Spatial and Temporal Protein Modules Signatures Associated with Alzheimer Disease in 3xTg-AD Mice Are Restored by Early Ubiquinol Supplementation

Despite its robust proteopathic nature, the spatiotemporal signature of disrupted protein modules in sporadic Alzheimer's disease (AD) brains remains poorly understood. This considered oxidative stress contributes to AD progression and early intervention with coenzyme Q10 or its reduced form, ubiquinol, delays the progression of the disease. Using MALDI-MSI and functional bioinformatic analysis, we have developed a protocol to express how deregulated protein modules arise from hippocampus and cortex in the AD mice model 3xTG-AD in an age-dependent manner. This strategy allowed us to identify which modules can be efficiently restored to a non-pathological condition by early intervention with ubiquinol. Indeed, an early deregulation of proteostasis-related protein modules, oxidative stress and metabolism has been observed in the hippocampus of 6-month mice (early AD) and the mirrored in cortical regions of 12-month mice (middle/late AD). This observation has been validated by IHC using mouse and human brain sections, suggesting that these protein modules are also affected in humans. The emergence of disrupted protein modules with AD signature can be prevented by early dietary intervention with ubiquinol in the 3xTG-AD mice model.A pesar de su robusta naturaleza proteopática, la firma espaciotemporal de los módulos de proteínas interrumpidos en los cerebros de la enfermedad de Alzheimer (EA) esporádica sigue siendo poco conocida. Este considerado estrés oxidativo contribuye a la progresión de la EA y la intervención precoz con coenzima Q10 o su forma reducida, el ubiquinol, retrasa la progresión de la enfermedad. Usando MALDI-MSI y análisis bioinformático funcional, hemos desarrollado un protocolo para expresar cómo surgen módulos de proteína desregulados del hipocampo y la corteza en el modelo de ratones AD 3xTG-AD de una manera dependiente de la edad. Esta estrategia nos permitió identificar qué módulos se pueden restaurar de manera eficiente a una condición no patológica mediante una intervención temprana con ubiquinol. De hecho, una desregulación temprana de los módulos proteicos relacionados con la proteostasis, Se ha observado estrés oxidativo y metabolismo en el hipocampo de ratones de 6 meses (EA temprana) y se refleja en regiones corticales de ratones de 12 meses (EA media/tardía). Esta observación ha sido validada por IHC utilizando secciones de cerebro humano y de ratón, lo que sugiere que estos módulos de proteína también se ven afectados en humanos. La aparición de módulos de proteínas interrumpidos con la firma AD puede prevenirse mediante una intervención dietética temprana con ubiquinol en el modelo de ratones 3xTG-AD

CoQ10 reduces glioblastoma growth and infiltration through proteome remodeling and inhibition of angiogenesis and inflammation

Purpose: Most monotherapies available against glioblastoma multiforme (GBM) target individual hallmarks of this aggressive brain tumor with minimal success. In this article, we propose a therapeutic strategy using coenzyme Q10 (CoQ10) as a pleiotropic factor that crosses the blood-brain barrier and accumulates in cell membranes acting as an antioxidant, and in mitochondrial membranes as a regulator of cell bioenergetics and gene expression. Methods: Xenografts of U251 cells in nu/nu mice were used to assay tumor growth, hypoxia, angiogenesis, and inflammation. An orthotopic model was used to explore microglial infiltration, tumor growth, and invasion into the brain parenchyma. Cell proliferation, migration, invasion, proteome remodeling, and secretome were assayed in vitro. Conditioned media were used to assay angiogenesis, monocyte chemoattraction, and differentiation into macrophages in vitro. Results: CoQ10 treatment decreased tumor volume in xenografts and orthotopic models, although its effect on tumor cell proliferation was not direct. Tumors from mice treated with CoQ10 were less hypoxic and vascularized, having less infiltration from inflammatory cells. Treatment-induced downregulation of HIF-1α and NF-kB led to a complete remodeling of the tumor cells proteome and secretome, impacting angiogenesis, monocyte infiltration, and their differentiation into macrophages. Besides, tumor cell migration and invasion were drastically restricted by mechanisms involving modulation of the actin cytoskeleton and downregulation of matrix metalloproteases (MMPs). Conclusions: CoQ10 has a pleiotropic effect on GBM growth, targeting several hallmarks simultaneously. Thus, its integration into current treatments of this fatal disease should be considered. Keywords: Angiogenesis; Coenzyme Q10; Glioblastoma; Inflammation; Invasion.Propósito: La mayoría de las monoterapias disponibles contra el glioblastoma multiforme (GBM) se dirigen a las características individuales de este tumor cerebral agresivo con un éxito mínimo. En este artículo proponemos una estrategia terapéutica utilizando la coenzima Q 10 (CoQ 10 ) como factor pleiotrópico que atraviesa la barrera hematoencefálica y se acumula en las membranas celulares actuando como antioxidante, y en las membranas mitocondriales como regulador de la bioenergética celular y gen expresión. Métodos: Se utilizaron xenoinjertos de células U251 en ratones nu/nu para analizar el crecimiento tumoral, la hipoxia, la angiogénesis y la inflamación. Se utilizó un modelo ortotópico para explorar la infiltración microglial, el crecimiento tumoral y la invasión del parénquima cerebral. Se ensayaron in vitro la proliferación celular, la migración, la invasión, la remodelación del proteoma y el secretoma. Se usaron medios acondicionados para analizar la angiogénesis, la quimioatracción de monocitos y la diferenciación en macrófagos in vitro. Resultados: el tratamiento con CoQ 10 disminuyó el volumen tumoral en xenoinjertos y modelos ortotópicos, aunque su efecto sobre la proliferación de células tumorales no fue directo. Los tumores de ratones tratados con CoQ 10 eran menos hipóxicos y vascularizados, con menos infiltración de células inflamatorias. La regulación a la baja inducida por el tratamiento de HIF-1α y NF-kB condujo a una remodelación completa del proteoma y el secretoma de las células tumorales, lo que impactó en la angiogénesis, la infiltración de monocitos y su diferenciación en macrófagos. Además, la migración e invasión de células tumorales se vieron drásticamente restringidas por mecanismos que involucran la modulación del citoesqueleto de actina y la regulación a la baja de las metaloproteasas de matriz (MMP). Conclusiones: CoQ 10 tiene un efecto pleiotrópico en el crecimiento de GBM, apuntando a varios sellos simultáneamente. Por lo tanto, se debe considerar su integración en los tratamientos actuales de esta enfermedad mortal

Imago & mirabilia : les formes del prodigi a la Mediterrània medieval

Hem organitzat el present volum a partir de tres àmbits que, sense cap pretensió totalitzadora ni teòrica, mostrin la vivacitat del prodigi medieval i la riquesa de la seva exploració. El primer àmbit és el titulat Geografies. El sagrat i el profà tracen una topografia del meravellós que omple la geografia d'indrets singulars, escenaris de tota mena de prodigis, alguns de remots o d'altres encara avinents. La tradicional història sagrada i l'heterogeni santoral, la literatura i els tractats pseudo-científics de l'antiguitat, les cròniques de viatgers i pelegrins o la mateixa cartografia, tot contribueix a fixar els indrets de la meravella com a lieux de mémoire. En efecte, el meravellós també respon a una topografia, a uns espais concrets on es troba, es reconeix i es difon; una memòria precisa on tothora són recordades les mirabilia. El segon àmbit del volum és Objectes. A l'edat mitjana, relíquies, objectes valuosos, rars o exòtics van ser buscats amb afany i els van creure portadors de virtuts prodigioses o reminiscències de criatures tan llunyanes com fabuloses. Presents a les corts, als tresors d'església o a les llars benestants, van esdevenir formes tangibles del sobrenatural. Alguns de procedents de l'Orient cristià van assolir una remarcable dimensió llegendària. I molts d'ells van desvetllar una arkhaiología, una «història de les coses antigues», amb la qual es va anar acompanyant l'objecte prodigiós d'una llegenda que reverberava la seva condició meravellosa i remota. Per últim, el tercer àmbit és Relats. Les narracions escrites i també els relats visuals van ser vehicles fonamentals per a la formació i la difusió del prodigi a l'edat mitjana. Les diverses formes de la meravella troben en la literatura profana o en l'hagiogràfica uns potents mitjans d'expressió i de la seva concreció. Cròniques, novel·les i relats hagiogràfics són portaveus de successos extraordinaris, i la seva enunciació o visualització és causa d'estupor. Miracle, llegenda i aventura esdevenen presències constants en la literatura i en les arts figuratives medievals

The CARMENES search for exoplanets around M dwarfs High-resolution optical and near-infrared spectroscopy of 324 survey stars

The CARMENES radial velocity (RV) survey is observing 324 M dwarfs to search for any orbiting planets. In this paper, we present the survey sample by publishing one CARMENES spectrum for each M dwarf. These spectra cover the wavelength range 520–1710 nm at a resolution of at least R >80 000, and we measure its RV, Hα emission, and projected rotation velocity. We present an atlas of high-resolution M-dwarf spectra and compare the spectra to atmospheric models. To quantify the RV precision that can be achieved in low-mass stars over the CARMENES wavelength range, we analyze our empirical information on the RV precision from more than 6500 observations. We compare our high-resolution M-dwarf spectra to atmospheric models where we determine the spectroscopic RV information content, Q, and signal-to-noise ratio. We find that for all M-type dwarfs, the highest RV precision can be reached in the wavelength range 700–900 nm. Observations at longer wavelengths are equally precise only at the very latest spectral types (M8 and M9). We demonstrate that in this spectroscopic range, the large amount of absorption features compensates for the intrinsic faintness of an M7 star. To reach an RV precision of 1 m s−1 in very low mass M dwarfs at longer wavelengths likely requires the use of a 10 m class telescope. For spectral types M6 and earlier, the combination of a red visual and a near-infrared spectrograph is ideal to search for low-mass planets and to distinguish between planets and stellar variability. At a 4 m class telescope, an instrument like CARMENES has the potential to push the RV precision well below the typical jitter level of 3–4 m s−1

Minimal information for studies of extracellular vesicles 2018 (MISEV2018):a position statement of the International Society for Extracellular Vesicles and update of the MISEV2014 guidelines

The last decade has seen a sharp increase in the number of scientific publications describing physiological and pathological functions of extracellular vesicles (EVs), a collective term covering various subtypes of cell-released, membranous structures, called exosomes, microvesicles, microparticles, ectosomes, oncosomes, apoptotic bodies, and many other names. However, specific issues arise when working with these entities, whose size and amount often make them difficult to obtain as relatively pure preparations, and to characterize properly. The International Society for Extracellular Vesicles (ISEV) proposed Minimal Information for Studies of Extracellular Vesicles (“MISEV”) guidelines for the field in 2014. We now update these “MISEV2014” guidelines based on evolution of the collective knowledge in the last four years. An important point to consider is that ascribing a specific function to EVs in general, or to subtypes of EVs, requires reporting of specific information beyond mere description of function in a crude, potentially contaminated, and heterogeneous preparation. For example, claims that exosomes are endowed with exquisite and specific activities remain difficult to support experimentally, given our still limited knowledge of their specific molecular machineries of biogenesis and release, as compared with other biophysically similar EVs. The MISEV2018 guidelines include tables and outlines of suggested protocols and steps to follow to document specific EV-associated functional activities. Finally, a checklist is provided with summaries of key points

A giant exoplanet orbiting a very-low-mass star challenges planet formation models

Surveys have shown that super-Earth and Neptune-mass exoplanets are more frequent than gas giants around low-mass stars, as predicted by the core accretion theory of planet formation. We report the discovery of a giant planet around the very-low-mass star GJ 3512, as determined by optical and near-infrared radial-velocity observations. The planet has a minimum mass of 0.46 Jupiter masses, very high for such a small host star, and an eccentric 204-day orbit. Dynamical models show that the high eccentricity is most likely due to planet-planet interactions. We use simulations to demonstrate that the GJ 3512 planetary system challenges generally accepted formation theories, and that it puts constraints on the planet accretion and migration rates. Disk instabilities may be more efficient in forming planets than previously thought

CARMENES: high-resolution spectra and precise radial velocities in the red and infrared

SPIE Astronomical Telescopes + Instrumentation (2018, Austin, Texas, United States

The CARMENES search for exoplanets around M dwarfs: High-resolution optical and near-infrared spectroscopy of 324 survey stars

The CARMENES radial velocity (RV) survey is observing 324 M dwarfs to search for any orbiting planets. In this paper, we present the survey sample by publishing one CARMENES spectrum for each M dwarf. These spectra cover the wavelength range 520–1710 nm at a resolution of at least R > 80 000, and we measure its RV, H emission, and projected rotation velocity. We present an atlas of high-resolution M-dwarf spectra and compare the spectra to atmospheric models. To quantify the RV precision that can be achieved in low-mass stars over the CARMENES wavelength range, we analyze our empirical information on the RV precision from more than 6500 observations. We compare our high-resolution M-dwarf spectra to atmospheric models where we determine the spectroscopic RV information content, Q, and signal-to-noise ratio. We find that for all M-type dwarfs, the highest RV precision can be reached in the wavelength range 700–900 nm. Observations at longer wavelengths are equally precise only at the very latest spectral types (M8 and M9).We demonstrate that in this spectroscopic range, the large amount of absorption features compensates for the intrinsic faintness of an M7 star. To reach an RV precision of 1 m/s in very low mass M dwarfs at longer wavelengths likely requires the use of a 10m class telescope. For spectral types M6 and earlier, the combination of a red visual and a near-infrared spectrograph is ideal to search for low-mass planets and to distinguish between planets and stellar variability. At a 4m class telescope, an instrument like CARMENES has the potential to push the RV precision well below the typical jitter level of 3–4 m/s