Visible and near-infrared observations of asteroid 2012 DA14 during its closest approach of February 15, 2013

Near-Earth asteroid 2012 DA14 made its closest approach on February 15, 2013, when it passed at a distance of 27,700 km from the Earth's surface. It was the first time an asteroid of moderate size was predicted to approach that close to the Earth, becoming bright enough to permit a detailed study from ground-based telescopes. Asteroid 2012 DA14 was poorly characterized before its closest approach. We acquired data using several telescopes on four Spanish observatories: the 10.4m Gran Telescopio Canarias (GTC) and the 3.6m Telescopio Nazionale Galileo (TNG), both in the El Roque de los Muchachos Observatory (ORM, La Palma); the 2.2m CAHA telescope, in the Calar Alto Observatory (Almeria); the f/3 0.77m telescope in the La Hita Observatory (Toledo); and the f/8 1.5m telescope in the Sierra Nevada Observatory (OSN, Granada). We obtained visible and near-infrared color photometry, visible spectra and time-series photometry. Visible spectra together with color photometry of 2012 DA14 show that it can be classified as an L-type asteroid, a rare spectral type with a composition similar to that of carbonaceous chondrites. The time-series photometry provides a rotational period of 8.95 +- 0.08 hours after the closest approach, and there are indications that the object suffered a spin-up during this event. The large amplitude of the light curve suggests that the object is very elongated and irregular, with an equivalent diameter of around 18m. We obtain an absolute magnitude of H_R = 24.5 +- 0.2, corresponding to H_V = 25.0 +- 0.2. The GTC photometry also gives H_V = 25.29 +- 0.14. Both values agree with the value listed at the Minor Planet Center shortly after discovery. From the absolute photometry, together with some constraints on size and shape, we compute a geometric albedo of p_V = 0.44 +- 0.20, which is slightly above the range of albedos known for L-type asteroids (0.082 - 0.405).Comment: 7 pages, 4 figures, 1 table. Accepted in A&A (June 17 2013

Influencia del cereal y el nivel de inclusión de fibra en el pienso sobre la productividad en pollitas de 0 a 17 semanas de edad.

La fibra ha sido considerada como un diluyente del pienso en monogástricos con efectos negativos sobre consumo y la digestibilidad de los nutrientes (Jansen and Carré, 1985). Sin embargo, estudios recientes (Mateos et al., 2012) han mostrado que la inclusión de cantidades moderadas de fibra en el pienso podría mejorar tanto la digestibilidad de los nutrientes como el crecimiento de las aves. La inclusión de fibra en piensos para broilers podría incrementar el tiempo de retención de la digesta en la parte superior del tracto digestivo, estimulando el funcionamiento de la molleja (Hetland et al. 2005) y la producción de HCl en el proventrículo (Duke, 1986). Un descenso del pH de la molleja favorece la producción de pepsina e incrementa la solubilidad de las sales minerales (Jiménez-Moreno et al. 2009). Por lo tanto, la inclusión de cantidades adecuadas de fibra podría beneficiar el desarrollo del tracto gastrointestinal (Mateos et al., 2012). Sin embargo, la información disponible sobre los efectos beneficiosos de la fibra dietética en pollitas es escasa (Frikha et al., 2009). De hecho, los autores no han encontrado ningún estudio publicado sobre los efectos de la inclusión de fibra sobre el crecimiento de pollitas de 0 a 17 sem de edad. La influencia de fuentes de fibra tales como la cascarilla de avena, pulpa de remolacha (PRE) o cascarilla de soja sobre el desarrollo del tracto gastrointestinal ha sido bien estudiada en broilers (González-Alvarado el al., 2010). Sin embargo, la información disponible sobre el uso de paja de cereales (PCE) en dietas para avicultura es muy limitada; aun siendo una fuente de fibra abundante. La hipótesis del presente ensayo fue que la inclusión de cantidades moderadas de fibra en piensos de pollitas podría mejorar el rendimiento productivo con una mejora de la utilización de los nutrientes. El objetivo del presente trabajo fue estudiar el efecto de la inclusión de diversas fuentes de fibra a diferentes niveles en el pienso de pollitas sobre los rendimientos productivos de 0 a 17 sem de edad

Influencia e la inclusión de fibra en el pienso sobre los rendimientos produtivos de pollitas rubias de 1 a 35 días de edad.

La fibra dietética representa la fracción indigestible de los ingredientes del pienso por lo que diluye el contenido en nutrientes del mismo (Rougière y Carré, 2010). Además, un aumento en el nivel de fibra del pienso puede reducir el consumo voluntario (Sklan et al., 2003), alterar el perfil de la flora gastrointestinal y aumentar la incidencia de procesos entéricos (Janssen and Carré, 1985). Sin embargo, estudios recientes muestran que la inclusión de ciertas fuentes de fibras a niveles adecuados podrían mejorar los rendimientos productivos y reducir la incidencia de problemas digestivos en aves (Mateos, 2012). En broilers, la inclusión de fibra adicional en el pienso mejoró la fisiología digestiva, aumentando el tamaño de la molleja, reduciendo el pH de la digesta de este órgano (Sacranie et al., 2012) y mejorando de los rendimientos productivos (González-Alvarado et al., 2010). Fuentes de fibra insoluble tales como la cascarilla de avena (CAV), la cascarilla de girasol (CGI) y la paja de cereales (PCE) podrían mejorar la fisiología del tracto gastrointestinal (TGI) y la digestibilidad de ciertos nutrientes cuando se incluyen en el pienso en cantidades moderadas (Hetland et al., 2003). Por otro lado, fuentes de fibra soluble, tal como la pulpa de remolacha (PRE), incrementan la viscosidad intestinal, lo que podría reducir el consumo de pienso (Jiménez-Moreno et al., 2010). Los autores no han encontrado estudio alguno sobre los efectos de la inclusión de fibra adicional en el pienso sobre los rendimientos productivos de pollitas comerciales. El objetivo del presente trabajo fue estudiar el efecto de incluir diversas fuentes de fibra a diferentes niveles en el pienso sobre los rendimientos productivos de pollitas de 1 a 35 d de edad

A semantic interoperability approach to support integration of gene expression and clinical data in breast cancer

[Abstract] Introduction. The introduction of omics data and advances in technologies involved in clinical treatment has led to a broad range of approaches to represent clinical information. Within this context, patient stratification across health institutions due to omic profiling presents a complex scenario to carry out multi-center clinical trials. Methods. This paper presents a standards-based approach to ensure semantic integration required to facilitate the analysis of clinico-genomic clinical trials. To ensure interoperability across different institutions, we have developed a Semantic Interoperability Layer (SIL) to facilitate homogeneous access to clinical and genetic information, based on different well-established biomedical standards and following International Health (IHE) recommendations. Results. The SIL has shown suitability for integrating biomedical knowledge and technologies to match the latest clinical advances in healthcare and the use of genomic information. This genomic data integration in the SIL has been tested with a diagnostic classifier tool that takes advantage of harmonized multi-center clinico-genomic data for training statistical predictive models. Conclusions. The SIL has been adopted in national and international research initiatives, such as the EURECA-EU research project and the CIMED collaborative Spanish project, where the proposed solution has been applied and evaluated by clinical experts focused on clinico-genomic studies.Instituto de Salud Carlos III, PI13/02020Instituto de Salud Carlos III, PI13/0028

Galaxy interactions I: Major and minor mergers

We study galaxy pair samples selected from the Sloan Digital Sky Survey (SDSS-DR7) and we perform an analysis of minor and major mergers with the aim of investigating the dependence of galaxy properties on interactions. We build a galaxy pair catalog requiring rp < 25 kpc h-1 and Delta V < 350 km s-1 within redshift z<0.1. By visual inspection of SDSS images we removed false identifications and we classify the interactions into three categories: pairs undergoing merging, M; pairs with evident tidal features, T; and non disturbed, N. We also divide the pair sample into minor and major interactions according to the luminosity ratio of the galaxy members. We study star formation activity through colors and star formation rates. We find that 10% of the pairs are classified as M. These systems show an excess of young stellar populations as inferred from the Dn(4000) spectral index, colors, and star formation rates of the member galaxies, an effect which we argue, is directly related to the ongoing merging process. We find 30% of the pairs exhibiting tidal features (T pairs) with member galaxies showing evidence of old stellar populations. Regardless of the color distribution, we find a prominent blue peak in the strongest mergers, while pairs with tidal signs under a minor merger show a strong red peak. Therefore, our results show that galaxy interactions are important in driving the evolution of galaxy bimodality. By adding stellar masses and star formation rates of the two members of the pairs, we explore the global efficiency of star formation of the pairs as a whole. We find that, at a given total stellar mass, major mergers are significantly more efficient (a factor 2) in forming new stars, with respect to both minor mergers or a control sample of non-interacting galaxies.Comment: 10 pages, 14 figures, submitted to A&

Preliminary characterization of columnar aerosol properties (AOD-AE) at the saharan tamanrasset (Algeria) station

Postprint (published version

Development and validation of a high performance liquid chromatography-tandem mass spectrometry method for the absolute analysis of 17 alpha D-amino acids in cooked meals

In the nutrition field, there is a lack of understanding about the impact that dietary chiral composition may have on health, especially regarding cooked meals. Chiral amino acids (AAs) are naturally present in food and their proportion may vary quite a lot. Besides, the D-amino acids (D-AAs) are present in very low concentration compared to L-AAs, so very sensitive methods are required for their accurate quantitation. Moreover, some of them have been described as indicators of quality and different food processes. In this research, we propose a robust method for the absolute quantitation and enantiomeric ratio of 17 D-AAs in cooked meals. The AAs were extracted from 1 g of the homogenised meal with methanol, derivatised with (S)-N-(4-nitrophenoxycarbonyl) phenylalanine methoxyethyl ester ((S)-NIFE) and analysed by RP-LC-MS/MS. The separation was carried out with an Acquity BEH C18 (100 mm x 2.1 mm, 1.7 µm) column at 70 ºC, with 10 mmol/L ammonium bicarbonate in water as eluent A and acetonitrile as eluent B at a 0.3 mL/min flow rate in gradient elution. The MS operated in positive electrospray ionisation method in multiple reaction monitoring (MRM) mode. Isotopically labelled AAs were used as internal standards for the quantitation. The method was validated for 17 D-AAs in the cooked food samples in terms of specificity, linearity, precision, accuracy, matrix effect and stability. LLOQ are 2.0 ng/mL for most of them. Additionally, linearity was also studied for L-AAs. After optimization and validation, the method was applied to real breakfast, lunch and dinner samples of cooked meals (n = 18) that were part of a diet with a very high concordance with WHO dietary guidelines. Level of concentration of major and minor D-AAs have been described per total daily intake and within each of the three main meals. This method can be used for quality control purposes as well as to investigate the role of chiral composition in food and clinical outcomes

Extreme Starbursts in the Local Universe

The "Extreme starbursts in the local universe" workshop was held at the Insituto de Astrofisica de Andalucia in Granada, Spain on 21-25 June 2010. Bearing in mind the advent of a new generation of facilities such as JWST, Herschel, ALMA, eVLA and eMerlin, the aim of the workshop was to bring together observers and theorists to review the latest results. The purpose of the workshop was to address the following issues: what are the main modes of triggering extreme starbursts in the local Universe? How efficiently are stars formed in extreme starbursts? What are the star formation histories of local starburst galaxies? How well do the theoretical simulations model the observations? What can we learn about starbursts in the distant Universe through studies of their local counterparts? How important is the role of extreme starbursts in the hierarchical assembly of galaxies? How are extreme starbursts related to the triggering of AGN in the nuclei of galaxies? Overall, 41 talks and 4 posters with their corresponding 10 minutes short talks were presented during the workshop. In addition, the workshop was designed with emphasis on discussions, and therefore, there were 6 discussion sessions of up to one hour during the workshop. Here is presented a summary of the purposes of the workshop as well as a compilation of the abstracts corresponding to each of the presentations. The summary and conclusions of the workshop along with a description of the future prospects by Sylvain Veilleux can be found in the last section of this document. A photo of the assistants is included.Comment: worksho

Factors influencing erythrocyte sedimentation rate in adults New evidence for an old test

The erythrocyte sedimentation rate (ESR) is a routine test for inflammation. Few studies have investigated the potential influence of lifestyle factors and common metabolic abnormalities on the ESR. This study investigates the influence of demographic factors, alcohol consumption, smoking, physical activity, obesity, and metabolic syndrome on the ESR in adults.This cross-sectional study covered 1472 individuals (44.5% males; age range, 18-91 years) randomly selected from the population of a Spanish municipality. The ESR was measured using a standardized method. We assessed habitual alcohol consumption in standard drinking units, along with tobacco smoking, regular physical exercise (by questionnaire), body mass index, and variables defining metabolic syndrome. Multivariate analyses were performed, including mean corpuscular volume and hemoglobin concentration in the models.The ESR was higher in females than in males, and increased steadily with age. Median ESR of females was 2-fold higher than that of males, and median ESR of individuals aged >65 years was 2-fold higher than that of individuals in the youngest category (ages 18-35 years). Body mass index, presence of metabolic syndrome, and smoking were independently and positively associated with higher ESR values. Light alcohol drinkers and individuals with high regular physical activity displayed lower ESR values than did alcohol abstainers and individuals with low physical activity, respectively.ESR varies greatly with age and sex, and corresponding reference values are proposed. Lifestyle factors (physical activity, smoking, and alcohol consumption) and common metabolic abnormalities (obesity and related metabolic syndrome) may also influence ESR values