Simultaneous Radio to (Sub-) mm-Monitoring of Variability and Spectral Shape Evolution of potential GLAST Blazars

The Large Area Telescope (LAT) instrument onboard GLAST offers a tremendous opportunity for future blazar studies. In order to fully benefit from its capabilities and to maximize the scientific return from the LAT, it is of great importance to conduct dedicated multi-frequency monitoring campaigns that will result comprehensive observations. Consequently, we initiated an effort to conduct a GLAST-dedicated, quasi-simultaneous, broad-band flux-density (and polarization) monitoring of potential GLAST blazars with the Effelsberg and OVRO radio telescopes (11cm to 7mm wavelength). Here, we present a short overview of these activities which will complement the multi-wavelengths activities of the GLAST/LAT collaboration towards the 'low-energy' radio bands. Further we will give a brief outlook including the extension of this coordinated campaign towards higher frequencies and future scientific aims.Comment: 3 pages, to appear in the Proceedings of the First GLAST Symposium, Stanford University, February 200

Signal processing in local neuronal circuits based on activity-dependent noise and competition

We study the characteristics of weak signal detection by a recurrent neuronal network with plastic synaptic coupling. It is shown that in the presence of an asynchronous component in synaptic transmission, the network acquires selectivity with respect to the frequency of weak periodic stimuli. For non-periodic frequency-modulated stimuli, the response is quantified by the mutual information between input (signal) and output (network's activity), and is optimized by synaptic depression. Introducing correlations in signal structure resulted in the decrease of input-output mutual information. Our results suggest that in neural systems with plastic connectivity, information is not merely carried passively by the signal; rather, the information content of the signal itself might determine the mode of its processing by a local neuronal circuit.Comment: 15 pages, 4 pages, in press for "Chaos

Testing Spallation Processes With Beryllium and Boron

The nucleosynthesis of Be and B by spallation processes provides unique insight into the origin of cosmic rays. Namely, different spallation schemes predict sharply different trends for the growth of LiBeB abundances with respect to oxygen. ``Primary'' mechanisms predict BeB $\propto$ O, and are well motivated by the data if O/Fe is constant at low metallicity. In contrast, ``secondary'' mechanisms predict BeB $\propto$ O$^2$ and are consistent with the data if O/Fe increases towards low metallicity as some recent data suggest. Clearly, any primary mechanism, if operative, will dominate early in the history of the Galaxy. In this paper, we fit the BeB data to a two-component scheme which includes both primary and secondary trends. In this way, the data can be used to probe the period in which primary mechanisms are effective. We analyze the data using consistent stellar atmospheric parameters based on Balmer line data and the continuum infrared flux. Results depend sensitively on Pop II O abundances and, unfortunately, on the choice of stellar parameters. When using recent results which show O/Fe increasing toward lower metallicity, a two-component Be-O fits indicates that primary and secondary components contribute equally at [O/H]$_{eq}$ = -1.8 for Balmer line data; and [O/H]$_{eq}$ = -1.4 to -1.8 for IRFM. We apply these constraints to recent models for LiBeB origin. The Balmer line data does not show any evidence for primary production. On the other hand, the IRFM data does indicate a preference for a two-component model, such as a combination of standard GCR and metal-enriched particles accelerated in superbubbles. These conclusions rely on a detailed understanding of the abundance data including systematic effects which may alter the derived O-Fe and BeB-Fe relations.Comment: 40 pages including 11 ps figures. Written in AASTe

A Consistency Test of Spectroscopic Gravities for Late-Type Stars

Chemical analyses of late-type stars are usually carried out following the classical recipe: LTE line formation and homogeneous, plane-parallel, flux-constant, and LTE model atmospheres. We review different results in the literature that have suggested significant inconsistencies in the spectroscopic analyses, pointing out the difficulties in deriving independent estimates of the stellar fundamental parameters and hence,detecting systematic errors. The trigonometric parallaxes measured by the HIPPARCOS mission provide accurate appraisals of the stellar surface gravity for nearby stars, which are used here to check the gravities obtained from the photospheric iron ionization balance. We find an approximate agreement for stars in the metallicity range -1 <= [Fe/H] <= 0, but the comparison shows that the differences between the spectroscopic and trigonometric gravities decrease towards lower metallicities for more metal-deficient dwarfs (-2.5 <= [Fe/H] <= -1.0), which casts a shadow upon the abundance analyses for extreme metal-poor stars that make use of the ionization equilibrium to constrain the gravity. The comparison with the strong-line gravities derived by Edvardsson (1988) and Fuhrmann (1998a) confirms that this method provides systematically larger gravities than the ionization balance. The strong-line gravities get closer to the physical ones for the stars analyzed by Fuhrmann, but they are even further away than the iron ionization gravities for the stars of lower gravities in Edvardsson's sample. The confrontation of the deviations of the iron ionization gravities in metal-poor stars reported here with departures from the excitation balance found in the literature, show that they are likely to be induced by the same physical mechanism(s).Comment: AAS LaTeX v4.0, 35 pages, 10 PostScript files; to appear in The Astrophysical Journa

Benchmarking a semiclassical impurity solver for dynamical-mean-field theory: self-energies and magnetic transitions of the single-orbital Hubbard model

An investigation is presented of the utility of semiclassical approximations for solving the quantum-impurity problems arising in the dynamical-mean-field approach to the correlated-electron models. The method is based on performing a exact numerical integral over the zero-Matsubara-frequency component of the spin part of a continuous Hubbard-Stratonovich field, along with a spin-field-dependent steepest descents treatment of the charge part. We test this method by applying it to one or two site approximations to the single band Hubbard model with different band structures, and comparing the results to quantum Monte-Carlo and simplified exact diagonalization calculations. The resulting electron self-energies, densities of states and magnetic transition temperatures show reasonable agreement with the quantum Monte-Carlo simulation over wide parameter ranges, suggesting that the semiclassical method is useful for obtaining a reasonable picture of the physics in situations where other techniques are too expensive.Comment: 14 pages, 15 figure

Caracteres morfo-agronômicos e bioquímicos de clones elite de mandioca de mesa com raízes de polpas amarelada e rosada.

A mandioca (Manihot esculenta Crantz) é considerada uma espécie relevante como fonte alimentícia para a população mundial, principalmente para os países subdesenvolvidos e emergentes. A mandioca é fornecedora de energia a partir do amido acumulado em suas raízes de reserva, mas é também importante destacar a presença dos carotenóides com atividade antioxidante. Nesse contexto, o presente trabalho teve como objetivo caracterizar, por meio de descritores morfológicos, agronômicos e bioquímicos, clones elite de mandioca de mesa de polpa aparelhada e rosada do programa de melhoramento genético de mandioca da Embrapa Cerrados. Foram caracterizados durante duas safras, 13 clones de mandioca de mesa com polpa amarelada e 8 clones com polpa rosada, em comparação com a variedade testemunha IAC 576-70 (BGMC 753). Para avaliar as características morfológicas foram obtidos 40 descritores qualitativos para cada clone. Tanto nos clones de polpas amarelada quanto naqueles de raízes de polpas rosada, houve diferenças morfológicas, demostrando que nenhum clone apresentou 100% de similaridade. O fator ano/safra não influenciou a expressão fenotípica dos caracteres aferidos. Com base no coeficiente cofenético, verificou-se elevado ajuste entre a representação gráfica via dendrograma de r = 0,80 nas raízes de polpa amarelada e r = 0,92 na rosada e a matriz de dissimilaridade genética. Entre os caracteres aferidos, os que apresentaram maior entropia nas raízes amarelada foram, a coloração da epiderme externa, forma do lóbulo central da folha e cor do córtex da raiz, ao passo que na rosada foi à cor do disco, forma do lóbulo central e cor do pecíolo. Foi realizada também a caracterização com base na altura da planta, altura da primeira ramificação, peso da parte aérea sem a cepa, produtividade em raízes, índices de amido nas raízes determinados por meio do método da balança hidrostática, tempo para a cocção e teor de ácido cianídrico nas raízes. Com base nos caracteres avaliados, os clones que se destacaram com polpa amarelada e rosada respectivamente, no caractere altura da primeira ramificação (273/08 e 259/08) e (390/08, 345/08 e a testemunha IAC 576-70), altura da planta (90/08, 272/08, 273/08, 497/08, 259/08 e 450/08) e (390/08, 345/08 e 378/08), peso da parte aérea sem a cepa (94/08 e 272/08) e (390/08, 406/08, 390/08, 378/08 e 341/08), porcentagem de amido nas raízes (26/08, 272/08, 259/08 e 450/08) e (378/08, 413/08, 390/08 e a testemunha IAC 576-70), produtividade de raízes (215/08) e (testemunha IAC 576-70, 341/08, 406/08, 390/08 e 387/08). Com relação ao tempo de cocção na safra 2011/2012, todos os clones necessitaram de tempo inferior a 30 minutos. Em relação ao teor de carotenóides totais nas raízes os clones de amarelada que se destacaram foram 91/08, 94/08, 215/08, 246/08, 272/08 e 497/08, e, naqueles de raízes rosada, os clones 406/08 e 341/08. Em relação ao teor de proteínas nas raízes amarelada, os clones 26/08, 90/08 e 91/08, foram os melhores enquanto nas raízes rosada se destacaram os clones 406/08 e a testemunha IAC 576-70. Os teores de HCN nas raízes de reserva de mandioca foram inferiores a 100 mg kg-1 em todos os clones avaliados. Diferenças significativas entre clones de mandioca de polpas amarelada e rosada foram verificadas para todas as características agronômicas, morfológicas e bioquímicas avaliadas. Os clones tiveram bom desempenho nas avaliações para o cultivo comercial na região do Cerrado e, alguns destes, têm potencial para utilização no melhoramento visando o incremento de carotenóides. ABSTRACT: Cassava (Manihot esculenta Crantz) is considered a relevant species as a food source for the world's population, particularly for developing and emerging countries. The cassava is a provider of energy from starch accumulated in their reserve roots, but it is also important to highlight the presence of carotenoids with antioxidant activity. In this context, this study aimed to characterize, using morphological, agronomic and biochemical, descriptors elite clones from sweet cassava of yellowish and pinkish pulps from the cassava breeding program at Embrapa Cerrados. They were characterized for two crops, 13 edible cassava clones with yellowish pulp and 8 clones with pinkish pulp, compared with the control variety IAC 576-70 (BGMC 753). To evaluate the morphological characteristics were obtained 40 qualitative descriptors for each clone. Both clones the yellowish pulp as those the roots the pinkish pulp, there was morphological differences among clones, showing that no clone showed 100% similarity. The year / crop factor did not influence the phenotypic expression of measured characters. Based on cofenetic coefficient, was found high fit between the graphical representation via dendrogram of r = 0.80 in the roots of yellowish pulp and r = 0.92 in the pinkish of genetic dissimilarity matrix. Among the measured characters, those with the highest entropy in the yellowish roots were, the color of the outer epidermis, the central lobe shape of the leaf and root cortex color, whereas the pinkish was the color to disc, central lobe shape and petiole color. We also performed the characterization based on plant height, the first branch point, and shoot weight without strain, productivity in roots, and index of starch in the roots determines by the method of hydrostatic balance, time for cooking and acid cyanide content in the roots. Based on the evaluated characters, clones stood out with pulps yellowish and pinkish respectively, characters height of the first branch (273/08 and 259/08) and (390/08, 345/08 and the witness IAC 576-70), plant height (90 / 08, 272/08, 273/08, 497/08, 259/08 and 450/08) and (390/08, 345/08 and 378/08), shoot weight without strain (94/08 and 272/08) and (390/08, 406/08, 390/08, 378/08 and 341/08), percentage of starch in the roots (26/08, 272/08, 259/08 and 450/08) and (378/08, 413/08, 390/08 and the witness IAC 576-70), roots of productivity (215/08) and (witnesses IAC 576-70, 341/08, 406/08, 390/08 and 387/08). Regarding the cooking time in the 2011/2012 harvest, all clones showed time less than 30 minutes. Regarding the total carotenoid content in the pulps clones of yellowish roots that stood out were 91/08, 94/08, 215/08, 246/08, 272/08 and 497/08, and, those the clones with pulp pinkish 406/08 and 341/08. Regarding the protein content in yellowish roots the clones 26/08, 90/08 and 91/08, was the best while the pinkish roots highlight clones 406/08 and witness IAC 576-70. The levels of HCN in reserve roots of cassava were less than 100 mg kg-1em all evaluated clones. Significant differences between yellowish and pinkish of pulps cassava clones were checked for all agronomic, morphological and biochemical characteristics evaluated. The clones had well in the ratings for commercial cultivation in the Cerrado region and some of these, clones has potential for use in breeding aimed at increase of carotenoids.Tese (Doutorado em Agronomia) -- Universidade de Brasília, Brasília, 2015. Orientador: Fabio Gelape Faleiro, Embrapa Cerrados. Co-orientador: Eduardo Alano Vieira, Embrapa Cerrados

Low Mass Companions for Five Solar-Type Stars from the Magellan Planet Search Program

We report low mass companions orbiting five Solar-type stars that have emerged from the Magellan precision Doppler velocity survey, with minimum (Msini) masses ranging from 1.2 to 25 Mjup. These nearby target stars range from mildly metal-poor to metal-rich, and appear to have low chromospheric activity. The companions to the brightest two of these stars have previously been reported from the CORALIE survey. Four of these companions (HD 48265-b, HD 143361-b, HD 28185-b, HD 111232-b) are low-mass Jupiter-like planets in eccentric intermediate and long-period orbits. On the other hand, the companion to HD 43848 appears to be a long period brown dwarf in a very eccentric orbit.Comment: Accepted for publication on ApJ, 26 pages, 10 figures, 7 table