Self-reported and measured cardiorespiratory fitness similarly predict cardiovascular disease risk in young adults

We aimed to (a) examine the validity and reliability of the International FItness Scale (IFIS) in Spanish young adults and (b) compare the capacity of self-reported vs measured fitness to predict cardiovascular disease (CVD) risk. The study comprised 276 participants (18–30 years). Fitness level (overall and specific components) was both self-reported (IFIS) and measured using standard fitness tests. Total and trunk fat was assessed by dual-energy X-ray absorptiometry. We computed a previously validated metabolic syndrome score. A separate sample of 181 of same age and characteristics fulfilled IFIS twice for reliability purposes. The results of the present study support the validity and reliability of self-reported fitness, as measured by IFIS, in Spanish young adults. Our data also suggest that not only measured cardiorespiratory fitness but also self-reported cardiorespiratory fitness predicts CVD risk, as assessed by adiposity and metabolic syndrome indicators. The associations for muscular fitness (both reported and measured) differed depending on how it was expressed (i.e., absolute vs relative terms). Self-reported fitness, as assessed by IFIS, can be a good alternative when physical fitness cannot be measured in large surveys.Nuestro objetivo fue (a) examinar la validez y confiabilidad de la Escala Internacional de Fitness (IFIS) en adultos jóvenes españoles y (b) comparar la capacidad del fitness autoinformado frente al medido para predecir el riesgo de enfermedad cardiovascular (ECV). El estudio comprendió a 276 participantes (18-30 años). El nivel de condición física (componentes generales y específicos) fue autoinformado (IFIS) y medido mediante pruebas de condición física estándar. La grasa total y del tronco se evaluó mediante absorciometría de rayos X de energía dual. Calculamos una puntuación de síndrome metabólico previamente validada. Una muestra separada de 181 de la misma edad y características cumplió IFIS dos veces para propósitos de confiabilidad. Los resultados del presente estudio respaldan la validez y la fiabilidad del estado físico autoinformado, medido por IFIS, en adultos jóvenes españoles. Nuestros datos también sugieren que no solo la aptitud cardiorrespiratoria medida sino también la aptitud cardiorrespiratoria autoinformada predicen el riesgo de ECV, según lo evaluado por los indicadores de adiposidad y síndrome metabólico. Las asociaciones para la condición física muscular (tanto informadas como medidas) diferían dependiendo de cómo se expresara (es decir, términos absolutos versus relativos). El estado físico autoinformado, según lo evaluado por IFIS, puede ser una buena alternativa cuando el estado físico no se puede medir en encuestas grandes

Sex differences on the relation among gross motor competence, cognition, and academic achievement in children

An association between gross motor competence (GMC) and academic achievement (AA) has been described, but the potential mechanisms behind this association are still unknown. It is not known either whether these mechanisms are similar for boys and girls. The aim of this study was to analyse whether the association between GMC and AA is mediated by executive functions (EFs), and to investigate whether this mediation differs by sex. This cross-sectional study involved 451 children aged 8 to 10 (234 girls; mean age 9.95 ± 0.59). The Movement Assessment Battery for Children-Second Edition (MABC-2), NIH Toolbox, and grades in language and mathematics were used to test GMC, EFs, and AA, respectively. Multifactorial structural equation model (SEM) was used to evaluate a possible relation between variables, controlling for confounders. The differences by sex were examined using a multi-group SEM approach. The results showed that EFs acted as a full mediator of the relationship between GMC and AA in boys (β = 0.14, p = 0.012) but not in girls (β = 0.10, p = 0.326). These results show that the benefit of GMC on AA is mediated by EFs in boys but not in girls. Nevertheless, these conclusions should be carefully considered due to the cross-sectional nature of the studySe ha descrito una asociación entre la competencia motora gruesa (GMC) y el rendimiento académico (AA), pero aún se desconocen los posibles mecanismos detrás de esta asociación. Tampoco se sabe si estos mecanismos son similares para niños y niñas. El objetivo de este estudio fue analizar si la asociación entre GMC y AA está mediada por funciones ejecutivas (FE), e investigar si esta mediación difiere según el sexo. Este estudio transversal involucró a 451 niños de 8 a 10 años (234 niñas; edad media 9,95 ± 0,59). La batería de evaluación de movimiento para niños, segunda edición (MABC-2), NIH Toolbox y las calificaciones en lenguaje y matemáticas se utilizaron para evaluar GMC, EF y AA, respectivamente. Se utilizó el modelo de ecuaciones estructurales multifactoriales (SEM) para evaluar una posible relación entre las variables, controlando los factores de confusión. Las diferencias por sexo se examinaron utilizando un enfoque SEM multigrupo. Los resultados mostraron que los EF actuaron como un mediador completo de la relación entre GMC y AA en niños (β  = 0,14, p  = 0,012) pero no en niñas ( β  = 0,10, p  = 0,326). Estos resultados muestran que el beneficio de GMC en AA está mediado por EF en niños pero no en niñas. Sin embargo, estas conclusiones deben ser consideradas cuidadosamente debido a la naturaleza transversal del estudio

Ivra: Romanas, visigodas y bizantinas. Una experiencia de innovación docente en clave de género

La experiencia que se presenta pretende, por un lado, cubrir la necesidad de crear unos materiales docentes en los que la transversalidad, la interdisciplinariedad y las competencias de género y ciudadanía fueran su hilo conductor con la finalidad de que se pudieran utilizar en los estudios jurídicos y, en especial, en el marco de las asignaturas relacionadas con el Derecho Romano. Por otra parte, pretende ser una experiencia en innovación docente, que ha derivado en la realización de investigación científica sobre la materia. Todo ello se ha llevado a cabo por un grupo esencialmente de profesoras de carácter interuniversitario y multidisciplinar. Además, la transferencia de resultados obtenidos ha sobrepasado el ámbito universitario para llegar a la sociedad en genera

Stabilization and reversal of child obesity in Andalusia using objective anthropometric measures by socioeconomic status

Background: Childhood obesity continues to be a significant public health issue worldwide. Recent national studies in Spain show a stable picture. However, prevalence and trends differ by socio-economic status, age, and region. We present the trend in childhood excess weight prevalence, aged 8–15 years, in Andalusia from 2011-2012 to 2015–2016 by socio-economic status. Results: Overall prevalence of excess weight decreased from 42.0% in 2011–2012 to 35.4% in 2015–2016. Overweight decreased from 28.2 to 24.2% and obesity from 13.8 to 11.2%. In 2011–2012 the prevalence of excess weight in boys was 46.0%and 37.9% in girls; in 2015–2016 the difference became significant with 41% of boys with excess weight compared with 30% in girls. Conclusions: Childhood excess weight prevalence in Andalusia has decreased slightly between 2011-2012 and 2015–2016. Notably, a decrease in obesity prevalence in girls aged 8–15 years was recorded. In 2011–2012 a social gradient for excess weight prevalence across three SES indicators was observed: in 2015–2016 this gradient disappeared. Nonetheless, prevalence remains too high

Plan de formación docente de jóvenes investigadores pre- y postdoctorales del Departamento de Farmacología y Toxicología.

Los objetivos que se han alcanzado son los siguientes: 1. Teniendo en cuenta los resultados obtenidos durante el curso 2018-19 (además de los resultados obtenidos en el curso 2017-18) los participantes han alcanzado una formación por encima de lo esperado en Farmacología habiendo asistido a una media de 57% del curso en su primer año de participación (cuando lo estipulado en el Plan de Formacion Docente es del 30%). Además, han superado un 42,3% de la materia entre su primer y segundo año con una calificación media de 8,3. 2. Los jóvenes investigadores han realizado una media de 10 horas de prácticas docentes contabilizando aquellas dedicadas a la asistencia a prácticas como oyentes, el ensayo de las prácticas con tutores y la impartición misma de las sesiones de prácticas. El número de horas está muy limitado por el bajo número de horas prácticas en las asignaturas de Farmacología del Dpto. y el elevado número de jóvenes investigadores incorporados al Dpto. 3. Con todo lo anterior, los jóvenes investigadores han alcanzado la formación en competencias docentes y las horas realizadas han sido acreditadas a las respectivas autoridades de sus becas/contratos. Su participación en la docencia práctica les permitirá en el futuro solicitar un certificado de actividades docentes emitido por las autoridades académicas de la Facultad de Medicina que avalaran su experiencia docente en solicitudes de acreditación a las diferentes figuras de profesor ante la ANECA. Además, el Dpto. de Farmacología y Toxicología ha emitido informes detallados de Aptitud Docente en Farmacología reflejando su participación en el Plan de Formación Docente del Dpto. que podrán ser consideradas en solicitudes a puestos docentes en el futuro

Propuesta de mejora del Sistema Interno de Garantía de Calidad de la Facultad de Medicina

La garantía de calidad en el ámbito universitario puede considerarse como la atención sistemática, estructurada y continua a las titulaciones ofertadas. La garantía de calidad se compromete a poner en marcha los medios que aseguren y demuestren la calidad de los programas formativos que se desarrollan en cada una de las titulaciones ofrecidas por la Universidad y así cumplir con la obligación que tiene con la sociedad. El presente proyecto nace como fruto de la responsabilidad adquirida para el cumplimiento de las funciones encomendadas y, con el objetivo de seguir adoptando una estrategia de mejora continua de la calidad de la docencia y satisfacción de los colectivos implicados en el proceso de enseñanza-aprendizaje (Profesorado, Estudiantes y PAS)

<i>Gaia</i> Data Release 1. Summary of the astrometric, photometric, and survey properties

Context. At about 1000 days after the launch of Gaia we present the first Gaia data release, Gaia DR1, consisting of astrometry and photometry for over 1 billion sources brighter than magnitude 20.7. Aims. A summary of Gaia DR1 is presented along with illustrations of the scientific quality of the data, followed by a discussion of the limitations due to the preliminary nature of this release. Methods. The raw data collected by Gaia during the first 14 months of the mission have been processed by the Gaia Data Processing and Analysis Consortium (DPAC) and turned into an astrometric and photometric catalogue. Results. Gaia DR1 consists of three components: a primary astrometric data set which contains the positions, parallaxes, and mean proper motions for about 2 million of the brightest stars in common with the HIPPARCOS and Tycho-2 catalogues – a realisation of the Tycho-Gaia Astrometric Solution (TGAS) – and a secondary astrometric data set containing the positions for an additional 1.1 billion sources. The second component is the photometric data set, consisting of mean G-band magnitudes for all sources. The G-band light curves and the characteristics of ∼3000 Cepheid and RR-Lyrae stars, observed at high cadence around the south ecliptic pole, form the third component. For the primary astrometric data set the typical uncertainty is about 0.3 mas for the positions and parallaxes, and about 1 mas yr−1 for the proper motions. A systematic component of ∼0.3 mas should be added to the parallax uncertainties. For the subset of ∼94 000 HIPPARCOS stars in the primary data set, the proper motions are much more precise at about 0.06 mas yr−1. For the secondary astrometric data set, the typical uncertainty of the positions is ∼10 mas. The median uncertainties on the mean G-band magnitudes range from the mmag level to ∼0.03 mag over the magnitude range 5 to 20.7. Conclusions. Gaia DR1 is an important milestone ahead of the next Gaia data release, which will feature five-parameter astrometry for all sources. Extensive validation shows that Gaia DR1 represents a major advance in the mapping of the heavens and the availability of basic stellar data that underpin observational astrophysics. Nevertheless, the very preliminary nature of this first Gaia data release does lead to a number of important limitations to the data quality which should be carefully considered before drawing conclusions from the data

Late orogenic doming in the Eastern Betics : final exhumation of the Nevado-Filabride complex and its relation to basin genesis.

The geometry, timing, and kinematics of late orogenic extension in the Betic Cordilleras pose the problem of a decoupling of upper crustal and lower crustal deformation regimes. Perpendicular directions of extension in metamorphic domes and nearby sedimentary basins remain unexplained. This paper puts kinematic constraints on the final exhumation of the Nevado-Filabride complex, focusing on the formation of metamorphic domes and their relations with the adjacent basins. Structural fabrics and kinematic indicators below the main shear zones as well as their relations with both published changing metamorphic P-T conditions and geochronological data were studied. Our approach describes (1) a consistent top-to-the-west shear parallel to dome axes of during D2 (i.e., during decompression) with distributed ductile flow and the onset of strain localization along major shear zones, (2) further strain localization along the major shear zones under greenschist facies conditions, during D3 leading to S-C′ mylonites formation accompanied with a rock strong thickness reduction, (3) the divergence of shear direction on either limbs of domes during D3 showing the appearance of the dome geometry, and (4) a local evolution toward N-S brittle extension (D4) in the upper plate and formation of sedimentary basins. Continuous ductile to brittle top-to-the-west shear is compatible with the slab retreat hypothesis from the Miocene; the formation of domes which adds gravitational forces responsible for the final stages of exhumation is thus characterized by important kinematics changes necessary to explain coeval N-S opened basins. Later, from the upper Tortonian, a contractional event (D5) amplified the earlier domal structures forming the present north vergent folds

Gaia Data Release 1: Testing parallaxes with local Cepheids and RR Lyrae stars

Context. Parallaxes for 331 classical Cepheids, 31 Type II Cepheids, and 364 RR Lyrae stars in common between Gaia and the Hipparcos and Tycho-2 catalogues are published in Gaia Data Release 1 (DR1) as part of the Tycho-Gaia Astrometric Solution (TGAS). Aims. In order to test these first parallax measurements of the primary standard candles of the cosmological distance ladder, which involve astrometry collected by Gaia during the initial 14 months of science operation, we compared them with literature estimates and derived new period-luminosity (PL), period-Wesenheit (PW) relations for classical and Type II Cepheids and infrared PL, PL-metallicity (PLZ), and optical luminosity-metallicity (M V -[Fe/H]) relations for the RR Lyrae stars, with zero points based on TGAS. Methods. Classical Cepheids were carefully selected in order to discard known or suspected binary systems. The final sample comprises 102 fundamental mode pulsators with periods ranging from 1.68 to 51.66 days (of which 33 with σ Ω /Ω < 0.5). The Type II Cepheids include a total of 26 W Virginis and BL Herculis stars spanning the period range from 1.16 to 30.00 days (of which only 7 with σ Ω /Ω < 0.5). The RR Lyrae stars include 200 sources with pulsation period ranging from 0.27 to 0.80 days (of which 112 with σ Ω /Ω < 0.5). The new relations were computed using multi-band (V,I,J,K s ) photometry and spectroscopic metal abundances available in the literature, and by applying three alternative approaches: (i) linear least-squares fitting of the absolute magnitudes inferred from direct transformation of the TGAS parallaxes; (ii) adopting astrometry-based luminosities; and (iii) using a Bayesian fitting approach. The last two methods work in parallax space where parallaxes are used directly, thus maintaining symmetrical errors and allowing negative parallaxes to be used. The TGAS-based PL,PW,PLZ, and M V - [Fe/H] relations are discussed by comparing the distance to the Large Magellanic Cloud provided by different types of pulsating stars and alternative fitting methods. Results. Good agreement is found from direct comparison of the parallaxes of RR Lyrae stars for which both TGAS and HST measurements are available. Similarly, very good agreement is found between the TGAS values and the parallaxes inferred from the absolute magnitudes of Cepheids and RR Lyrae stars analysed with the Baade-Wesselink method. TGAS values also compare favourably with the parallaxes inferred by theoretical model fitting of the multi-band light curves for two of the three classical Cepheids and one RR Lyrae star, which were analysed with this technique in our samples. The K-band PL relations show the significant improvement of the TGAS parallaxes for Cepheids and RR Lyrae stars with respect to the Hipparcos measurements. This is particularly true for the RR Lyrae stars for which improvement in quality and statistics is impressive. Conclusions. TGAS parallaxes bring a significant added value to the previous Hipparcos estimates. The relations presented in this paper represent the first Gaia-calibrated relations and form a work-in-progress milestone report in the wait for Gaia-only parallaxes of which a first solution will become available with Gaia Data Release 2 (DR2) in 2018. © ESO, 2017

Gaia Data Release 1: Open cluster astrometry: performance, limitations, and future prospects

Context. The first Gaia Data Release contains the Tycho-Gaia Astrometric Solution (TGAS). This is a subset of about 2 million stars for which, besides the position and photometry, the proper motion and parallax are calculated using Hipparcos and Tycho-2 positions in 1991.25 as prior information.Aims. We investigate the scientific potential and limitations of the TGAS component by means of the astrometric data for open clusters.Methods. Mean cluster parallax and proper motion values are derived taking into account the error correlations within the astrometric solutions for individual stars, an estimate of the internal velocity dispersion in the cluster, and, where relevant, the effects of the depth of the cluster along the line of sight. Internal consistency of the TGAS data is assessed.Results. Values given for standard uncertainties are still inaccurate and may lead to unrealistic unit-weight standard deviations of least squares solutions for cluster parameters. Reconstructed mean cluster parallax and proper motion values are generally in very good agreement with earlier HIPPARCOS-based determination, although the Gaia mean parallax for the Pleiades is a significant exception. We have no current explanation for that discrepancy. Most clusters are observed to extend to nearly 15 pc from the cluster centre, and it will be up to future Gaia releases to establish whether those potential cluster-member stars are still dynamically bound to the clusters.Conclusions. The Gaia DR1 provides the means to examine open clusters far beyond their more easily visible cores, and can provide membership assessments based on proper motions and parallaxes. A combined HR diagram shows the same features as observed before using the HIPPARCOS data, with clearly increased luminosities for older A and F dwarfs