Fingerprints of Anthocyanins and Flavonols in Wild Grapes (Vitis vinifera L. ssp. sylvestris (Gmelin) Hegi)

Phenolic compounds are a group of natural products that play an important role in the quality of wines. Most phenolic compounds present in wine are derived from those contained in grapes and extracted from skins, seeds, and pulp during the initial steps of winemaking. Among them, anthocyanins and flavonols are involved in the color of red wines as pigments or copigments and also as precursors of polymeric pigments after reaction with other phenols. Biosynthesis of those phenolics in grapes is regulated by different genes; thus, each grape genotype presents a characteristic phenolic fingerprint, which is modulated by different environmental conditions. In this chapter, the anthocyanins and flavonols composition of different genotypes of wild grapes preserved at El Encin Germplasm Bank has been examined in detail. Wild grapevines are a remarkable genetic resource that may be used in breeding programs to improve the phenolic composition of cultivated grapes and, hence, the quality of red wines

A small XY chromosomal region explains sex determination in wild dioecious V. vinifera and the reversal to hermaphroditism in domesticated grapevines

Publis014-agap-029Background In Vitis vinifera L., domestication induced a dramatic change in flower morphology: the wild sylvestris subspecies is dioecious while hermaphroditism is largely predominant in the domesticated subsp. V. v. vinifera. The characterisation of polymorphisms in genes underlying the sex-determining chromosomal region may help clarify the history of domestication in grapevine and the evolution of sex chromosomes in plants. In the genus Vitis, sex determination is putatively controlled by one major locus with three alleles, male M, hermaphrodite H and female F, with an allelic dominance M > H > F. Previous genetic studies located the sex locus on chromosome 2. We used DNA polymorphisms of geographically diverse V. vinifera genotypes to confirm the position of this locus, to characterise the genetic diversity and traces of selection in candidate genes, and to explore the origin of hermaphroditism. Results In V. v. sylvestris, a sex-determining region of 154.8 kb, also present in other Vitis species, spans less than 1% of chromosome 2. It displays haplotype diversity, linkage disequilibrium and differentiation that typically correspond to a small XY sex-determining region with XY males and XX females. In male alleles, traces of purifying selection were found for a trehalose phosphatase, an exostosin and a WRKY transcription factor, with strikingly low polymorphism levels between distant geographic regions. Both diversity and network analysis revealed that H alleles are more closely related to M than to F alleles. Conclusions Hermaphrodite alleles appear to derive from male alleles of wild grapevines, with successive recombination events allowing import of diversity from the X into the Y chromosomal region and slowing down the expansion of the region into a full heteromorphic chromosome. Our data are consistent with multiple domestication events and show traces of introgression from other Asian Vitis species into the cultivated grapevine gene pool. La vigne domestiquée, Vitis vinifera ssp. vinifera, cultivée pour la production de fruit et de vin à travers le monde, dérive de la vigne sauvage, Vitis vinifera ssp. sylvestris, sous-espèce endémique de l'Eurasie. Au cours de la domestication, le système de reproduction a évolué de la diécie à l'hermaphrodisme. Nous montrons que la région du sexe est sous le contrôle d'une région chromosomique qui couvre au maximum 154kpbp, moins de 1% du chromosome 2. La caractérisation de ce locus en terme de diversité haplotypique, de signature de sélection et de déséquilibre de liaison a permis de révéler un système de détermination sexuelle de type XY. La petite taille de cette région chromosomique semble indiquer un stade très précoce dans l'évolution de chromosomes sexuels, malgré que la diécie soit le trait ancestral chez toutes les espèces de Vitis, ayant divergé du sous-genre Muscadinia il y a plusieurs millions d'années. L'analyse des distances génétiques entre haplotypes dans le locus du sexe a révélé que l'hermaphrodisme observé chez la vigne domestiquée résulte de la mutation de l'allèle mâle présent chez la vigne sauvage. Le réseau d'haplotypes a montré qu'en plus de la contribution de V. sylvestris, une autre espèce de Vitis asiatique a pu contribuer à la constitution du génome actuel de la vigne cultivée moderne. Ces travaux résultent d'une collaboration entre l'équipe DAAV d'AGAP et l'UMR CBAE (Montpellier)

Urban resilience profile of Cozumel Island, Mexico

La determinación de perfiles de resiliencia urbana es una línea de trabajo que instauró el gobierno de México en el año 2016. Su primera versión fue a nivel nacional con la generación de un reporte de 17 ciudades. Los principales resultados arrojaron una deficiencia técnico metodológico para hacer frente al desastre y se reconoce la necesidad de elaborar perfiles que consideren el “sentir” local y la participación de los habitantes. Así, el presente estudio tiene como finalidad la determinación del perfil de resiliencia de los asentamientos humanos de la isla de Cozumel, lugar con más de 85 mil habitantes y con impacto de huracanes de categoría 4. Se parte de la técnica de los 10 esenciales, cuyas secciones se enriquecieron con preguntas específicas a manera de indicadores. Se estableció el relevamiento de información a través de un muestreo representativo a nivel municipal –manzana, recopilando datos de 519 hogares en los meses de junio y julio del año 2018. Finalmente, se resume que el grado de resiliencia de la isla de Cozumel es de 5.18, considerando como medio, y con retos significativos en la capacidad social e institucional para hacer frente a la gestión integral de riesgo ante desastres.The determination of urban resilience profiles is a line of work established by the government of Mexico in 2016. Its first version was nationwide with the generation of a report of 17 cities. The main results showed a methodological technical deficiency to face the disaster and the need to elaborate profiles that consider the local & quot; feeling" and the participation of the inhabitants is recognized. Thus, the present study aims to determine the resilience profile of the human settlements on the island of Cozumel, an island with more than 85 thousand inhabitants and with the impact of category 4 hurricanes; for this, it is based on the technique of the 10 essentials, whose sections were enriched with specific questions as indicators. The survey of information was established through a representative sample at the municipal level – block, collecting data from 519 households in the months of June and July 2018. Finally, it is summarized that the degree of resilience of the island of Cozumel is 5.18 , considering as a means, and with significant challenges in the social and institutional capacity to face the integral management of disaster risk

Estudios sobre violencia en la educación. Enfoques, textos y contextos

El concepto de la violencia ha estado sobre la palestra desde el principio de nuestras sociedades. No obstante, en la práctica sus facetas son múltiples y en diversos ámbitos, lo que ha dado lugar a especulaciones acerca de los medios y los fines. Esto mismo incita a reflexionar en lo axiológico, pues la violencia alberga en sí un elemento adicional de arbitrariedad y, por lo tanto, se relaciona con aspectos fundamentales del derecho o los derechos humanos. En los ámbitos educativos han aparecido nuevas formas de violencia personal, que se reflejan en el bullying y el mobbing. En el ámbito universitario, existe un malestar que no se palía con estímulos o clientelismos y que se refiere a un tipo de violencia particular soterrada por las políticas públicas y el intervencionismo del Estado, los cuales han provocado tensiones entre las comunidades académicas; éstas tienen que ver con la defensa de los principios de libertad y autonomía de cátedra e investigación. En algunos casos, dichas voces han formulado críticas a los programas impuestos, ya que éstos se establecen sin reflexionar en los costos sociales que provocan en el trabajo académico y científico. De esas formas de violencia se quiere dar cuenta en esta obra, la cual fue desarrollada por la Red de Cuerpos Académicos en Política, Educación y Universidad

Advanced Virgo Plus: Future Perspectives

While completing the commissioning phase to prepare the Virgo interferometer for the next joint Observation Run (O4), the Virgo collaboration is also finalizing the design of the next upgrades to the detector to be employed in the following Observation Run (O5). The major upgrade will concern decreasing the thermal noise limit, which will imply using very large test masses and increased laser beam size. But this will not be the only upgrade to be implemented in the break between the O4 and O5 observation runs to increase the Virgo detector strain sensitivity. The paper will cover the challenges linked to this upgrade and implications on the detector's reach and observational potential, reflecting the talk given at 12th Cosmic Ray International Seminar - CRIS 2022 held in September 2022 in Napoli

The Advanced Virgo+ status

The gravitational wave detector Advanced Virgo+ is currently in the commissioning phase in view of the fourth Observing Run (O4). The major upgrades with respect to the Advanced Virgo configuration are the implementation of an additional recycling cavity, the Signal Recycling cavity (SRC), at the output of the interferometer to broaden the sensitivity band and the Frequency Dependent Squeezing (FDS) to reduce quantum noise at all frequencies. The main difference of the Advanced Virgo + detector with respect to the LIGO detectors is the presence of marginally stable recycling cavities, with respect to the stable recycling cavities present in the LIGO detectors, which increases the difficulties in controlling the interferometer in presence of defects (both thermal and cold defects). This work will focus on the interferometer commissioning, highlighting the control challenges to maintain the detector in the working point which maximizes the sensitivity and the duty cycle for scientific data taking

Multi-messenger observations of a binary neutron star merger

On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of ~1.7 s with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg2 at a luminosity distance of 40+8-8 Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 Mo. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at ~40 Mpc) less than 11 hours after the merger by the One- Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ~10 days. Following early non-detections, X-ray and radio emission were discovered at the transient’s position ~9 and ~16 days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta

NEOTROPICAL XENARTHRANS: a data set of occurrence of xenarthran species in the Neotropics

Xenarthrans – anteaters, sloths, and armadillos – have essential functions for ecosystem maintenance, such as insect control and nutrient cycling, playing key roles as ecosystem engineers. Because of habitat loss and fragmentation, hunting pressure, and conflicts with 24 domestic dogs, these species have been threatened locally, regionally, or even across their full distribution ranges. The Neotropics harbor 21 species of armadillos, ten anteaters, and six sloths. Our dataset includes the families Chlamyphoridae (13), Dasypodidae (7), Myrmecophagidae (3), Bradypodidae (4), and Megalonychidae (2). We have no occurrence data on Dasypus pilosus (Dasypodidae). Regarding Cyclopedidae, until recently, only one species was recognized, but new genetic studies have revealed that the group is represented by seven species. In this data-paper, we compiled a total of 42,528 records of 31 species, represented by occurrence and quantitative data, totaling 24,847 unique georeferenced records. The geographic range is from the south of the USA, Mexico, and Caribbean countries at the northern portion of the Neotropics, to its austral distribution in Argentina, Paraguay, Chile, and Uruguay. Regarding anteaters, Myrmecophaga tridactyla has the most records (n=5,941), and Cyclopes sp. has the fewest (n=240). The armadillo species with the most data is Dasypus novemcinctus (n=11,588), and the least recorded for Calyptophractus retusus (n=33). With regards to sloth species, Bradypus variegatus has the most records (n=962), and Bradypus pygmaeus has the fewest (n=12). Our main objective with Neotropical Xenarthrans is to make occurrence and quantitative data available to facilitate more ecological research, particularly if we integrate the xenarthran data with other datasets of Neotropical Series which will become available very soon (i.e. Neotropical Carnivores, Neotropical Invasive Mammals, and Neotropical Hunters and Dogs). Therefore, studies on trophic cascades, hunting pressure, habitat loss, fragmentation effects, species invasion, and climate change effects will be possible with the Neotropical Xenarthrans dataset

Population of Merging Compact Binaries Inferred Using Gravitational Waves through GWTC-3

We report on the population properties of compact binary mergers inferred from gravitational-wave observations of these systems during the first three LIGO-Virgo observing runs. The Gravitational-Wave Transient Catalog 3 (GWTC-3) contains signals consistent with three classes of binary mergers: binary black hole, binary neutron star, and neutron star-black hole mergers. We infer the binary neutron star merger rate to be between 10 and 1700 Gpc-3 yr-1 and the neutron star-black hole merger rate to be between 7.8 and 140 Gpc-3 yr-1, assuming a constant rate density in the comoving frame and taking the union of 90% credible intervals for methods used in this work. We infer the binary black hole merger rate, allowing for evolution with redshift, to be between 17.9 and 44 Gpc-3 yr-1 at a fiducial redshift (z=0.2). The rate of binary black hole mergers is observed to increase with redshift at a rate proportional to (1+z)κ with κ=2.9-1.8+1.7 for z≲1. Using both binary neutron star and neutron star-black hole binaries, we obtain a broad, relatively flat neutron star mass distribution extending from 1.2-0.2+0.1 to 2.0-0.3+0.3M⊙. We confidently determine that the merger rate as a function of mass sharply declines after the expected maximum neutron star mass, but cannot yet confirm or rule out the existence of a lower mass gap between neutron stars and black holes. We also find the binary black hole mass distribution has localized over- and underdensities relative to a power-law distribution, with peaks emerging at chirp masses of 8.3-0.5+0.3 and 27.9-1.8+1.9M⊙. While we continue to find that the mass distribution of a binary's more massive component strongly decreases as a function of primary mass, we observe no evidence of a strongly suppressed merger rate above approximately 60M⊙, which would indicate the presence of a upper mass gap. Observed black hole spins are small, with half of spin magnitudes below χi≈0.25. While the majority of spins are preferentially aligned with the orbital angular momentum, we infer evidence of antialigned spins among the binary population. We observe an increase in spin magnitude for systems with more unequal-mass ratio. We also observe evidence of misalignment of spins relative to the orbital angular momentum