Multiwavelength study of quiescent states of MrK 421 with unprecedented hard x-Ray coverage provided by NuStar in 2013

We present coordinated multiwavelength observations of the bright, nearby BL Lacertae object Mrk 421 taken in 2013 January–March, involving GASP-WEBT, Swift, NuSTAR, Fermi-LAT, MAGIC, VERITAS, and other collaborations and instruments, providing data from radio to very high energy (VHE) γ-ray bands. NuSTAR yielded previously unattainable sensitivity in the 3–79 keV range, revealing that the spectrum softens when the source is dimmer until the X-ray spectral shape saturates into a steep G » 3 power law, with no evidence for an exponential cutoff or additional hard components up "aprox" 80keV. For the first time, we observed both the synchrotron and the inverse-Compton peaks of the spectral energy distribution (SED) simultaneously shifted to frequencies below the typical quiescent state by an order of magnitude. The fractional variability as a function of photon energy shows a double-bump structure that relates to the two bumps of the broadband SED. In each bump, the variability increases with energy, which, in the framework of the synchrotron self-Compton model, implies that the electrons with higher energies are more variable. The measured multi band variability, the significant X-ray-toVHE correlation down to some of the lowest fluxes ever observed in both bands, the lack of correlation between optical/UV and X-ray flux, the low degree of polarization and its significant (random) variations, the short estimated electron cooling time, and the significantly longer variability timescale observed in the NuSTAR light curves point toward in situ electron acceleration and suggest that there are multiple compact regions contributing to the broadband emission of Mrk 421 during low-activity states.

Limits to dark matter annihilation cross-section from a combined analysis of MAGIC and Fermi-LAT observations of dwarf satellite galaxies

We present the first joint analysis of gamma-ray data from the MAGIC Cherenkov telescopes and the Fermi Large Area Telescope (LAT) to search for gamma-ray signals from dark matter annihilation in dwarf satellite galaxies. We combine 158 hours of Segue 1 observations with MAGIC with 6-year observations of 15 dwarf satellite galaxies by the Fermi-LAT. We obtain limits on the annihilation cross-section for dark matter particle masses between 10 GeV and 100 TeV – the widest mass range ever explored by a single gamma-ray analysis. These limits improve on previously published Fermi-LAT and MAGIC results by up to a factor of two at certain masses. Our new inclusive analysis approach is completely generic and can be used to perform a global, sensitivity-optimized dark matter search by combining data from present and future gamma-ray and neutrino detectors.

Diseño y validación de políticas de transmisión de datos en redes inalámbricas de sensores de bajo consumo

El envejecimiento de la poblaci on, el sobrepeso, y el aumento de enfermedades cr onicas, tales como: afecciones cardiacas, diabetes e hipertensi on, plantean nuevos retos al sistema de salud p ublica. En este contexto, las redes de sensores inal ambricas corporales (Wireless Body Area Networks (WBAN)/Wireless Body Sensor Networks (WBSN)) tienen gran potencial para revolucionar el sistema de salud ya que facilitan el seguimiento, la monitorizaci on y el diagn ostico de pacientes en casa, mejorando as su calidad de vida y reduciendo los costes asociados la asistencia sanitaria. Las redes WBAN/WBSN est an constituidas por nodos sensores que miden diferentes variables siol ogicas y cin eticas y disponen de interfaces inal ambricas de bajo coste para transmitir en tiempo real la informaci on a dispositivos en otros niveles de la red. En este tipo de redes, la transmisi on inal ambrica de datos es probablemente la tarea que presenta mayor consumo de energ a, por lo que dicho consumo debe ser reducido para maximizar su vida util. Adicionalmente, en escenarios WBAN/WBSN, el cuerpo humano juega un papel muy importante en la calidad de la comunicaci on. El cuerpo act ua como un canal de comunicaci on para la propagaci on de ondas electromagn eticas, por lo que el comportamiento de este tipo de canal representa un conjunto unico de desaf os para la transferencia able de datos...

Deep observation of the NGC1275 region with MAGIC: search of diffuse gamma-ray emission from cosmic rays in the Perseus cluster

Clusters of galaxies are expected to be reservoirs of cosmic rays (CRs) that should produce diffuse γ-ray emission due to their hadronic interactions with the intra-cluster medium. The nearby Perseus cool-core cluster, identified as the most promising target to search for such an emission, has been observed with the MAGIC telescopes at very-high energies (VHE, E ≥ 100 GeV) for a total of 253 hr from 2009 to 2014. The active nuclei of NGC 1275, the central dominant galaxy of the cluster, and IC 310, lying at about 0.6º from the centre, have been detected as point-like VHE γ-ray emitters during the first phase of this campaign. We report an updated measurement of the NGC 1275 spectrum, which is described well by a power law with a photon index Γ = 3.6 ± 0.2_(stat) ± 0.2_(syst) between 90 GeV and 1200 GeV. We do not detect any diffuse γ-ray emission from the cluster and so set stringent constraints on its CR population. To bracket the uncertainties over the CR spatial and spectral distributions, we adopt different spatial templates and power-law spectral indexes α. For α = 2.2, the CR-to-thermal pressure within the cluster virial radius is constrained to be ≤ 1 − 2%, except if CRs can propagate out of the cluster core, generating a flatter radial distribution and releasing the CR-to-thermal pressure constraint to ≤ 20%. Assuming that the observed radio mini-halo of Perseus is generated by secondary electrons from CR hadronic interactions, we can derive lower limits on the central magnetic field, B_(0), that depend on the CR distribution. For α = 2.2, B_(0) ≥ 5 − 8 µG, which is below the ∼25 µG inferred from Faraday rotation measurements, whereas for α ≤ 2.1, the hadronic interpretation of the diffuse radio emission contrasts with our γ-ray flux upper limits independently of the magnetic field strength.

Validando buenas prácticas en la docencia de Trabajo Social: en el camino de la innovación didáctica

Durante el curso pasado, la red REDITS avanzó en la identificación de diversas estrategias para mejorar la adquisición de competencias que quedaron volcadas en la memoria del proyecto desarrollado. Siguiendo con el trabajo iniciado, la red se propuso una labor de transferencia de conocimientos comparativos en prácticas docentes innovadoras para formación en competencias entre cuatro universidades españolas y una italiana. Este objetivo supone que una vez realizada una primera identificación de posibles buenas prácticas, debe realizarse su validación antes de replicarla. Una vez concluido ese trabajo se las incorporará a una Guía de buenas prácticas en didáctica de TS. Asimismo, del proceso de validación surgen debates y propuestas de análisis para supervisión y sistematización de la práctica en TS. Para este curso se seleccionaron dos buenas prácticas, la supervisión educativa y la realización de una experiencia de elaboración y edición de una revista desde criterios científicos. En la primera práctica se trabajó desde la evaluación mediante la aplicación de un cuestionario aplicado a diversas universidades con experiencia en este tipo de actividad y en el segundo caso al tratarse de una experiencia más novedosa se realizó su sistematización, recogiendo paralelamente el nivel de satisfacción del estudiantado con la práctica.