Una Especie Nueva de Tillus Olivier, 1790 (Coleoptera Cleridae) de la Peninsula Ibérica

6 páginas, 2 figuras et al..[EN] Tillus ibericus sp. nov. is described from the Comunidad Autónoma de Madrid (Spain) and it is compared to the western Palaearctic species of the genus Tillus Olivier, 1790. Tillus ibericus is easily distinguished from all other species of the genus by the structure of the elytral sculpture and its characteristic coloration. This new species shares a general habitus and characters from the antennae, and general body stucture with T. flabellicornis Fairmaire, 1866, a species from northern Africa. All preexisting records of T. flabellicornis in the Iberian Peninsula correspond to T. ibericus.[ES]Se describe Tillus ibericus sp. nov. de la Comunidad Autónoma de Madrid (España) y se compara con las otras especies del género Tillus Olivier, 1790 de la región Paleártica occidental. Tillus ibericus se distingue con facilidad de las especies próximas por la estructura del punteado elitral y por su coloración característica. La especie nueva comparte un aspecto general y caracteres de la estructura del cuerpo y de las antenas con T. flabellicornis Fairmaire, 1866 del Norte de África. Todas las citas anteriores de T. flabellicornis de la Península Ibérica corresponden a T. ibericus sp. nov.Peer reviewe

Designación del neotipo de Ochodaeus montanus Fuente (Coleoptera, Ochodaeidae)

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Caracterización taxonómica, distribución y primeros registros europeos de Apalus cinctus (Pic, 1896) (Coleoptera, Meloidae)

In this study we clarify the taxonomic status and geographic distribution of Apalus cinctus (Pic, 1896), a Mediterranean species included in the group of Apalus bimaculatus (Linnaeus, 1760). Apalus cinctus was only known from a few North African localities mentioned in the original description, and was considered of uncertain taxonomic status. The review of detailed photographs of the type specimen and the study of recently captured specimens allow us to discuss its taxonomic position and to define its diagnostic characters, validating its specific status. Capture or observation of specimens assignable to Apalus cinctus in continental Spain (León, Zamora and Huesca), extends the geographic range of the species considerably, including it within the European Fauna. We question the presence of Apalus bimaculatus in the Iberian peninsula and North Africa, suggesting that it is possibly replaced by A. cinctus.En este estudio se clarifica el estatus taxonómico y la distribución geográfica de Apalus cinctus (Pic, 1896), especie mediterránea que se integra en el grupo de Apalus bimaculatus (Linnaeus, 1760). Apalus cinctus sólo se conocía por su descripción original a partir de algunas localidades norteafricanas y se consideraba como un taxon con estatus taxonómico incierto. El examen de fotografías detalladas del tipo de Apalus cinctus y el estudio de nuevo material capturado recientemente nos permite discutir su posición taxonómica y definir sus caracteres diagnósticos, validando su estatus específico. La captura u observación de ejemplares asignables a Apalus cinctus en España continental (León, Zamora y Huesca), amplía considerablemente la distribución de la especie y permite incluirla dentro de la Fauna Europea. Se cuestiona la presencia de Apalus bimaculatus en la Península Ibérica y en el Norte de África, donde posiblemente sea reemplazada por A. cinctus

Estudio de las características físico–químicas de las aguas del Balneario de San Nicolás (Almería)

Las aguas del balneario de San Nicolás, de Alhama de Almería, fueron declaradas de utilidad pública por Real Orden de 16 de mayo de 1877, bajo la denominación de aguas de Alhama la Seca; en 1928 fue confirmada la utilidad pública de las aguas minero-medicinales de Alhama de Almería. Existen diferentes estudios de las aguas de este balneario, especialmente en el siglo XIX, en los que se comenta el tipo de aguas y su clasificación, y la mayoría de autores hacen referencia a una temperatura de las mismas superior a 40ºC. Se analizaron las aguas correspondientes al origen del manantial, a una de las bañeras y a la fuente que se encuentra en uno de los patios. Las aguas surgen a una temperatura de 48ºC; su pH es cercano a 8. El residuo seco, a 180ºC, es superior a 600 mg/L. La dureza es cercana a 500 mg/L de CaCO3, y predomina el calcio, cuyo contenido es ligeramente superior a 100 mg/L. De los aniones, bicarbonatos y sulfatos son mayoritarios; el contenido de estos últimos, ligeramente superior a los 200 mg/L, permite considerar estas aguas como sulfatadas. Los fluoruros se encuentran en cantidad ligeramente superior a 1 mg/L, lo que indica que se pueden considerar fluoradas. Los análisis realizados nos indican que se trata de aguas hipertermales, de mineralización media, muy duras, sulfatadas y fluoradas

TOI-1235 b: A Keystone Super-Earth For Testing Radius Valley Emergence Models Around Early M Dwarfs

Small planets on close-in orbits tend to exhibit envelope mass fractions of either effectively zero or up to a few percent depending on their size and orbital period. Models of thermally driven atmospheric mass loss and of terrestrial planet formation in a gas-poor environment make distinct predictions regarding the location of this rocky/nonrocky transition in period–radius space. Here we present the confirmation of TOI-1235 b (P = 3.44 days, ${r}_{{\rm{p}}}={1.738}_{-0.076}^{+0.087}$ ${R}_{\oplus }$), a planet whose size and period are intermediate between the competing model predictions, thus making the system an important test case for emergence models of the rocky/nonrocky transition around early M dwarfs (R s = 0.630 ± 0.015 ${R}_{\odot }$, M s = 0.640 ± 0.016 ${M}_{\odot }$). We confirm the TESS planet discovery using reconnaissance spectroscopy, ground-based photometry, high-resolution imaging, and a set of 38 precise radial velocities (RVs) from HARPS-N and HIRES. We measure a planet mass of ${6.91}_{-0.85}^{+0.75}$ ${M}_{\oplus }$, which implies an iron core mass fraction of ${20}_{-12}^{+15}$% in the absence of a gaseous envelope. The bulk composition of TOI-1235 b is therefore consistent with being Earth-like, and we constrain an H/He envelope mass fraction to be \u3c0.5% at 90% confidence. Our results are consistent with model predictions from thermally driven atmospheric mass loss but not with gas-poor formation, suggesting that the former class of processes remains efficient at sculpting close-in planets around early M dwarfs. Our RV analysis also reveals a strong periodicity close to the first harmonic of the photometrically determined stellar rotation period that we treat as stellar activity, despite other lines of evidence favoring a planetary origin ($P={21.8}_{-0.8}^{+0.9}$ days, ${m}_{{\rm{p}}}\sin i={13.0}_{-5.3}^{+3.8}$ ${M}_{\oplus }$) that cannot be firmly ruled out by our data

Comparative study of enteric viruses, coliphages and indicator bacteria for evaluating water quality in a tropical high-altitude system

<p>Abstract</p> <p>Background</p> <p>Bacteria used as indicators for pathogenic microorganisms in water are not considered adequate as enteric virus indicators. Surface water from a tropical high-altitude system located in Mexico City that receives rainwater, treated and non-treated wastewater used for irrigation, and groundwater used for drinking, was studied.</p> <p>Methods</p> <p>The presence of enterovirus, rotavirus, astrovirus, coliphage, coliform bacteria, and enterococci was determined during annual cycles in 2001 and 2002. Enteric viruses in concentrated water samples were detected by reverse transcriptase-polymerase chain reaction (RT-PCR). Coliphages were detected using the double agar layer method. Bacteria analyses of the water samples were carried out by membrane filtration.</p> <p>Results</p> <p>The presence of viruses and bacteria in the water used for irrigation showed no relationship between current bacterial indicator detection and viral presence. Coliphages showed strong association with indicator bacteria and enterovirus, but weak association with other enteric viruses. Enterovirus and rotavirus showed significant seasonal differences in water used for irrigation, although this was not clear for astrovirus.</p> <p>Conclusion</p> <p>Coliphages proved to be adequate faecal pollution indicators for the irrigation water studied. Viral presence in this tropical high-altitude system showed a similar trend to data previously reported for temperate zones.</p

Early Release Science of the Exoplanet WASP-39b with JWST NIRSpec G395H

Measuring the abundances of carbon and oxygen in exoplanet atmospheres is considered a crucial avenue for unlocking the formation and evolution of exoplanetary systems. Access to an exoplanet's chemical inventory requires high-precision observations, often inferred from individual molecular detections with low-resolution space-based and high-resolution ground-based facilities. Here we report the medium-resolution (R$\sim$600) transmission spectrum of an exoplanet atmosphere between 3-5 $\mu$m covering multiple absorption features for the Saturn-mass exoplanet WASP-39b, obtained with JWST NIRSpec G395H. Our observations achieve 1.46x photon precision, providing an average transit depth uncertainty of 221 ppm per spectroscopic bin, and present minimal impacts from systematic effects. We detect significant absorption from CO$_2$ (28.5$\sigma$) and H$_2$O (21.5$\sigma$), and identify SO$_2$ as the source of absorption at 4.1 $\mu$m (4.8$\sigma$). Best-fit atmospheric models range between 3 and 10x solar metallicity, with sub-solar to solar C/O ratios. These results, including the detection of SO$_2$, underscore the importance of characterising the chemistry in exoplanet atmospheres, and showcase NIRSpec G395H as an excellent mode for time series observations over this critical wavelength range.Comment: 44 pages, 11 figures, 3 tables. Resubmitted after revision to Natur

Guidelines for the use and interpretation of assays for monitoring autophagy (4th edition)1.

In 2008, we published the first set of guidelines for standardizing research in autophagy. Since then, this topic has received increasing attention, and many scientists have entered the field. Our knowledge base and relevant new technologies have also been expanding. Thus, it is important to formulate on a regular basis updated guidelines for monitoring autophagy in different organisms. Despite numerous reviews, there continues to be confusion regarding acceptable methods to evaluate autophagy, especially in multicellular eukaryotes. Here, we present a set of guidelines for investigators to select and interpret methods to examine autophagy and related processes, and for reviewers to provide realistic and reasonable critiques of reports that are focused on these processes. These guidelines are not meant to be a dogmatic set of rules, because the appropriateness of any assay largely depends on the question being asked and the system being used. Moreover, no individual assay is perfect for every situation, calling for the use of multiple techniques to properly monitor autophagy in each experimental setting. Finally, several core components of the autophagy machinery have been implicated in distinct autophagic processes (canonical and noncanonical autophagy), implying that genetic approaches to block autophagy should rely on targeting two or more autophagy-related genes that ideally participate in distinct steps of the pathway. Along similar lines, because multiple proteins involved in autophagy also regulate other cellular pathways including apoptosis, not all of them can be used as a specific marker for bona fide autophagic responses. Here, we critically discuss current methods of assessing autophagy and the information they can, or cannot, provide. Our ultimate goal is to encourage intellectual and technical innovation in the field