R-Band Imaging of Fields Around 1<z<2 Radiogalaxies

We have taken deep $R$-band images of fields around five radiogalaxies: 0956+47, 1217+36, 3C256, 3C324 and 3C294 with $1<z<2$ . 0956+47 is found to show a double nucleus. Our data on 1217+36 suggest the revision of its classification as a radiogalaxy. We found a statistically significant excess of bright ($19.5<R<22$) galaxies on scales of 2 arcmin around the radiogalaxies (which have $R \approx 21.4$) in our sample. The excess has been determined empirically to be at $\gtrsim 99.5\%$ level. It is remarkable that this excess is not present for $22<R<23.75$ galaxies within the same area, suggesting that the excess is not physically associated to the galaxies but due to intervening groups and then related to gravitational lensing.Comment: 20 pages, uuencoded compressed PostScript including tables. Figures available upon request. To appear in the March 1995 issue of The Astronomical Journa

Impact of prior accumulated work and intensity on power output in elite/international level road cyclists—a pilot study

Background. This study aimed to investigate the impact of the intensity of prior accumulated work on the decline in power output in elite/international level road cyclists, comparing the effects of prior continuous moderate intensity versus intermittent high intensity cycling.Methods. Nine elite/international level road cyclists (age 26.2 +/- 4.0 years; body mass: 66.6 +/- 5.5 kg; height: 176 +/- 0.4 cm) conducted a 12-min field test (12 min(fresh)) during two consecutive training camps. Participants then performed both a 150-min moderate intensity continuous (MIC) work bout or a 150-min high intensity intermittent (HII) race simulation in randomized order, cross-over design. After each condition a 12-min field test (12 min(fatigue)) was completed.Results. Absolute and relative 12min(fresh) power output were not significantly different between training camps (p&gt;0.05). The 12 min(fatigue) power after HII was significantly lower than 12min(fatigue) after MIC (Delta=14W; p=0.014). Participants recorded more percentage time (%Time) in heart rate (HR) zone 3 (Delta=9.2%; p=0.003) and power output band between 5.0-7.9W.kg(-1) (Delta=8.9%; p=0.002) as well as higher total work (Delta=237 kJ; p &lt;= 0.001) during HII.Conclusion. These findings reveal that the decline in power output is higher after HII compared to MIC cycling work bouts. This suggests that the quantification of total work and intensity should be used in conjunction to predict a distinctive decline in power output. Future research is required to better understand the mechanisms of endurance "durability" in elite/international level road cyclists

Seeking the Ultraviolet Ionizing Background at z~3 with the Keck Telescope

We describe the initial results of a deep long-slit emission line search for redshifted (2.7<z<4.1) Lyman-alpha. These observations are used to constrain the fluorescent Ly-alpha emission from the population of clouds whose absorption produces the higher-column-density component of the Ly-alpha forest in quasar spectra. We use the results to set an upper limit on the ultraviolet ionizing background. Our spectroscopic data obtained with the Keck II telescope at lambda/(Delta lambda FWHM)~2000 reveals no candidate Ly-alpha emission over the wavelength range of 4500-6200 Ang along a 3 arcmin slit in a 5400 s integration. Our 3 sigma upper bound on the mean intensity of the ionizing background at the Lyman limit is J(nu 0) < 2E-21 erg/s/cm**2/Hz/sr for 2.7<z<3.1 (where we are most sensitive), assuming Lyman limit systems have typical radii of 70 kpc (q_0=0.5, H_0=50 km/s/Mpc). This constraint is more than an order of magnitude more stringent than any previously published direct limit. However, it is still a factor of three above the ultraviolet background level expected due to the integrated light of known quasars at z~3. This pilot study confirms the conclusion of Gould \& Weinberg (1996) that integrations of several hours on a 10-m class telescope should be capable of measuring J(nu 0) at high redshift.Comment: 22 pages, 2 postscipt figures. Latex requires aaspp4.sty and epsf.sty (included). Accepted for publication in the Astronomical Journal (Nov 1998

A wot-based method for creating digital sentinel twins of iot devices

The data produced by sensors of IoT devices are becoming keystones for organizations to conduct critical decision-making processes. However, delivering information to these processes in real-time represents two challenges for the organizations: the first one is achieving a constant dataflow from IoT to the cloud and the second one is enabling decision-making processes to retrieve data from dataflows in real-time. This paper presents a cloud-based Web of Things method for creating digital twins of IoT devices (named sentinels).The novelty of the proposed approach is that sentinels create an abstract window for decision-making processes to: (a) find data (e.g., properties, events, and data from sensors of IoT devices) or (b) invoke functions (e.g., actions and tasks) from physical devices (PD), as well as from virtual devices (VD). In this approach, the applications and services of decision-making processes deal with sentinels instead of managing complex details associated with the PDs, VDs, and cloud computing infrastructures. A prototype based on the proposed method was implemented to conduct a case study based on a blockchain system for verifying contract violation in sensors used in product transportation logistics. The evaluation showed the effectiveness of sentinels enabling organizations to attain data from IoT sensors and the dataflows used by decision-making processes to convert these data into useful information

Educational Strategies to Promote Adherence to Treatment in Patients with Cardiovascular Disease

Introduction: Educational material is a key strategy for primary health care promotion. Purpose: To design and validate educational material adapted to the population and aimed to increase knowledge about adherence to the treatment of arterial hypertension and diabetes mellitus. Methodology: Methodological study for the design of educational material for people with diabetes mellitus and high blood pressure. For the design, content validity tests were carried out, with the participation of six experts in health education and six patients with chronic diseases. Validation was performed pursuant to the attraction, understanding, engagement, and acceptance criteria. Results: The validation confirmed that all items and criteria were above the minimal expected range. Conclusion: The design and validation of educational material provide elements that improve the education of patients about their pathologies and their adherence to treatment

Factores con mayor influencia sobre la elección de alimentos en la población española

Fundamentos: Encuesta poblacional dirigida a conocer los factores que influyen en la elección de los alimentos de la población española. Métodos: Análisis de una muestra de todo el territorio español compuesta por 1009 individuos y seleccionada por un procedimiento aleatorio multietápico. Este estudio corresponde a la participación española en un estudio europeo sobre las actitudes de la población frente a la alimentación, nutrición y salud dirigido por el Instituto Europeo de Estudios Nutricionales de Dublín. Se determinó el porcentaje de individuos que situó a alguno de los cinco factores mencionados con más frecuencia (calidad, precio, dieta sana, condicionantes españoles, sabor) entre las tres primeras influencias en la elección de alimentos. Se ajustó un modelo multivariante para identificar los factores asociados a la elección de una dieta sana como una de las tres primeras influencias en la alimentación.Resultados: El precio influía más en los individuos de mayor edad, en niveles socioeconómicos más bajos y en individuos con menor nivel educativo. Fue mayor el impacto del precio en las mujeres de la zona Norte, Noreste y Noroeste. El sexo, la distribución geográfica, la edad y el nivel educativo presentaron un efecto independiente y significativo sobre la importancia concedida por la población a la elección de una dieta sana. Conclusiones: Los resultados sugieren la necesidad de una mayor educación sobre dieta y salud especialmente en hombre jóvenes, personas con menor nivel educativo y mujeres del Noroeste del país

Determinación reciente de la colesterolemia en población adulta sana de Pamplona

RESUMEN: Objetivo: Los objetivos del estudio fueron estimar la proporción de la población adulta sana de Pamplona que había determinado recientemente su colesterolemia e identificar los factores asociados a esta determinación. Métodos: Estudio transversal con entrevista personal a 1066 habitantes de Pamplona seleccionados por muestreo de rutas aleatorias. Se estratificó la ciudad en tres áreas urbanas según el nivel socioeconómico (alto, medio, bajo). La participación fue de un 91,8%. Utilizando como variable dependiente la determinación del colesterol total en los últimos 5 años, y como variables independientes la edad, el sexo, el nivel socioeconómico y el hábito tabáquico, se calcularon las odds ratios (OR) univariantes y se ajustó un modelo de regresión logística. Resultados: El 71,2% de la muestra estudiada (IC 95%: 68,3-74,O) se había determinado el colesterol en los últimos cinco años. Los no fumadores conocían más su colesterolemia que los fumadores con una OR ajustada de 1,38 (IC 95%: 1 ,O-1,9); los hombres lo conocían más que las mujeres (OR ajustada de 1,5; IC 95% 1,l-2,O). El conocimiento era menos frecuente en el grupo de edad 30 años. La determinación de la colesterolemia se daba más en los individuos de nivel socioeconómico medio y alto (OR ajustadas 3,2; IC 95% 2,2-4,7 y 1,6; IC 95% 1,l-2,3), respectivamente. Conclusiones: La determinación reciente del colesterol era más frecuente en individuos de mayor edad y en varones. La determinación de la colesterolemia era menos frecuente en algunos grupos con peor perfil de riesgo coronario (menor nivel socioeconómico y fumadores). Estos resultados sugieren la necesidad de intervenciones para mejorar el conocimientoy control de la colesterolemia en adultos sanos

Observational constraints to boxy/peanut bulge formation time

Boxy/peanut bulges are considered to be part of the same stellar structure as bars and both could be linked through the buckling instability. The Milky Way is our closest example. The goal of this letter is determining if the mass assembly of the different components leaves an imprint in their stellar populations allowing to estimate the time of bar formation and its evolution. To this aim we use integral field spectroscopy to derive the stellar age distributions, SADs, along the bar and disc of NGC 6032. The analysis shows clearly different SADs for the different bar areas. There is an underlying old (>=12 Gyr) stellar population for the whole galaxy. The bulge shows star formation happening at all times. The inner bar structure shows stars of ages older than 6 Gyrs with a deficit of younger populations. The outer bar region presents a SAD similar to that of the disc. To interpret our results, we use a generic numerical simulation of a barred galaxy. Thus, we constrain, for the first time, the epoch of bar formation, the buckling instability period and the posterior growth from disc material. We establish that the bar of NGC 6032 is old, formed around 10 Gyr ago while the buckling phase possibly happened around 8 Gyr ago. All these results point towards bars being long-lasting even in the presence of gas.Comment: Accepted for publication in MNRAS Letter