Jet precession in the active nucleus of M81. Ongoing VLBI monitoring

In a recent publication, we reported results of a multi-frequency VLBI campaign of observations of the Active Galactic Nucleus (AGN) in galaxy M\,81, phase-referenced to the supernova SN\,1993J. We were able to extract precise information on the relative astrometry of the AGN radio emission at different epochs and frequencies. We found strong evidence of precession in the AGN jet (i.e., a systematic evolution in the jet inclination at each frequency) coupled to changes in the overall flux density at the different frequencies. In these proceedings, we summarise the main contents of our previous publication and we report on (preliminary) new results from our follow-up VLBI observations, now phase-referenced to the young supernova SN2008iz. We also briefly discuss how these results match the picture of our previously-reported precession model.Comment: 6 pages, 3 figures. Proceedings of EVN meeting 201

La evaluación por competencias de los casos prácticos sobre Derechos Fundamentales

En este trabajo, exponemos una experiencia docente de evaluación de los casos prácticos sobre derechos fundamentales a través de diversas herramientas que permiten objetivar esta tarea mediante la parcelación de la actividad en pequeñas unidades de observación y con referencia a cada una de las competencias trabajadas como son las rúbricas, escalas de valoración, listas de control, etc. A través de ello, se consigue no sólo dar publicidad a los criterios de evaluación y asegurar la transparencia del proceso, sino además proporcionar al alumnado una guía útil que le permite conocer cuál es su progreso y mejorar en su avance, convirtiéndose así en un elemento esencial del proceso formativo del estudiante.In this piece of work, we present a teaching experience in relation to the assessment of case studies on fundamental rights through several tools which allow us to establish some objective criteria to asses this task by means of the division of that task into parcels which involve small observation units and in relation to each competence in work such as rubrics, assessment scales, control lists, etc. When doing this, we achieve not only the publishing of the assessment criteria and the openness of the process but also we provide the students with an useful guide which allows them to know their progress and to improve that progress so it becomes and essential element in the students' formative process

Nota sobre equidae de Galicia

[Resumen] Se recogen en esta nota los primeros datos numéricos sobre f6siles cuaternarios de Galicia. Si bien estos hallazgos habían sido mencionados repetidamente en la literatura existente sobre el cuaternario de Galicia, no existían, hasta el momento, más que referencias indirectas a los mismos.La rareza en el descubrimiento de restos fósiles en el registro cuaternario gallego, justifica con creces la escasez de referencias sobre la 10calizaci6n estratigráfica de estos fósiles.[Abstract] This note deals with the first numerical data about quaternary fossils in Galicia. The finds refered here was repeatedly mentioned in the literature concerning the Galicia's quaternary, but don't had, to the moment, others than indirect references to them.The scarcity in quaternary fossil data from Galicia, balance the inexistence of references concerning the stratigraphic situation of that fossil

Serendipitous discovery of the long-sought AGN in Arp 299-A

Context: The dusty nuclear regions of luminous infra-red galaxies (LIRGs) are heated by either an intense burst of massive star formation, an active galactic nucleus (AGN), or a combination of both. Disentangling the contribution of each of those putative dust-heating agents is a challenging task, and direct imaging of the innermost few pc can only be accomplished at radio wavelengths, using very high-angular resolution observations. Aims: We observed the nucleus A of the interacting starburst galaxy Arp 299, using very long baseline interferometry (VLBI) radio observations at 1.7 and 5.0 GHz. Our aim was to characterize the compact sources in the innermost few pc region of Arp 299-A, as well as to detect recently exploded core-collapse supernovae. Methods: We used the European VLBI Network (EVN) to image the 1.7 and 5.0 GHz compact radio emission of the parsec-scale structure in the nucleus of Arp 299-A with milliarcsecond resolution. Results: Our EVN observations show that one of the compact VLBI sources, A1, previously detected at 5.0 GHz, has a flat spectrum between 1.7 and 5.0 GHz and is the brightest source at both frequencies. Our 1.7 GHz EVN image shows also diffuse, low-surface brightness emission extending westwards from A1 and displays a prominent core-jet structure. Conclusions: The morphology, radio luminosity, spectral index and ratio of radio-to-X-ray emission of the A1-A5 region is consistent with a low-luminosity AGN (LLAGN), and rules out the possibility that it is a chain of young radio supernovae (RSNe) and supernova remnants (SNRs). We therefore conclude that A1-A5 is the long-sought AGN in Arp 299-A. This finding may suggest that both starburst and AGN are frequently associated phenomena in mergers.Comment: Accepted for publication in Letters to Astronomy and Astrophysics on 12 August 2010. 4 pages, 1 figur

Gaining assurance in a voter-verifiable voting system

The literature on e-voting systems has many examples of discussion of the correctness of the computer and communication algorithms of such systems, as well as discussions of their vulnerabilities. However, a gap in the literature concerns the practical need (before adoption of a specific e-voting system) for a complete case demonstrating that the system as a whole has sufficiently high probability of exhibiting the desired properties when in use in an actual election. This paper discusses the problem of producing such a case, with reference to a specific system: a version of the Prêt à Voter scheme for voter-verifiable e-voting. We show a possible organisation of a case in terms of four main requirements – accuracy, privacy, termination and ‘trustedness’– and show some of the detailed organisation that such a case should have, the diverse kinds of evidence that needs to be gathered and some of the interesting difficulties that arise

Optical detection of the radio supernova SN 2000ft in the circumnuclear region of the luminous infrared galaxy NGC 7469

SN 2000ft is detected in two independent Planetary Camera images (F547W and F814W) taken May 13, 2000, about two months before the predicted date of the explosion (July 19, 2000), based on the analysis of its radio light evolution by Alberdi and collaborators. The apparent optical magnitudes and red color of SN 2000ft indicate that it is observed through an extinction of at least A$_V$= 3.0 magnitudes. The extinction corrected lower limit to the absolute visual magnitude (M$_V$ $\leq -$ 18.0), identifies SN 2000ft as a luminous supernova in the optical, as other luminous radio supernovae before. SN 2000ft exploded in a region located at only 0.1 arcsec (i.e. 34 +/- 3 pc) west of a faint cluster (C24). No parent cluster is identified within the detection limits of the HST short exposures. The unambiguous detection of SN 2000ft in the visual shows that multi-epoch sub-arcsecond (FWHM less than 0.1 arcsec) optical imaging is also a valid tool that should be explored further to detect supernovae in the dusty (circum)nuclear regions of (U)LIRGs

El equus stenonis cocchi como indicador biostatigráfico del plio-pleistoceno en Italia y España

[Resumen] Se esquematiza la cronoestratigrafía de los principales yacimientos de Vertebrados italianos del Plio-pleistoceno, de el Villafranquiense medio al Galerino. Se estudia, desde un punto de vista evolutivo, la presencia de las distintas formas de Equus stenonis Cocchi hasta la llegada de Equus caballus Linn. La comparación de los distintos estadios evolutivos de E. stenonis y su fauna acompañante permiten la elaboración de un Cuadro sinóptico en el cual los yacimientos españoles con Equus se correlacionan con sus sincrónicos italianos sobre una base estratigráfica comparada (BONADONNA, 1982; ARIAS et all., 1982) con los principales eventos geológicos en Europa[Abstract] The chronostratigraphy of the Plio-pleistocene marnmals italian deposits from middle Villafranchian to Galerian is surnmarized. The presence of different forms of Equus stenonis Cocchi until the appearance of the first kinds of Equus caballus Linn. is studied by an evolutive point of view. The comparison among the different evolutive levels of Equus stenonis and the associated fauna allow us to build a synoptic Table in which the spanish deposits with Equus are correlate to analogous italian ones ln a stratigraphic scale yet compared (BONADONNA, 1982; ARIAS et all., 1982) to the most important geological event ln Europ

The connection between radio and high energy emission in black hole powered systems in the SKA era

Strong evidence exists for a highly significant correlation between the radio flux density and gamma-ray energy flux in blazars revealed by Fermi. However, there are central issues that need to be clarified in this field: what are the counterparts of the about 30% of gamma-ray sources that are as yet unidentified? Are they just blazars in disguise or they are something more exotic, possibly associated with dark matter? How would they fit in the radio-gamma ray connection studied so far? With their superb sensitivity, SKA1-MID and SKA1-SUR will help to resolve all of these questions. Even more, while the radio-MeV/GeV connection has been firmly established, a radio-VHE connection has been entirely elusive so far. The advent of CTA in the next few years and the expected CTA-SKA1 synergy will offer the chance to explore this connection, even more intriguing as it involves the opposite ends of the electromagnetic spectrum and the acceleration of particles up to the highest energies. We are already preparing to address these questions by exploiting data from the various SKA pathfinders and precursors. We have obtained 18 cm European VLBI Network observations of E>10 GeV sources, with a detection rate of 83%. Moreover, we are cross correlating the Fermi catalogs with the MWA commissioning survey: when faint gamma-ray sources are considered, pure positional coincidence is not significant enough for selecting counterparts and we need an additional physical criterion to pinpoint the right object. It can be radio spectral index, variability, polarization, or compactness, needing high angular resolution in SKA1-MID; timing studies can also reveal pulsars, which are often found from dedicated searches of unidentified gamma-ray sources. SKA will be the ideal instrument for investigating these characteristics in conjunction with CTA. (abridged)Comment: 12 pages, to be published in the proceedings of "Advancing Astrophysics with the Square Kilometre Array", PoS(AASKA14)15

Use of computer-aided detection (CAD) tools in screening mammography: a multidisciplinary investigation

We summarise a set of analyses and studies conducted to assess the effects of the use of a computer-aided detection (CAD) tool in breast screening. We have used an interdisciplinary approach that combines: (a) statistical analyses inspired by reliability modelling in engineering; (b) experimental studies of decisions of mammography experts using the tool, interpreted in the light of human factors psychology; and (c) ethnographic observations of the use of the tool both in trial conditions and in everyday screening practice. Our investigations have shown patterns of human behaviour and effects of computer-based advice that would not have been revealed by a standard clinical trial approach. For example, we found that the negligible measured effect of CAD could be explained by a range of effects on experts' decisions, beneficial in some cases and detrimental in others. There is some evidence of the latter effects being due to the experts using the computer tool differently from the intentions of the developers. We integrate insights from the different pieces of evidence and highlight their implications for the design, evaluation and deployment of this sort of computer tool