bluuebunny/crossref_metadata_2025_split huggingface dataset:
Qualidade de vida de indivíduos com lesão medular praticantes de Basquetebol em cadeira de rodas
Authors: Rodrigues Fernanda Dos Reis , Filho Agege Haidar , Haidar Adelzir Malheiros E S. C. B. , Soares Karla Virgínia Bezerra de Castro , Carvalho Sarah Tarcisia Rebelo Ferreira de 
Published: August 2017

Introdução: Lesão medular é uma injúria à medula espinhal que danifica a rede neural do indivíduo, causando alterações na coordenação motora e sensorial e no controle autônomo dos órgãos. Tais lesões podem ser irreversíveis, levando a consequências sociais e econômicas para o paciente, a família e a sociedade. Objetivo: Comparar a qualidade de vida de indivíduos com lesão medular praticantes de basquetebol em cadeira de rodas e de indivíduos com lesão medular não praticantes deste esporte. Material e método: Estudo comparativo e descritivo do tipo transversal, com abordagem quantitativa, com 20 cadeirantes do gênero masculino, portadores de lesão medular, sendo 10 praticantes de basquetebol e 10 não praticantes, com idade de 20 a 55 anos, da cidade de Marabá-PA. A qualidade de vida foi avaliada através da Versão Brasileira d o SF-36. A análise dos dados foi realizada utilizando-se o programa SPSS 18.0, considerando p≤0,05. Resultados: Os participantes lesados medulares que praticavam basquetebol em cadeira de rodas apresentaram escores significativamente superiores em relação aos aspectos referentes à capacidade funcional, aspectos físicos e vitalidade da qualidade de vida quando comparados de indivíduos com lesão medular não praticantes de basquetebol em cadeira de rodas. Conclusão: Considera-se que o basquetebol em cadeira de rodas pode ser uma importante estratégia terapêutica capaz de influenciar a qualidade de vida de seus praticantes.Palavras-chave: Qualidade de vida; Lesão medular; Basquetebol em cadeira de rodas.
Psicologia
Authors: Azevedo Kaline Silva 
Published: August 2017

MAISTO, Alberto A. et al. São Luís: Universidade CEUMA /PEARSON, 2013, 173p. A Universidade CEUMA estabeleceu, em seu percurso acadêmico, a coautoria e promoção de trabalhos científicos, não só dos seus pesquisadores quanto também de estudiosos de outras instituições, inclusive, um trabalho de parceria com as editoras. Este é o caso da parceria com a Editora PEARSON.O trabalho PSICOLOGIA, em tão boa hora editado, vem servindo o Curso de Psicologia e áreas afins. Trata-se, então, de uma obra escrita por um grupo de autores americanos, de consagrado conceito internacional.Maisto, Morris, Sobral, Robbins e Judge expõem, com refinamento didático, todo um conjunto epistemológico sobre a Ciência da Alma. E o fazem de modo interessante e instrutivo.O livro contém três unidades e vinte e quatro itens que se distribuem em conteúdos que perpassam pelos métodos de pesquisa em psicologia, ética, carreiras em psicologia, tipos de equipes, características do trabalho e outros assuntos importantes. Cento e setenta e três páginas, um largo anexo com referências, boxes com estudos de caso, tópicos para exercícios em grupo, questões para revisão, “ponto e contraponto”, constituem o estofo epistemológico do trabalho. Também algumas páginas em que os autores discutem tópicos ilustrativos, a exemplo de “mito ou ciência”, comportamento organizacional, diferenças culturais no trabalho etc.Um ponto interessante consiste na utilização de fotografias pertinentes aos assuntos trabalhados. Deste modo, fotografias obtidas nos próprios ambientes estudados, além daquelas que ilustram consagrados experts da Psicologia. Este trabalho é bastante indicado para interessados em Psicologia, cultura laboral e relacionamento humano. ¹ Psicóloga especialista em Psicologia Geriátrica, Mestranda em Psicologia em Educação para a Saúde, ex-chefa do CRAS – Colinas/MA. Professora na Universidade CEUMA.
Desafios da Educação Profissional: por um trabalho pedagógico no Ensino Médio Integrado
Authors: Maraschin Mariglei Severo 
Published: August 2017

Como uma das formas de oferta da Educação Profissional, tem-se o Ensino Médio Integrado, sendo esta uma das funções dos Institutos Federais. Reconhece-se, neste sentido, a importância de olhar para essa etapa de formação com o objetivo de ver avanços e ir além. Assim, o objetivo deste texto é tecer uma avaliação dos últimos anos da trajetória da Educação Profissional no Brasil e destacar desafios para o Ensino Médio Integrado, incluindo a Educação de Jovens e Adultos. Acredita-se que é chegada a hora de investir fortemente em um trabalho pedagógico, trabalho este que envolve pessoas para o objetivo do Ensino Médio Integrado: integração e criticidade. O artigo destacará os avanços da Educação Profissional, os desafios e o caminho que se quer chegar. A partir da pesquisa bibliográfica, busca-se trazer problematizações para a melhoria do Ensino Médio Integrado, em especial olhando para os dados do Rio Grande do Sul, a partir de um trabalho pedagógico crítico e integrado. Muitos são os desafios, mas acredita-se na efetivação de uma política de formação integrada como opção para a melhoria do Ensino Médio.
Importância da fibra alimentar na nutrição de animais não ruminantes
Authors: Goulart Fernanda Rodrigues , Adoriam Taida Juliana , Mombach Patrícia Inês , Da Silva Leila Picolli 
Published: August 2017

Por muito tempo, a fi bra da dieta representou a porção inerte do alimento em razão do seu baixo teor de energia. Além disso, essa fração também foi considerada como nutriente indesejável na dieta de monogástricos, em razão, principalmente, dos efeitos negativos de sua presença, como seu efeito diluidor de energia. Porém, esses efeitos podem estar relacionados à quantifi caçãoerrônea dessa fração. Quando as fi bras são determinadas de forma correta e adicionadas em quantidades adequadas, os efeitos deste nutriente trazem vários benefícios aos animais. As fi bras alimentares são formadas por polissacarídeos não amiláceos, dentre os quais podemos destacar a celulose, hemicelulose, pectinas, gomas, mucilagens, β-glicanas, entre outras. Frações essasque vêm recebendo grande atenção, devido às suas propriedades prebióticas. A principal ação prebiótica ocorre pela ativação do metabolismo de um grupo de bactérias benéfi cas do trato gastrointestinal, promovendo aumento na produção de ácidos graxos de cadeia curta e do número de vilos no íleo, o que permite aumento na área absortiva intestinal e consequentemente melhora no desempenho animal.
Management urbaner Wälder zwischen Ansprüchen der Gesellschaft und Besitzerzielen
Authors: Lupp Gerd , Börtitz Katharina , Kantelberg Valerie , Koch Marc , Pauleit Stephan 
Published: August 2017

Management of urban woodlands between demands of society and owner objectives
Urban woodlands provide numerous ecosystem services for the society. However, they depend on the management goals, motivations and interests of the forest owners. In the Munich Metropolitan Region, it was examined how the population perceive the woodlands and which services of the woodlands are most important for them. On the other hand management goals, interests and motivation of forest owners were assessed by interviewing representatives of state, communal and private forest owners in urban area. It turned out that both population and forest owners had quite similar ideas about the services urban woodlands should deliver. For many forest owners, timber production was of little importance. The main objective was creating and maintaining stable and ecologically valuable mixed stands. In the everyday perception of the population, there is a deep fear of losing woodlands for urban development. Forest management actions are often associated with a general loss of forest. To avoid conflicts, communication and information should be improved. To provide attractive forest consultancy for urban woodland owners, forest authorities and forest associations should include topics such as forest aesthetics, nature conservation, pest control, legal duty to maintain safety, recreation and visitor management.
iPTF15eqv: Multiwavelength Exposé of a Peculiar Calcium-rich Transient
Authors: Milisavljevic Dan , Patnaude Daniel J. , Raymond John C. , Drout Maria R. , Margutti Raffaella , Kamble Atish , Chornock Ryan , Guillochon James , Sanders Nathan E. , Parrent Jerod T. , Lovisari Lorenzo , Chilingarian Igor V. , Challis Peter , Kirshner Robert P. , Penny Matthew T. , Itagaki Koichi , Eldridge J. J. , Moriya Takashi J. 
Published: August 2017

Abstract
The progenitor systems of the class of “Ca-rich transients” is a key open issue in time domain astrophysics. These intriguing objects exhibit unusually strong calcium line emissions months after explosion, fall within an intermediate luminosity range, are often found at large projected distances from their host galaxies, and may play a vital role in enriching galaxies and the intergalactic medium. Here we present multiwavelength observations of iPTF15eqv in NGC 3430, which exhibits a unique combination of properties that bridge those observed in Ca-rich transients and SNe Ib/c. iPTF15eqv has among the highest [Ca ii]/[O i] emission line ratios observed to date, yet is more luminous and decays more slowly than other Ca-rich transients. Optical and near-infrared photometry and spectroscopy reveal signatures consistent with the supernova explosion of a

star that was stripped of its H-rich envelope via binary interaction. Distinct chemical abundances and ejecta kinematics suggest that the core collapse occurred through electron-capture processes. Deep limits on possible radio emission made with the Jansky Very Large Array imply a clean environment (n ≲ 0.1 cm−3) within a radius of

cm. Chandra X-ray Observatory observations rule out alternative scenarios involving the tidal disruption of a white dwarf (WD) by a black hole, for masses >100 M
⊙. Our results challenge the notion that spectroscopically classified Ca-rich transients only originate from WD progenitor systems, complicate the view that they are all associated with large ejection velocities, and indicate that their chemical abundances may vary widely between events.
Influence of Intermittency on the Quasi-perpendicular Scaling in Three-dimensional Magnetohydrodynamic Turbulence
Authors: Yang Liping , He Jiansen , Tu Chuanyi , Li Shengtai , Zhang Lei , Wang Xin , Marsch Eckart , Wang Linghua 
Published: August 2017

Abstract
Solar wind fluctuations reveal the ubiquity of intermittency, which is believed to affect the spectral signatures of turbulence. In this work, based on simulation of driven compressible MHD turbulence, we apply the wavelet technique to the magnetic field and velocity to identify intermittency, and we analyze the influence of the intermittency on the quasi-perpendicular scaling in the inertial range. The numerical results show that the original magnetic and velocity fluctuations are anisotropic, and have a power anisotropy with a spectral index approaching the Iroshnikov–Kraichnan

scaling in the direction quasi-perpendicular to the local mean magnetic field. As in observations of the solar wind fluctuations, as the scale decreases in the simulation, the calculated probability distribution functions (pdfs) of the wavelet coefficients become extended on both tails of the non-Gaussian distribution, with a rapid increase in flatness. After intermittency has been removed from the driven turbulence, at each scale, the pdfs approach a Gaussian distribution, with the flatness being ∼3. Meanwhile, the quasi-perpendicular scaling for both fluctuations becomes steeper and close to a Kolmogorov

scaling, which may be a result of the stronger intermittency in the quasi-perpendicular direction and at the smaller scales. These results suggest that there is intermittency superposed on the “background” turbulence that seems to have the Kolmogorov scaling, whereby the overall slope is getting flatter with the involvement of intermittency.
Is There a Temperature Limit in Planet Formation at 1000 K?
Authors: Demirci Tunahan , Teiser Jens , Steinpilz Tobias , Landers Joachim , Salamon Soma , Wende Heiko , Wurm Gerhard 
Published: August 2017

Abstract
Dust drifting inward in protoplanetary disks is subject to increasing temperatures. In laboratory experiments, we tempered basaltic dust between 873 K and 1273 K and find that the dust grains change in size and composition. These modifications influence the outcome of self-consistent low speed aggregation experiments showing a transition temperature of 1000 K. Dust tempered at lower temperatures grows to a maximum aggregate size of 2.02 ± 0.06 mm, which is 1.49 ± 0.08 times the value for dust tempered at higher temperatures. A similar size ratio of 1.75 ± 0.16 results for a different set of collision velocities. This transition temperature is in agreement with orbit temperatures deduced for observed extrasolar planets. Most terrestrial planets are observed at positions equivalent to less than 1000 K. Dust aggregation on the millimeter-scale at elevated temperatures might therefore be a key factor for terrestrial planet formation.
13C Isotopic Fractionation of HC3N in Two Starless Cores: L1521B and L134N (L183)
Authors: Taniguchi Kotomi , Ozeki Hiroyuki , Saito Masao 
Published: August 2017

Abstract
We observed the

rotational lines of the normal species and three 13C isotopologues of HC3N at the 45 GHz band toward two low-mass starless cores, L1521B and L134N (L183), using the Nobeyama 45 m radio telescope in order to study the main formation pathways of HC3N in each core. The abundance ratios of the three 13C isotopologues in L1521B are derived to be [H13CCCN]:[HC13CCN]:[HCC13CN] = 0.98 (±0.14):1.00:1.52 (±0.16) (

). The fractionation pattern is consistent with that at the cyanopolyyne peak in Taurus Molecular Cloud-1. This fractionation pattern suggests that the main formation pathway of HC3N is the neutral–neutral reaction between C2H2 and CN. On the other hand, their abundance ratios in L134N are found to be [H13CCCN]:[HC13CCN]:[HCC13CN] = 1.5 (±0.2):1.0:2.1 (±0.4) (

), which are different from those in L1521B. From this fractionation pattern, we propose that the reaction between HNC and CCH is a possible main formation pathway of HC3N in L134N. We find out that the main formation pathways of the same molecule are not common even in similar physical conditions. We discuss the possible factors that could make a difference in the fractionation pattern between L134N and L1521B/TMC-1.
CMB Polarization B-mode Delensing with SPTpol and Herschel
Authors: Manzotti A. , Story K. T. , Wu W. L. K. , Austermann J. E. , Beall J. A. , Bender A. N. , Benson B. A. , Bleem L. E. , Bock J. J. , Carlstrom J. E. , Chang C. L. , Chiang H. C. , Cho H-M. , Citron R. , Conley A. , Crawford T. M. , Crites A. T. , de Haan T. , Dobbs M. A. , Dodelson S. , Everett W. , Gallicchio J. , George E. M. , Gilbert A. , Halverson N. W. , Harrington N. , Henning J. W. , Hilton G. C. , Holder G. P. , Holzapfel W. L. , Hoover S. , Hou Z. , Hrubes J. D. , Huang N. , Hubmayr J. , Irwin K. D. , Keisler R. , Knox L. , Lee A. T. , Leitch E. M. , Li D. , McMahon J. J. , Meyer S. S. , Mocanu L. M. , Natoli T. , Nibarger J. P. , Novosad V. , Padin S. , Pryke C. , Reichardt C. L. , Ruhl J. E. , Saliwanchik B. R. , Sayre J. T. , Schaffer K. K. , Smecher G. , Stark A. A. , Vanderlinde K. , Vieira J. D. , Viero M. P. , Wang G. , Whitehorn N. , Yefremenko V. , Zemcov M. 
Published: August 2017

Abstract
We present a demonstration of delensing the observed cosmic microwave background (CMB) B-mode polarization anisotropy. This process of reducing the gravitational-lensing-generated B-mode component will become increasingly important for improving searches for the B modes produced by primordial gravitational waves. In this work, we delens B-mode maps constructed from multi-frequency SPTpol observations of a 90 deg2 patch of sky by subtracting a B-mode template constructed from two inputs: SPTpol E-mode maps and a lensing potential map estimated from the Herschel 500 μm map of the cosmic infrared background. We find that our delensing procedure reduces the measured B-mode power spectrum by

% in the multipole range

this is shown to be consistent with expectations from simulations and to be robust against systematics. The null hypothesis of no delensing is rejected at

. Furthermore, we build and use a suite of realistic simulations to study the general properties of the delensing process and find that the delensing efficiency achieved in this work is limited primarily by the noise in the lensing potential map. We demonstrate the importance of including realistic experimental non-idealities in the delensing forecasts used to inform instrument and survey-strategy planning of upcoming lower-noise experiments, such as CMB-S4.
A Search for FRB 121102-like Persistent Radio-luminous Sources—Candidates and Implications for the FRB Rate and Searches
Authors: Ofek Eran O. 
Published: August 2017

Abstract
The localization of the repeating fast radio burst (FRB), FRB 121102, suggests that it is associated with a persistent radio-luminous compact source in the FRB host galaxy. Using the FIRST radio catalog, I present a search for luminous persistent sources in nearby galaxies, with radio luminosities

of the FRB 121102 persistent source luminosity. The galaxy sample contains about 30% of the total galaxy g-band luminosity within

Mpc, in a footprint of 10,600 deg2. After rejecting sources likely due to active galactic nuclei activity or background sources, I am left with 11 candidates that are presumably associated with galactic disks or star-formation regions. At least some of these candidates are likely to be due to chance alignment. In addition, I find 85 sources within

of galactic nuclei. Assuming that the radio persistent sources are not related to galactic nuclei and that they follow the galaxy g-band light, the 11 sources imply a 95% confidence upper limit on the space density of luminous persistent sources of

Mpc−3, and that at any given time only a small fraction of galaxies host a radio-luminous persistent source (

). Assuming a persistent source lifetime of 100 years, this implies a birth rate of

yr−1 Mpc−3. Given the FRB volumetric rate, and assuming that all FRBs repeat and are associated with persistent radio sources, this sets a lower limit on the rate of FRB events per persistent source of

yr−1. I argue that these 11 candidates are good targets for FRB searches and I estimate the FRB event rate from these candidates.
Bioclimatic approach to assessing the potential impact of climate change on two flea beetle (Coleoptera: Chrysomelidae) species in Canada
Authors: Olfert O. , Weiss R.M. , Elliott R.H. , Soroka J.J. 
Published: August 2017

AbstractBoth the striped flea beetle,Phyllotreta striolata(Fabricius), and crucifer flea beetle,Phyllotreta cruciferae(Goeze) (Coleoptera: Chrysomelidae), are invasive alien species to North America. In western Canada, they are the most significant insect pests of cruciferous (Brassicaceae) crops. Climate is the one of the most dominant factors regulating the geographic distribution and population density of most insect species. Recent bioclimatic simulation models of the two flea beetle species fostered a better understanding of how the two species responded to selected climate variables. They demonstrated that selected climate variables increased population densities and geographic range of the two species. General circulation model inputs were applied in this study to assess the impact of a changing climate on the response ofP. cruciferae and P. striolatapopulations. Model output, using the climate change scenarios, predicted that bothP. cruciferaeandP. striolatapopulations will shift north in future climates and the degree of geographic overlap between these two species will be greater than for current climate. This suggests that the two species could potentially cause economic losses over an expanded area in the future.
Exploring Vital Sign Data Quality in Electronic Health Records with Focus on Emergency Care Warning Scores
Authors: Chen Rong , Blomqvist Hans , Koch Sabine , Skyttberg Niclas 
Published: August 2017

Summary
Background: Computerized clinical decision support and automation of warnings have been advocated to assist clinicians in detecting patients at risk of physiological instability. To provide reliable support such systems are dependent on high-quality vital sign data. Data quality depends on how, when and why the data is captured and/or documented.
Objectives: This study aims to describe the effects on data quality of vital signs by three different types of documentation practices in five Swedish emergency hospitals, and to assess data fitness for calculating warning and triage scores. The study also provides reference data on triage vital signs in Swedish emergency care.
Methods: We extracted a dataset including vital signs, demographic and administrative data from emergency care visits (n=335027) at five Swedish emergency hospitals during 2013 using either completely paper-based, completely electronic or mixed documentation practices. Descriptive statistics were used to assess fitness for use in emergency care decision support systems aiming to calculate warning and triage scores, and data quality was described in three categories: currency, completeness and correctness. To estimate correctness, two further categories –plausibility and concordance –were used.
Results: The study showed an acceptable correctness of the registered vital signs irrespectively of the type of documentation practice. Completeness was high in sites where registrations were routinely entered into the Electronic Health Record (EHR). The currency was only acceptable in sites with a completely electronic documentation practice.
Conclusion: Although vital signs that were recorded in completely electronic documentation practices showed plausible results regarding correctness, completeness and currency, the study concludes that vital signs documented in Swedish emergency care EHRs cannot generally be considered fit for use for calculation of triage and warning scores. Low completeness and currency were found if the documentation was not completely electronic.
Citation: Skyttberg N, Chen R, Blomqvist H, Koch S. Exploring Vital Sign Data Quality in Electronic Health Records with Focus on Emergency Care Warning Scores. Appl Clin Inform 2017; 8: 880–892 https://doi.org/10.4338/ACI-2017-05-RA-0075
Pulmonary embolism four days after interruption of therapy with rivaroxaban
Authors: Göndör Gabor , Stöllberger Claudia 
Published: August 2017

SummaryThrombosis after cessation of anticoagulation, also named rebound thrombosis, is a matter of concern and controversy. There are only few published data about occurrence of rebound thrombosis associated with non-vitamin K-antagonist oral anticoagulant drugs (NOACs). We report on a 58-year-old male with paroxysmal atrial fibrillation (AF) with a CHA2DS2VASC score of 4 who developed central pulmonary embolism four days after interruption of rivaroxaban because of parotid surgery. He had received 40 mg enoxaparin/d. The parotid gland was partially resected within 6 hours without blood loss. Pulmonary embolism and AF occurred on the first postoperative day. He recovered with low-molecular-weight heparin in therapeutic dosages and amiodarone and was discharged with phenprocoumon. The relevance of a rivaroxaban rebound phenomenon, manifesting as arterial embolism, stroke or venous thromboembolism should be clarified. It should be assessed if rebound-phenomena also exist for the NOACs dabigatran, apixaban and edoxaban. Thus, the randomized trials and registries investigating patients with AF or venous thromboembolism should be re-analysed and, based on these data, recommendations should be developed for situations in which NOAC-therapy has to be interrupted or ceased.