education Funding Council for England.