92 research outputs found

    Study of MTHFR C677T polymorphism in neonates with isolated congenital heart disease in a Colombian population

    Get PDF
    IntroducciĂłn: El estudio del papel de polimorfismos en genes de las vĂ­as metabĂłlicas de la homocisteĂ­na-metionina y el ĂĄcido fĂłlico en anomalĂ­as congĂ©nitas, es cada vez mĂĄs importante debido a que sus efectos podrĂ­an ser modulados.Objetivo: Determinar si la presencia del polimorfismo C677T en el gen de la metilentetrahidrofolato reductasa (MTHFR) se asocia con el desarrollo de cardiopatĂ­as congĂ©nitas aisladas.MĂ©todos: Se compararon las frecuencias alĂ©licas y genotĂ­picas del polimorfismo en 34 reciĂ©n nacidos con cardiopatĂ­as congĂ©nitas aisladas y en 102 individuos sanos. La genotipificaciĂłn se hizo mediante la reacciĂłn en cadena de la polimerasa (PCR) y se determinĂł el genotipo por medio de la tĂ©cnica de polimorfismo de longitud de los fragmentos de restricciĂłn (RFLP).Resultados: No se encontraron diferencias estadĂ­sticamente significativas en las frecuencias alĂ©licas ni genotĂ­picas entre los grupos de casos y controles. Sin embargo, se observĂł una tendencia estadĂ­stica para un posible efecto protector del genotipo TT.ArtĂ­culo original269-277The research of the role of gene polymorphisms in the metabolic pathways of homocysteine-me-thionine and folic acid in congenital malformations is very important because its effect could be modulated. Objetive: The aim of this study was to determine whether the C677T polymorphism in the gene of the enzyme methylenetetrahydrofolate reductase (NÍTHFR) was associated with the development of isolated congenital heart disease. Methodology: We compared the allele and genotype frequencies of this polymorphism in 34 infants with isolated congenital heart defects and 102 healthy individuals. Genotyping was performed by Polymerase Chain Reaction (PCR) and with the technique Restriction Fragment Length Polymorphism (RFLP). Results: There were no statistically significant differences in allele or genotype frequencies between case and control groups. Although our results show no statistically significant differences between the groups assessed there was a statistical trend for a possible protective effect of TT genotype against the development of congenital heart disease

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

    Full text link
    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

    Full text link
    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

    GuĂ­as colombianas de cardiologĂ­a sĂ­ndrome coronario agudo sin elevaciĂłn del ST

    Get PDF
    Las enfermedades cardiovasculares constituyen la principal causa de muerte en los paĂ­ses industrializadosy en los paĂ­ses en vĂ­a de desarrollo. Dentro de estas patologĂ­as la enfermedad coronaria es la manifes-taciĂłn mĂĄs prevalente y se asocia con alta mortalidad y morbilidad. Las presentaciones clĂ­nicas de laenfermedad coronaria isquĂ©mica incluyen, isquemia silente, angina de pecho estable, falla cardĂ­aca,angina inestable, infarto agudo del miocardio y muerte sĂșbita. En esta primera entrega se tratarĂĄ elsĂ­ndrome coronario agudo sin elevaciĂłn del ST que incluye la angina inestable y el infarto agudo delmiocardio sin elevaciĂłn del ST.Q4121-27

    Clonal chromosomal mosaicism and loss of chromosome Y in elderly men increase vulnerability for SARS-CoV-2

    Full text link
    The pandemic caused by severe acute respiratory syndrome coronavirus 2 (SARS-CoV-2, COVID-19) had an estimated overall case fatality ratio of 1.38% (pre-vaccination), being 53% higher in males and increasing exponentially with age. Among 9578 individuals diagnosed with COVID-19 in the SCOURGE study, we found 133 cases (1.42%) with detectable clonal mosaicism for chromosome alterations (mCA) and 226 males (5.08%) with acquired loss of chromosome Y (LOY). Individuals with clonal mosaic events (mCA and/or LOY) showed a 54% increase in the risk of COVID-19 lethality. LOY is associated with transcriptomic biomarkers of immune dysfunction, pro-coagulation activity and cardiovascular risk. Interferon-induced genes involved in the initial immune response to SARS-CoV-2 are also down-regulated in LOY. Thus, mCA and LOY underlie at least part of the sex-biased severity and mortality of COVID-19 in aging patients. Given its potential therapeutic and prognostic relevance, evaluation of clonal mosaicism should be implemented as biomarker of COVID-19 severity in elderly people. Among 9578 individuals diagnosed with COVID-19 in the SCOURGE study, individuals with clonal mosaic events (clonal mosaicism for chromosome alterations and/or loss of chromosome Y) showed an increased risk of COVID-19 lethality

    Anales del III Congreso Internacional de Vivienda y Ciudad "Debate en torno a la nueva agenda urbana"

    Get PDF
    Acta de congresoEl III Congreso Internacional de Vivienda y Ciudad “Debates en torno a la NUEVa Agenda Urbana”, ha sido una apuesta de alto compromiso por acercar los debates centrales y urgentes que tensionan el pleno ejercicio del derecho a la ciudad. Para ello las instituciones organizadoras (INVIHAB –Instituto de InvestigaciĂłn de Vivienda y HĂĄbitat y MGyDH-MaestrĂ­a en GestiĂłn y Desarrollo Habitacional-1), hemos convidado un espacio que se concretĂł con potencia en un debate transdisciplinario. ConvocĂł a intelectuales de prestigio internacional, investigadores, acadĂ©micos y gestores estatales, y en una metodologĂ­a de innovaciĂłn articulĂł las voces acadĂ©micas con las de las organizaciones sociales y/o barriales en el Foro de las Organizaciones Sociales que tuvo su espacio propio para dar voz a quienes estĂĄn trabajando en los desafĂ­os para garantizar los derechos a la vivienda y los bienes urbanos en nuestras ciudades del Siglo XXI

    Multiple Scenario Generation of Subsurface Models:Consistent Integration of Information from Geophysical and Geological Data throuh Combination of Probabilistic Inverse Problem Theory and Geostatistics

    Get PDF
    Neutrinos with energies above 1017 eV are detectable with the Surface Detector Array of the Pierre Auger Observatory. The identification is efficiently performed for neutrinos of all flavors interacting in the atmosphere at large zenith angles, as well as for Earth-skimming \u3c4 neutrinos with nearly tangential trajectories relative to the Earth. No neutrino candidates were found in 3c 14.7 years of data taken up to 31 August 2018. This leads to restrictive upper bounds on their flux. The 90% C.L. single-flavor limit to the diffuse flux of ultra-high-energy neutrinos with an E\u3bd-2 spectrum in the energy range 1.0 7 1017 eV -2.5 7 1019 eV is E2 dN\u3bd/dE\u3bd < 4.4 7 10-9 GeV cm-2 s-1 sr-1, placing strong constraints on several models of neutrino production at EeV energies and on the properties of the sources of ultra-high-energy cosmic rays

    The Helicobacter pylori Genome Project : insights into H. pylori population structure from analysis of a worldwide collection of complete genomes

    Get PDF
    Helicobacter pylori, a dominant member of the gastric microbiota, shares co-evolutionary history with humans. This has led to the development of genetically distinct H. pylori subpopulations associated with the geographic origin of the host and with differential gastric disease risk. Here, we provide insights into H. pylori population structure as a part of the Helicobacter pylori Genome Project (HpGP), a multi-disciplinary initiative aimed at elucidating H. pylori pathogenesis and identifying new therapeutic targets. We collected 1011 well-characterized clinical strains from 50 countries and generated high-quality genome sequences. We analysed core genome diversity and population structure of the HpGP dataset and 255 worldwide reference genomes to outline the ancestral contribution to Eurasian, African, and American populations. We found evidence of substantial contribution of population hpNorthAsia and subpopulation hspUral in Northern European H. pylori. The genomes of H. pylori isolated from northern and southern Indigenous Americans differed in that bacteria isolated in northern Indigenous communities were more similar to North Asian H. pylori while the southern had higher relatedness to hpEastAsia. Notably, we also found a highly clonal yet geographically dispersed North American subpopulation, which is negative for the cag pathogenicity island, and present in 7% of sequenced US genomes. We expect the HpGP dataset and the corresponding strains to become a major asset for H. pylori genomics

    Observation of gravitational waves from the coalescence of a 2.5−4.5 M⊙ compact object and a neutron star

    Get PDF

    Search for eccentric black hole coalescences during the third observing run of LIGO and Virgo

    Get PDF
    Despite the growing number of confident binary black hole coalescences observed through gravitational waves so far, the astrophysical origin of these binaries remains uncertain. Orbital eccentricity is one of the clearest tracers of binary formation channels. Identifying binary eccentricity, however, remains challenging due to the limited availability of gravitational waveforms that include effects of eccentricity. Here, we present observational results for a waveform-independent search sensitive to eccentric black hole coalescences, covering the third observing run (O3) of the LIGO and Virgo detectors. We identified no new high-significance candidates beyond those that were already identified with searches focusing on quasi-circular binaries. We determine the sensitivity of our search to high-mass (total mass M>70 M⊙) binaries covering eccentricities up to 0.3 at 15 Hz orbital frequency, and use this to compare model predictions to search results. Assuming all detections are indeed quasi-circular, for our fiducial population model, we place an upper limit for the merger rate density of high-mass binaries with eccentricities 0<e≀0.3 at 0.33 Gpc−3 yr−1 at 90\% confidence level
    • 

    corecore