18 research outputs found

    Increasing significance of external quality assurance in higher education: current strategies applied by European agencies

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    [EN] Quality assurance of higher education programmes and institutions has been one of the cornerstones of the Bologna process since its creation. However, after more than one decade of implementation of the European quality assurance framework, many national systems are suffering from the so-called “evaluation fatigue”. From a thorough revision of key sectorial sources, this paper identifies a number of strategies currently being tested by European quality assurance agencies aimed at increasing significance and reducing bureaucracy of external quality assurance processes. http://ocs.editorial.upv.es/index.php/HEAD/HEAD18Sánchez Chaparro, T.; Gomez Frías, V. (2018). Increasing significance of external quality assurance in higher education: current strategies applied by European agencies. Editorial Universitat Politècnica de València. 1413-1420. https://doi.org/10.4995/HEAD18.2018.8215OCS1413142

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

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    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

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    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

    To Which World Regions Does the Valence-Dominance Model of Social Perception Apply?

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    Over the past 10 years, Oosterhof and Todorov’s valence–dominance model has emerged as the most prominent account of how people evaluate faces on social dimensions. In this model, two dimensions (valence and dominance) underpin social judgements of faces. Because this model has primarily been developed and tested in Western regions, it is unclear whether these findings apply to other regions. We addressed this question by replicating Oosterhof and Todorov’s methodology across 11 world regions, 41 countries and 11,570 participants. When we used Oosterhof and Todorov’s original analysis strategy, the valence–dominance model generalized across regions. When we used an alternative methodology to allow for correlated dimensions, we observed much less generalization. Collectively, these results suggest that, while the valence–dominance model generalizes very well across regions when dimensions are forced to be orthogonal, regional differences are revealed when we use different extraction methods and correlate and rotate the dimension reduction solution

    Nanosecond-level time synchronization of autonomous radio detector stations for extensive air showers

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

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    Prototype muon detectors for the AMIGA component of the Pierre Auger Observatory

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    Studies of Cosmic Ray Composition and Air Shower Structure with the Pierre Auger Observatory : Presentations for the 31st International Cosmic Ray Conference, Lodz , Poland, July 2009

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    Interpretation of the depths of maximum of extensive air showers measured by the Pierre Auger Observatory

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    Ultrahigh Energy Neutrinos at the Pierre Auger Observatory

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