Análisis del desempeño del lenguaje en sujetos con demencia tipo alzheimer (dta)

Antecedentes: la demencia tipo Alzheimer representaun 50-70% de las enfermedadesdemenciales. Su prevalencia es del 3-5% en personasmayores de 65 años y su incidencia de 1-2% al año en la población general; se caracterizapor alteraciones progresivas en la memoria, ellenguaje, la atención, el comportamiento y la presenciade déficit visoespaciales.Objetivo: hacer un análisis descriptivo-comparativode una muestra poblacional con demenciatipo Alzheimer, en especial una descripciónfenomenológica de las alteraciones del lenguajepresentes en esa población.Métodos: como criterios de inclusión se usaron:diagnóstico de demencia tipo Alzheimer, dominanciamanual derecha, escolaridad superior aquinto de primaria y capacidad para rendir laspruebas propuestas. Se comparó el rendimientoen las subpruebas de lenguaje del examenmínimo del estado mental (MMSE); en denominacióny fluidez semántica y fonológica y seanalizó el deterioro lingüístico en dos estadiosde la demencia tipo Alzheimer.Resultados: en el estadio leve se evidenciandéficit ligeros en todas las pruebas. Sinembargolos dominios con rendimiento más bajo fueronla fluidez fonológica y semántica. En el estadiomoderado se evidenciaron diferencias en el rendimiento;las tareas de denominación, fluidez semánticay fluidez fonológica tuvieron rendimientomás bajo.Conclusiones: el lenguaje es un dominio quesuele comprometerse en la demencia tipoAlzheimer. Los resultados reflejan el deterioroprogresivo de la habilidad lingüística, manifiestoen un amplio rango de frecuencia entre el estadio leve y el moderado de la demencia.Existe un perfil similar de deterioro para losestadios leve y moderado con patrones independientesen las pruebas específicas

Measurement of the cosmic ray spectrum above 4×10184{\times}10^{18} eV using inclined events detected with the Pierre Auger Observatory

A measurement of the cosmic-ray spectrum for energies exceeding $4{\times}10^{18}$ eV is presented, which is based on the analysis of showers with zenith angles greater than $60^{\circ}$ detected with the Pierre Auger Observatory between 1 January 2004 and 31 December 2013. The measured spectrum confirms a flux suppression at the highest energies. Above $5.3{\times}10^{18}$ eV, the "ankle", the flux can be described by a power law $E^{-\gamma}$ with index $\gamma=2.70 \pm 0.02 \,\text{(stat)} \pm 0.1\,\text{(sys)}$ followed by a smooth suppression region. For the energy ($E_\text{s}$) at which the spectral flux has fallen to one-half of its extrapolated value in the absence of suppression, we find $E_\text{s}=(5.12\pm0.25\,\text{(stat)}^{+1.0}_{-1.2}\,\text{(sys)}){\times}10^{19}$ eV.Comment: Replaced with published version. Added journal reference and DO

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

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

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

Multiple star systems in the Orion nebula

This is the author accepted manuscript. The final fersion is available from EDP Sciences via the DOI in this record.This work presents an interferometric study of the massive-binary fraction in the Orion Trapezium cluster with the recently comissioned GRAVITY instrument. We observed a total of 16 stars of mainly OB spectral type. We find three previously unknown companions for θ1 Ori B, θ2 Ori B, and θ2 Ori C. We determined a separation for the previously suspected companion of NU Ori. We confirm four companions for θ1 Ori A, θ1 Ori C, θ1 Ori D, and θ2 Ori A, all with substantially improved astrometry and photometric mass estimates. We refined the orbit of the eccentric high-mass binary θ1 Ori C and we are able to derive a new orbit for θ1 Ori D. We find a system mass of 21.7 M⊙ and a period of 53 days. Together with other previously detected companions seen in spectroscopy or direct imaging, eleven of the 16 high-mass stars are multiple systems. We obtain a total number of 22 companions with separations up to 600 AU. The companion fraction of the early B and O stars in our sample is about two, significantly higher than in earlier studies of mostly OB associations. The separation distribution hints toward a bimodality. Such a bimodality has been previously found in A stars, but rarely in OB binaries, which up to this point have been assumed to be mostly compact with a tail of wider companions. We also do not find a substantial population of equal-mass binaries. The observed distribution of mass ratios declines steeply with mass, and like the direct star counts, indicates that our companions follow a standard power law initial mass function. Again, this is in contrast to earlier findings of flat mass ratio distributions in OB associations. We excluded collision as a dominant formation mechanism but find no clear preference for core accretion or competitive accretion.Marie Skłodowska-Curie Grant AgreementFCT-PortugalERC Starting Gran

The PAU survey: close galaxy pairs identification and analysis

Galaxy pairs constitute the initial building blocks of galaxy evolution, which is driven through merger events and interactions. Thus, the analysis of these systems can be valuable in understanding galaxy evolution and studying structure formation. In this work, we present a new publicly available catalogue of close galaxy pairs identified using photometric redshifts provided by the Physics of the Accelerating Universe Survey (PAUS). To efficiently detect them, we take advantage of the high-precision photo−z (σ68 < 0.02) and apply an identification algorithm previously tested using simulated data. This algorithm considers the projected distance between the galaxies (rp < 50 kpc), the projected velocity difference (ΔV < 3500 km s−1) and an isolation criterion to obtain the pair sample. We applied this technique to the total sample of galaxies provided by PAUS and to a subset with high-quality redshift estimates. Finally, the most relevant result we achieved was determining the mean mass for several subsets of galaxy pairs selected according to their total luminosity, colour, and redshift, using galaxy–galaxy lensing estimates. For pairs selected from the total sample of PAUS with a mean r-band luminosity 1010.6 h−2 L⊙, we obtain a mean mass of M200 = 1012.2 h−1 M⊙, compatible with the mass–luminosity ratio derived for elliptical galaxies. We also study the mass-to-light ratio M/L as a function of the luminosity L and find a lower M/L (or steeper slope with L) for pairs than the one extrapolated from the measurements in groups and galaxy clusters.The PAU Survey is partially supported by MINECO under grants CSD2007-00060, AYA2015-71825, ESP2017-89838, PGC2018-094773, PGC2018-102021, PID2019-111317GB, SEV-2016-0588, SEV-2016-0597,MDM-2015-0509 and Juan de la Cierva fellowship and LACEGAL and EWC Marie Sklodowska-Curie grant numbers 734374 and 776247 with ERDF funds from the EU Horizon 2020 Programme, some of which include ERDF funds from the European Union. IEEC and IFAE are partially funded by the CERCA and Beatriu de Pinos program of the Generalitat de Catalunya. Funding for PAUS has also been provided by Durham University (via the ERC StG DEGAS-259586), ETH Zurich, Leiden University (via ERC StG ADULT-279396 and Netherlands Organisation for Scientific Research (NWO) Vici grant 639.043.512), University College London and from the European Union’s Horizon 2020 research and innovation programme under the grant agreement number 776247 EWC. This project has received funding from the European Union’s Horizon 2020 Research and Innovation Programme under the Marie Sklodowska-Curie grant agreement number 734374. This work was also partially supported by the Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET, Argentina) and the Secretaría de Ciencia y Tecnología de la Universidad Nacional de Córdoba (SeCyT-UNC, Argentina). This work has been also partially supported by the Polish National Agency for Academic Exchange (Bekker grant BPN/BEK/2021/1/00298/DEC/1), the European Union’s Horizon 2020 Research and Innovation programme under the Marie Sklodowska-Curie grant agreement (number 754510). H. Hildebrandt is supported by a Heisenberg grant of the Deutsche Forschungsgemeinschaft (Hi 1495/5-1) as well as an ERC consolidator grant (number 770935). A. Wittje is supported by the DFG (SFB 1491).Peer reviewe

Análisis del desempeño del lenguaje en sujetos con demencia tipo Alzheimer (DTA)

Antecedentes: la demencia tipo Alzheimer representa un 50-70% de las enfermedades demenciales. Su prevalencia es del 3-5% en personas mayores de 65 años y su incidencia de 1- 2% al año en la población general; se caracteriza por alteraciones progresivas en la memoria, el lenguaje, la atención, el comportamiento y la presencia de déficit visoespaciales. Objetivo: hacer un análisis descriptivo-comparativo de una muestra poblacional con demencia tipo Alzheimer, en especial una descripción fenomenológica de las alteraciones del lenguaje presentes en esa población. Métodos: como criterios de inclusión se usaron: diagnóstico de demencia tipo Alzheimer, dominancia manual derecha, escolaridad superior a quinto de primaria y capacidad para rendir las pruebas propuestas. Se comparó el rendimiento en las subpruebas de lenguaje del examen mínimo del estado mental (MMSE); en denominación y fluidez semántica y fonológica y se analizó el deterioro lingüístico en dos estadios de la demencia tipo Alzheimer. Resultados: en el estadio leve se evidencian déficit ligeros en todas las pruebas. Sinembargo los dominios con rendimiento más bajo fueron la fluidez fonológica y semántica. En el estadio moderado se evidenciaron diferencias en el rendimiento; las tareas de denominación, fluidez semántica y fluidez fonológica tuvieron rendimiento más bajo. Conclusiones: el lenguaje es un dominio que suele comprometerse en la demencia tipo Alzheimer. Los resultados reflejan el deterioro progresivo de la habilidad lingüística, manifiesto en un amplio rango de frecuencia entre el estadio leve y el moderado de la demencia. Existe un perfil similar de deterioro para los estadios leve y moderado con patrones independientes en las pruebas específicas

Evaluación de métodos para medir la actividad inhibitoria de extractos vegetales nativos del departamento de Sucre sobre bacterias y levaduras patógenas

The objective of this study was to evaluate the efficiency of two methods for measuring inhibitory activity of native ethanolic extracts plant of the Department of Sucre on bacteria and yeast human pathogenic. Sampling was conducted in the municipalities of Morroa and Sincelejo. The leaves of the plants Melia azederach, Sapium sp, Jatropha gossypilia, Psidium guajava, Origanum vulgare, Melissa officinalis, Eucalyptus sp and Cymbopogon citratus were processed using the methods of percolation and Soxhlet for the extraction of the extract. Methods were tested on agar hole method (Method 1) and the sensitive disk method (method 2) to measure the inhibitory effect on Pseudomonas aeruginosa, Klebsiella oxytoca, Enterococcus faecalis, Escherichia coli, and Bulkolderia glumaea Zygosaccharomyces microellipsoides. The results demonstrate that the method 2 allows greater efficiency and interpretation of results with regard to method 1 where there was diffusion of the extracts in the hole, which creates interference in the measurement. This is the first work in the department of Sucre where two methods are evaluated to determine inhibitory activity of a large group of native plants on pathogenic bacteria and yeast.El objetivo del presente trabajo fue evaluar la eficiencia de dos métodos para medir actividad inhibitoria de extractos vegetales etanólicos nativos del Departamento de Sucre sobre bacterias y levadura patógenas de humanos y plantas. Los muestreos se realizaron en los municipios de Morroa y Sincelejo. Las hojas de las plantas Melia Azederach, Sapium sp, Jatropha gossypilia, Psidium guajava, Origanum vulgare Melissa officinalis, Eucalyptus sp y Cymbopogon citratus fueron procesadas utilizando los métodos de percolación y de soxhlet para la extracción de los extractos. Se evaluaron los métodos de orificio sobre agar (método 1) y el método de disco sensitivos (método 2) para medir el efecto inhibitorio sobre Pseudomonas aeruginosa, Klebsiella oxytoca, Enterococcus faecalis, Escherichia coli, Bulkolderia glumaea y Zygosaccharomyces microellipsoides. Los resultados obtenidos demuestran que el método 2 permite una mayor eficacia e interpretación de los resultados con relación al método 1 donde se observó difusión de los extractos en el orificio, lo cual crea interferencia en la medición. Este es el primer trabajo en el departamento de Sucre donde se evalúan dos métodos para determinar actividad inhibitoria de un grupo amplio de plantas nativas sobre bacterias y levadura patógenas

Acute effect of three different exercise training modalities on executive function in overweight inactive men: A secondary analysis of the BrainFit study

7 páginasThere is currently a consensus about the positive effects of physical exercise on cognition. However, the exercise intensity-dependent effect on executive function remains unclear. Thus, the aim of this study was to compare the acute effects of high-intensity aerobic interval training (HIIT), progressive resistance training (PRT), or combined training (PRT + HIIT) on executive function indicators in overweight inactive adult men (aged 18–30 years old). The participants were screened and excluded for medical conditions known to impact cognitive functioning, which was measured with the Montreal Cognitive Assessment (MoCA) screening cognitive test. A randomised, parallel-group clinical trial was conducted among 36 adults who were randomly assigned to a HIIT (n = 12), PRT (n = 7), PRT + HIIT (n = 7), or control group (n = 10) until the energy expenditure of 400–500 kcal. Cognitive inhibition and attention capacity were examined using the Stroop test and d2 test of attention, respectively, and were obtained pre-exercise for baseline measurement and 1 min post-exercise for each exercise training modality. Cognitive inhibition measured by the Stroop test was improved after the HIIT protocol for the domains of reading by +5.89 (η2 = 0.33), colour naming +9.0 (η2 = 0.60), interference +10.1 (η2 = 0.39), and index interference +6.0 (η2 = 0.20). Additionally, the PRT + HIIT group had an increase for the reading condition of +7.1 (η2 = 0.40), colour naming +7.5 (η2 = 0.80), and interference +5.8 (η2 = 0.39). In regard to attentional capacity, the HIIT group elicited small to medium improvements in the concentration level domain of +21.7 (η2 = 0.44), total performance domain +56.6 (η2 = 0.50), and consistency domain −3.0 (η2 = 0.27). These results were similar in the PRT and PRT + HIIT groups in the concentration level and items-processed domains (P < 0.05). In conclusion, acute HIIT and PRT + HIIT sessions reported important effect sizes than PRT alone for cognitive inhibition and attention capacity. Taken together, the results suggest that even short-term exercise interventions can enhance overweight adults' executive functions