Marginación y esperanza de vida en los municipios de Coahuila durante la pandemia por COVID-19

Introduction: A health condition of great impact on life expectancy in different populations and countries has been the Covid-19 pandemic. Objective: To calculate life expectancy comparing 2019 with 2020 and analyzed its relationship with indicators of the marginalization at the municipal level for the state of Coahuila in the context of Covid-19 pandemic. Material and method: Life expectancy was calculated using mortality data for 2019 and 2020 from the Ministry of Health and demographic and marginalization indicators were obtained from the National Population Council. The Shapiro-Wilk test was applied to the variables under study and those that has a normal distribution where analyzed with variance hypothesis test (ANOVA), followed by the Bonferroni post-hoc test. Variables that where found to be significant in the ANOVA test where subjected to a multiple regression to identify predictors. Kruskal-Wallis and Games Howell tests were performed with variables that did not have a normal distribution. Results: Variables that showed a positive and significant directionality were the percentage of population greater than 5 000 inhabitants and the natural logarithm of the population size of the municipalities. This latter variable was the only predictor of the loss in years of life expectancy. Conclusion: The natural logarithm of population size was the only predictor of the drop in years of life expectancy.Introducción: Una condición sanitaria de gran impacto en la esperanza de vida en diferentes poblaciones y países ha sido la pandemia por el Covid-19. Objetivo: Calcular la esperanza de vida (EV) comparando 2019 con 2020 y analizar su relación con indicadores de marginación a nivel municipal para el estado de Coahuila en el contexto de la pandemia por Covid-19. Material y Método: La EV se calculó con información de mortalidad para 2019 y 2020 de la Secretaría de Salud y demográfica e indicadores de marginación del Consejo Nacional de Población. Se aplicó la prueba de Shapiro-Wilk a las variables bajo estudio y aquellas que tuvieron una distribución normal fueron analizadas con la prueba de hipótesis de varianza (ANOVA), seguida de la prueba pos-hoc de Bonferroni. Las variables que resultaron significativas en la prueba de ANOVA fueron sujetas a un análisis de regresión lineal múltiple para identificar predictores. Con las variables que no se distribuyeron normalmente se hicieron pruebas de Kruskal-Wallis y post-hoc de Games-Howell. Resultados: Las variables que resultaron ser estadísticamente significativas y que mostraron una direccionalidad positiva fueron el porcentaje de población mayor a 5 000 habitantes y el logaritmo natural del tamaño de la población de los municipios. Conclusión: De las variables analizadas el logaritmo natural del tamaño de la población fue el único predictor capaz de modelar la caída en años de la esperanza de vida

P050 Oral inflammatory changes associated with inflammatory bowel disease in spondyloarthritis associated with early endoscopic findings

BACKGROUND: Spondyloarthritis (SpA) is a heterogeneous group of chronic autoinflammatory disorders that can present extra-articular gastrointestinal manifestations. Among them is mainly inflammatory bowel disease (IBD). Although IBD mainly affects the intestinal tract, it can include early manifestations evident in the oral cavity. No comparative data on these oral manifestations in patients with SpA were found in the literature. OBJECTIVE: To identify oral clinical manifestations due to changes in the oral mucosa associated with IBD in patients with SpA without a diagnosis of IBD and associate them with endoscopic and histological findings. METHODS: 80 patients with SpA and 52 healthy controls were evaluated. They were assessed intra- and extra-orally, following the modified World Health Organization guideline. In addition, by clinical parameters of rheumatological, gastrointestinal and laboratory activity. Ileocolonoscopy was performed with digital chromoendoscopy with magnification and histological analysis. Comparative analyzes were performed by Chi square tests, Fisher's exact tests, confirmed by univariate regression and discriminant analysis of multiple correspondences. Institutional ethics committee approval cod-2017-023. RESULTS: The patients with SpA had 56% male gender, mean age of 42.8 years (SD ± 10.4) and a BMI in the range of 23.9 - 28.4. The healthy controls, 54% of the male gender with an average age of 41 years (SD ± 13.6) and a body mass index-BMI in the range of 22.9 - 27.6. The patients reported smoking only in 6.2%, however as a smoking history in 31% and passive smokers (15%), the majority employed (41%), married (56%) and professionals (49%). Of the healthy controls, they smoked (15%), with a history of smoking (31%), passive smokers (21%), the majority employed (77%), with their own home (67%), and professionals (54%). The patients with SpA reported a greater presence of some signs and symptoms of gastrointestinal origin 69%, while in the controls it was 7.7% (p = 0.001). Forty one of them were referred to colonoscopy with magnification being in 17.1 % changes in the mucosa of the rectum and in the same frequency changes in the mucosa of the sigmoid colon. Regarding the ileum, changes in the mucosa were evidenced in 41.5% of the cases. The presence of oral lesions was evident and predominated in them (63%) compared to controls p = 0.050. The main oral lesions associated with IBD were gingivitis (55%) (p = 0.001), followed by aphthous stomatitis (3.8%), angular cheilitis (2.6%) and perioral erythema with scaling (1.3%). 100% of the patients who presented alteration of the colonic mucosa presented oral lesions associated with IBD (p = 0039), which was also significantly associated with the presence of gingivitis/aphthous stomatitis (p = 0.029). CONCLUSION: Patients with SpA without a diagnosis of IBD have more oral signs and symptoms compared to healthy controls. Gingivitis is important given its association with early endoscopic and histological findings. Manifestations in the oral cavity can precede intestinal manifestations, therefore the clinical assessment by the oral pathologist in conjunction with gastroenterology and rheumatology allows a timely referral to gastroenterology and an endoscopic and histological evaluation, impacting the quality of life of patients

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

A search for ultra-high-energy photons at the Pierre Auger Observatory exploiting air-shower universality

The Pierre Auger Observatory is the most sensitive detector to primary photons with energies above ∼0.2 EeV. It measures extensive air showers using a hybrid technique that combines a fluorescence detector (FD) with a ground array of particle detectors (SD). The signatures of a photon-induced air shower are a larger atmospheric depth at the shower maximum (X$_{max}$) and a steeper lateral distribution function, along with a lower number of muons with respect to the bulk of hadron-induced background. Using observables measured by the FD and SD, three photon searches in different energy bands are performed. In particular, between threshold energies of 1-10 EeV, a new analysis technique has been developed by combining the FD-based measurement of X$_{max}$ with the SD signal through a parameter related to its muon content, derived from the universality of the air showers. This technique has led to a better photon/hadron separation and, consequently, to a higher search sensitivity, resulting in a tighter upper limit than before. The outcome of this new analysis is presented here, along with previous results in the energy ranges below 1 EeV and above 10 EeV. From the data collected by the Pierre Auger Observatory in about 15 years of operation, the most stringent constraints on the fraction of photons in the cosmic flux are set over almost three decades in energy

Study on multi-ELVES in the Pierre Auger Observatory

Since 2013, the four sites of the Fluorescence Detector (FD) of the Pierre Auger Observatory record ELVES with a dedicated trigger. These UV light emissions are correlated to distant lightning strikes. The length of recorded traces has been increased from 100 μs (2013), to 300 μs (2014-16), to 900 μs (2017-present), to progressively extend the observation of the light emission towards the vertical of the causative lightning and beyond. A large fraction of the observed events shows double ELVES within the time window, and, in some cases, even more complex structures are observed. The nature of the multi-ELVES is not completely understood but may be related to the different types of lightning in which they are originated. For example, it is known that Narrow Bipolar Events can produce double ELVES, and Energetic In-cloud Pulses, occurring between the main negative and upper positive charge layer of clouds, can induce double and even quadruple ELVES in the ionosphere. This report shows the seasonal and daily dependence of the time gap, amplitude ratio, and correlation between the pulse widths of the peaks in a sample of 1000+ multi-ELVES events recorded during the period 2014-20. The events have been compared with data from other satellite and ground-based sensing devices to study the correlation of their properties with lightning observables such as altitude and polarity