Community Voices: Integrating Local and International Partnerships through Storytelling

This essay describes a new global service-learning project focused on integrating local and international partnerships through storytelling. Providence College faculty and students partnered with a local organization, CityArts, and an international organization, Waves of Hope, to empower young people to share their stories through a community lens. Using art and literacy in transnational contexts, the voices and images depict beauty and justice in communities, while also representing a more collaborative model of engagement

FeNi-based magnetoimpedance multilayers: Tailoring of the softness by magnetic spacers

The microstructure and magnetic properties of sputtered permalloy films and FeNi(170 nm)/X/FeNi(170 nm) (X=Co, Fe, Gd, Gd-Co) sandwiches were studied. Laminating of the thick FeNi film with various spacers was done in order to control the magnetic softness of FeNi-based multilayers. In contrast to the Co and Fe spacers, Gd and Gd-Co magnetic spacers improved the softness of the FeNi/X/FeNi sandwiches. The magnetoimpedance responses were measured for [FeNi/Ti(6 nm)] 2/FeNi and [FeNi/Gd(2 nm)] 2/FeNi multilayers in a frequency range of 1-500 MHz: for all frequencies under consideration the highest magnetoimpedance variation was observed for [FeNi/Gd(2 nm)] 2/FeNi multilayers. © 2012 American Institute of Physics

Survey for Emission-Line Galaxies: Universidad Complutense de Madrid List 3

A new low-dispersion objective-prism search for low-redshift (z<0.045) emission-line galaxies (ELG) has been carried out by the Universidad Complutense de Madrid with the Schmidt Telescope at the Calar-Alto Observatory. This is a continuation of the UCM Survey, which was performed by visual selection of candidates in photographic plates via the presence of the Halpha+[NII]6584 blend in emission. In this new list we have applied an automatic procedure, fully developed by us, for selecting and analyzing the ELG candidates on the digitized images obtained with the MAMA machine. The analyzed region of the sky covers 189 square degrees in nine fields near R.A.=14h & 17h, Dec=25 deg. The final sample contains 113 candidates. Special effort has been made to obtain a large amount of information directly from our uncalibrated plates by using several external calibrations. The parameters obtained for the ELG candidates allow for the study of the statistical properties for the sample.Comment: 13 pages, 18 PostScript figures, 6 JPEG figures, Table 2 corrected. Accepted for publication in Astrophysical Journal Supplements, also available at http://www.ucm.es/info/Astrof/opera/LIST3_ApJS99

HetSAGE: Heterogenous Graph Neural Network for Relational Learning

This paper aims to bridge this gap between neuro-symbolic learning (NSL) and graph neural networks (GNN) approaches and provide a comparative study. We argue that the natural evolution of NSL leads to GNNs, while the logic programming foundations of NSL can bring powerful tools to improve the way how information is represented and pre-processed for the GNN. In order to make this comparison, we propose HetSAGE, a GNN architecture that can efficiently deal with the resulting heterogeneous graphs that represent typical NSL learning problems. We show that on CORA, MUTA188 and MovieLens our approach outperforms the state-of-the-art in NSL

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

Boron in Very Metal-Poor Stars

We have observed the B I 2497 A line to derive the boron abundances of two very metal-poor stars selected to help in tracing the origin and evolution of this element in the early Galaxy: BD +23 3130 and HD 84937. The observations were conducted using the Goddard High Resolution Spectrograph on board the Hubble Space Telescope. A very detailed abundance analysis via spectral synthesis has been carried out for these two stars, as well as for two other metal-poor objects with published spectra, using both Kurucz and OSMARCS model photospheres, and taking into account consistently the NLTE effects on the line formation. We have also re-assessed all published boron abundances of old disk and halo unevolved stars. Our analysis shows that the combination of high effective temperature (Teff > 6000 K, for which boron is mainly ionized) and low metallicity ([Fe/H]<-1) makes it difficult to obtain accurate estimates of boron abundances from the B I 2497 A line. This is the case of HD 84937 and three other published objects (including two stars with [Fe/H] ~ -3), for which only upper limits can be established. BD +23 3130, with [Fe/H] ~ -2.9 and logN(B)_NLTE=0.05+/-0.30, appears then as the most metal-poor star for which a firm measurement of the boron abundance presently exists. The evolution of the boron abundance with metallicity that emerges from the seven remaining stars with Teff < 6000 K and [Fe/H]<-1, for which beryllium abundances were derived using the same stellar parameters, shows a linear increase with a slope ~ 1. Furthermore, the B/Be ratio found is constant at a value ~ 20 for stars in the range -3<[Fe/H]<-1. These results point to spallation reactions of ambient protons and alpha particles with energetic particles enriched in CNO as the origin of boron and beryllium in halo stars.Comment: 38 pages, 11 Encapsulated Postscript figures (included), uses aaspp4.sty. Accepted for publication in The Astrophysical Journal. The preprint is also available at: http://www.iac.es/publicaciones/preprints.htm

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

Oxygen abundances in unevolved metal-poor stars from near-UV OH lines

We have performed a detailed oxygen abundance analysis of 23 metal-poor (-3.0<[Fe/H]<-0.3) unevolved halo stars and one giant through the OH bands in the near UV, using high-resolution echelle spectra. Oxygen is found to be overabundant with respect to iron in these stars, with the [O/Fe] ratio increasing from 0.6 to 1 between [Fe/H]=-1.5 and -3.0. The behavior of the oxygen overabundance with respect to [Fe/H] is similar to that seen in previous works based on OI IR triplet data (Abia and Rebolo 1989; Tomkin et al. 1992; Cavallo, Pilachowski, and Rebolo 1997). Contrary to the previously accepted picture, our oxygen abundances, derived from low-excitation OH lines, agree well with those derived from high-excitation lines of the triplet. For nine stars in common with Tomkin et al. we obtain a mean difference of 0.00+/-0.11 dex with respect to the abundances determined from the triplet using the same stellar parameters and model photospheres. For four stars in our sample we have found measurements of the [OI] 6300 A line in the literature, from which we derive oxygen abundances consistent (average difference 0.09 dex) with those based on OH lines, showing that the long standing controversy between oxygen abundances from forbidden and permitted lines in metal-poor unevolved stars can be resolved. Our new oxygen abundances show a smooth extension of the Edvardsson et al.'s (1993) [O/Fe] versus metallicity curve to much lower abundances, with a slope -0.31+/- 0.11 (taking into account the error bars in both oxygen abundances and metallicities) in the range -3<[Fe/H]<-1.Comment: 17 pages, 8 figures, 3 table