Journal articles: 'Othlo'

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Dana, Kathleen Osgood, and Daniel Katz. "Otelo." World Literature Today 69, no. 3 (1995): 617. http://dx.doi.org/10.2307/40151521.

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Navarro Martínez, Rocío, Ana María Pérez-García, Ricardo Pérez-Martínez, Miguel Cerviño, Jesús Gallego, Ángel Bongiovanni, Laia Barrufet, et al. "The OTELO survey." Astronomy & Astrophysics 653 (September 2021): A24. http://dx.doi.org/10.1051/0004-6361/202140353.

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Aims. We study a sample of Hβ emission line sources at z ∼ 0.9 to identify the star-forming galaxies sample and characterise them in terms of line luminosity, stellar mass, star formation rate, and morphology. The final aim is to obtain the Hβ luminosity function of the star-forming galaxies at this redshift. Methods. We used the red tunable filter of the instrument Optical System for Imaging low Resolution Integrated Spectroscopy (OSIRIS) at Gran Telescopio de Canarias to obtain the pseudo spectra of emission line sources in the OTELO field. From these pseudo spectra, we identified the objects with Hβ emission. As the resolution of the pseudo spectra allowed us to separate Hβ from [O III], we were able to derive the Hβ flux without contamination from its adjacent line. Using data from the extended OTELO catalogue, we discriminated AGNs and studied the star formation rate, the stellar mass, and the morphology of the star-forming galaxies. Results. We find that our sample is located on the main sequence of star-forming galaxies. The sources are morphologically classified, mostly as disc-like galaxies (76%), and 90% of the sample are low-mass galaxies (M* < 1010 M⊙). The low-mass star-forming galaxies at z ∼ 0.9 that were detected by OTELO present similar properties as low-mass star-forming galaxies in the local universe, suggesting that these kinds of objects do not have a favorite epoch of formation and star formation enhancement from z ∼ 1 to now. Our sample of 40 Hβ star-forming galaxies include the faintest Hβ emitters detected so far. This allows us to constrain the faint end of the luminosity function for the Hβ line alone with a minimum luminosity of log L = 39 erg s−1, which is a hundred times fainter than previous surveys. The dust-corrected OSIRIS Tunable Emission Line Object survey (OTELO) Hβ luminosity function established the faint-end slope as α = −1.36 ± 0.15. We increased the scope of the analysis to the bright end by adding ancillary data from the literature, which was not dust-corrected in this case. The obtained slope for this extended luminosity function is α = −1.43 ± 0.12.

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Cedrés, B., Á. Bongiovanni, M. Cerviño, J. Nadolny, J. Cepa, J. A. de Diego, A. M. Pérez García, et al. "The OTELO survey." Astronomy & Astrophysics 649 (May 2021): A73. http://dx.doi.org/10.1051/0004-6361/202039880.

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Aims. In this paper, we aim to study the main properties and luminosity function (LF) of the [O II]3727 emitters detected in the OTELO survey in order to characterise the star formation processes in low-mass galaxies at z ∼ 1.43 and to constrain the faint-end of the LF. Methods. Here, we describe the selection method and analysis of the emitters obtained from narrow-band scanning techniques. In addition, we present several relevant properties of the emitters and discuss the selection biases and uncertainties in the determination of the LF and the star formation rate density (SFRD). Results. We confirmed a total of 60 sources from a preliminary list of 332 candidates as [O II]3727 emitters. Approximately 93% of the emitters have masses in the range of 108 < M*/M⊙ < 109. All of our emitters are classified as late-type galaxies, with a lower value of (u − v) when compared with the rest of the emitters of the OTELO survey. We find that the cosmic variance strongly affects the normalisation (ϕ*) of the LF and explains the discrepancy of our results when compared with those obtained from surveys of much larger volumes. However, we are able to determine the faint-end slope of the LF, namely, α = −1.42 ± 0.06, by sampling the LF down to ∼1 dex lower than in previous works. We present our calculation of the SFRD of our sample and compare it to the value obtained in previous studies from the literature.

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Bongiovanni, Ángel, Marina Ramón-Pérez, Ana María Pérez García, Jordi Cepa, Miguel Cerviño, Jakub Nadolny, Ricardo Pérez Martínez, et al. "The OTELO survey." Astronomy & Astrophysics 631 (October 14, 2019): A9. http://dx.doi.org/10.1051/0004-6361/201833294.

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Context. The evolution of galaxies through cosmic time is studied observationally by means of extragalactic surveys. The usefulness of these surveys is greatly improved by increasing the cosmological volume, in either depth or area, and by observing the same targets in different wavelength ranges. A multi-wavelength approach using different observational techniques can compensate for observational biases. Aims. The OTELO survey aims to provide the deepest narrow-band survey to date in terms of minimum detectable flux and emission line equivalent width in order to detect the faintest extragalactic emission line systems. In this way, OTELO data will complements other broad-band, narrow-band, and spectroscopic surveys. Methods. The red tunable filter of the OSIRIS instrument on the 10.4 m Gran Telescopio Canarias (GTC) is used to scan a spectral window centred at 9175 Å, which is free from strong sky emission lines, with a sampling interval of 6 Å and a bandwidth of 12 Å in the most deeply explored EGS region. Careful data reduction using improved techniques for sky ring subtraction, accurate astrometry, photometric calibration, and source extraction enables us to compile the OTELO catalogue. This catalogue is complemented with ancillary data ranging from deep X-ray to far-infrared, including high resolution HST images, which allow us to segregate the different types of targets, derive precise photometric redshifts, and obtain the morphological classification of the extragalactic objects detected. Results. The OTELO multi-wavelength catalogue contains 11 237 entries and is 50% complete at AB magnitude 26.38. Of these sources, 6600 have photometric redshifts with an uncertainty δ zphot better than 0.2 (1+zphot). A total of 4336 of these sources correspond to preliminary emission line candidates, which are complemented by 81 candidate stars and 483 sources that qualify as absorption line systems. The OTELO survey results will be released to the public on the second half of 2019.

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Ramón-Pérez, Marina, Ángel Bongiovanni, Ana María Pérez García, Jordi Cepa, Maritza A. Lara-López, José A. de Diego, Emilio Alfaro, et al. "The OTELO survey." Astronomy & Astrophysics 631 (October 14, 2019): A10. http://dx.doi.org/10.1051/0004-6361/201833295.

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Aims. We take advantage of the capability of the OTELO survey to obtain the Hα luminosity function (LF) at z ∼ 0.40. Because of the deepest coverage of OTELO, we are able to determine the faint end of the LF, and thus better constrain the star formation rate and the number of galaxies at low luminosities. The AGN contribution to this LF is estimated as well. Methods. We make use of the multiwavelength catalogue of objects in the field compiled by the OTELO survey, which is unique in terms of minimum flux and equivalent width. We also take advantage of the pseudo-spectra built for each source, which allow the identification of emission lines and the discrimination of different types of objects. Results. The Hα luminosity function at z ∼ 0.40 is obtained, which extends the current faint end by almost 1 dex, reaching minimal luminosities of log10Llim = 38.5 erg s−1 (or ∼0.002 M⊙ yr−1). The AGN contribution to the total Hα luminosity is estimated. We find that no AGN should be expected below a luminosity of log10L = 38.6 erg s−1. From the sample of non-AGN (presumably, pure SFG) at z ∼ 0.40 we estimated a star formation rate density of ρSFR = 0.012 ± 0.005 M⊙ yr−1 Mpc−3.

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Ramón-Pérez, Marina, Ángel Bongiovanni, Ana María Pérez García, Jordi Cepa, Jakub Nadolny, Irene Pintos-Castro, Maritza A. Lara-López, et al. "The OTELO survey." Astronomy & Astrophysics 631 (October 14, 2019): A11. http://dx.doi.org/10.1051/0004-6361/201833296.

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Aims. We take advantage of the capabilities of the OSIRIS Tunable Emission Line Object (OTELO) survey to select and study the AGN population in the field. In particular, we aim to perform an analysis of the properties of these objects, including their demography, morphology, and IR luminosity. Focusing on the population of Hα emitters at z ∼ 0.4, we also aim to study the environments of AGN and non-AGN galaxies at that redshift. methods. We make use of the multiwavelength catalogue of objects in the field compiled by the OTELO survey, unique in terms of minimum flux and equivalent width. We also take advantage of the pseudo-spectra built for each source, which allow the identification of emission lines and the discrimination of different types of objects. Results. We obtained a sample of 72 AGNs in the field of OTELO, selected with four different methods in the optical, X-rays, and mid-infrared bands. We find that using X-rays is the most efficient way to select AGNs. An analysis was performed on the AGN population of OTELO in order to characterise its members. At z ∼ 0.4, we find that up to 26% of our Hα emitters are AGNs. At that redshift, AGNs are found in identical environments to non-AGNs, although they represent the most clustered group when compared to passive and star-forming galaxies. The majority of our AGNs at any redshift were classified as late-type galaxies, including a 16% proportion of irregulars. Another 16% of AGNs show signs of interactions or mergers. Regarding the infrared luminosity, we are able to recover all the luminous infrared galaxies (LIRGs) in the field of OTELO up to z ∼ 1.6. We find that the proportion of LIRGs and ultra-luminous infraed galaxies (ULIRGs) is higher among the AGN population, and that ULIRGs show a higher fraction of AGNs than LIRGs.

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Bongiovanni, Ángel, Marina Ramón-Pérez, Ana María Pérez García, Miguel Cerviño, Jordi Cepa, Jakub Nadolny, Ricardo Pérez Martínez, et al. "The OTELO survey." Astronomy & Astrophysics 635 (March 2020): A35. http://dx.doi.org/10.1051/0004-6361/201833656.

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Context. The OSIRIS Tunable Filter Emission Line Object (OTELO) survey is a very deep, blind exploration of a selected region of the Extended Groth Strip and is designed for finding emission-line sources (ELSs). The survey design, observations, data reduction, astrometry, and photometry, as well as the correlation with ancillary data used to obtain a final catalogue, including photo-z estimates and a preliminary selection of ELS, were described in a previous contribution. Aims. Here, we aim to determine the main properties and luminosity function (LF) of the [O III] ELS sample of OTELO as a scientific demonstration of its capabilities, advantages, and complementarity with respect to other surveys. Methods. The selection and analysis procedures of ELS candidates obtained using tunable filter pseudo-spectra are described. We performed simulations in the parameter space of the survey to obtain emission-line detection probabilities. Relevant characteristics of [O III] emitters and the LF ([O III]), including the main selection biases and uncertainties, are presented. Results. From 541 preliminary emission-line source candidates selected around z = 0.8, a total of 184 sources were confirmed as [O III] emitters. Consistent with simulations, the minimum detectable line flux and equivalent width in this ELS sample are ∼5 × 10−19 erg s−1 cm2 and ∼6 Å, respectively. We are able to constrain the faint-end slope (α = −1.03 ± 0.08) of the observed LF ([O III]) at a mean redshift of z = 0.83. This LF reaches values that are approximately ten times lower than those from other surveys. The vast majority (84%) of the morphologically classified [O III] ELSs are disc-like sources, and 87% of this sample is comprised of galaxies with stellar masses of M⋆ < 1010 M⊙.

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Bongiovanni, Ángel, Marina Ramón-Pérez, Ana María Pérez García, Miguel Cerviño, Jordi Cepa, Jakub Nadolny, Ricardo Pérez Martínez, et al. "The OTELO survey." Astronomy & Astrophysics 637 (May 2020): C2. http://dx.doi.org/10.1051/0004-6361/201833656e.

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Nadolny, Jakub, Maritza A. Lara-López, Miguel Cerviño, Ángel Bongiovanni, Jordi Cepa, José A. de Diego, Ana María Pérez García, et al. "The OTELO survey." Astronomy & Astrophysics 636 (April 2020): A84. http://dx.doi.org/10.1051/0004-6361/201936205.

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Context. A sample of low-mass Hα emission line sources at z ∼ 0.4 was studied in the context of the mass-metallicty relation (MZR) and its possible evolution. We drew our sample from the OSIRIS Tunable Emission Line Object (OTELO) survey, which exploits the red tunable filter of OSIRIS at the Gran Telescopio Canarias to perform a blind narrow-band spectral scan in a selected field of the Extended Groth Strip. We were able to directly measure emission line fluxes and equivalent widths from the analysis of OTELO pseudo-spectra. Aims. This study aims to explore the MZR in the very low-mass regime. Our sample reaches stellar masses (M*) as low as 106.8 M⊙, where 63% of the sample have M* < 109 M⊙. We also explore the relation of the star formation rate (SFR) and specific SFR with M* and gas-phase oxygen abundances, as well as the M*-size relation and the morphological classification. Methods. The M* were estimated using synthetic rest-frame colours. Using an χ2 minimization method, we separated the contribution of [N II]λ6583 to the Hα emission lines. Using the N2 index, we separated active galactic nuclei from star-forming galaxies (SFGs) and estimated the gas metallicity. We studied the morphology of the sampled galaxies qualitatively (visually) and quantitatively (automatically) using high-resolution data from the Hubble Space Telescope-ACS. The physical size of the galaxies was derived from the morphological analysis using GALAPAGOS2/GALFIT, where we fit a single-Sérsic 2D model to each source. Results. We find no evidence for an MZR evolution from comparing our very low-mass sample with local SFGs from the Sloan Digital Sky Survey. Furthermore, the same is true for M*-size and M*-SFR relations, as we deduce from comparison with recent literature. Morphologically, our sample is mostly (63%) populated by late-type galaxies, with 13% of early-type sources. For the first time, we identify one possible candidate outlier in the MZR at z = 0.4. The stellar-mass, metallicity, colour, morphology, and SFR of this source suggest that it is compatible with a transitional dwarf galaxy.

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Esteban-Jiménez, Ó., C. Navarro-Pemán, and F. González-Rubio. "Síndrome de Otelo." SEMERGEN - Medicina de Familia 42, no. 1 (January 2016): 63–65. http://dx.doi.org/10.1016/j.semerg.2014.10.016.

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Costa, Luciana Fidelis de Souza da, and Marta Helena Caetano. "A VISITA DE "OTELO" A "DOM CASMURRO" DEIXA MARCAS DE DESDÊMONA EM CAPITU." Linguagens - Revista de Letras, Artes e Comunicação 11, no. 1 (June 17, 2017): 109. http://dx.doi.org/10.7867/1981-9943.2017v11n1p109-118.

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O ciúme é o tema fundamental na tragédia de William Shakespeare, na obra Otelo, através da personagem Otelo por Desdêmona, sua esposa. Desdêmona é estrangulada pelo marido, que acredita que ela tenha cometido o adultério com seu grande amigo, Cássio. Essa temática shakespeariana também é refletida na obra Dom Casmurra, de Machado de Assis, com a desconfiança do personagem Bentinho, que acredita que sua esposa Capitu cometeu o adultério com seu amigo, Escobar. Bentinho, após assistir a peça teatral Otelo, de Shakespeare, imagina-se no papel de Otelo e Capitu, o da personagem Desdêmona. Capitu é apresentada na obra machadiana através dos olhos de Bentinho, o narrador-personagem e é somente através do seu depoimento, que é possível conhecer as características de Capitu. Cada vez mais, autores e críticos trazem a personagem Capitu para a atualidade, discutindo-a, analisando-a ou comparando-a com Desdêmona. Essa análise contínua comprova a imortalidade do perfil feminino de Capitu.

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Hirano, Luis Felipe Kojima. "O imaginário da branquitude à luz da trajetória de Grande Otelo: raça, persona e estereótipo em sua perfomance artística." Afro-Ásia, no. 48 (December 2013): 77–125. http://dx.doi.org/10.1590/s0002-05912013000200003.

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Este artigo pretende esboçar a trajetória de mais de 70 anos de Sebastião Bernardes de Souza Prata, Grande Otelo, em diálogo com os diferentes períodos do cinema brasileiro e com os debates raciais no Brasil. Se no campo cinematográfico ele conseguiu, ainda que em meio a tensões, variar seus papéis conforme as novas tendências do debate racial, entre as décadas de 1940 e 1980 houve sempre um hiato entre suas opiniões e as reivindicações da militância negra. A partir de Grande Otelo, seus personagens e suas posições políticas, busca-se por um lado discutir os conceitos de estereótipo e persona em intersecção com raça, corpo e gênero para analisar os dilemas que distintas convenções do cinema brasileiro impõem à representação do negro; por outro, examinar certos debates raciais pelo contraste com as percepções de Grande Otelo.

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Santos, Octávio Henrique Chames dos. "Uma tentativa de comparação entre as personagens Luís Padilha, de S. Bernardo, de Graciliano Ramos, e Iago, de Otelo, de William Shakespeare." Palimpsesto - Revista do Programa de Pós-Graduação em Letras da UERJ 20, no. 35 (May 13, 2021): 623–41. http://dx.doi.org/10.12957/palimpsesto.2021.57311.

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Sobre S. Bernardo, de Graciliano Ramos (2018), Juarez Filho (2006) indaga: “quem teria sido o Iago em São Bernardo?”, referindo-se ao personagem shakespeariano da tragédia Otelo (2017). Em nosso artigo, propomos uma resposta a essa provocação. Baseando-nos nas características atribuídas a Iago por críticos como Bloom (1998) e no exame de excertos de Otelo e, em especial, de S. Bernardo, buscamos sustentar que o ex-proprietário da fazenda S. Bernardo, Luís Padilha, assume esse papel.

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KEENER, CRAIG S. "Otho: A Targeted Comparison of Suetonius's Biography and Tacitus's History, with Implications for the Gospels' Historical Reliability." Bulletin for Biblical Research 21, no. 3 (January 1, 2011): 331–55. http://dx.doi.org/10.2307/26424373.

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Abstract A majority of scholars today recognize that the Gospels are ancient biographies. This recognition has implications for our valuation of the information content in the Gospels. Biographies written as soon after the subject's life as the Gospels normally include substantial historical information. The biographies of the later emperors in Suetonius offer a reasonable test case. Comparing Suetonius's biography of Otho with information about Otho in Tacitus's Histories, as well as Plutarch's biographies of Galba and Otho, confirms that Suetonius, whatever his other agendas, did not invent material freely but depended heavily on preexisting historical information.

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Mattick, Paul. "Otho Rühle e o movimento operário alemão – Parte I." Revista Novos Rumos 53, no. 1 (June 30, 2016): 3–22. http://dx.doi.org/10.36311/0102-5864.2016.v53n1.02.p3.

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Nesta edição da Seção Clássicos/Documentos da Revista Novos Rumos, apresentamos o texto de Paul Mattick "Otho Rühle e omovimento operário alemão" (parte II). Extraído de: Comunismo Anti-Bolchevique. Londres: Merlin Press, 1978. Tradução de Angélica Lovatto. O alemão Otho Rühle (1874-1943) foi fundador (junto com Karl Liebknecht, Rosa Luxemburgo, entre outros) da Liga Espartaquista (1916).

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Mattick, Paul. "Otho Rühle e o movimento operário alemão – Parte II." Revista Novos Rumos 53, no. 2 (December 20, 2016): 3–17. http://dx.doi.org/10.36311/0102-5864.2016.v53n2.02.p3.

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Nesta edição da Seção Clássicos/Documentos da Revista Novos Rumos, apresentamos o texto de Paul Mattick "Otho Rühle e omovimento operário alemão" (parte II). Extraído de: Comunismo Anti-Bolchevique. Londres: Merlin Press, 1978. Tradução de Angélica Lovatto. O alemão Otho Rühle (1874-1943) foi fundador (junto com Karl Liebknecht, Rosa Luxemburgo, entre outros) da Liga Espartaquista (1916).

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Alves, Murilo Cavalcante. "Otelo, a tragédia da alteridade." Revista Investigações 32, no. 1 (September 30, 2019): 343. http://dx.doi.org/10.51359/2175-294x.2019.240708.

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O artigo aborda a tragédia shakespeariana Otelo sob o ponto de vista da alteridade, e não do ciúme, como está sendo tradicionalmente analisada pela fortuna crítica do dramaturgo inglês. Nessa perspectiva, problematiza o papel relevante, mas usualmente ignorado, do epíteto "o mouro de Veneza", adicionado ao título da tragédia.

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Thompson, Glen. "Otelo Burningand Zulu surfing histories." Journal of African Cultural Studies 26, no. 3 (August 11, 2014): 324–40. http://dx.doi.org/10.1080/13696815.2014.940037.

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Mellen, Gregory R. "WHEN GOOD MEN DO NOTHING: AN EMENDATION IN TACITUS, HISTORIAE 1.38.3." Classical Quarterly 68, no. 1 (May 2018): 343–46. http://dx.doi.org/10.1017/s0009838818000198.

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In January of the year a.d. 69, Marcus Salvius Otho, disappointed in his attempt to be named Galba's heir and successor, fomented revolt among the praetorian guard. Trading on the praetorians’ own discontent at not receiving the donative, he began to win over the soldiers’ favour. Tacitus relates that, when the attitude of the soldiers seemed ripe (haud dubiae iam in castris omnium mentes, Hist. 1.36.1), Otho himself came forth and began to implore them directly (nec deerat Otho protendens manus adorare uolgum, iacere oscula, et omnia seruiliter pro dominatione, Hist. 1.36.3); and after he accepted the oath of loyalty from the entire classicorum legio (Hist. 1.36.3), he felt ready to hold a speech encouraging the men to complete the deed by ousting Galba.

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Rosa, Janaina Mirian, and Ketlyn Mara Rosa. "The temptation scene in Orson Welles' and Folias d'Arte's adaptations of "Othello"." Em Tese 21, no. 2 (January 29, 2016): 124. http://dx.doi.org/10.17851/1982-0739.21.2.124-135.

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O objetivo deste artigo é oferecer uma analogia quanto à representação da chamada cena da tentação no filme de Orson Welles intitulado Othello (1952) e na produção teatral de Otelo pelo grupo Folias d'Arte, que estreou em São Paulo no ano de 2003, ambas adaptações da peça de William Shakespeare. A cena da tentação é considerada pelos críticos como um momento crucial da peça, já que refere-se ao momento em que Iago astutamente reuni todas as suas forças como estrategista para influenciar os pensamentos de Otelo com a idéia de que Desdemona está traindo o Mouro com Cássio−e Iago atinge seu objetivo com sucesso.

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de Diego, José A., Jakub Nadolny, Ángel Bongiovanni, Jordi Cepa, Mirjana Pović, Ana María Pérez García, Carmen P. Padilla Torres, et al. "Galaxy classification: deep learning on the OTELO and COSMOS databases." Astronomy & Astrophysics 638 (June 2020): A134. http://dx.doi.org/10.1051/0004-6361/202037697.

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Context. The accurate classification of hundreds of thousands of galaxies observed in modern deep surveys is imperative if we want to understand the universe and its evolution. Aims. Here, we report the use of machine learning techniques to classify early- and late-type galaxies in the OTELO and COSMOS databases using optical and infrared photometry and available shape parameters: either the Sérsic index or the concentration index. Methods. We used three classification methods for the OTELO database: (1) u − r color separation, (2) linear discriminant analysis using u − r and a shape parameter classification, and (3) a deep neural network using the r magnitude, several colors, and a shape parameter. We analyzed the performance of each method by sample bootstrapping and tested the performance of our neural network architecture using COSMOS data. Results. The accuracy achieved by the deep neural network is greater than that of the other classification methods, and it can also operate with missing data. Our neural network architecture is able to classify both OTELO and COSMOS datasets regardless of small differences in the photometric bands used in each catalog. Conclusions. In this study we show that the use of deep neural networks is a robust method to mine the cataloged data.

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Peterson, Bhekizizwe. "Otelo Burning(dir. Sara Blecher, 2011)." Journal of African Cultural Studies 26, no. 3 (August 11, 2014): 341–44. http://dx.doi.org/10.1080/13696815.2014.896189.

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Rubio-Nazabal, Eduardo, Purificación Álvarez-Pérez, Teresa Lema-Facal, and Soledad López-Facal. "Síndrome de Otelo secundario a zonisamida." Medicina Clínica 142, no. 3 (February 2014): 133–34. http://dx.doi.org/10.1016/j.medcli.2013.03.006.

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Zabalza Estévez, Ramón J. "Síndrome de Otelo inducido por pramipexol." Revista de Neurología 54, no. 08 (2012): 509. http://dx.doi.org/10.33588/rn.5408.2012036.

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De Freitas Moraes, Camila, and Roseane Torres de Madeiro. "VIOLÊNCIA CONJUGAL E CIÚME NUMA PERSPECTIVA PSICANALÍTICA A PARTIR DE ‘OTELO – O MOURO DE VENEZA’." Psicanálise & Barroco em Revista 16, no. 1 (December 4, 2018): 79–95. http://dx.doi.org/10.9789/1679-9887.2018.v16i1.79-95.

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Pretende-se, no presente estudo, analisar as questões que permeiam a violência conjugal, a partir da obra shakespeariana, em especial, no que tange à temática dos ciúmes de Otelo por sua esposa Desdêmona, e sua interface com a obra freudiana. E é a partir desse prisma que se busca conceituar a violência conjugal em articulação com os conceitos psicanalíticos, para que, então, se possa investigar os aspectos subjetivos que se entrelaçam na relação amorosa em que a mulher é agredida por seu companheiro em função de um afeto como o ciúme. Ao fim, nota-se que Otelo passa a crer na suposta infidelidade de sua esposa. Seu ciúme consome-lhe a sanidade, fazendo-o construir um processo delirante que o leva a matar seu objeto de amor.PALAVRAS-CHAVE: Psicanálise. Literatura. Ciúme. Violência Conjugal. Mulher.

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Schrankel, Kenneth. "Otho D. Easterday (1924–1997)." Regulatory Toxicology and Pharmacology 27, no. 3 (June 1998): 199. http://dx.doi.org/10.1006/rtph.1998.1214.

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Diego, Marcelo. "O Hamlet brasileiro de Machado de Assis." Remate de Males 39, no. 2 (September 12, 2019): 741–67. http://dx.doi.org/10.20396/remate.v39i2.8655531.

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Este ensaio parte de uma provocação em relação à contribuição crítica seminal de Helen Caldwell (com o seu O Otelo brasileiro de Machado de Assis, de 1960), para discutir o diálogo intertextual de Dom Casmurro com o Hamlet de Shakespeare. Para tanto, dá particular atenção à centralidade, no interior do romance e da peça, da figuração do teatro, ou melhor, de processos de encenação; figuração que se dá por meio do desnudamento de uma consciência cênica, de uma forma teatral e de uma visão do mundo como representação. Por fim, sugere que, assim como o resgate da presença de Otelo em Dom Casmurro, então, abriu caminho para que a crítica literária debatesse questões candentes do seu tempo, a recuperação da presença de Hamlet em Dom Casmurro possibilita que a crítica cultural discuta algumas das questões mais prementes dos dias atuais.

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28

Modisane, Litheko. "Otelo Burning: On the turbulence of freedom." Journal of African Cultural Studies 26, no. 3 (August 11, 2014): 345–47. http://dx.doi.org/10.1080/13696815.2014.935709.

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29

Miranda, Célia Maria Arns de. "Otelo do Folias D’arte: canções como enquadramento épico." Letras, no. 51 (December 18, 2015): 135. http://dx.doi.org/10.5902/2176148523550.

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No espetáculo Otelo, realizado pelo Grupo Folias D’Arte (2003-2004), a reflexão sobre o fazer teatral torna-se um procedimento imperativo. Marco Antonio Rodrigues (encenador), através da inserção das músicas “New York, New York ”(Frank Sinatra) e “The End” (The Doors), que desempenham uma função de enquadramento épico e de comentário crítico da ação, identifica o referente contemporâneo ao estabelecer o diálogo entre a cultura-fonte e a cultura-alvo.

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30

Ick, Judy Celine. "Otelo, Intercultural Spectatorship, and Ocular Proof." Asian Theatre Journal 28, no. 1 (2011): 129–48. http://dx.doi.org/10.1353/atj.2011.0018.

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31

Roelen, J. C. P. F., H. van den Elst, C. E. Dreef, G. A. van der Marel, and J. H. van Boom. "Synthesis of alkylphosphon(othio)ate analogues of DNA." Tetrahedron Letters 33, no. 17 (April 1992): 2357–60. http://dx.doi.org/10.1016/s0040-4039(00)74210-9.

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32

Roche, Paul. "The Public Imagery of the Emperor Otho." Historia 57, no. 1 (2008): 108–23. http://dx.doi.org/10.25162/historia-2008-0007.

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33

Roche, P. A. "The Execution of L. Salvius Otho Cocceianus." Classical Quarterly 53, no. 1 (May 2003): 319–22. http://dx.doi.org/10.1093/cq/53.1.319.

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34

Guskov, Evgenii A. "The Praetorian Metilius Pudens and the Civil War in Rome." Vestnik of Saint Petersburg University. History 67, no. 1 (2022): 113–27. http://dx.doi.org/10.21638/11701/spbu02.2022.108.

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This paper is concerned with a dedicatory stele of some Metilius Pudens, named a warrior of the XIX praetorian cohort in its text. According to paleographic features, it is dated to the second half of the first century A. D. The inscription was published only in 1995, but has not attracted wide attention of researchers yet. The role of Pudens in the events of 69 is unknown due to the scanty content of the stele. The article proves that Pudens could only serve in the guard of Julii-Claudii and during the civil war fought first on the side of Otho. Then, like many former Othonians, he supported the party of Vespasian and was eventually enrolled in his praetorium, which could comprise 20 000 people. The article presents information about the conditions of service and resignation of Metilius Pudens, and describes the organization of the new guard, consisting of soldiers of the Flavian legions, former praetorians of Otho and legionaries of Vitellius. The long duration of Metilius Pudent’s service was due to the need to maintain a group balance in the Flavian guard. Taking into account the large proportion of former Vitellian soldiers in the new corps, the new administration pursued a cautious demobilization policy in order to break mutual responsibility and prevent a repeat of the situation with the Praetorians of Otho, who, having been dismissed by Vitellius, came out in support of Vespasian. Since the Othonians were absolutely loyal to the new authorities in gratitude for the possibility of rehabilitation after the humiliation by Vitellius in April 69, they were seen as a counterweight to the Vitellians.

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35

Miranda, C. A., and C. F. P. Carneiro. "A Universalidade da Tragédia Otelo, o Mouro de Veneza." Revista Scripta Alumni, no. 14 (December 30, 2015): 194–210. http://dx.doi.org/10.18304/1984-6614/scripta.alumni.n14p194-210.

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36

Miranda, C. A. "Otelo e o Engajamento Político-Cultural do Folias D'arte." Revista Scripta Uniandrade, no. 6 (December 30, 2008): 285–300. http://dx.doi.org/10.18305/1679-5520/scripta.uniandrade.n6p285-300.

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37

Cepa, J., A. M. Pérez-García, A. Bongiovanni, E. J. Alfaro, H. Castañeda, J. Gallego, J. I. González-Serrano, M. Sánchez-Portal, and J. J. González. "OTELO survey: deepBVRIbroad-band photometry of the Groth strip." Astronomy & Astrophysics 490, no. 1 (August 1, 2008): 1–14. http://dx.doi.org/10.1051/0004-6361:200810092.

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38

Keynes, Simon. "A lost cartulary of St Albans Abbey." Anglo-Saxon England 22 (December 1993): 253–79. http://dx.doi.org/10.1017/s0263675100004403.

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It would be a truism among Anglo-Saxonists to say that we depend for our knowledge of a fair proportion of pre-Conquest literary and historical texts on the labours of scholars active in the sixteenth, seventeenth and early eighteenth centuries. Among the many important texts which were casualties, for example, of the Cotton fire on 23 October 1731, and for which we now depend on early modern transcripts and printed editions, one thinks immediately of Asser's Life of King Alfred and of the poem on the battle of Maldon (in Cotton Otho A. xii), of manuscript G of the Anglo-Saxon Chronicle (in Cotton Otho B. xi), and of Ealdorman Æthelweard's Chronicle (in Cotton Otho A. x). Should one choose to venture into the realm of Anglo-Saxon charters, the importance of antiquarian transcripts of manuscripts now lost becomes ever more apparent. The most spectacular addition to the corpus of charters made since the publication of Professor Sawyer's catalogue in 1968 arose from the examination of a sixteenth-century cartulary of Ilford Hospital preserved at Hatfield House, which proved to contain the texts of eleven pre-Conquest charters derived ultimately from the archives of Barking abbey in Essex; of course this manuscript is an ‘original’ cartulary, as opposed to an antiquarian transcript, but it serves here as a salutary reminder of the treasures which may lurk as yet unidentified in libraries and archives throughout the country. Other ‘discoveries’ include a seventeenth-century copy of a charter by which King Edgar granted an estate at Ballidon, in Derbyshire, to his thegn Æthelferth, Sir Henry Spelman's extracts from a lost cartulary of Abbotsbury abbey, and notes made by the jurist John Selden from a charter-roll formerly preserved in the archives of St Paul's Cathedral in London.

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39

MICHAEL B. CHARLES and EVA ANAGNOSTOU-LAOUTIDES. "UNMANNING AN EMPEROR: OTHO IN THE LITERARY TRADITION." Classical Journal 109, no. 2 (2014): 199. http://dx.doi.org/10.5184/classicalj.109.2.0199.

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CHARLES, MICHAEL B., and EVA ANAGNOSTOU-LAOUTIDES. "UNMANNING AN EMPEROR: OTHO IN THE LITERARY TRADITION." Classical Journal 109, no. 2 (2013): 199–222. http://dx.doi.org/10.1353/tcj.2013.0000.

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41

Martin, Thomas R., Plutarch, Christopher Ehrhardt, Douglas Little, and C. F. Konrad. "Plutarch's "Lives of Galba and Otho": A Companion." Classical World 90, no. 1 (1996): 69. http://dx.doi.org/10.2307/4351914.

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42

Lara-López, M. A., J. Cepa, H. Castañeda, A. M. Pérez García, A. Bongiovanni, A. Ederoclite, M. Fernández Lorenzo, M. Pović, and M. Sánchez-Portal. "OTELO Survey: Optimal Emission-Line Flux Determination with OSIRIS/GTC." Publications of the Astronomical Society of the Pacific 122, no. 898 (December 2010): 1495–509. http://dx.doi.org/10.1086/657509.

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43

Lara-López, M. A., J. Cepa, H. Castañeda, A. M. Pérez García, A. Bongiovanni, A. Ederoclite, M. Fernández Lorenzo, et al. "OTELO Survey: Optimal Emission-Line Flux Determination with OSIRIS/GTC." Publications of the Astronomical Society of the Pacific 123, no. 900 (February 2011): 252. http://dx.doi.org/10.1086/658901.

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44

Espárrago-Llorca, Guadalupe, Laura Carrión-Expósito, Antonio Baena-Baldomero, Sergio Ruiz-Doblado, and Eloisa López-Garzón. "Síndrome de Otelo (delirio celotípico monosintomático) inducido por agonistas dopaminérgicos." Psiquiatría Biológica 18, no. 2 (April 2011): 68–71. http://dx.doi.org/10.1016/j.psiq.2011.08.002.

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45

ROELEN, H. C. P. F., H. VAN DEN ELST, C. E. DREEF, G. A. VAN DER MAREL, and J. H. VAN BOOM. "ChemInform Abstract: Synthesis of Alkylphosphon(othio)ate Analogues of DNA." ChemInform 23, no. 43 (August 21, 2010): no. http://dx.doi.org/10.1002/chin.199243255.

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46

Pimenta, Daniele. "Grande Otelo: Sobre ser um artista popular no Brasil do século XX." Urdimento - Revista de Estudos em Artes Cênicas 2, no. 41 (September 15, 2021): 1–25. http://dx.doi.org/10.5965/1414573102412021e0301.

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Este texto foi escrito com o intuito de estimular reflexões sobre a trajetória de Grande Otelo, considerando o contexto social e artístico do período em que ele viveu e refletindo sobre questões que determinaram o modo como desenvolveu sua carreira. Para essa contextualização, foram abordados aspectos de sua trajetória que coincidem com características das carreiras de outros artistas da cena popular no período, no teatro e no circo, como o trabalho desde a infância, a especialização da atuação e escolhas estéticas guiadas pelo constante cuidado em agradar ao público.

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47

Edwards, A. S. G., and Elizabeth J. Bryan. "Collaborative Meaning in Medieval Scribal Culture: The Otho Lazamon." Modern Language Review 98, no. 2 (April 2003): 422. http://dx.doi.org/10.2307/3737825.

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48

Pelle, S. "Newly Recovered English Homilies from Cotton Otho A. xiii." Review of English Studies 65, no. 269 (September 16, 2013): 193–218. http://dx.doi.org/10.1093/res/hgt056.

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49

Mag, Matthias, Jochen Muth, Kerstin Jahn, Anusch Peyman, Gerhard Kretzschmar, Joachim W. Engels, and Eugen Uhlmann. "Synthesis and binding properties of oligodeoxynucleotides containing phenylphosphon(othio)ate linkages." Bioorganic & Medicinal Chemistry 5, no. 12 (December 1997): 2213–20. http://dx.doi.org/10.1016/s0968-0896(97)00164-8.

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50

Bianconcini Anjos, Ana Paula. "A adaptação cinematográfica de Uma Tragédia Americana e Otelo em Match Point." Ilha do Desterro A Journal of English Language, Literatures in English and Cultural Studies 70, no. 1 (January 27, 2017): 161. http://dx.doi.org/10.5007/2175-8026.2017v70n1p161.

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http://dx.doi.org/10.5007/2175-8026.2017v70n1p161O artigo retoma o histórico das adaptações cinematográficas do romance Uma Tragédia Americana (1925), de Theodore Dreiser, recuperando as discussões sobre a cena do afogamento. Os estudos de Sergei Eisenstein sobre o uso do monólogo interior no cinema e o comentário de Bertolt Brecht a respeito da trilha sonora na adaptação do romance de Dreiser oferecem importante ponto de entrada para a análise do filme Match Point (2005), de Woody Allen. Em Match Point, o uso da trilha sonora, notadamente a colagem com a ópera Otelo (1887), de Giuseppe Verdi, permite que o espectador reflita sobre as possibilidades narrativas da adaptação para o cinema.

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Journal articles on the topic 'Othlo'

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