National evaluation of the neighbourhood nurseries: impact report

This study assessed the impact of NNI on parental employment, use of formal childcare, and take-up of benefits and tax credits, particularly for disadvantaged groups such as lone parents, low income families and ethnic minority groups

Hierarchical Event Descriptors (HED): Semi-Structured Tagging for Real-World Events in Large-Scale EEG.

Real-world brain imaging by EEG requires accurate annotation of complex subject-environment interactions in event-rich tasks and paradigms. This paper describes the evolution of the Hierarchical Event Descriptor (HED) system for systematically describing both laboratory and real-world events. HED version 2, first described here, provides the semantic capability of describing a variety of subject and environmental states. HED descriptions can include stimulus presentation events on screen or in virtual worlds, experimental or spontaneous events occurring in the real world environment, and events experienced via one or multiple sensory modalities. Furthermore, HED 2 can distinguish between the mere presence of an object and its actual (or putative) perception by a subject. Although the HED framework has implicit ontological and linked data representations, the user-interface for HED annotation is more intuitive than traditional ontological annotation. We believe that hiding the formal representations allows for a more user-friendly interface, making consistent, detailed tagging of experimental, and real-world events possible for research users. HED is extensible while retaining the advantages of having an enforced common core vocabulary. We have developed a collection of tools to support HED tag assignment and validation; these are available at hedtags.org. A plug-in for EEGLAB (sccn.ucsd.edu/eeglab), CTAGGER, is also available to speed the process of tagging existing studies

Swift observations of GRB 060614: an anomalous burst with a well behaved afterglow

GRB 060614 is a remarkable GRB observed by Swift with puzzling properties, which challenge current progenitor models. The lack of any bright SN down to very strict limits and the vanishing spectral lags are typical of short GRBs, strikingly at odds with the long (102s) duration of this event. Here we present spectral and temporal analysis of the Swift observations. We show that the burst presents standard optical, UV and X-ray afterglows. An achromatic break is observed simultaneously in optical and X-rays, at a time consistent with the break in the R-band light curve measured by the VLT. The achromatic behaviour and the consistent post-break decay slopes make GRB 060614 one of the best examples of a jet break for a Swift burst. The optical, UV and X-rays afterglow light curves have also an earlier break at ~30 ks. In the optical, there is strong spectral evolution around this break, suggesting the passage of a break frequency through the optical/UV band. The very blue spectrum at early times and the trend in the light curves (rising at low frequencies, and decaying at higher energies) suggest this may be the injection frequency. The early X-ray light curve is well interpreted as the X-ray counterpart of the burst extended emission. Spectral analysis of BAT/XRT data in the 80s overlap time show that the Ep of the burst has decreased to as low as 8keV at the beginning of the XRT observation. The Ep continues to decrease through the XRT energy band and exits it at about 500s after the trigger. The average Ep of the burst is likely < 24 keV but larger than 8 keV. The initial peak observed by BAT is however distinctly harder than the rest with Ep ~300 keV as measured by Konus Wind. Considering the time-averaged spectral properties, GRB 060614 is consistent with the Eiso-Ep_rest, Egamma-Ep_rest, and Liso-Ep correlations.Comment: 20 pages, 9 figures, 8 tables. Abstract shortened for posting on astro-ph. Accepted for publication by A&

Discriminación del comportamiento del turismo en función de la tecnología utilizada. Comparativa entre destinos rurales y urbanos

La tecnología ha cambiado definitivamente el paradigma del turismo. En el modelo de comportamiento del turista, para cada una de las etapas que configuran el viaje, la tecnología ha influido y alterado las mismas tanto antes de la compra, durante como en los momentos posteriores del viaje. No obstante, esa tendencia a construir negocios y destinos donde prevalecen los criterios tecnológicos y la apuesta por la conectividad universal del turista debe también considerar las diferentes actitudes y necesidades de la demanda pues es posible que no todos los turistas pueden tener la exigencia de estar conectados, de ser medidos y estar presente en todas las aplicaciones disponibles. Este trabajo tiene como fin determinar desde una segmentación del mercado qué atributos, o servicios, resultan más críticas para diferenciar tipos de turistas en función de su comportamiento y uso de las TICs. Se han estudiado las diferencias entre un turismo que acude a un destino de ciudad frente a un destino rural, analizando las relaciones entre las aplicaciones tecnológicas, redes sociales… y su uso en el destino por parte del turista. Se ha podido determinar indicadores a partir de la segmentación estratégica de experiencias turísticas desde el uso y disponibilidad de las tecnologías de la información Para ello se han utilizado los datos obtenidos a través de sendos estudios realizados en el marco del proyecto CSO2014-59193-R1.Este trabajo se ha desarrollado en el marco del Proyecto de Investigación «Nuevos enfoques para la planificación y gestión del territorio turístico: conceptualización, análisis de experiencias y problemas. Definición de modelos operativos para destinos turísticos inteligentes» (Proyecto CSO2014-59193-R) del Programa Estatal de I+D+I del Ministerio de Economía y Competitividad

El mazateco de Oaxaca

El proyecto analiza la variación y el cambio en la fonología, léxico, morfología y sintaxis del mazateco que se habla en las Regiones de la Cuenca y la Cañada (Santo Domingo del Río, Xalapa de Díaz, Huautla de Jiménez y Santa María Asunción) del estado de Oaxaca de la República Mexican

Structure and Stability of an Amorphous Metal

Using molecular dynamics simulations, with a realistic many-body embedded-atom potential, and a novel method to characterize local order, we study the structure of pure nickel during the rapid quench of the liquid and in the resulting glass. In contrast with previous simulations with pair potentials, we find more crystalline order and fewer icosahedra for slower quenching rates, resulting in a glass less stable against crystallization. It is shown that there is not a specific amorphous structure, only the arrest of the transition from liquid to crystal, resulting in small crystalline clusters immersed in an amorphous matrix with the same structure of the liquid.Comment: 4 pages, 4 ps figs., to appear in Phys. Rev. Let

Discovery of a Supernova Explosion at Half the Age of the Universe and its Cosmological Implications

The ultimate fate of the universe, infinite expansion or a big crunch, can be determined by measuring the redshifts, apparent brightnesses, and intrinsic luminosities of very distant supernovae. Recent developments have provided tools that make such a program practicable: (1) Studies of relatively nearby Type Ia supernovae (SNe Ia) have shown that their intrinsic luminosities can be accurately determined; (2) New research techniques have made it possible to schedule the discovery and follow-up observations of distant supernovae, producing well over 50 very distant (z = 0.3 -- 0.7) SNe Ia to date. These distant supernovae provide a record of changes in the expansion rate over the past several billion years. By making precise measurements of supernovae at still greater distances, and thus extending this expansion history back far enough in time, we can distinguish the slowing caused by the gravitational attraction of the universe's mass density Omega_M from the effect of a possibly inflationary pressure caused by a cosmological constant Lambda. We report here the first such measurements, with our discovery of a Type Ia supernova (SN 1997ap) at z = 0.83. Measurements at the Keck II 10-m telescope make this the most distant spectroscopically confirmed supernova. Over two months of photometry of SN 1997ap with the Hubble Space Telescope and ground-based telescopes, when combined with previous measurements of nearer SNe Ia, suggests that we may live in a low mass-density universe. Further supernovae at comparable distances are currently scheduled for ground and space-based observations.Comment: 12 pages and 4 figures (figure 4 is repeated in color and black and white) Nature, scheduled for publication in the 1 January, 1998 issue. Also available at http://www-supernova.lbl.go