Glutathione reductase gsr-1 is an essential gene required for Caenorhabditis elegans early embryonic development

Glutathione is the most abundant thiol in the vast majority of organisms and is maintained in its reduced form by the flavoenzyme glutathione reductase. In this work, we describe the genetic and functional analysis of the Caenorhabditis elegans gsr-1 gene that encodes the only glutathione reductase protein in this model organism. By using green fluorescent protein reporters we demonstrate that gsr-1 produces two GSR-1 isoforms, one located in the cytoplasm and one in the mitochondria. gsr-1 loss of function mutants display a fully penetrant embryonic lethal phenotype characterized by a progressive and robust cell division delay accompanied by an aberrant distribution of interphasic chromatin in the periphery of the cell nucleus. Maternally expressed GSR-1 is sufficient to support embryonic development but these animals are short-lived, sensitized to chemical stress and have increased mitochondrial fragmentation and lower mitochondrial DNA content. Furthermore, the embryonic lethality of gsr-1 worms is prevented by restoring GSR-1 activity in the cytoplasm but not in mitochondria. Given the fact that the thioredoxin redox systems are dispensable in C. elegans, our data support a prominent role of the glutathione reductase/glutathione pathway in maintaining redox homeostasis in the nematode

On Quantum Effects in a Theory of Biological Evolution

We construct a descriptive toy model that considers quantum effects on biological evolution starting from Chaitin's classical framework. There are smart evolution scenarios in which a quantum world is as favorable as classical worlds for evolution to take place. However, in more natural scenarios, the rate of evolution depends on the degree of entanglement present in quantum organisms with respect to classical organisms. If the entanglement is maximal, classical evolution turns out to be more favorable

Role of glutathione reductase in proteostasis regulation

Trabajo presentado en la V Spanish Worm Meeting, celebrada en Salamanca el 5 y 6 de marzo de 2015.Peer Reviewe

Towards a DNA-vaccine against African swine fever: an ongoing effort

Trabajo presentado en el 6th International Symposium on Emerging and Re-emerging pig Diseases, celebrado en Barcelona (España) del 12 al 15 de julio de 2011

The Sensitivity of HAWC to High-Mass Dark Matter Annihilations

The High Altitude Water Cherenkov (HAWC) observatory is a wide field-of-view detector sensitive to gamma rays of 100 GeV to a few hundred TeV. Located in central Mexico at 19 degrees North latitude and 4100 m above sea level, HAWC will observe gamma rays and cosmic rays with an array of water Cherenkov detectors. The full HAWC array is scheduled to be operational in Spring 2015. In this paper, we study the HAWC sensitivity to the gamma-ray signatures of high-mass (multi- TeV) dark matter annihilation. The HAWC observatory will be sensitive to diverse searches for dark matter annihilation, including annihilation from extended dark matter sources, the diffuse gamma-ray emission from dark matter annihilation, and gamma-ray emission from non-luminous dark matter subhalos. Here we consider the HAWC sensitivity to a subset of these sources, including dwarf galaxies, the M31 galaxy, the Virgo cluster, and the Galactic center. We simulate the HAWC response to gamma rays from these sources in several well-motivated dark matter annihilation channels. If no gamma-ray excess is observed, we show the limits HAWC can place on the dark matter cross-section from these sources. In particular, in the case of dark matter annihilation into gauge bosons, HAWC will be able to detect a narrow range of dark matter masses to cross-sections below thermal. HAWC should also be sensitive to non-thermal cross-sections for masses up to nearly 1000 TeV. The constraints placed by HAWC on the dark matter cross-section from known sources should be competitive with current limits in the mass range where HAWC has similar sensitivity. HAWC can additionally explore higher dark matter masses than are currently constrained.Comment: 15 pages, 4 figures, version to be published in PR

Estudio teórico y experimental del sistema 9 Be + 51 V y sistemas similares

En este trabajo de tesis se presenta el estudio sistemático de los sistemas 7Li + 51V, 9Be + 51V y 8B + 58Ni. Para los sistemas ( 7Li, 9 Be) + 51V se midieron las secciones eficaces de fusión a energías cercanas a la barrera Coulombiana (EB,lab=11.75 y 16.16 MeV, respectivamente) empleando la técnica de rayos γ. El experimento para medir la fusión se llevó a cabo en el Laboratorio del Acelerador Tan- dem, del Instituto Nacional de Investigaciones Nucleares (ININ), siendo éstas las primeras mediciones realizadas para estos proyectiles a las energías consideradas. De forma simultánea, se hizo el análisis de los posibles núcleos residuales usando los códigos computacionales de fusión-evaporación PACE2, LILITA y CASCADE. Los resultados obtenidos fueron comparados con los datos experimentales me- didos. De forma preliminar, para el sistema 7Li + 51V, se hicieron cálculos usando la teoría de canales acoplados de reacción para estimar la contribución de la sección eficaz de transferencia de un protón a la producción del núcleo residual 52Cr. Para el sistema 8B + 58Ni, se hizo un análisis teórico de canales acoplados con el continuo discretizado y canales acoplados de reacción para estudiar los procesos de rompimiento y de transfe- rencia de un protón, 58Ni(8B,7Be)59Cu, a energías alrededor de la barrera Coulombiana (EB,lab=22.95 MeV). Para calcular las secciones eficaces correspondientes se usó un potencial de Modelo Óptico se- mimicroscópico, el cual combina un potencial real de doble convolución, un potencial de polarización y un potencial imaginario tipo Woods-Saxon. A partir de la comparación de nuestros cálculos con datos experimentales se determinaron los factores espectroscópicos Sexpt y astrofísicos S17(0) del protón en la interacción 8B → 7Be+p

VAMOS: a Pathfinder for the HAWC Gamma-Ray Observatory

VAMOS was a prototype detector built in 2011 at an altitude of 4100m a.s.l. in the state of Puebla, Mexico. The aim of VAMOS was to finalize the design, construction techniques and data acquisition system of the HAWC observatory. HAWC is an air-shower array currently under construction at the same site of VAMOS with the purpose to study the TeV sky. The VAMOS setup included six water Cherenkov detectors and two different data acquisition systems. It was in operation between October 2011 and May 2012 with an average live time of 30%. Besides the scientific verification purposes, the eight months of data were used to obtain the results presented in this paper: the detector response to the Forbush decrease of March 2012, and the analysis of possible emission, at energies above 30 GeV, for long gamma-ray bursts GRB111016B and GRB120328B.Comment: Accepted for pubblication in Astroparticle Physics Journal (20 pages, 10 figures). Corresponding authors: A.Marinelli and D.Zaboro

Glucose Starvation Boosts Entamoeba histolytica Virulence

The unicellular parasite, Entamoeba histolytica, is exposed to numerous adverse conditions, such as nutrient deprivation, during its life cycle stages in the human host. In the present study, we examined whether the parasite virulence could be influenced by glucose starvation (GS). The migratory behaviour of the parasite and its capability to kill mammalian cells and to lyse erythrocytes is strongly enhanced following GS. In order to gain insights into the mechanism underlying the GS boosting effects on virulence, we analyzed differences in protein expression levels in control and glucose-starved trophozoites, by quantitative proteomic analysis. We observed that upstream regulatory element 3-binding protein (URE3-BP), a transcription factor that modulates E.histolytica virulence, and the lysine-rich protein 1 (KRiP1) which is induced during liver abscess development, are upregulated by GS. We also analyzed E. histolytica membrane fractions and noticed that the Gal/GalNAc lectin light subunit LgL1 is up-regulated by GS. Surprisingly, amoebapore A (Ap-A) and cysteine proteinase A5 (CP-A5), two important E. histolytica virulence factors, were strongly down-regulated by GS. While the boosting effect of GS on E. histolytica virulence was conserved in strains silenced for Ap-A and CP-A5, it was lost in LgL1 and in KRiP1 down-regulated strains. These data emphasize the unexpected role of GS in the modulation of E.histolytica virulence and the involvement of KRiP1 and Lgl1 in this phenomenon