The influence of halo assembly on galaxies and galaxy groups

In this paper, we study the variations of groups (galaxy properties according to the assembly history in Sloan Digital Sky Survey Data Release 6 (SDSS-DR6) selected groups. Using mock SDSS group catalogues, we find two suitable indicators of group formation time: (i) the isolation of the group, defined as the distance to the nearest neighbour ill terms of its virial radius and 00 the concentration. measured as the groups inner density calculated using the fifth nearest bright galaxy to the groups centre. Groups Within narrow ranges of Mass ill the mock catalO-Lie show increasing Ifl-OLIP alle With isolation and concentration. However, in the observational data the stellar age, as indicated by the spectral type, only shows a correlation with concentration. We study groups of similar mass and different assembly history. finding important differences ill their galaxy population. Particularly, ill high-mass SDSS groups. the number of members. mass-to-light ratios, red galaxy fractions and the magnitude difference between the brightest and second-brightest group galaxies, show different trends as a function of isolation and concentration, even when it is expected that the latter two quantities correlate with group age. Conversely. low-mass SDSS groups appear to be less sensitive to their assembly history. The correlations detected in the SDSS are not consistent with the trends measured in the mock catalogues. However, discrepancies can he explained in terms of the disagreement found in the a-e-isolation trends, suggesting that the model might be overestimating the effects of, environment, We discuss how the modelling of the cold gas ill satellite galaxies could be responsible for this problem. These results call be Used to improve our Understanding of the evolution of galaxies ill high-density environments.

THE VORONOI TESSELLATION CLUSTER FINDER IN 2+1 DIMENSIONS

We present a detailed description of the Voronoi Tessellation (VT) cluster finder algorithm in 2+1 dimensions, which improves on past implementations of this technique. The need for cluster finder algorithms able to produce reliable cluster catalogs up to redshift 1 or beyond and down to 10(13.5) solar masses is paramount especially in light of upcoming surveys aiming at cosmological constraints from galaxy cluster number counts. We build the VT in photometric redshift shells and use the two-point correlation function of the galaxies in the field to both determine the density threshold for detection of cluster candidates and to establish their significance. This allows us to detect clusters in a self-consistent way without any assumptions about their astrophysical properties. We apply the VT to mock catalogs which extend to redshift 1.4 reproducing the ACDM cosmology and the clustering properties observed in the Sloan Digital Sky Survey data. An objective estimate of the cluster selection function in terms of the completeness and purity as a function of mass and redshift is as important as having a reliable cluster finder. We measure these quantities by matching the VT cluster catalog with the mock truth table. We show that the VT can produce a cluster catalog with completeness and purity > 80% for the redshift range up to similar to 1 and mass range down to similar to 10(13.5) solar masses.

Segregation effects according to the evolutionary stage of galaxy groups

We study segregation phenomena in 57 groups selected from the 2dF Percolation-Inferred Galaxy Groups (2PIGG) catalogue of galaxy groups. The sample corresponds to those systems located in areas of at least 80 per cent redshift coverage out to 10 times the radius of the groups. The dynamical state of the galaxy systems was determined after studying their velocity distributions. We have used the Anderson-Darling test to distinguish relaxed and non-relaxed systems. This analysis indicates that 84 per cent of groups have galaxy velocities consistent with the normal distribution, while 16 per cent of them have more complex underlying distributions. Properties of the member galaxies are investigated taking into account this classification. Our results indicate that galaxies in Gaussian groups are significantly more evolved than galaxies in non-relaxed systems out to distances of similar to 4R(200), presenting significantly redder (B - R) colours. We also find evidence that galaxies with M(R) <= -21.5 in Gaussian groups are closer to the condition of energy equipartition.

Caracterização de remanescentes de aglomerados abertos na galáxia

o presente trabalho busca ampliar o conhecimento das relações entre aglomerados abertos de estrelas e seus remanescentes. Do ponto de vista observacional, um remanescente pode ser definido como uma concentração pouco povoada de estrelas resultante da evolução dinâmica de um sistema inicialmente mais massivo. Apesar do avanços no conhecimento teórico a respeito desses objetos e, nos últimos anos, da busca pela identificação observacional dos mesmos ter aumep.tado, muitas questões permanecem em aberto. Assim, no presente estudo serão analisados 23 candidatos a remanescentes através de dados fotométricos, espectroscópicos e de movimentos próprios. Esses dados fornecem informações sobre os objetos e seus campos. Por meio destas, buscam-se estabelecer critérios de definição de remanescentes de aglomerados abertos, levando-se em conta incertezas observacionais. Os dados fotométricos no infravermelho oriundos do catálogo The Two Micron Ali sky Survey possibilitam, nesse estudo, (i) estudar as propriedades estruturais dos objetos por meio dos perfis de densidade radial de estrelas; (ii) testar a semelhanças entre objetos e campos através de um método estatístico de comparação entre distribuições de estrelas no plano do diagrama cor-magnitude e, (iii) obter idades, avermelhamentos e distâncias com o uso de diagramas cor-magnitude, além de distinguir os objetos em função de um índice de ajuste de isócronas. Os dados espectroscópicos obtidos através de observações óticas no Complejo Astronómico EI Leoncito (Argentina) fornecem para 12 objetos da amostra informações adicionais de avermelhamentos e idades. Os dados cinemáticos extraídos do The Second U. S. Naval Observatory CCD Astrograph Catalog permitem, por sua vez, uma comparação objetiva entre a distribuição de movimentos próprios dos objetos e campos próximos de grande ângulo sólido O emprego desses métodos complementares se mostra essencial no estudo em função da carência de dados completos para os candidatos a remanescentes. No que diz respeito à amostra, em geral não é possível afirmar individualmente qual objeto caracteriza-se de forma definitiva como um remanescente de aglomerado aberto devido à incompleteza dos dados, às incertezas observacionais e à baixa estatística. Entretanto, os métodos desenvolvidos permitem uma análise objetiva e sugerem a presença de remanescentes de aglomerados abertos na amostra. Além disso, há evidência da presença de binarismo, o que é esperado para sistemas evoluídos dinamicamente. Portanto, pode-se inferir sobre estágios evolutivos para remanescentes a partir das distribuições de movimento próprio de suas estrelas e de seu mapeamento no diagrama cor-magnitude.

Identificação das condições gerais de conservação dos reservatórios integrantes do sistema de abastecimento de água de Natal

Infrastructure works are included in strategic areas for the social development. For that matter that all of the investments are very important for the social development. When the population has enough water and an acceptable quality, and it includes a wastewater gathering and its treatment, the whole society became less susceptible to the water diseases. Even the Water Supply and the Sewage depend for its perfect operation of reservoirs, or of the accumulation of water to provide the popular necessity, either due to retention or for the treatment wastewarer. These structures present very specific environmental conditions, because the microclimate created around them, like high environmental humidity and for the existence of many harmful substances for the concrete, such as chloride ions presents in water. The reservoir that compose the System of Water Supply of Natal were built between 1970s and 1980s, a period whom the technical and scientific community did not have in-depth studies about the reinforced concrete mechanism of deterioration. Therefore, these reservoirs have been suffered accelerated deterioration progress, and they have been shown many pathological manifestations strikingly visible. In front of all these problems this academic work aims to identify the generally conditions of conservation of all the reservoirs components of the Water Supply System of Natal. This academic work objectives to develop a recuperation plan for use in these reservoirs, in this academic work it was achieved all the survey of pathological manifestation existing in each reservoir. It was made with local visits, photographic recorders of all manifestations viii and realization of in loco tests. The other step consisted in a application of GDE/UnB metodolgy reformulated by Fonseca (2007). In the step of local visits in each reservoir it was evaluated carbonation depth, by spreading a phenolphthalein solution with 1% of concentration; evaluation of contamination of chlorides, by spreading silver nitrate solution with 1% of concentration, and evaluation of width cracks. After the conclusion of all the testings, it was established that all reservoir, studied in this academic work, have showed an advanced deteriorating condition. It´s presents prevalent pathological manifestations as unacceptable cracks, spots, efflorescence and reinforcement corrosion, and in some cases, chlorides contamination. After the conclusion of the testings and its concatenation it was able to implementing, using GDE/UnB methodology, the order of the restoration its service life and initial safety conditions

Observational Characterization of the Downward Atmospheric Longwave Radiation at the Surface in the City of São Paulo

Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)

The stable archipelago in the region of the Pallas and Hansa dynamical families

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Efeitos de tempestades magnéticas em sinais de gps, em Natal, Brasil

Satellites signals present disturbances (scintillations), due to presence of irregularities in the ionospheric plasma. In the present work, we dedicate to the study of the attenuation of these scintillations that is, an improvement in the signal, during the main magnetic storm phase during the period of October 2006 to February 2007. Using amplitude of scintillation 1.5GHz (L1) data of the net of satellites GPS, in the ionospheric station of Natal (5.84o S, 35.20o O, -20o dip) and geomagnetic indices, during the minimum solar cycle (referred to as cycle 23), demonstrating its anti-correlation between magnetic activity (Kp) and index of scintillation () (Bonelli2005 method, that works for solar maximum, Bonelli(2005)). These results show that these storms correspond to category I of Aarons (1991). The magnetic storms can generate irregularities when the electric feld of penetration eastward on the pre-reversal hour intensificating that and can too generate irregularities on midnight and sunlight period. The limitation of the method applied here is that it is not considering some storms that had also occurred during equinox and summer in the Brazilian region. For this reason, we will use additional data of the stations of São João de Cariri (Imager and Photometer) and of the station at Fortaleza (Digissonde data), as aid to analyze these storms. The storms that had been left out by the applied method, fit in the other two categories of Aarons, with one only exception (storm of January, 02). We show that in the day of the main phase of the magnetic storm, and with presence of bubbles (according to data of the Imager and Photometer), the speed of vertical drift ~E ~B (hF=t) is below 20m/s, that is the threshold found for Anderson al., (2004) (>20m/s as condition favorable to the formation of irregularities and increase in the scintillation index). This reduction of the speed is due to solar minimum

Cosmic microwave background and large-scale structure constraints on a simple quintessential inflation model

We derive constraints on a simple quintessential inflation model, based on a spontaneously broken Phi(4) theory, imposed by the Wilkinson Microwave Anisotropy Probe three-year data (WMAP3) and by galaxy clustering results from the Sloan Digital Sky Survey (SDSS). We find that the scale of symmetry breaking must be larger than about 3 Planck masses in order for inflation to generate acceptable values of the scalar spectral index and of the tensor-to-scalar ratio. We also show that the resulting quintessence equation of state can evolve rapidly at recent times and hence can potentially be distinguished from a simple cosmological constant in this parameter regime.

Diversidade de pulgões e de seus parasitóides e predadores na cultura da alfafa

O objetivo deste trabalho foi verificar a diversidade de pulgões, seus predadores e parasitóides, e a influência de fatores climáticos nas suas populações. Foram realizadas coletas semanais no período de abril/1995 a março/1996, no campo de alfafa da Universidade Federal de Lavras (UFLA), em Lavras, MG. As espécies de pulgões coletadas foram Therioaphis trifolii (Monel) f. maculata, Acyrthosiphon pisum (Harris), A. kondoi Shinji e Aphis craccivora Kock, presentes na cultura durante todo o período de estudo, com picos populacionais em novembro/1995, julho/1995, dezembro/1995 e abril/1996, respectivamente. Foram amostrados insetos predadores das famílias Coccinellidae, Syrphidae, Anthocoridae, Geocoridae e Chrysopidae, tendo as duas últimas ocorrência esporádica. Espécies da família Coccinellidae ocorreram durante todo o período amostral, apresentando o pico populacional no final de dezembro/1995, com precipitação de 20 mm e temperatura de 22,6ºC. A família Syrphidae alcançou maiores números em abril, à precipitação de 53 mm e temperatura de 21ºC. A família Anthocoridae não se manteve por todo o período amostral, porém um pico populacional ocorreu no final de dezembro nas mesmas condições que aquele apresentado pela família Coccinellidae. Os parasitóides da família Aphididae alcançaram pico em junho/1995, à temperatura de 16ºC.

Avaliação e intervenção de bebês em instituição de acolhimento infantil

O presente estudo aborda a avaliação e intervenção com bebês em uma instituição de acolhimento infantil na cidade de Belém-Pa, através da aplicação da Escala de Desenvolvimento do Comportamento da Criança – EDCC e de um programa de atividades elaborado pela pesquisadora para a estimulação precoce/essencial das habilidades motoras, cognitivas, linguagem e afetivas. Dados referentes à história pregressa de todas as crianças envolvidas no estudo também foram considerados e obtidos por meio de relatos informais da equipe da instituição de acolhimento e através de documentos (prontuários) junto à direção. Participaram do estudo quatro bebês, com idade entre seis a onze meses, que não apresentavam disfunções neurológicas e com o maior tempo de permanência na instituição. A abordagem metodológica utilizada foi qualitativa, com característica descritiva e interventiva de pesquisa. A avaliação com a utilização da EDCC no período pré-intervenção demonstrou que todos os bebês participantes da pesquisa obtiveram a pontuação “4” referente a classificação “bom” da escala, sendo que inicialmente apresentaram dificuldades na realização de comportamentos que envolvem a linguagem e a interação social. Na reavaliação, a maioria dos bebês participantes manteve a pontuação “4” com apenas um evoluindo para “5” (excelente), visto que obtiveram melhora significativa nos comportamentos que exigiam a interação com outra pessoa. Assim como através do programa de estimulação, as crianças evoluíram na aquisição das habilidades motoras e afetivo-sociais. Os bebês passaram a demonstrar comportamentos como olhar nos olhos, sorrisos, reconhecimento do rosto do adulto, vocalizações, entre outros. Isto evidenciou que o contexto de acolhimento pode ser um fator de proteção para a infância que encontra-se em situação de vulnerabilidade. Por fim, propõe-se que estudos futuros possam reconhecer a importância da avaliação do desenvolvimento infantil em contextos institucionais e de propostas de estimulação que possam ser incorporadas no cotidiano desses ambientes.

A multidomain approach to asteroid families' identification

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Dynamical evolution and chronology of the Hygiea asteroid family

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Search for Gravitational Waves Associated with gamma-ray Bursts Detected by the Interplanetary Network

We present the results of a search for gravitational waves associated with 223 gamma-ray bursts (GRBs) detected by the InterPlanetary Network (IPN) in 2005-2010 during LIGO's fifth and sixth science runs and Virgo's first, second, and third science runs. The IPN satellites provide accurate times of the bursts and sky localizations that vary significantly from degree scale to hundreds of square degrees. We search for both a well-modeled binary coalescence signal, the favored progenitor model for short GRBs, and for generic, unmodeled gravitational wave bursts. Both searches use the event time and sky localization to improve the gravitational wave search sensitivity as compared to corresponding all-time, all-sky searches. We find no evidence of a gravitational wave signal associated with any of the IPN GRBs in the sample, nor do we find evidence for a population of weak gravitational wave signals associated with the GRBs. For all IPN-detected GRBs, for which a sufficient duration of quality gravitational wave data are available, we place lower bounds on the distance to the source in accordance with an optimistic assumption of gravitational wave emission energy of 10(-2)M(circle dot)c(2) at 150 Hz, and find a median of 13 Mpc. For the 27 short-hard GRBs we place 90% confidence exclusion distances to two source models: a binary neutron star coalescence, with a median distance of 12 Mpc, or the coalescence of a neutron star and black hole, with a median distance of 22 Mpc. Finally, we combine this search with previously published results to provide a population statement for GRB searches in first-generation LIGO and Virgo gravitational wave detectors and a resulting examination of prospects for the advanced gravitational wave detectors.