Adaptaciones curriculares en el área de Matemáticas para el alumnado de altas capacidades

La publicación pretende despertar el interés del alumnado de altas capacidades por las matemáticas y sus formas de razonamiento. Desarrollar su pensamiento crítico y creativo, así como proporcionar al docente apoyo para la elaboración de adaptaciones curriculares para este alumnado, proporcionando una colección de materiales en los que se abordan los diferentes contenidos de Matemáticas del segundo ciclo de E.S.O. a través de actividades más complejas que las habituales en este nivel educativo y que requieren de un mayor nivel de abstracción.AsturiasUniversidad de Oviedo. Facultad de Formación del Profesorado y Educación; Campus de Llamaquique, Calle Aniceto Sela, s. n.; 33005 Oviedo; +34985103215; +34985103214; [email protected]

Adaptaciones curriculares en el área de Matemáticas para el alumnado de altas capacidades

La publicación pretende despertar el interés del alumnado de altas capacidades por las matemáticas y sus formas de razonamiento. Desarrollar su pensamiento crítico y creativo, así como proporcionar al docente apoyo para la elaboración de adaptaciones curriculares para este alumnado, proporcionando una colección de materiales en los que se abordan los diferentes contenidos de Matemáticas del segundo ciclo de E.S.O. a través de actividades más complejas que las habituales en este nivel educativo y que requieren de un mayor nivel de abstracción.AsturiasUniversidad de Oviedo. Facultad de Formación del Profesorado y Educación; Campus de Llamaquique, Calle Aniceto Sela, s. n.; 33005 Oviedo; +34985103215; +34985103214; [email protected]

VIII Jornadas de Intercambio de Experiencias Educativas : Avilés, 16, 17 y 18 de Noviembre de 2009

Comunicaciones presentadas en las VIII Jornadas de Intercambio de Experiencias Educativas, celebradas en el Centro del Profesorado y de Recursos de Avilés en noviembre de 2009, acompañadas en cada caso de las correspondientes presentaciones y aplicaciones empleadas en la exposición y de fragmentos videográficos relativos a cada intervención. En la línea de ediciones anteriores de las Jornadas, continúan su apuesta por dar a conocer experiencias educativas de centro y de aula. La selección de experiencias se ha llevado a cabo utilizando el mismo protocolo que en años anteriores. A partir de la valoración de las memorias presentadas por la totalidad de Seminarios y Grupos de Trabajo desarrollados en este C.P.R. durante el curso escolar 2008-2009, se ha efectuado la correspondiente selección teniendo en cuenta criterios de calidad y proyección en las actividades de aula. Se han incluido en la presente edición experiencias procedente de ámbitos geográficos próximos, en función de la valía y oportunidad de la temática abordada, pudiendo diferenciarse en conjunto tres grandes temáticas: el tratamiento de la diversidad desde la dimensión de las altas capacidades, las bibliotecas escolares en distintos tipos de centros y el tratamiento de las Tecnologías de la Información y la Comunicación desde la doble perspectiva de un modelo de integración de las TIC en un centro educativo y la elaboración de aplicaciones para la pizarra digital interactiva.AsturiasUniversidad de Oviedo. Facultad de Formación del Profesorado y Educación; Campus de Llamaquique, Calle Aniceto Sela, s. n.; 33005 Oviedo; +34985103215; +34985103214; [email protected]

Chasing Gravitational Waves with the Chereknov Telescope Array

Presented at the 38th International Cosmic Ray Conference (ICRC 2023), 2023 (arXiv:2309.08219)2310.07413International audienceThe detection of gravitational waves from a binary neutron star merger by Advanced LIGO and Advanced Virgo (GW170817), along with the discovery of the electromagnetic counterparts of this gravitational wave event, ushered in a new era of multimessenger astronomy, providing the first direct evidence that BNS mergers are progenitors of short gamma-ray bursts (GRBs). Such events may also produce very-high-energy (VHE, > 100GeV) photons which have yet to be detected in coincidence with a gravitational wave signal. The Cherenkov Telescope Array (CTA) is a next-generation VHE observatory which aims to be indispensable in this search, with an unparalleled sensitivity and ability to slew anywhere on the sky within a few tens of seconds. New observing modes and follow-up strategies are being developed for CTA to rapidly cover localization areas of gravitational wave events that are typically larger than the CTA field of view. This work will evaluate and provide estimations on the expected number of of gravitational wave events that will be observable with CTA, considering both on- and off-axis emission. In addition, we will present and discuss the prospects of potential follow-up strategies with CTA

Chasing Gravitational Waves with the Chereknov Telescope Array

Presented at the 38th International Cosmic Ray Conference (ICRC 2023), 2023 (arXiv:2309.08219)2310.07413International audienceThe detection of gravitational waves from a binary neutron star merger by Advanced LIGO and Advanced Virgo (GW170817), along with the discovery of the electromagnetic counterparts of this gravitational wave event, ushered in a new era of multimessenger astronomy, providing the first direct evidence that BNS mergers are progenitors of short gamma-ray bursts (GRBs). Such events may also produce very-high-energy (VHE, > 100GeV) photons which have yet to be detected in coincidence with a gravitational wave signal. The Cherenkov Telescope Array (CTA) is a next-generation VHE observatory which aims to be indispensable in this search, with an unparalleled sensitivity and ability to slew anywhere on the sky within a few tens of seconds. New observing modes and follow-up strategies are being developed for CTA to rapidly cover localization areas of gravitational wave events that are typically larger than the CTA field of view. This work will evaluate and provide estimations on the expected number of of gravitational wave events that will be observable with CTA, considering both on- and off-axis emission. In addition, we will present and discuss the prospects of potential follow-up strategies with CTA

Performance of a proposed event-type based analysis for the Cherenkov Telescope Array

The Cherenkov Telescope Array (CTA) will be the next-generation observatory in the field of very-high-energy (20 GeV to 300 TeV) gamma-ray astroparticle physics. Classically, data analysis in the field maximizes sensitivity by applying quality cuts on the data acquired. These cuts, optimized using Monte Carlo simulations, select higher quality events from the initial dataset. Subsequent steps of the analysis typically use the surviving events to calculate one set of instrument response functions (IRFs). An alternative approach is the use of event types, as implemented in experiments such as the Fermi-LAT. In this approach, events are divided into sub-samples based on their reconstruction quality, and a set of IRFs is calculated for each sub-sample. The sub-samples are then combined in a joint analysis, treating them as independent observations. This leads to an improvement in performance parameters such as sensitivity, angular and energy resolution. Data loss is reduced since lower quality events are included in the analysis as well, rather than discarded. In this study, machine learning methods will be used to classify events according to their expected angular reconstruction quality. We will report the impact on CTA high-level performance when applying such an event-type classification, compared to the classical procedure

Chasing Gravitational Waves with the Chereknov Telescope Array

Presented at the 38th International Cosmic Ray Conference (ICRC 2023), 2023 (arXiv:2309.08219)2310.07413International audienceThe detection of gravitational waves from a binary neutron star merger by Advanced LIGO and Advanced Virgo (GW170817), along with the discovery of the electromagnetic counterparts of this gravitational wave event, ushered in a new era of multimessenger astronomy, providing the first direct evidence that BNS mergers are progenitors of short gamma-ray bursts (GRBs). Such events may also produce very-high-energy (VHE, > 100GeV) photons which have yet to be detected in coincidence with a gravitational wave signal. The Cherenkov Telescope Array (CTA) is a next-generation VHE observatory which aims to be indispensable in this search, with an unparalleled sensitivity and ability to slew anywhere on the sky within a few tens of seconds. New observing modes and follow-up strategies are being developed for CTA to rapidly cover localization areas of gravitational wave events that are typically larger than the CTA field of view. This work will evaluate and provide estimations on the expected number of of gravitational wave events that will be observable with CTA, considering both on- and off-axis emission. In addition, we will present and discuss the prospects of potential follow-up strategies with CTA