From stellar to planetary composition: Galactic chemical evolution of Mg/Si mineralogical ratio

Aims. The main goal of this work is to study element ratios that are important for the formation of planets of different masses. Methods. We study potential correlations between the existence of planetary companions and the relative elemental abundances of their host stars. We use a large sample of FGK-type dwarf stars for which precise Mg, Si, and Fe abundances have been derived using HARPS high-resolution and high-quality data. Results. A first analysis of the data suggests that low-mass planet host stars show higher [Mg/Si] ratios, while giant planet hosts present [Mg/Si] that is lower than field stars. However, we found that the [Mg/Si] ratio significantly depends on metallicity through Galactic chemical evolution. After removing the Galactic evolution trend only the difference in the [Mg/Si] elemental ratio between low-mass planet hosts and non-hosts was present in a significant way. These results suggest that low-mass planets are more prevalent around stars with high [Mg/Si]. Conclusions. Our results demonstrate the importance of Galactic chemical evolution and indicate that it may play an important role in the planetary internal structure and composition. The results also show that abundance ratios may be a very relevant issue for our understanding of planet formation and evolution.

Megabenthic communities in the waters around Svalbard during POLARSTERN cruise ARK-VIII/2 (EPOS II)

Composition and distribution of megabenthic communities around Svalbard were investigated in June/July 1991 with 20 Agassiz trawl and 5 bottom trawl hauls in depths between 100 and 2100 m. About 370 species, ranging from sponges to fish, were identified in the catches. Species numbers per station ranged from 21 to 86. Brittle stars, such as Ophiacantha bidentata, Ophiura sarsi and Ophiocten sericeum, were most important in terms of constancy and relative abundance in the catches. Other prominent faunal elements were eunephthyid alcyonarians, bivalves, shrimps, sea stars and fish (Gadidae, Zoarcidae, Cottidae). Multivariate analyses of the species and environmental data sets showed that the spatial distribution of the megabenthos was characterized by a pronounced depth zonation: abyssal, bathyal, off-shore shelf and fjordic communities were discriminated. However, a gradient in sediment properties, especially the organic carbon content, seemed to superimpose on the bathymetric pattern. Both main factors are interpreted as proxies of the average food availability, which is, hence, suggested to have the strongest influence in structuring megabenthic communities off Svalbard.

Validated sample ages from 823 EPD sites

The number of well-dated pollen diagrams in Europe has increased considerably over the last 30 years and many of them have been submitted to the European Pollen Database (EPD). This allows for the construction of increasingly precise maps of Holocene vegetation change across the continent. Chronological information in the EPD has been expressed in uncalibrated radiocarbon years, and most chronologies to date are based on this time scale. Here we present new chronologies for most of the datasets stored in the EPD based on calibrated radiocarbon years. Age information associated with pollen diagrams is often derived from the pollen stratigraphy itself or from other sedimentological information. We reviewed these chronological tie points and assigned uncertainties to them. The steps taken to generate the new chronologies are described and the rationale for a new classification system for age uncertainties is introduced. The resulting chronologies are fit for most continental-scale questions. They may not provide the best age model for particular sites, but may be viewed as general purpose chronologies. Taxonomic particularities of the data stored in the EPD are explained. An example is given of how the database can be queried to select samples with appropriate age control as well as the suitable taxonomic level to answer a specific research question.

¿Quién protagoniza y cómo la historia escolar? La enseñanza de la historia de los otros y las otras en los textos de estudio de Historia de Chile de educación primaria

El currículum de historia escolar y los libros de texto no han evolucionado al ritmo de la investigación histórica. Así puede comprobarse analizando quiénes son los seleccionados para protagonizar los hechos y los procesos históricos. Ni en el currículum ni en los manuales de didáctica de la historia ni en los libros de texto se concede la importancia que se debería a las mujeres, los niños y niñas, a los miembros de cualquier minoría, a los pobres, a los homosexuales, a aquellas personas y grupos que no pertenecen a la elite y a la minoría dirigente. En este trabajo presentamos algunas reflexiones sobre los protagonistas, sobre los actores, de la historia desde la historiografía y desde la didáctica de la historia y analizamos su tratamiento en libros de texto de historia de la educación primaria chilena

¿Quién protagoniza y cómo la historia escolar? La enseñanza de la historia de los otros y las otras en los textos de estudio de Historia de Chile de educación primaria

El currículum de historia escolar y los libros de texto no han evolucionado al ritmo de la investigación histórica. Así puede comprobarse analizando quiénes son los seleccionados para protagonizar los hechos y los procesos históricos. Ni en el currículum ni en los manuales de didáctica de la historia ni en los libros de texto se concede la importancia que se debería a las mujeres, los niños y niñas, a los miembros de cualquier minoría, a los pobres, a los homosexuales, a aquellas personas y grupos que no pertenecen a la elite y a la minoría dirigente. En este trabajo presentamos algunas reflexiones sobre los protagonistas, sobre los actores, de la historia desde la historiografía y desde la didáctica de la historia y analizamos su tratamiento en libros de texto de historia de la educación primaria chilena

¿Quién protagoniza y cómo la historia escolar? La enseñanza de la historia de los otros y las otras en los textos de estudio de Historia de Chile de educación primaria

El currículum de historia escolar y los libros de texto no han evolucionado al ritmo de la investigación histórica. Así puede comprobarse analizando quiénes son los seleccionados para protagonizar los hechos y los procesos históricos. Ni en el currículum ni en los manuales de didáctica de la historia ni en los libros de texto se concede la importancia que se debería a las mujeres, los niños y niñas, a los miembros de cualquier minoría, a los pobres, a los homosexuales, a aquellas personas y grupos que no pertenecen a la elite y a la minoría dirigente. En este trabajo presentamos algunas reflexiones sobre los protagonistas, sobre los actores, de la historia desde la historiografía y desde la didáctica de la historia y analizamos su tratamiento en libros de texto de historia de la educación primaria chilena

Seawater carbonate chemistry, mass, size and regenerative capacity of Luidia clathrata during experiments, 2011

The present study examines sublethal effects of near-future (year 2100) ocean acidification (OA) on regenerative capacity, biochemical composition, and behavior of the sea star Luidia clathrata, a predominant predator in sub-tropical soft-bottom habitats. Two groups of sea stars, each with two arms excised, were maintained on a formulated diet in seawater bubbled with air alone (pH 8.2, approximating a pCO2 of 380 µatm) or with a controlled mixture of air/C02 (pH 7.8, approximating a pCO2 of 780 µatm). Arm length, total body wet weight, and righting responses were measured weekly. After 97 days, a period of time sufficient for 80% arm regeneration, pyloric caecal indices, and protein, carbohydrate, lipid, and ash levels were determined for body wall and pyloric caecal tissues of intact and regenerating arms of individuals held in both seawater pH treatments. The present study indicates that predicted near-term levels of ocean acidification (seawater pH 7.8) do not significantly impact whole animal growth, arm regeneration rates, biochemical composition, or righting behavior in this common soft bottom sea star.

Biogenic and environmental fluctuations of temperature and pH in a novel mesocosm concept ("Kiel Outdoor Benthocosms") April 2013 to September 2014

The Kiel Outdoor Benthocosm infrastructure (Kiel, Germany,N 54°19.8'; E 010°09.0') allows combining natural in-situ fluctuations on all environmental variables with the controlled manipulation of treatment factors. The environmental fluctuations are admitted by a continuous flow-through of fjord water. The treatment is applied by delta-treatments which shift the mean of target variables (temperature and pH in this case) while maintaining the frequency and amplitude of natural fluctuations. The data presented here show the treatment levels and the continuously logged temperature and pH conditions in the experimental tanks. The dynamics of temperature and pH are driven by (i) in situ variability, (ii) the treatments imposed and (iii) the biology of the biota in the tanks. These contained macroalgal communities with associated mesograzers, mussels, and sea stars. The data set comprised 5 experimental runs: spring experiment (4.4.-19.6.2013), summer experiment 1 (4.7.-17.9.2013), autumn experiment (10.10-17.12.2013), winter experiment (16.1. - 1.4.2014), summer experiment 2 (10.7. - 26.9.2014).

The VLT/NaCo large program to probe the occurrence of exoplanets and brown dwarfs at wide orbits II. Survey description, results, and performances

Context. Young, nearby stars are ideal targets for direct imaging searches for giant planets and brown dwarf companions. After the first-imaged planet discoveries, vast efforts have been devoted to the statistical analysis of the occurence and orbital distributions of giant planets and brown dwarf companions at wide (>= 5-6 AU) orbits. Aims. In anticipation of the VLT/SPHERE planet-imager, guaranteed-time programs, we have conducted a preparatory survey of 86 stars between 2009 and 2013 to identify new faint comoving companions to ultimately analyze the occurence of giant planets and brown dwarf companions at wide (10-2000 AU) orbits around young, solar-type stars. Methods. We used NaCo at VLT to explore the occurrence rate of giant planets and brown dwarfs between typically 0.1 and 8 ''. Diffraction-limited observations in H-band combined with angular differential imaging enabled us to reach primary star-companion brightness ratios as small as 10(-6) at 1.5 ''. Repeated observations at several epochs enabled us to discriminate comoving companions from background objects. Results. During our survey, twelve systems were resolved as new binaries, including the discovery of a new white dwarf companion to the star HD8049. Around 34 stars, at least one companion candidate was detected in the observed field of view. More than 400 faint sources were detected; 90% of them were in four crowded fields. With the exception of HD8049 B, we did not identify any new comoving companions. The survey also led to spatially resolved images of the thin debris disk around HD61005 that have been published earlier. Finally, considering the survey detection limits, we derive a preliminary upper limit on the frequency of giant planets for the semi-major axes of [10, 2000] AU: typically less than 15% between 100 and 500 AU and less than 10% between 50 and 500 AU for exoplanets that are more massive than 5 M-Jup and 10 M-Jup respectively, if we consider a uniform input distribution and a confidence level of 95%. Conclusions. The results from this survey agree with earlier programs emphasizing that massive, gas giant companions on wide orbits around solar-type stars are rare. These results will be part of a broader analysis of a total of similar to 210 young, solar-type stars to bring further statistical constraints for theoretical models of planetary formation and evolution.

From regression estimates to document tables: output formatting using -estout-

Postestimation processing and formatting of regression estimates for input into document tables are tasks that many of us have to do. However, processing results by hand can be laborious, and is vulnerable to error. There are therefore many benefits to automation of these tasks while at the same time retaining user flexibility in terms of output format. The estout package meets these needs. estout assembles a table of coefficients, "significance stars", summary statistics, standard errors, t/z statistics, p-values, confidence intervals, and other statistics calculated for up to twenty models previously fitted and stored by estimates store. It then writes the table to the Stata log and/or to a text file. The estimates are formatted optionally in several styles: html, LaTeX, or tab-delimited (for input into MS Excel or Word). There are a large number of options regarding which output is formatted and how. This talk will take users through a range of examples, from relatively basic simple applications to complex ones.

The Islamic Crossed-Arch Domes in Cordoba: Geometry and Structural Analysis of the “Capilla de Villaviciosa”

Crossed-arch domes are a singular type of ribbed vaults. Their characteristic feature is that the ribs that form the vault are intertwined, forming polygons or stars, leaving an empty space in the centre. The earliest known vaults of this type are found in the Great Mosque of Córdoba, built ca. 960 a.C. The type spread through Spain, and the north of Africa in the 10th to the 16th Centuries, and was used by Guarini and Vittone in the 17th and 18th Centuries in Italy. However, it was used only in a few buildings. Though the literature about the structural behaviour of ribbed Gothic vaults is extensive, so far no structural analysis of crossed arch domes has been made. The purpose of this work is, first to show the way to attack such an analysis within the frame of Modern Limit Analysis of Masonry Structures (Heyman 1995), and then to apply the approach to study the stability of the dome of the Capilla de Villaviciosa. The work may give some clues to art and architectural historians to understand better the origin and development of Islamic dome architecture.

Sistemas de control de roturas en presas y caracterización de sistemas hidráulicos

Este proyecto nace de la necesidad de automatizar el estudio de sistemas hidráulicos y de control de roturas en presas. Para realizar el estudio de sistemas hidráulicos se usarán un número indeterminado de sensores de nivel, presión y caudal. El número de sensores que se pueden utilizar viene determinado por el material disponible. Estos sensores se conectarán a unas tarjetas de National Instruments modelo NI 9208 y éstas a su vez a un chasis modelo CompactDAQ NI-9174 con cuatro ranuras. Conectando este chasis al ordenador podremos obtener los datos provenientes de los sensores. También se podrá controlar una válvula para determinar la cantidad de agua que fluye en nuestro experimento. Está válvula está conectada a una tarjeta NI-9264 que se conectará al chasis en su última posición Para detectar y estudiar posibles roturas en presas se dispone de un motor y un láser con los cuales se puede barrer la superficie de una presa y obtener una imagen en tres dimensiones de la misma procesando los datos provenientes del laser. Para recoger los datos de los sensores y controlar una válvula se ha desarrollado una aplicación utilizando LabVIEW, un programa creado por National Instruments. Para poder controlar el motor y el láser se parte de una aplicación que ya estaba realizada en LabVIEW. El objetivo ha sido detectar y corregir una serie de errores en la misma. Dentro del proyecto, además de la explicación detallada de la aplicación para los sensores y la válvula, y las pruebas realizadas para detectar y corregir los errores de la aplicación del láser y el motor, existe: una breve introducción a la programación en LabVIEW, la descripción de los pasos realizados para el conexionado de los sensores con las tarjetas, los manuales de usuario de las aplicaciones y la descripción de los equipos utilizados. This project stars from the need to automate the study of hydraulic systems and control dam breaks. For the study of hydraulic systems it will be used an unspecified number of level, pressure and flow sensors. The number of sensors that can be used is determined by the available material. These sensors are connected to a NI 9208 National Instruments target and these cards to a NI-9174 CompactDAQ chassis with four slots. Connecting the chassis to a computer we will obtain data from the sensors. We also can control a valve to determine the amount of water flowing in our experiment. This valve is connected to a NI-9264 card and this card to the last position of the chassis. To detect and study dams breakage it used a motor and a laser. With these two devices we can scan the surface of a dam and obtain a three-dimensional image processing data from the laser. To collect data from the sensors and control the valve it has developed an application using LabVIEW, a program created by National Instruments. To control the motor and the laser it is used an application that was already created using LabVIEW. The aim of this part has been detect and correct a number of errors in this application. Within the project, in addition to the detailed explanation of the application for sensors and valve, and tests to detect and correct errors in the application of lasers and the motor, there is: a brief introduction to programming in LabVIEW, the description of the steps taken for connecting the sensors with cards, user manuals and application description of the equipment used.

Can Jupiters be found by monitoring Galactic bulge microlensing events from northern sites?

In 1998 the EXPORT team monitored microlensing event light curves using a charge-coupled device (CCD) camera on the IAC 0.8-m telescope on Tenerife to evaluate the prospect of using northern telescopes to find microlens anomalies that reveal planets orbiting the lens stars. The high airmass and more limited time available for observations of Galactic bulge sources make a northern site less favourable for microlensing planet searches. However, there are potentially a large number of northern 1-m class telescopes that could devote a few hours per night to monitor ongoing microlensing events. Our IAC observations indicate that accuracies sufficient to detect planets can be achieved despite the higher airmass.

Biosensing comparison between different geometries based on vertical submicron-structrures made of SU-8 resist

Previous work of the research group [1-4] demonstrated the viability of using periodic lattices of micro and nanopillars, called Bio-photonic sensing Cells (BICELLs), as an optical biosensor vertically characterized by visible spectrometry. Also we have studied theoretically [5] the performance of the BICELLs by 2D and 3D simulation in orde r to optimize the biosensing response. In this work we present the fabrication and biosensing comparison of different geometrical parameters on periodic lattices of pillars in order to discuss theoretical conclusions with these results. In this way, we have explored the biosensing response of other patter ns such as crosses, stars, cylinders, concentrical cylinders (Figure 1). Also we introduced a novel method to test the BICELLs in a cost-effective way by using an ultra-thin film of SU-8 spin-coated onto the patterns to reproduce the effect of a biofilm attached to the biosensor surface. Finally we have tested the biosensing response of the different geometries by the well-known Bovine Serum Albumin (BSA) immunoassay and compared with the theoretical simulation.