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5. 'AGRO SEM PARTIDO'? COERÇÃO E CONSENSO - A INVESTIDA DO AGRONEGÓCIO NA EDUCAÇÃO BRASILEIRA

Author

Tássia Gabriele Balbi de Figueredo e Cordeiro

Subjects
Special aspects of education, LC8-6691, Labor market. Labor supply. Labor demand, HD5701-6000.9, Labor policy. Labor and the state, HD7795-8027
Abstract

Neste artigo analisamos a inserção do agronegócio na educação, especificamente, a campanha De Olho no Material Escolar e seus atravessamentos com os procedimentos do Escola sem Partido. Para tanto, realizamos pesquisa bibliográfica e documental acerca das temáticas em questão. Como resultado, observamos indícios de que o De Olho no Material Escolar compõe uma frente de expansão político-ideológica do agronegócio que busca, por meio da combinação entre força e consenso, interferir nos rumos da educação brasileira, reproduzindo de forma mais sofisticada os métodos desenvolvidos pelo Escola sem Partido. Palavra-chave: Agronegócio; Questão Agrária; Educação.

Published
2022
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6. Identification of Cucumisin (Cuc m 1), a subtilisin‐like endopeptidase, as the major allergen of melon fruit

Author

Cuesta‐Herranz, J., Pastor, C., Figueredo, E., Vidarte, L., De Las Heras, M., Durán, D., Fernández‐Caldas, E., De Miguel, J., Vivanco, F., Pastor Vargas, Carlos, Vivanco Martínez, Fernando, Cuesta‐Herranz, J., Pastor, C., Figueredo, E., Vidarte, L., De Las Heras, M., Durán, D., Fernández‐Caldas, E., De Miguel, J., Vivanco, F., Pastor Vargas, Carlos, and Vivanco Martínez, Fernando

Abstract

Background: Allergenic components in melon extracts have not been described in spite of the fact that melon (Cucumis melo) is a frequent allergy-eliciting fruit. The aim of this study was to evaluate allergenic components in melon extract and to report the identification of cucumisin as a major melon allergen. Materials and methods: Sera from 35 patients allergic to melon were selected on the basis of clinical symptoms, skin prick tests and oral challenge test. Allergenic components were detected by sodium dodecyl sulphate polyacrylamide gel electrophoresis and immunoblotting. Molecular characterization of IgE-binding bands was performed by N-terminal amino acid sequencing. Results: More than 10 IgE-binding bands, between 10 and 80 kDa, were identified in melon extract. Out of them, four IgE-binding bands were major allergens: 14 kDa, 36 kDa, 54 kDa and 67 kDa. These major allergens, except 14 kDa band, showed the same N-terminal sequence: T-T-R-S-W-D-F-L. Research conducted with protein databases identified this N-terminal sequence as cucumisin, an alkaline serine protease, which shares structural homology with microbial subtilisin. The molecular mass of the identified bands corresponds with different molecular forms of cucumisin produced during the processing or degradation of the enzyme: 67 kDa native cucumisin, 54 kDa mature cucumisin and 36 kDa NH2-terminal cucumisin fragment. Conclusion: Cucumisin (Cuc m 1) and several N-terminal cucumisin fragments are the major allergens of melon. The ubiquitous distribution of this protein family (cucumisin-like proteases) in many plant species and its high structural similarity suggest its potential role as a new panallergen in plant foods., Depto. de Bioquímica y Biología Molecular, Fac. de Ciencias Químicas, TRUE, pub

Published
2024

7. The Stellar Content of Obscured Galactic Giant HII Regions. VII. W3

Author

Navarete, F., Figueredo, E., Damineli, A., Moisés, A. P., Blum, R. D., and Conti, P. S.

Subjects
Astrophysics - Astrophysics of Galaxies
Abstract

Spectrophotometric distances in the K band have been reported by different authors for a number of obscured Galactic HII regions. Almost 50% of them show large discrepancies compared to the classical method using radial velocities measured in the radio spectral region. In order to provide a crucial test of both methods, we selected a target which does not present particular difficulty for any method and which has been measured by as many techniques as possible. The W3 star forming complex, located in the Perseus arm, offers a splendid opportunity for such a task. We used the NIFS spectrograph on the Frederick C. Gillett Gemini North telescope to classify candidate "naked photosphere" OB stars based on 2MASS photometry. Two of the targets are revealed to be mid O-type main sequence stars leading to a distance of d = 2.20 kpc. This is in excellent agreement with the spectrophotometric distance derived in the optical band (d = 2.18 kpc, Humphreys 1978) and with a measurement of the W3 trigonometric parallax (d = 1.95 kpc, Xu et al. 2006). Such results confirm that the spectrophotometric distances in the K band are reliable. The radio derived kinematic distance, on the contrary, gives a distance twice as large (d = 4.2 kpc, Russeil 2003). This indicates that this region of Perseus arm does not follow the Galactic rotation curve, and this may be the case also for other HII regions for which discrepancies have been found.

Published
2011
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8. Spectrophotometric Distances to Galactic H\,{\sc{ii}} Regions

Author

Moisés, A. P., Damineli, A., Figuerêdo, E., Blum, R. D., Conti, P. S., and Barbosa, C. L.

Subjects
Astrophysics - Solar and Stellar Astrophysics
Abstract

We present a near infrared study of the stellar content of 35 H\,{\sc{ii}} regions in the Galactic plane. In this work, we have used the near infrared domain $J-$, $H-$ and $K_{s}-$ band color images to visually inspect the sample. Also, color-color and color-magnitude diagrams were used to indicate ionizing star candidates, as well as, the presence of young stellar objects such as classical TTauri Stars (CTTS) and massive young stellar objects (MYSOs). We have obtained {\it Spitzer} IRAC images for each region to help further characterize them. {\it Spitzer} and near infrared morphology to place each cluster in an evolutionary phase of development. {\it Spitzer} photometry was also used to classify the MYSOs. Comparison of the main sequence in color-magnitude diagrams to each observed cluster was used to infer whether or not the cluster kinematic distance is consistent with brightnesses of the stellar sources. We find qualitative agreement for a dozen of the regions, but about half the regions have near infrared photometry that suggests they may be closer than the kinematic distance. A significant fraction of these already have spectrophotometric parallaxes which support smaller distances. These discrepancies between kinematic and spectrophotometric distances are not due to the spectrophotometric methodologies, since independent non-kinematic measurements are in agreement with the spectrophotometric results. For instance, trigonometric parallaxes of star-forming regions were collected from the literature and show the same effect of smaller distances when compared to the kinematic results. In our sample of H\,{\sc{ii}} regions, most of the clusters are evident in the near infrared images. Finally, it is possible to distinguish among qualitative evolutionary stages for these objects., Comment: 59 pages, 146 figures and 4 tables. MNRAS accepted

Published
2010
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9. Far-infrared all sky diffuse mapping with AKARI

Author

Doi, Y., Azkonaga, M. Etxaluze, White, Glenn J., Figueredo, E., Chinone, Y., Hattori, M., Nakagawa, T., Yamauchi, C., Shibai, H., and team, the AKARI Diffuse Map

Subjects
Astrophysics - Galaxy Astrophysics
Abstract

We discuss the capability of AKARI in recovering diffuse far-infrared emission, and examine the achieved reliability. Critical issues in making images of diffuse emission are the transient response and long-term stability of the far-infrared detectors. Quantitative evaluation of these characteristics are the key to achieving sensitivity comparable to or better than that for point sources (< 20 -- 95 MJy sr-1). We describe current activity and progress toward the production of high quality images of the diffuse far-infrared emission using the AKARI all-sky survey data., Comment: 4 pages, 8 figures, to appear in the Proceedings of the Conference "AKARI, a light to illuminate the misty Universe", Fukutake Hall, The University of Tokyo, Japan, 16-19 February 2009

Published
2009

10. High Spatial Resolution Spectroscopy of W51 IRS2E and IRS2W: Two Very Massive Young Stars in Early Formation Stages

Author

Barbosa, C. L., Blum, R. D., Conti, P. S., Damineli, A., and Figueredo, E.

Subjects
Astrophysics
Abstract

We present $K$-band spectra of the near infrared counterparts to IRS2E and IRS2W which is associated with the ultracompact HII region W51d, both of them embedded sources in the Galactic compact HII region W51 IRS2. The high spatial resolution observations were obtained with the laser guide star facility and Near infrared Integral Field Spectrograph (NIFS) mounted at the Gemini North observatory. The spectrum of the ionizing source of W51d shows the photospheric features NIII (21155 \AA) in emission and HeII (21897 \AA) in absorption which lead us to classify it as an young O3 type star. We detected CO overtone in emission at 23000 \AA in the spectrum of IRS2E, suggesting that it is a massive young object still surrounded by an accretion disc, probably transitioning from the hot core phase to an ultracompact HII region., Comment: Accepted by ApJ Letters

Published
2008
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11. The Stellar Content of Obscured Galactic Giant HII Regions. VI: W51A

Author

Figueredo, E., Blum, R. D., Damineli, A., Conti, P. S., and Barbosa, C. L.

Subjects
Astrophysics
Abstract

We present K-band spectra of newly born OB stars in the obscured Galactic giant H II region W51A and ~ 0.8'' angular resolution images in the J, H and K_S-bands. Four objects have been spectroscopically classified as O-type stars. The mean spectroscopic parallax of the four stars gives a distance of 2.0 \pm 0.3 kpc (error in the mean), significantly smaller than the radio recombination line kinematic value of 5.5 kpc or the values derived from maser propermotion observations (6--8 kpc). The number of Lyman continuum photons from the contribution of all massive stars (NLyc ~ 1.5 x 10^{50} s^{-1}) is in good agreement with that inferred from radio recombination lines (NLyc = 1.3 x 10^{50} s^{-1}) after accounting for the smaller distance derived here. We present analysis of archival high angular resolution images (NAOS CONICA at VLT and T-ReCS at Gemini) of the compact region W51 IRS2. The K_S--band images resolve the infrared source IRS~2 indicating that it is a very young compact HII region. Sources IRS2E was resolved into compact cluster (within 660 AU of projected distance) of 3 objects, but one of them is just bright extended emission. W51d1 and W51d2 were identified with compact clusters of 3 objects (maybe 4 in the case of W51d1) each one. Although IRS~2E is the brightest source in the K-band and at 12.6 \micron, it is not clearly associated with a radio continuum source. Our spectrum of IRS~2E shows, similar to previous work, strong emission in Br$\gamma$ and HeI, as well as three forbidden emission lines of FeIII and emission lines of molecular hydrogen (H_2) marking it as a massive young stellar object., Comment: 31 pages and 9 figures, submitted to AJ

Published
2008
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12. The Infrared Astronomical Mission AKARI

Author

Murakami, H., Baba, H., Barthel, P., Clements, D. L., Cohen, M., Doi, Y., Enya, K., Figueredo, E., Fujishiro, N., Fujiwara, H., Fujiwara, M., Garcia-Lario, P., Goto, T., Hasegawa, S., Hibi, Y., Hirao, T., Hiromoto, N., Hong, S. S., Imai, K., Ishigaki, M., Ishiguro, M., Ishihara, D., Ita, Y., Jeong, W. -S., Jeong, K. S., Kaneda, H., Kataza, H., Kawada, M., Kawai, T., Kawamura, A., Kessler, M. F., Kester, Do, Kii, T., Kim, D. C., Kim, W., Kobayashi, H., Koo, B. C., Kwon, S. M., Lee, H. M., Lorente, R., Makiuti, S., Matsuhara, H., Matsumoto, T., Matsuo, H., Matsuura, S., Mueller, T. G., Murakami, N., Nagata, H., Nakagawa, T., Naoi, T., Narita, M., Noda, M., Oh, S. H., Ohnishi, A., Ohyama, Y., Okada, Y., Okuda, H., Oliver, S., Onaka, T., Ootsubo, T., Oyabu, S., Pak, S., Park, Y. S., Pearson, C. P., Rowan-Robinson, M., Saito, T., Sakon, I., Salama, A., Sato, S., Savage, R. S., Serjeant, S., Shibai, H., Shirahata, M., Sohn, J. J., Suzuki, T., Takagi, T., Takahashi, H., Tanabe, T., Takeuchi, T. T., Takita, S., Thomson, M., Uemizu, K., Ueno, M., Usui, F., Verdugo, E., Wada, T., Wang, L., Watabe, T., Watarai, H., White, G. J., Yamamura, I., Yamauchi, C., and Yasuda, A.

Subjects
Astrophysics
Abstract

AKARI, the first Japanese satellite dedicated to infrared astronomy, was launched on 2006 February 21, and started observations in May of the same year. AKARI has a 68.5 cm cooled telescope, together with two focal-plane instruments, which survey the sky in six wavelength bands from the mid- to far-infrared. The instruments also have the capability for imaging and spectroscopy in the wavelength range 2 - 180 micron in the pointed observation mode, occasionally inserted into the continuous survey operation. The in-orbit cryogen lifetime is expected to be one and a half years. The All-Sky Survey will cover more than 90 percent of the whole sky with higher spatial resolution and wider wavelength coverage than that of the previous IRAS all-sky survey. Point source catalogues of the All-Sky Survey will be released to the astronomical community. The pointed observations will be used for deep surveys of selected sky areas and systematic observations of important astronomical targets. These will become an additional future heritage of this mission., Comment: 13 pages, 4 figures, and 3 tables. Accepted for publication in the AKARI special issue of the Publications of the Astronomical Society of Japan

Published
2007
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13. Discovery and identification of the very high redshift afterglow of GRB 050904

Author

Haislip, J., Nysewander, M., Reichart, D., Levan, A., Tanvir, N., Cenko, S., Fox, D., Price, P., Castro-Tirado, A., Gorosabel, J., Evans, C., Figueredo, E., MacLeod, C., Kirschbrown, J., Jelinek, M., Guziy, S., Postigo, A. de Ugarte, Cypriano, E., LaCluyze, A., Graham, J., Priddey, R., Chapman, R., Rhoads, J., Fruchter, A., Lamb, D., Kouveliotou, C., Wijers, R., Schmidt, B., Soderberg, A., Kulkarni, S., Harrison, F., Moon, D., Gal-Yam, A., Kasliwal, M., Hudec, R., Vitek, S., Kubanek, P., Crain, J., Foster, A., Bayliss, M., Clemens, J., and Bartelme, J.

Subjects
Astrophysics
Abstract

In 2000, Lamb and Reichart predicted that gamma-ray bursts (GRBs) and their afterglows occur in sufficient numbers and at sufficient brightnesses at very high redshifts (z > 5) to eventually replace quasars as the preferred probe of element formation and reionization in the early universe and to be used to characterize the star-formation history of the early universe, perhaps back to when the first stars formed. Here we report the discovery of the afterglow of GRB 050904 and the identification of GRB 050904 as the first very high redshift GRB. We measure its redshift to be 6.39(+0.11,-0.12), which is consistent with the reported spectroscopic redshift (6.29 +/- 0.01). Furthermore, just redward of Ly-alpha the flux is suppressed by a factor of three on the first night, but returns to expected levels by the fourth night. We propose that this is due to absorption by molecular hydrogen that was excited to rovibrational states by the GRB's prompt emission, but was then overtaken by the jet. Now that very high redshift GRBs have been shown to exist, and at least in this case the afterglow was very bright, observing programs that are designed to capitalize on this science will likely drive a new era of study of the early universe, using GRBs as probes., Comment: Submitted to Nature, 11 pages, 3 figures, LaTeX

Published
2005
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14. The Stellar Content of Obscured Galactic Giant HII Regions V: G333.1--0.4

Author

Figueredo, E., Blum, R. D., Damineli, A., and Conti, P. S.

Subjects
Astrophysics
Abstract

We present high angular resolution near--infrared images of the obscured Galactic Giant HII (GHII) region G333.1--0.4 in which we detect an OB star cluster. For G333.1--0.4, we find OB stars and other massive objects in very early evolutionary stages, possibly still accreting. We obtained $K$--band spectra of three stars; two show O type photospheric features, while the third has no photospheric features but does show CO 2.3 $\mu$m band--head emission. This object is at least as hot as an early B type star based on its intrinsic luminosity and is surrounded by a circumstellar disc/envelope which produces near infrared excess emission. A number of other relatively bright cluster members also display excess emission in the $K$--band, indicative of disks/envelopes around young massive stars. Based upon the O star photometry and spectroscopy, the distance to the cluster is 2.6 $\pm$ 0.4 kpc, similar to a recently derived kinematic (near side) value. The slope of the $K$--band luminosity function is similar to those found in other young clusters. The mass function slope is more uncertain, and we find $-1.3 \pm 0.2 < \Gamma < -1.1 \pm 0.2$- for stars with M $> 5$ M$_\odot$ where the upper an lower limits are calculated independently for different assumptions regarding the excess emission of the individual massive stars. The number of Lyman continuum photons derived from the contribution of all massive stars in the cluster is 0.2 $\times$ $10^{50}$ $s^{-1}$ $< NLyc < 1.9$ $\times$ $10^{50}$ $s^{-1}$. The integrated cluster mass is 1.0 $\times$ $10^{3}$ $M_\odot < M_{cluster} < 1.3$ $\times$ $10^{3}$ $M_\odot$., Comment: 31 pages, including 12 figures and 3 tables. Accepted for publication in the AJ

Published
2004
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15. The Stellar Content of Obscured Galactic Giant H II Regions IV.: NGC3576

Author

Figueredo, E., Blum, R. D., Damineli, A., and Conti, P. S.

Subjects
Astrophysics
Abstract

We present deep, high angular resolution near-infrared images of the obscured Galactic Giant H II region NGC3576. Our images reach objects to ~3M_sun. We collected high signal-to-noise K-band spectra of eight of the brightest objects, some of which are affected by excess emission and some which follow a normal interstellar reddening law. None of them displayed photospheric features typical of massive OB type stars. This indicates that they are still enshrouded in their natal cocoons. The K-band brightest source (NGC3576 #48) shows CO 2.3 micron bandhead emission, and three others have the same CO feature in absorption. Three sources display spatially unresolved H_2 emission, suggesting dense shocked regions close to the stars. We conclude that the remarkable object NGC3576 #48 is an early-B/late-O star surrounded by a thick circumstellar disk. A number of other relatively bright cluster members also display excess emission in the K-band, indicative of reprocessing disks around massive stars (YSOs). Such emission appears common in other Galactic Giant H II regions we have surveyed. The IMF slope of the cluster, Gamma = -1.51, is consistent with Salpeter's distribution and similar to what has been observed in the Magellanic Cloud clusters and in the periphery of our Galaxy., Comment: 14 pages, 11 figures, accepted for publication in AJ

Published
2002
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16. Atitudes de profissionais da saúde em relação ao comportamento suicida

Author

Bárbara Diniz Storino, Carolina Figueredo e Campos, Luciana Coutinho de Oliveira Chicata, Mariana de Almeida Campos, Mayra Soares da Costa Matos, Roberta Martins Carvalho Mesquita Nunes, and Carlos Eduardo Leal Vidal

Subjects
suicídio, profissional de saúde, atitude, atenção básica à saúde, Public aspects of medicine, RA1-1270
Abstract

Resumo Introdução O suicídio ocupa um lugar de destaque entre os agravos que atingem as populações devido ao grande impacto familiar, psicossocial e econômico. A atenção básica à saúde é o primeiro local onde são atendidos indivíduos que apresentam comportamento suicida, e as atitudes dos profissionais podem ser determinantes para a evolução dos casos. Objetivo Verificar as atitudes de profissionais da atenção básica diante do comportamento suicida. Método Estudo transversal, com aplicação do Questionário de Atitudes em Relação ao Comportamento Suicida aos profissionais da atenção básica do município de Barbacena-MG. Resultados A maioria da amostra foi representada por agentes de saúde, do sexo feminino, com idade entre 30-39 anos e com instrução média. Foram observadas mais atitudes positivas entre os médicos e os enfermeiros quando comparados aos outros profissionais. Não foram verificadas diferenças significativas das atitudes em relação ao sexo e à idade dos participantes. Conclusão Os técnicos de enfermagem e os agentes de saúde apresentaram atitudes mais negativas em relação aos demais. Esse é um dado que deve ser levado em conta nos programas de capacitação. O treinamento dos profissionais deve contemplar habilidades cognitivas e mudanças nas atitudes que possam favorecer a empatia e a compreensão do comportamento suicida, priorizando a capacitação dos agentes de saúde.

Published
2018
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17. EMPREENDEDORISMO FEMININO: O PERFIL GERENCIAL DA MULHER EMPREENDEDORA DA CIDADE DE BACABAL-MA

Author

Ana Paula da Cunha Costa, Pauliane de Sousa Freitas, Marcus Vinicius Gomes Frota, Francisco de Sousa Lima Neto, and Simone Maria de Figueredo E Silva

Subjects
General Medicine
Abstract

O empreendedorismo feminino tem se tornado cada vez mais visível nas organizações e nos negócios em geral. As experiências bem sucedidas de empresas criadas por mulheres, bem como a sobrevivência do número significativo de novos empreendimentos geridos por estas, tem sido um fator de grande relevância para a realização de estudos e pesquisas. O objetivo desse estudo é analisar o perfil gerencial das mulheres empreendedoras na cidade Bacabal-MA, bem como verificar o comportamento estratégico, identificar sua capacidade criativa e verificar a formalização de seus empreendimentos. O presente artigo foi desenvolvido através de uma pesquisa descritiva junto a 50 empreendedoras em diferentes setores de atividades, no qual os dados foram levantados por meio da aplicação de questionários correspondendo a uma pesquisa quanti-qualitativa. Através da análise de dados constatou-se que as empreendedoras tem iniciado sua atividade em sua maioria pela vontade de ter o próprio negócio, uma vez que suas características mais marcantes foram capacidade de organização, relação interpessoal, praticidade, e a valorização da criatividade, posto pelas empreendedoras como diferencial competitivo, fazendo uso de uma gestão mais flexível e uma visão mais estratégica. Pode-se perceber ainda, que as empreendedoras pesquisadas são comprometidas e responsáveis com seus negócios, posto que, quase em sua totalidade já iniciaram sua atividade na formalidade, estão a mais de 10 anos no mercado e já tinham um conhecimento prévio de sua área de atuação. Os resultados permitiram concluir, que o perfil gerencial adotado por elas, tem contribuído para o sucesso e a sobrevivência significativa dos seus empreendimentos.

Published
2023
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18. Uma análise da dor do membro fantasma

Author

Ferreira, Thomaz Mota Cabo, primary, Bullos, Bernardo Silva, additional, Costa, Ana Clara Martins da, additional, Silva, Thales Figueredo e, additional, Ferreira, Igor Azevedo, additional, Marins, Amanda Souza, additional, and Siqueira, Emílio Conceição de, additional

Published
2023
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19. The Stellar Population of Embedded Galactic Massive Star Clusters

Author

Damineli, A., Blum, R. D., Conti, P. S., Figuerêdo, E., Barbosa, C. L., Appenzeller, I., Bahcall, J. N., Bertola, F., Cassinelli, J. P., Cesarsky, C. J., Engvold, O., McCray, R., Murdin, P. G., Pacini, F., Radhakrishnan, V., Sato, K., Shu, F. H., Somov, B. V., Sunyaev, R. A., Tanaka, Y., Tremaine, S., Weiss, N.O., Burton, W.B., editor, Kuijpers, J. M. E., editor, Van Den Heuvel, E. P. J., editor, Van Der Laan, H., editor, Lépine, Jacques, editor, and Gregorio-Hetem, Jane, editor

Published
2003
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20. ¿'AGRO SIN PARTIDO'? COERCIÓN Y CONSENSO - LA INSERCIÓN DE EL AGRONEGOCIO EN LA EDUCACIÓN BRASILEÑA

Author

Balbi de Figueredo e Cordeiro, Tássia Gabriele

Abstract

This article analyzes the insertion of agribusiness into education, specifically, the campaign De Olho no Material Escolar and its crossings with the procedures of Escola sem Partido movement. To this end, we conducted bibliographical and documentary research on the topics in question. As a result, we observed compelling evidence that De Olho no Material Escolar is part of a political-ideological expansion of agribusiness that seeks to influence Brazilian educational practices, through the combination of strength and consensus, reproducing the strategies applied by Escola sem Partido in a more sophisticated way.Keyword: Agribusiness; Agrarian question; Education. En este artículo analizamos la inserción del agronegocio en la educación, en concreto, la campaña De Olho no Material Escolar y sus articulaciones con los trámites de la Escola sem Partido. Para ello, realizamos una investigación bibliográfica y documental sobre los temas en cuestión. Como resultado, observamos evidencias de que De Olho no Material Escolar es parte de una expansión político-ideológica del agronegocio que busca, a través de la combinación de fuerza y consenso, interferir en la dirección de la educación brasileña, reproduciendo de manera más sofisticada los métodos desarrollados por la Escola sem Partido.Palabra clave: Agronegocio; Cuestión agraria; Educación. Palabra clave: Agronegocio; Cuestión agraria; Educación. Neste artigo analisamos a inserção do agronegócio na educação, especificamente, a campanha De Olho no Material Escolar e seus atravessamentos com os procedimentos do Escola sem Partido. Para tanto, realizamos pesquisa bibliográfica e documental acerca das temáticas em questão. Como resultado, observamos indícios de que o De Olho no Material Escolar compõe uma frente de expansão político-ideológica do agronegócio que busca, por meio da combinação entre força e consenso, interferir nos rumos da educação brasileira, reproduzindo de forma mais sofisticada os métodos desenvolvidos pelo Escola sem Partido.Palavra-chave: Agronegócio; Questão Agrária; Educação.

Published
2022
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21. Uma análise da dor do membro fantasma

Author

Thomaz Mota Cabo Ferreira, Bernardo Silva Bullos, Ana Clara Martins da Costa, Thales Figueredo e Silva, Igor Azevedo Ferreira, Amanda Souza Marins, and Emílio Conceição de Siqueira

Abstract

Objetivo: Analisar as características da dor do membro fantasma (DMF). Revisão bibliográfica: A DMF é uma condição debilitante caracterizada por sensações dolorosas na parte ausente do membro amputado. A DMF ocorre em até 85% dos amputados, tornando-se a condição de dor crônica mais comum em pessoas que sofreram amputações de membros. Múltiplas teorias foram propostas para explicar o mecanismo subjacente da DMF, sendo a reorganização cortical a mais comum. Existem dois picos de aparecimento da DMF, sendo um até a primeira semana de amputação e o outro com um ano com sensações dolorosas variando entre aguda, tiro, queimação, latejante, esfaqueamento e dor. Considerações finais: A dor do membro fantasma está associada a sofrimento pessoal, interferência nas atividades diárias gerais, incapacidade e redução da qualidade de vida relacionada à saúde. Nesse contexto, torna-se essencial o reconhecimento e tratamento adequado desta condição, visando a melhora da qualidade de vida. Na atualidade, a terpêutica da DMF é feita através de mecanismos farmacológicos como a gabapentina, morfina, cetamina e dextrometorfano e tratamentos não farmacológicos como a terapia dos espelhos.

Published
2023
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24. Alternativa restauradora por meio de endocrown: uma revisão da literatura

Author

João Nilton Lopes de Sousa, Rodrigo Alves Ribeiro, José Henrique de Araújo Cruz, Bárbara Vanessa De Brito Monteiro, Daniela Lima Cristino, Monnyk Stefane Figueredo e Silva, and Rodrigo Araújo Rodrigues

Subjects
Orthodontics, Physics, Fatigue resistance, CEREC, All ceramic, Resin coating, Resin composite, INT, Clinical performance, General Medicine, Load bearing
Abstract

Introdução: A coroa endocrown é uma restauração indireta confeccionada em cerâmica adesiva em monobloco e cimentada com técnicas adesivas. A coroa possui como retenção a câmara pulpar do dente tratado endodonticamente sem que se utilizem os condutos. Dentes tratados endodonticamente possuem redução da rigidez e resistência devido à perda da integridade estrutural. Este fato pode acarretar em longo prazo falhas biomecânicas. Objetivo: Realizar uma revisão de literatura do tipo narrativa acerca das principais características das endocrowns. Metodologia: A pesquisa foi realizada no período de 20 de Janeiro a 02 de Abril de 2019. Foram utilizados artigos científicos das seguintes bases de dados: SCIELO (Scientific Eletronic Library Online), BVS (Biblioteca Virtual em Saúde), e monografias que atendiam aos requisitos no período entre 2008 a 2019, com exceção de artigos clássicos, em língua nacional, português, bem como em inglês e espanhol. Foram utilizados como descritores isolados, ou combinados, para a busca: "Endocrown”, “Endocrown Prótese”, “Endocrown Prosthesis”, “Endocrown Prótesis”, com um resultado de 31 artigos utilizados. Conclusão: As endocrowns são indicadas para dentes posteriores tratados endodonticamente, confeccionada na maioria das vezes por dissilicato de lítio e apresenta estudos que comprovem que o risco de fratura é inferior às reabilitações sob uso de retentores intrarradiculares. Sob boa indicação e avaliação, é possível obter previsibilidade de sucesso, porém, ainda são necessários mais pesquisas para comprovar cada vez mais a eficácia dessa alternativa.Descritores: Prótese Dentária; Prótese Parcial Fixa; Odontologia.ReferênciasRocca GT, Rizcalla N, Krejci I. Fiber-reinforced resin coating for endocrown preparations: a technical report. Oper Dent. 2013;38(3):242-48.Borges Junior HE, Sábio S, Bender KRF, Costa YM, Mondelli J. Endocrown – avaliação da resistência dos cimentos dentários. Rev Odontol Araçatuba. 2013;34(2):23-6.Dejak B, Młotkowski A. 3D-Finite element analysis of molars restored with endocrowns and posts during masticatory simulation. Dent Mater. 2013;29(12):e309-17.Chang CY, Kuo JS, Lin YS, Chang YH. Fracture resistance and failure modes of CEREC endo-crowns and conventional post and core-supported CEREC crowns. J Dent Sci 2009;4(3):110-17.Carlos RB, Thomas Nainan M, Pradhan S, Sharma R, Benjamin S, Rose R. Restoration of endodontically treated molars using all ceramic endocrowns. Cape Rep Dent. 2013;2013:210763.Magne P, Knezevic A. Simulated fatigue resistance of composite resin versus porcelain CAD/CAM overlay restorations on endodontically treated molars. Quintessence Int. 2009;40(2):125-33.Biacchi GR, Mello B, Basting RT. The endocrown: an alternative approach for restoring extensively damaged molars. J Esthet Restor Dent. 2013;25(6):383-90.Dietschi D, Duc O, Krejci I, Sadan A. Biomechanical considerations for the restoration of endodontically treated teeth: a systematic review of the literature, Part II (Evaluation of fatigue behavior, interfaces, and in vivo studies). Quintessence Int. 2008;39(2):117-29.Mörmann WH, Bindl A, Lüthy H, Rathke A. Effects of preparation and luting system on all-ceramic computer-generated crowns. Int J Prosthodont. 1998;11(4):333-39.Bernardo WM, Nobre MRC, Jatene FB. A prática clinica baseada em evidências. Parte II: buscando as evidências em fontes de informação. Rev Assoc Med Bras. 2004;50(1):104-8.Zavanelli AC, Zavanelli RA, Mazaro JVQ, Lemos CAA, Dias ES, Silva EV, Pinto RC. Coroas Endoncrown: uma revisão de literatura e relato de caso. Arch Health Invest. 2017;6(8):382-89.Rocca GT, Saratti CM, Cattani-Lorente M, Feilzer AJ, Scherrer S, Krejci I. The effect of a fiber reinforced cavity configuration on load bearing capacity and failure mode of endodontically treated molars restored with CAD/CAM resin composite overlay restorations. J Dent. 2015;43(9):1106-15.Gresnigt MM, Özcan M, van den Houten ML, Schipper L, Cune MS. Fracture strength, failure type and Weibull characteristics of lithium disilicate and multiphase resin composite endocrowns under axial and lateral forces. Dent Mater. 2016;32(5):607-14.Rocca GT, Sedlakova P, Saratti CM, Sedlacek R; Gregor L; Rizcalla N et al. Fatigue behavior of resin-modified monolithic CAD-CAM RNC crowns and endocrowns. Dent Mater. 2016;32(12):e338-50.Fages M, Bennasar B. The endocrown: a different type of all-ceramic reconstruction for molars. J Can Dent Assoc. 2013;79:d140.Hayes A, Duvall N, Wajdowicz M, Roberts H. Effect of Endocrown Pulp Chamber Extension Depth on Molar Fracture Resistance. Oper Dent. 2017;42(3):327-34.Gaintantzopoulou MD, El-Damanhoury HM. Effect of Preparation Depth on the Marginal and Internal Adaptation of Computer-aided Design/Computer-assisted Manufacture Endocrowns. Oper Dent. 2016;41(6):607-16.Baratieri LN, Monteiro S JR. Coroas posteriores endocrown. In: Baratieri L N. Odontologia restauradora: fundamentos e técnicas, São Paulo: Santos, 2010. v. 2, cap.30, p.738-55.Rocca GT, Saratti CM, Poncet A, Feilzer AJ, Krejci I. The influence of FRCs reinforcement on marginal adaptation of CAD/CAM composite resin endocrowns after simulated fatigue loading. Odontology. 2016;104(2):220-32.Sedrez-Porto JA, Rosa WL, da Silva AF, Münchow EA, Pereira-Cenci T. Endocrown restorations: A systematic review and meta-analysis. J Dent. 2016;52:8-14.Borgia Botto E, Barón R, Borgia JL. Endocrown: Estudio clínico retrospectivo de una serie de pacientes, en un período de 8 a 19 años. Odontoestomatología 2016;18(28):48-59.Rayyan MR, Alauti RY, Abanmy MA, AlReshaid RM, Bin Ahmad HA. Endocrowns versus post-core retained crowns for restoration of compromised mandibular molars: an in vitro study. Int J Comput Dent. 2019;22(1):39-44.Silva ACC, Santos FB. Opções protéticas para dentes posteriores tratados endodonticamente: revisão de literatura [monografia]. Lagarto - SE: Departamento de Odontologia de Lagarto da Universidade Federal de Sergipe – UFS; 2018.El-Damanhoury HM, Haj-Ali RN, Platt JA. Fracture resistance and microleakage of endocrowns utilizing three CAD-CAM blocks. Oper Dent. 2015;40(2):201-10.Valentina V, Aleksandar T, Dejan L, Vojkan L. Restoring endodontically treated teeth with all-ceramic endo-crowns - case report. Serbian Dent J 2008;55:54-64.Tysowsky GW. The science behind lithium disilicate: a metal-free alternative. Dent Today. 2009;28(3):112-13.Qin F, Zheng S, Luo Z, Li Y, Guo L, Zhao Y et al. Evaluation of machinability and flexural strength of a novel dental machinable glass-ceramic. J Dent. 2009;37(10):776-80.El Ghoul W, Özcan M, Silwadi M, Salameh Z. Fracture resistance and failure modes of endocrowns manufactured with different CAD/CAM materials under axial and lateral loading. J Esthet Restor Dent. 2019;31(4):378-87. El Ghoul WA, Özcan M, Ounsi H, Tohme H, Salameh Z. Effect of different CAD-CAM materials on the marginal and internal adaptation of endocrown restorations: An in vitro study. J Prosthet Dent. 2020;123(1):128-34.Zou Y, Bai J, Xiang J. Clinical performance of CAD/CAM-fabricated monolithic zirconia endocrowns on molars with extensive coronal loss of substance. Int J Comput Dent. 2018;21(3):225-32.

Published
2020
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27. A photometric redshift of z = 6.39 ± 0.12 for GRB 050904

Author

Haislip, J. B., Nysewander, M. C., Reichart, D. E., Levan, A., Tanvir, N., Cenko, S. B., Fox, D. B., Price, P. A., Castro-Tirado, A. J., Gorosabel, J., Evans, C. R., Figueredo, E., MacLeod, C. L., Kirschbrown, J. R., Jelinek, M., Guziy, S., de Ugarte Postigo, A., Cypriano, E. S., LaCluyze, A., Graham, J., Priddey, R., Chapman, R., Rhoads, J., Fruchter, A. S., Lamb, D. Q., Kouveliotou, C., Wijers, R. A. M. J., Bayliss, M. B., Schmidt, B. P., Soderberg, A. M., Kulkarni, S. R., Harrison, F. A., Moon, D. S., Gal-Yam, A., Kasliwal, M. M., Hudec, R., Vitek, S., Kubanek, P., Crain, J. A., Foster, A. C., Clemens, J. C., Bartelme, J. W., Canterna, R., Hartmann, D. H., Henden, A. A., Klose, S., Park, H.-S., Williams, G. G., Rol, E., O'Brien, P., Bersier, D., Prada, F., Pizarro, S., Maturana, D., Ugarte, P., Alvarez, A., Fernandez, A. J. M., Jarvis, M. J., Moles, M., Alfaro, E., Ivarsen, K. M., Kumar, N. D., Mack, C. E., Zdarowicz, C. M., Gehrels, N., Barthelmy, S., and Burrows, D. N.

Published
2006

31. Mites in Madrid

Author

Sastre, J, Iraola, V, Figueredo, E, Tornero, P, and Fernandez-Caldas, E

Published
2002

38. Beer-induced anaphylaxis

Author

Figueredo, E., Quirce, S., Lahoz, C., del Amo, A., de las Heras, M., and Sastre, J.

Published
1998

40. Anaphylactic reaction to methotrexate

Author

Lluch-Bernal, M., Cuesta-Herranz, J., De las Heras, M., Figueredo, E., Umpierrez, A., Fernandez, M., Novalbos, A., Casimiro, C., and Sastre, J.

Published
1997

41. Anaphylaxis to dexamethasone

Author

Figueredo, E., Cuesta-Herranz, J., De Las Heras, M., Lluch-Bernal, M., Umpierrez, A., and Sastre, J.

Published
1997

42. UM ESFORÇO DE PESQUISA: PENSAR A EDUCAÇÃO DE JOVENS SURDOS NA TENSÃO ENTRE O MAIOR E O MENOR DA EDUCAÇÃO

Author

Anelice Astrid Ribetto and Luma Balbi de Figueredo E Cordeiro

Subjects
General Medicine
Abstract

Este ensaio tem como objetivo central dar a ver e enunciar as tensõesentre Histórias e Políticas da Educação de Surdos e as histórias escolaresde quatro jovens surdos em Rio Bonito. Trabalhamos em diálogo com ométodo deleuzeguatarriano de cartografia e produzimos umdeslocamento do conceito de literatura menor para a noção de históriamenor. A "história menor" é aqui entendida como um dispositivoinstituinte que nos ajuda a pensar as trajetórias escolares das pessoassurdas como micropolíticas de resistência às formas que majoritariamentevêm sendo inventadas e, em decorrência destas invenções, produzindoefeitos de exclusão escolar.

Published
2017
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45. Frecuencia de Hipertensión Arterial en pacientes de primera consulta en consultorio externo de la Primera Cátedra de Clínica Médica, Hospital de Clínicas, año 2012

Author

Ortiz Galeano, I, Brizuela, M, Cardenas, M, Figueredo, E, and Chirico Achinelli, C

Subjects
cardiovascular risk factors, frecuencia, hipertensión arterial, hypertension, consultorio, frequency, factores de riesgo cardiovascular, outpatient care
Abstract

La hipertensión arterial es un factor de riesgo para el desarrollo de enfermedades cardiovasculares, principales causas de mortalidad en todo el mundo. El objetivo de este trabajo fue determinar la frecuencia de hipertensión arterial y su asociación con otros factores de riesgo cardiovascular en pacientes de primera consulta en el consultorio de la Primera Cátedra de Clínica Médica del Hospital de Clínicas, FCM, UNA en 2012. Se realizó unestudio observacional, descriptivo, retrospectivo, con componente analítico en el que se estudió a pacientes entre 18 y 90 años, seleccionados por muestreo aleatorio simple. En el periodo de estudio se registraron 4.046 historias clínicas en primera consulta, y 3.854 fueron consideradas para la aleatorización. Se estudiaron las variables demográficas, antropométricas, bioquímicas, presencia de hipertensión arterial, diabetes mellitus tipo 2, consumo de alcohol y tabaco. Se analizaron las historias clínicas de 457 pacientes con una edad media de 44,13±17 años; 48,23±18 años en hombres y 46,61±11 años en mujeres,300 (66%) fueron mujeres. La frecuencia de la hipertensión arterial± IC95%fue de30,41±4,2%, sin diferencia significativa entre mujeres y hombres (32,33±4,3% versus 28±4,1%). La obesidad fue el factor de riesgo cardiovascular más frecuente. Alrededor del 60% de los pacientes presentaba uno o más factores de riesgo cardiovascular.La hipertensión arterial se asoció conla obesidad (OR:4,427; IC95%: 2,345-4,876; p=0,032), la diabetes (OR: 2,141; IC 95%: 1,261-2,347; p=0,005) y niveles de c-HDL

Published
2014

46. Surgical treatments for esophageal cancers

Author

Allum, WH, Bonavina, L, Cassivi, SD, Cuesta, MA, Dong, ZM, Felix, VN, Figueredo, E, Gatenby, PAC, Haverkamp, L, Ibraev, MA, Krasna, MJ, Lambert, R, Langer, R, Lewis, MPN, Nason, KS, Parry, K, Preston, SR, Ruurda, JP, Schaheen, LW, Tatum, RP, Turkin, IN, Van Der Horst, S, Van Der Peet, DL, Van Der Sluis, PC, Van Hillegersberg, R, Wormald, JCR, Wu, PC, Zonderhuis, BM, Surgery, and CCA - Innovative therapy

Subjects
Article
Abstract

The following, from the 12th OESO World Conference: Cancers of the Esophagus, includes commentaries on the role of the nurse in preparation of esophageal resection (ER); the management of patients who develop high‐grade dysplasia after having undergone Nissen fundoplication; the trajectory of care for the patient with esophageal cancer; the influence of the site of tumor in the choice of treatment; the best location for esophagogastrostomy; management of chylous leak after esophagectomy; the optimal approach to manage thoracic esophageal leak after esophagectomy; the choice for operational approach in surgery of cardioesophageal crossing; the advantages of robot esophagectomy; the place of open esophagectomy; the advantages of esophagectomy compared to definitive chemoradiotherapy; the pathologist report in the resected specimen; the best way to manage patients with unsuspected positive microscopic margin after ER; enhanced recovery after surgery for ER: expedited care protocols; and long‐term quality of life in patients following esophagectomy.

Published
2014
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47. Atitudes de profissionais da saúde em relação ao comportamento suicida.

Author

Diniz Storino, Bárbara, Figueredo e Campos, Carolina, de Oliveira Chicata, Luciana Coutinho, de Almeida Campos, Mariana, da Costa Matos, Mayra Soares, Carvalho Mesquita Nunes, Roberta Martins, and Leal Vidal, Carlos Eduardo

Abstract

Background: Suicide and suicide attempts occupy a prominent place among diseases affecting the population due to their great impact on family, psychosocial and economy. Health professionals' attitudes are important since their knowledge and view about suicide can significantly influence their behavior toward patients. Objective: To verify the attitudes of health care professionals towards the suicidal patients. Method: This is a cross-sectional study in which we applied the Suicide Behavior Attitude Questionnaire to health care professionals in the city of Barbacena, Minas Gerais. Results: The majority of the sample was represented by health agents, female, age between 30 and 39 years, with average level of education. Doctors and nurses had the most positive attitudes when compared to other professionals. There were no significant differences in attitudes regarding gender and age of participants. Conclusion: The results indicated that nursing technicians and health agents presented more negative attitudes when compared to doctors and nurses. This is a relevant fact and should be taken into account by the training programs. The training of professionals should contemplate cognitive skills and changes in attitudes that may favor the empathy and understanding of these behaviors. [ABSTRACT FROM AUTHOR]

Published
2018
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48. Release of the AKARI-FIS Bright Source Catalogue β-1

Author

Yamamura, I., Makiuti, S., Ikeda, N., Fukuda, Y., Yamauchi, C., Hasegawa, S., Nakagawa, T., Narumi, H., Baba, H., Takagi, T., Jeong, W. -S, Oh, S. H., Lee, H. M., Savage, R., Rahman, N., Thomson, M., Oliver, S., Figueredo, E., Stephen Serjeant, Glenn White, Chris Pearson, Wang, L., Rowan-Robinson, M., Kester, Do, Wolk, G., Barthel, P., Salama, A., Alfageme, C., García-Lario, P., Stephenson, C., Cohen, M., Mueller, T. G., and Astronomy

Abstract

The AKARI; satellite has made an All-Sky Survey at six bands in the mid- and far-infrared spectral region. One of the primary goals of the AKARI survey is to produce all-sky infrared source catalogues. We report the release of the first version of the AKARI FIS Bright Source Catalogue (β-1) for four of the six wavelengths (65, 90, 140, 160 μm), containing ˜ 63,000 sources. The detection limit of the most sensitive band (90 μm) is ˜1.3 Jy, corresponding approximately to a 10 σ noise level. The photometric accuracy is 30-60%, depending on the band, and the position uncertainty, currently dominated by the FIS data processing, is 4-5 arcsec. The catalogue was prepared for initial scientific validation by the AKARI science team. The revised version will enter the public domain in Autumn 2009. The two other wavelength bands (9 & 18 μm) data are processed separately for the IRC point source catalogues.

Published
2009

49. A photometric redshift of z = 6.39 ± 0.12 for GRB 050904

Author

Ivarsen, K.M., Levan, A., Fernandez, A.J.M., Barthelmy, S., MacLeod, C.L., Hartmann, D.H., Canterna, R., Moon, D.S., Bayliss, M.B., Tanvir, N., Gorosabel, J., Zdarowicz, C.M., Lamb, D.Q., Kulkarni, S.R., Fruchter, A.S., Gehrels, N., Moles, M., Hudec, R., Alvarez, A., Bartelme, J.W., Guziy, S., Kirschbrown, J.R., Evans, C.R., Castro-Tirado, A.J., Price, P.A., Rol, E., Williams, G.G., Prada, F., Bersier, D., Chapman, R., Alfaro, E., Crain, J.A., Priddey, R., Reichart, D.E., Rhoads, J., Mack, C.E., Kasliwal, M.M., Clemens, J.C., De Ugarte Postigo, A., Foster, A.C., Jelinek, M., Park, H.-S., Maturana, D., Burrows, D.N., O'Brien, P., Soderberg, A.M., Kubanek, P., Graham, J., LaCluyze, A., Kumar, N.D., Ugarte, P., Gal-Yam, A., Cenko, S.B., Haislip, J.B., Klose, S., Henden, A.A., Vitek, S., Pizarro, S., Jarvis, M.J., Schmidt, B.P., Fox, D.B., Nysewander, M.C., Wijers, R.A.M.J., Figueredo, E., Cypriano, E.S., Kouveliotou, C., and Harrison, F.A.

Abstract

Gamma-ray bursts (GRBs) and their afterglows are the most brilliant transient events in the Universe. Both the bursts themselves and their afterglows have been predicted to be visible out to redshifts of z ≈ 20, and therefore to be powerful probes of the early Universe1,2. The burst GRB 000131, at z = 4.50, was hitherto the most distant such event identified3. Here we report the discovery of the bright near-infrared afterglow of GRB 050904 (ref. 4). From our measurements of the near-infrared afterglow, and our failure to detect the optical afterglow, we determine the photometric redshift of the burst to be z = 6.39-0.12+0.11 (refs 5-7). Subsequently, it was measured8 spectroscopically to be z = 6.29 ± 0.01, in agreement with our photometric estimate. These results demonstrate that GRBs can be used to trace the star formation, metallicity, and reionization histories of the early Universe.

Published
2006
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