Permeability of phospholipid membranes and human red blood cell membranes to hydrogen peroxide

Resumen del Conference paper presentado a SfRBM 28th Annual ConferenceHydrogen peroxide (H2O2) is an oxygen-derived oxidant involved in multiple redox processes in the cell, ranging from physiological signaling pathways to oxidative damage reactions when it is found at higher concentrations. In the vascular system, H2O2 is metabolized mainly by red blood cells (RBC) due to their very efficient antioxidant systems and high membrane permeability. However, the information regarding H2O2 transport in the human RBC membrane is limited, as neither the exact value of the permeability coefficient (Pm) nor the permeation mechanisms are known. To explore whether H2O2 permeates through the lipid fraction or protein channels, we studied H2O2 solubility in organic solvents and its permeability in lipid membranes, in order to compare with the RBC membrane. Through measurements of partition constants, we found that H2O2 is 14 and 122000 times less soluble in octanol and hexadecane than in water, anticipating a large thermodynamic barrier to H2O2 permeation by lipid membranes. The Pm in phospholipid membranes of different compositions, determined using the catalase-latency method, varied from 4×10-4 to 5×10-3 cm s-1, at 37°C. On the other hand, in human RBC we determined a Pm of 1.6×10-3 cm s-1. After obtaining these results, we evaluated the potential role of aquaporins as H2O2 transporters by checking the effect of aquaporin inhibitors in H2O2 consumption by RBC, and also by studying H2O2 permeability in RBC devoid of either aquaporin 1 or aquaporin 3. Surprisingly, we could not detect any differences in H2O2 permeability in any case. Altogether, these results provide new information on lipid membrane permeability to H2O2 and a new value for the Pm in human RBC, which was previously unknown. Additionally, they indicate that H2O2 is not transported by aquaporins in human RBC membranes, suggesting simple diffusion or a still unidentified membrane protein as a more probable pathway.ANII: ANII: FMV_1_2019_15559

Anatomy of a post-starburst minor merger: a multi-wavelength WFC3 study of NGC 4150

(Abridged) We present a spatially-resolved near-UV/optical study of NGC 4150, using the Wide Field Camera 3 (WFC3) on board the Hubble Space Telescope. Previous studies of this early-type galaxy (ETG) indicate that it has a large reservoir of molecular gas, exhibits a kinematically decoupled core (likely indication of recent merging) and strong, central H_B absorption (indicative of young stars). The core of NGC 4150 shows ubiquitous near-UV emission and remarkable dusty substructure. Our analysis shows this galaxy to lie in the near-UV green valley, and its pixel-by-pixel photometry exhibits a narrow range of near-UV/optical colours that are similar to those of nearby E+A (post-starburst) galaxies. We parametrise the properties of the recent star formation (age, mass fraction, metallicity and internal dust content) in the NGC 4150 pixels by comparing the observed near-UV/optical photometry to stellar models. The typical age of the recent star formation (RSF) is around 0.9 Gyrs, consistent with the similarity of the near-UV colours to post-starburst systems, while the morphological structure of the young component supports the proposed merger scenario. The RSF metallicity, representative of the metallicity of the gas fuelling star formation, is around 0.3 - 0.5 Zsun. Assuming that this galaxy is a merger and that the gas is sourced mainly from the infalling companion, these metallicities plausibly indicate the gas-phase metallicity (GPM) of the accreted satellite. Comparison to the local mass-GPM relation suggests (crudely) that the mass of the accreted system is around 3x10^8 Msun, making NGC 4150 a 1:20 minor merger. A summation of the pixel RSF mass fractions indicates that the RSF contributes about 2-3 percent of the stellar mass. This work reaffirms our hypothesis that minor mergers play a significant role in the evolution of ETGs at late epochs.Comment: 28 pages, 2 tables, accepted for publication in Ap

The permeability of human red blood cell membranes to hydrogen peroxide is independent of aquaporins

Hydrogen peroxide (H2O2) not only is an oxidant but also is an important signaling molecule in vascular biology, mediating several physiological functions. Red blood cells (RBCs) have been proposed to be the primary sink of H2O2 in the vasculature because they are the main cellular component of blood with a robust antioxidant defense and a high membrane permeability. However, the exact permeability of human RBC to H2O2 is neither known nor is it known if the mechanism of permeation involves the lipid fraction or protein channels. To gain insight into the permeability process, we measured the partition constant of H2O2 between water and octanol or hexadecane using a novel double-partition method. Our results indicated that there is a large thermodynamic barrier to H2O2 permeation. The permeability coefficient of H2O2 through phospholipid membranes containing cholesterol with saturated or unsaturated acyl chains was determined to be 4 × 10−4 and 5 × 10−3 cm s−1, respectively, at 37 °C. The permeability coefficient of human RBC membranes to H2O2 at 37 °C, on the other hand, was 1.6 × 10−3 cm s−1. Different aquaporin-1 and aquaporin-3 inhibitors proved to have no effect on the permeation of H2O2. Moreover, human RBCs devoid of either aquaporin-1 or aquaporin-3 were equally permeable to H2O2 as normal human RBCs. Therefore, these results indicate that H2O2 does not diffuse into RBCs through aquaporins but rather through the lipid fraction or a still unidentified membrane protein.ANII: FCE_2017_136043ANII: FMV_2019_155597CSIC: I+D_2014_C632-348CSIC: 2018_4

Moda sostenible. Diseñando modelos de economía circular en la región

El PAP Moda Sostenible: Diseñando modelos de economía circular en la región, tiene como objetivo general: activar economías locales, involucrando a los pequeños productores de la región en el sistema de la moda, desde una perspectiva sostenible. Como metodología se utiliza un modelo circular de moda sostenible1 basado en los tres pilares de la sostenibilidad: desarrollo económico, cuidado ambiental y cohesión social, con el que se busca incrementar los ingresos de los artesanos y productores de la comunidad destino, fortalecer el tejido social de los involucrados, gestionar de manera adecuada los recursos naturales con los que se trabaje y generar vínculos entre los consumidores y los productores. Durante este primer periodo se plantearon tres objetivos clave, que permitieron obtener resultados favorables: 1. Se realizaron manuales y fichas derivadas del análisis de los recursos naturales y humanos de la organización destino, que permitieron generar las primeras líneas de acción y propuestas de mejora. 2. Se creó una línea de productos viable y asequible para incrementar ingresos inmediatos en la comunidad destino que permitirá invertir en los desarrollos de mejora posteriores. Se creo @parakata una marca con identidad que ofrece los productos de los artesanos productores, con una línea de accesorios que ya se encuentra en fase de testeo dentro del mercado meta y una propuesta museográfica que se implementará para atraer nuevos clientes y aliados al lugar de origen de la producción artesanal (Casita de Piedra Cetcaser). 3. Se fortalecieron habilidades de los artesanos y productores tras detectar áreas de oportunidad para posibles mejoras integrales que se abordaron bajo manuales y capacitaciones en línea. Ofreciendo con esto a los beneficiarios, herramientas para prepararse y apropiarse de los productos y servicios diseñados en colaboración con las alumnas del PAP, permitiendo así su sostenibilidad a lo largo del tiempoITESO, A.C

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

Pan-cancer Alterations of the MYC Oncogene and Its Proximal Network across the Cancer Genome Atlas

Although theMYConcogene has been implicated incancer, a systematic assessment of alterations ofMYC, related transcription factors, and co-regulatoryproteins, forming the proximal MYC network (PMN),across human cancers is lacking. Using computa-tional approaches, we define genomic and proteo-mic features associated with MYC and the PMNacross the 33 cancers of The Cancer Genome Atlas.Pan-cancer, 28% of all samples had at least one ofthe MYC paralogs amplified. In contrast, the MYCantagonists MGA and MNT were the most frequentlymutated or deleted members, proposing a roleas tumor suppressors.MYCalterations were mutu-ally exclusive withPIK3CA,PTEN,APC,orBRAFalterations, suggesting that MYC is a distinct onco-genic driver. Expression analysis revealed MYC-associated pathways in tumor subtypes, such asimmune response and growth factor signaling; chro-matin, translation, and DNA replication/repair wereconserved pan-cancer. This analysis reveals insightsinto MYC biology and is a reference for biomarkersand therapeutics for cancers with alterations ofMYC or the PMN