Descripción de dos nuevas subespecies del género Lepidocyrtus Bourlet, 1839 (Collembola, Entomobryidae) de La Península Ibérica

Specimens of Lepidocyrtus lusitanicus from the Iberian Peninsula have been studied. Two new taxa have been found: Lepidocyrtus lusitanicus nigrus ssp. n. and Lepidocyrtus lusitanicus piezoensis ssp. n.; they are separated from the main species on the basis of colour. The other two taxa in this species, Lepidocyrtus lusitanicus lusitanicus and L. lusitanicus coloratus comb. n. and their distribution maps have also been studied. At the same time a key and distribution of all species of this genus for the Iberian Peninsula is given.Se hace un estudio de Lepidocyrtus lusitanicus Gama, 1964, encontrándose dos nuevos taxones, L. lusitanicus nigrus ssp. n. y L. lusitanicus piezoensis ssp. n. Difieren de la especie principal en la distinta coloración corporal. También se estudian los otros dos taxones de esta especie L. lusitanicus lusitanicus y L. lusitanicus coloratus comb. n., con sus mapas de distribución. Al mismo tiempo se efectúa una clave de las especies de este género para la Península Ibérica

Stachorutes cabagnerensis sp. n., Collembola (Neanuridae) de la región central de España, y una aproximación preliminar a la filogenia del género

A new species of the genus Stachorutes, Stachorutes cabagnerensis n. sp., from central Spain is described. It is characterized by the presence of 6+6 eyes in the head, retinaculum 2+2 teeth, dentes with 5 hairs, and the absence of mucron. A phylogenetic analysis of this genus was attempted. Potential synapomorphies supporting the monophyly of Stachorutes are presented. One member of the genus (the Nearctic S. navajellus) appears as a basal form, phylogenetically distant from the remaining (Old World) species. There is evidence for a monophyletic infrageneric clade with the species S. dematteisi, S. jizuensis and S. sphagnophilus. However, more information is required for further phylogenetic resolution.Se describe una nueva especie del genero Stachorutes de la region central de España. Stachorutes cabagnerensis nov. sp. se caracteriza por la presencia de 6+6 ojos en la cabeza, retinaculum con 2+2 dientes y 5 sedas en cada rama del dentes; la furca carece de mucrón. Se ha efectuado un análisis filogenético. Las sinapomorfias potenciales establecen la monofilia del género. Una especie del mismo, S. navajellus, aparece como forma basal, filogenéticamente distante del resto de especies (Viejo Mundo). Se podría establecer un clado infragenérico con las especies S. dematteisi, S. jizuensis y S. sphagnophilus. Sin embargo, se precisa de mayor información para poder confirmarlo

Dos nuevas especies de Pseudosinella Schäffer, 1897 (Collembola, Entomobryidae) de Castilla-La Mancha

Two new species of Pseudosinella (Collembola, Entomobryidae), P. lafargensis sp. n. and P. cementensis sp. n., have been found in Castilla-La Mancha, where the number of citations of this genus is very few.Se han encontrado dos nueva especies de Pseudosinella (Collembola, Entomobryidae), P. lafargensis sp. n. y P. cementensis sp. n., en Castilla-La Mancha, en donde el número de citas de este género es muy reducido

Nueva especie de Pseudosinella Schaeffer, 1897 de la Península Ibérica (Collembola, Entomobryidae)

A new species of Pseudosinella, P. soriensis sp. n. is described and a new key to worldwide species of the petterseni group, to which the new species belongs, is made.Se describe una nueva especie de Pseudosinella de la Península Ibérica, P. soriensis sp. n., al mismo tiempo que se da una clave de todas las especies del grupo petterseni, al que pertenece la especie

Las comunidades de insectos del Parque Regional de la Cuenca Alta del Manzanares (centro de España): estado de conservación

The Parque Regional de la Cuenca Alta del Manzanares (PRCAM) is a protected area at the North of Madrid. Eight sampling sites were selected representing different ecosystems and land uses. In these sites we studied the communities of four insect groups: Collembolla, Chrysomelida, Curculionoidea and Papilionoidea and Hesperioidea. The objetive of the study was to assess the conservation status of the Park ecosystems and the paralelism of the results in these four insect groups. The results show that the Park ecosystems are heavily disturbed. The lowland areas being damaged to a greater extent. On the other hand the four groups have a different behaviour in similar conditions. This shows the importance of gathering information from different groups in order to assess or manage the biological diversity of an area.El Parque Regional de la Cuenca Alta del Manzanares (PRCAM) es un área protegida del norte de Madrid. En el se han elegido ocho puntos representativos de sus ecosistemas y del uso del territorio. En estos puntos se han estudiado las comunidades de cuatro grupos de insectos: Colémbolos, Crisomélidos, Curculiónidos y Mariposas. El objetivo del estudio es valorar el estado de conservación de los ecosistemas del parque, y el grado de paralelismo de la información suministrada por los cuatro grupos de insectos sobre unas mismas áreas. Los resultados indican que los ecosistemas del Parque están muy alterados. El grado de deterioro es mayor en las zonas de menor altitud. Por otro lado las comunidades de estos cuatro grupos de insectos responden de formas distintas ante situaciones idénticas. De ello se deduce la importancia de tener en cuenta varios grupos de organismos a la hora de manejar o valorar la diversidad biológica de un zona

Detection of norovirus in saliva samples from acute gastroenteritis cases and asymptomatic subjects : Association with age and higher shedding in stool

Norovirus infections are a leading cause of acute gastroenteritis outbreaks worldwide and across all age groups, with two main genogroups (GI and GII) infecting humans. The aim of our study was to investigate the occurrence of norovirus in saliva samples from individuals involved in outbreaks of acute gastroenteritis in closed and semiclosed institutions, and its relationship with the virus strain, virus shedding in stool, the occurrence of symptoms, age, and the secretor status of the individual. Epidemiological and clinical information was gathered from norovirus outbreaks occurring in Catalonia, Spain during 2017-2018, and stool and saliva samples were collected from affected and exposed resident individuals and workers. A total of 347 saliva specimens from 25 outbreaks were analyzed. Further, 84% of individuals also provided a paired stool sample. For GII infections, norovirus was detected in 17.9% of saliva samples from symptomatic cases and 5.2% of asymptomatic individuals. Positivity in saliva occurred in both secretors and nonsecretors. None of the individuals infected by norovirus GI was positive for the virus in saliva. Saliva positivity did not correlate with any of the studied symptoms but did correlate with age ≥ 65 years old. Individuals who were positive in saliva showed higher levels of virus shedding in stool. Mean viral load in positive saliva was 3.16 ± 1.08 log10 genome copies/mL, and the predominance of encapsidated genomes was confirmed by propidium monoazide (PMA)xx-viability RTqPCR assay. The detection of norovirus in saliva raises the possibility of oral-to-oral norovirus transmission during the symptomatic phase and, although to a lesser extent, even in cases of asymptomatic infections

Potassium and Sodium Transport in Yeast

[EN] As the proper maintenance of intracellular potassium and sodium concentrations is vital for cell growth, all living organisms have developed a cohort of strategies to maintain proper monovalent cation homeostasis. In the model yeast Saccharomyces cerevisiae, potassium is accumulated to relatively high concentrations and is required for many aspects of cellular function, whereas high intracellular sodium/potassium ratios are detrimental to cell growth and survival. The fact that S. cerevisiae cells can grow in the presence of a broad range of concentrations of external potassium (10 M–2.5 M) and sodium (up to 1.5 M) indicates the existence of robust mechanisms that have evolved to maintain intracellular concentrations of these cations within appropriate limits. In this review, current knowledge regarding potassium and sodium transporters and their regulation will be summarized. 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The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation

WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, will see first light in late 2022. WEAVE comprises a new 2-degree field-of-view prime-focus corrector system, a nearly 1000-multiplex fibre positioner, 20 individually deployable 'mini' integral field units (IFUs), and a single large IFU. These fibre systems feed a dual-beam spectrograph covering the wavelength range 366$-$959\,nm at $R\sim5000$, or two shorter ranges at $R\sim20\,000$. After summarising the design and implementation of WEAVE and its data systems, we present the organisation, science drivers and design of a five- to seven-year programme of eight individual surveys to: (i) study our Galaxy's origins by completing Gaia's phase-space information, providing metallicities to its limiting magnitude for $\sim$3 million stars and detailed abundances for $\sim1.5$ million brighter field and open-cluster stars; (ii) survey $\sim0.4$ million Galactic-plane OBA stars, young stellar objects and nearby gas to understand the evolution of young stars and their environments; (iii) perform an extensive spectral survey of white dwarfs; (iv) survey $\sim400$ neutral-hydrogen-selected galaxies with the IFUs; (v) study properties and kinematics of stellar populations and ionised gas in $z<0.5$ cluster galaxies; (vi) survey stellar populations and kinematics in $\sim25\,000$ field galaxies at $0.3\lesssim z \lesssim 0.7$; (vii) study the cosmic evolution of accretion and star formation using $>1$ million spectra of LOFAR-selected radio sources; (viii) trace structures using intergalactic/circumgalactic gas at $z>2$. Finally, we describe the WEAVE Operational Rehearsals using the WEAVE Simulator.Comment: 41 pages, 27 figures, accepted for publication by MNRA

The wide-field, multiplexed, spectroscopic facility WEAVE : survey design, overview, and simulated implementation

Funding for the WEAVE facility has been provided by UKRI STFC, the University of Oxford, NOVA, NWO, Instituto de Astrofísica de Canarias (IAC), the Isaac Newton Group partners (STFC, NWO, and Spain, led by the IAC), INAF, CNRS-INSU, the Observatoire de Paris, Région Île-de-France, CONCYT through INAOE, Konkoly Observatory (CSFK), Max-Planck-Institut für Astronomie (MPIA Heidelberg), Lund University, the Leibniz Institute for Astrophysics Potsdam (AIP), the Swedish Research Council, the European Commission, and the University of Pennsylvania.WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, will see first light in late 2022. WEAVE comprises a new 2-degree field-of-view prime-focus corrector system, a nearly 1000-multiplex fibre positioner, 20 individually deployable 'mini' integral field units (IFUs), and a single large IFU. These fibre systems feed a dual-beam spectrograph covering the wavelength range 366-959 nm at R ∼ 5000, or two shorter ranges at R ∼ 20,000. After summarising the design and implementation of WEAVE and its data systems, we present the organisation, science drivers and design of a five- to seven-year programme of eight individual surveys to: (i) study our Galaxy's origins by completing Gaia's phase-space information, providing metallicities to its limiting magnitude for ∼ 3 million stars and detailed abundances for ∼ 1.5 million brighter field and open-cluster stars; (ii) survey ∼ 0.4 million Galactic-plane OBA stars, young stellar objects and nearby gas to understand the evolution of young stars and their environments; (iii) perform an extensive spectral survey of white dwarfs; (iv) survey  ∼ 400 neutral-hydrogen-selected galaxies with the IFUs; (v) study properties and kinematics of stellar populations and ionised gas in z 1 million spectra of LOFAR-selected radio sources; (viii) trace structures using intergalactic/circumgalactic gas at z > 2. Finally, we describe the WEAVE Operational Rehearsals using the WEAVE Simulator.PostprintPeer reviewe

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