671 research outputs found
Dans l'ombre chaude de l'Islam.
No full text"Notes sur la vie et les œuvres d'Isabelle Eberhardt," signed V. B. : p. [315]-363.At head of title: Isabelle Eberhardt and Victor Barrucand.Mode of access: Internet
Educational Narrative: Grace Eberhardt
No full textAs a part of the University of Puget Sound\u27s African American Studies Public Scholarship course, students were required to review their educational experiences from pre-k to the present. The goal of this assignment was for them to assess the ways in which they were treated based on their marginalizations or their privileges. Students provided three terms for what their narrative would share — the terms were not to be included in their narrative. After reading their narratives aloud, a class discussion connected their terms to the associated experiences. There are a total of four narratives in this issue, three are also accompanied with a voice recording by the author. The following is one such narrative
Imperial Performativity: the Life, Transgressions, and Writings of Isabelle Eberhardt under the Lens of Queer Theory
No full textAn examination of Isabelle Eberhardt\u27s life and writings with regard to gender norms and imperialist expectations in French-controlled Algeria. The PDF includes the author\u27s entry submission essay for the 2011 Undergraduate Research Awards
Ida von Hahn-Hahn und Isabelle Eberhardt. Ausbruch aus Restriktionen – Auf der Suche nach sich selbst
No full textThe following thesis compares the travelogue Orientalische Briefe by the German author Ida von Hahn-Hahn with the travel journals Mes Journaliers by the French author Isabelle Eberhardt, in the context of how each woman represents herself as a female traveler and author. The comparative study analyzes whether both authors in these texts deal with the issue of breaking out of social and cultural restrictions while traveling to the ‘Orient’. The overall question of my thesis concerns what kind of filters did they use to speak about the ‘cultural other’.
The personal backgrounds of Ida von Hahn-Hahn and Isabelle Eberhardt differ in several aspects. The German author Ida von Hahn-Hahn visited the ‘Orient’ in 1843 temporarily and each place on only one occasion whereas the French author Isabelle Eberhardt constantly traveled at the end of the 19th century and at the same time she turned North Africa into her new home. These texts were analyzed in the context of gender discourse analysis, focusing on the discourse of feminity in the 19th century and the discourse of the Western world about the ‘Orient’. The comparison showed similarities and differences in the way both authors present themselves and the ‘Arab woman’ by (de-)constructing pre-existing ‘images’.
In my analysis I was able to demonstrate that both authors consciously deal with the western femininity discourse of the 19th century and the Western discourse about the ‘Orient’ by selecting similar motives. Even though their results are quite different, both authors clearly use the ‘Orient’ to express their search of one’s self
Mulher, islã e literatura: os avatares de Isabelle Eberhardt
No full textThis work was developed though reading three books of Isabelle Eberhardt: Pages d'lslam, Notes de Route and Amours Nômades, as well as reading of criticai works of this author and studying in depth aspects of the Islamic religion and situation of woman in the Islamism, as well as her achieve on the society that the author lived, include striking and predominant influence the French occupation in the countries that are part of Maghreb (North African countries), especially Tunisia, Algeria and Morocco.Desenvolvido através da leitura de três obras a escritora argelina de origem suíça Isabelle Eberhardt: Pages d’Islam, Notes de Route e Amours Nomades, assim como a leitura da fortuna crítica dessa autora e as obras que estudam em profundidade os aspectos da religião islâmica e a situação da mulher no seio do islamismo, bem como seu alcance sobre a sociedade em que a autora viveu, incluindo a influência marcante e preponderante da ocupação francesa nos países que compõem o Magrebe (países do norte da África), mais especificamente a Tunísia, a Argélia e o Marrocos
TOI-6695: A Pair of Near-resonant Massive Planets Observed with TESS from the WINE Survey
No full textEberhardt, Jan et al.-- Full list of authors: Eberhardt, Jan; Trifonov, Trifon; Henning, Thomas; Tala Pinto, Marcelo; Brahm, Rafael; Jordán, Andrés; Espinoza, Nestor; Jones, Matías I.; Hobson, Melissa J.; Rojas, Felipe I.; Schlecker, Martin; Acuña, Lorena; Burn, Remo; Boyle, Gavin; Leiva, Rodrigo; McCormac, James; Dunckel, Nicholas; Dragomir, Diana; Crane, Jeffrey D.; Shectman, Stephen; Teske, Johanna K.; Osip, David; Gupta, Arvind F.; Ulmer-Moll, Solène; Bouchy, François; Lendl, Monika; Gandolfi, Davide; Ricker, George R.; Jenkins, Jon M.; Seager, Sara; Winn, Joshua N.We present the discovery and characterization of a pair of warm Jovian-mass exoplanets orbiting the Sun-like star TOI-6695, based on Transiting Exoplanet Survey Satellite (TESS) transits and precise radial velocity (RV) measurements obtained with FEROS, HARPS, CHIRON, CORALIE, and PFS. The transiting exoplanet TOI-6695b has an orbital period of ∼80.4 days, a radius of 0.85Rjup, and a mass of 0.21Mjup. The outer planet has a minimum mass of 1.45Mjup and an orbital period of about 242.4 days, confidently constrained by the Doppler time-series data. The TOI-6695 exoplanet system exhibits transit-timing variations due to the dynamical interaction of the planets, which reside near a 3:1 mean-motion resonance. We modeled the TOI-6695 system's orbital and dynamical configuration by performing self-consistent N-body fits of TESS photometry, ground-based photometry from Observatoire Moana, and precise RV data, all of which are consistent with the presence of a warm Jovian-mass duo of exoplanets. *Based on observations collected at the European Organization for Astronomical Research in the Southern Hemisphere under MPG programmes 0100.A-9007(A), 0104.A-9007(A), 0108.A-9003(A), 0109.A-9003(A), 105.20GX.001 (PI Brahm), 105.20L0.001 (PI Bouchy), 106.21ER.001 (PI Brahm),106.21TJ.001 (PI Gandolfi), 108.22A8.001 (PI Brahm), 109.239V.001 (PI Brahm), 110.23YQ.001 (PI Brahm), and 112.25W1.001 (PI Brahm). This paper includes data gathered with the 6.5 m Magellan Telescopes located at Las Campanas Observatory, Chile. © 2025 The Author(s).This research has made use of the Exoplanet Follow-up Observation Program website, which is operated by the California Institute of Technology, under contract with the National Aeronautics and Space Administration under the Exoplanet Exploration Program. Resources supporting this work were provided by the NASA High-End Computing (HEC) Program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center for the production of the SPOC data products. We acknowledge the use of public TESS data from pipelines at the TESS Science Office and at the TESS Science Processing Operations Center. This paper includes data collected by the TESS mission, which are publicly available from the Mikulski Archive for Space Telescopes (MAST) operated by the Space Telescope Science Institute (STScI). Funding for the TESS mission is provided by NASA's Science Mission Directorate. T.T. acknowledges support by the BNSF program "VIHREN-2021" project No. KP-06-DV/5. R.B. acknowledges support from FONDECYT Project 1241963 and from ANID—Millennium Science Initiative—ICN12_009. R.Bu. acknowledges the financial support from DFG under Germany's Excellence Strategy EXC 2181/1-390900948, Exploratory project EP 8.4 (the Heidelberg STRUCTURES Excellence Cluster). The results reported herein benefitted from collaborations and/or information exchange within NASA's Nexus for Exoplanet System Science (NExSS) research coordination network sponsored by NASA's Science Mission Directorate under Agreement No. 80NSSC21K0593 for the program "Alien Earths." D.D. acknowledges support from the TESS Guest Investigator Program grant 80NSSC23K0769, and from the NASA Exoplanet Research Program grant 18-2XRP18_2-0136. M.T.P. acknowledges the support of Fondecyt-ANID fellowship no. 3210253 and ASTRON-0037. A.J. acknowledges support from ANID Millennium Science Initiative IM23-0001 and Fondecyt project 1251439.
Some of the observations in this paper made use of the NN-EXPLORE Exoplanet and Stellar Speckle Imager (NESSI). NESSI was funded by the NASA Exoplanet Exploration Program and the NASA Ames Research Center. NESSI was built at the Ames Research Center by Steve B. Howell, Nic Scott, Elliott P. Horch, and Emmett Quigley. This work made use of tpfplotter by J. Lillo-Box (publicly available at www.github.com/jlillo/tpfplotter), which also made use of the python packages astropy, lightkurve, matplotlib and numpy. This research has made use of tglc, which is available at https://github.com/TeHanHunter/TESS_Gaia_Light_Curve and is listed with doi:10.17909/610m-9474. The TESS data used for this analysis can be accessed via doi:10.17909/vwtg-p336. This work has been carried out within the framework of the NCCR PlanetS supported by the Swiss National Science Foundation under grants 51NF40_182901 and 51NF40_205606.
J.E. acknowledges the use of ChatGPT, which has been used on rare occasions for the purpose of rephrasing repetitive sentences. The outputs have been checked for their correctness and no original content has been created.Peer reviewe
Dekonstrukcja orientalistycznych stereotypów w dziennikach z podróży Isabelle Eberhardt
No full textThe article examines the role of Orientalist stereotypes in Isabelle Eberhardt’s travel short stories. It questions the oversimplified view which considers stereotyping as an individual cognitive process that helps individuals simplify their understanding of people from different cultures. It also shows that this is an ideological construct overloaded with racial attitudes, sexist, and gender issues. The author emphasizes that stereotypes reveal a cognitive bias due to generalizations, out-group homogeneity, and categorizations, and cannot be isolated from their ideological motivations, especially in the context of colonialism. Selected travel short stories by Eberhardt are analyzed: Le Magicien, Le Meddah, Criminel, Fiancée, Le portrait de l’Ouled-Naïl, and La Derouïcha, in accordance with the theory of Palestinian-American philosopher Edward Said, expressed in his book Orientalism, so as to demonstrate the major tropes of Orientalist stereotypes and their functioning in the aforementioned texts. Said asserts that the European prejudiced perspective on the East is the result of stereotypical images, which were built in a context of domination of the Orient. Other theorists are also relied upon, such as Frantz Fanon and Achille Mbembe, Gayatri C. Spivak, Ania Loomba, and Meyda Yeğenoğlu, in order to consider the link between Orientalist discourse and issues of ethnicity and gender. The intersectional approach allows us to examine the Orientalist stereotypes and to deconstruct the racist and sexist constructions underlying Eberhardt’s texts. It also provides a broader conception of stereotyping, which considers the nexus between Orientalist discourse, race, gender, and sexuality. The research shows that the author adopts the scrutinizing gaze of the colonizer and creates binary oppositions between Western, civilized personas and their uncivilized, Oriental counterparts. Moreover, it uses degrading and dehumanizing stereotypes which implicitly justify the “civilizing mission” undertaken by the Occident.W artykule zbadano rolę stereotypów orientalistycznych w opowiadaniach podróżniczych Isabelle Eberhardt. Podważono uproszczony pogląd, który traktuje stereotypy jako indywidualny proces poznawczy, pomagający jednostkom uprościć ich rozumienie ludzi z różnych kultur. Jednocześnie wykazano, że jest to ideologiczna konstrukcja przeciążona postawami rasowymi, seksizmem i kwestiami płci. Autorka podkreśla, że stereotypy ujawniają uprzedzenia poznawcze z powodu uogólnień, jednorodności i kategoryzacji grup zewnętrznych i nie można ich odizolować od ich ideologicznych motywacji, zwłaszcza w kontekście kolonializmu. Analizie poddano wybrane opowiadania Eberhardt: Le Magicien, Le Meddah, Criminel, Fiancée, Le portrait de l’Ouled-Naïl oraz La Derouïcha, zgodnie z teorią palestyńsko-amerykańskiego filozofa Edwarda Saida wyrażoną w książce Orientalizm, aby zademonstrować główne tropy stereotypów orientalistycznych i ich funkcjonowanie w tych tekstach. Said twierdzi, że europejska uprzedzona perspektywa na Wschód jest wynikiem stereotypowych obrazów, które zostały zbudowane w kontekście dominacji Orientu. Powołuje się również na innych teoretyków, takich jak Frantz Fanon i Achille Mbembe, Gayatri C. Spivak, Ania Loomba i Meyda Yeğenoğlu, aby rozważyć związek między dyskursem orientalistycznym oraz kwestiami etnicznymi i płciowymi. Podejście interseksjonalne pozwala badać stereotypy orientalistyczne oraz dekonstruować rasistowskie i seksistowskie konstrukcje leżące u podstaw tekstów Eberhardt, a także zapewnia szerszą koncepcję stereotypizacji, w której uwzględniany jest związek między dyskursem orientalistycznym, rasą, płcią i seksualnością. Autorka ta przyjmuje badawcze spojrzenie kolonizatora oraz tworzy binarne opozycje między zachodnimi cywilizowanymi personami a ich nieokrzesanymi orientalnymi odpowiednikami. Ponadto posługuje się poniżającymi i nieludzkimi stereotypami, które implicite usprawiedliwiają „misję cywilizacyjną” podjętą przez Okcydent
supplemental_table_1 - Processing Escape Mechanisms Through Altered Proteasomal Cleavage of Epitopes Affect Immune Response in Pulmonary Neuroendocrine Tumors
No full textsupplemental_table_1 for Processing Escape Mechanisms Through Altered Proteasomal Cleavage of Epitopes Affect Immune Response in Pulmonary Neuroendocrine Tumors by Michael Wessolly, Robert F. H. Walter, Claudia Vollbrecht, Robert Werner, Sabrina Borchert, Jan Schmeller, Elena Mairinger, Thomas Herold, Anna Streubel, Daniel C. Christoph, Wilfried E. E. Eberhardt, Jens Kollmeier, Thomas Mairinger, Kurt W. Schmid, Jeremias Wohlschlaeger, Thomas Hager, and Fabian D. Mairinger in Technology in Cancer Research & Treatment</p
supplemental_table_2 - Processing Escape Mechanisms Through Altered Proteasomal Cleavage of Epitopes Affect Immune Response in Pulmonary Neuroendocrine Tumors
No full textsupplemental_table_2 for Processing Escape Mechanisms Through Altered Proteasomal Cleavage of Epitopes Affect Immune Response in Pulmonary Neuroendocrine Tumors by Michael Wessolly, Robert F. H. Walter, Claudia Vollbrecht, Robert Werner, Sabrina Borchert, Jan Schmeller, Elena Mairinger, Thomas Herold, Anna Streubel, Daniel C. Christoph, Wilfried E. E. Eberhardt, Jens Kollmeier, Thomas Mairinger, Kurt W. Schmid, Jeremias Wohlschlaeger, Thomas Hager, and Fabian D. Mairinger in Technology in Cancer Research & Treatment</p
Three Warm Jupiters around Solar-analog Stars Detected with TESS
No full textFull list of the authors: Eberhardt, Jan; Hobson, Melissa J.; Henning, Thomas; Trifonov, Trifon; Brahm, Rafael; Espinoza, Nestor; Jordán, Andrés; Thorngren, Daniel; Burn, Remo; Rojas, Felipe I.; Sarkis, Paula; Schlecker, Martin; Tala Pinto, Marcelo; Barkaoui, Khalid; Schwarz, Richard P.; Suarez, Olga; Guillot, Tristan; Triaud, Amaury H. M. J.; Günther, Maximilian N.; Abe, Lyu; Boyle, Gavin; Leiva, Rodrigo; Suc, Vincent; Evans, Phil; Dunckel, Nick; Ziegler, Carl; Falk, Ben; Fong, William; Rudat, Alexander; Shporer, Avi; Striegel, Stephanie; Watanabe, David; Jenkins, Jon M.; Seager, Sara; Winn, Joshua N.We report the discovery and characterization of three giant exoplanets orbiting solar-analog stars, detected by the TESS space mission and confirmed through ground-based photometry and radial velocity measurements taken at La Silla observatory with FEROS. TOI-2373 b is a warm Jupiter orbiting its host star every ∼13.3 days, and is one of the most massive known exoplanet with a precisely determined mass and radius around a star similar to the Sun, with an estimated mass of m = 9.3 − 0.2 + 0.2 M jup and a radius of r = 0.93 − 0.2 + 0.2 R jup . With a mean density of ρ = 14.4 − 1.0 + 0.9 g cm − 3 , TOI-2373 b is among the densest planets discovered so far. TOI-2416 b orbits its host star on a moderately eccentric orbit with a period of ∼8.3 days and an eccentricity of e = 0.32 − 0.02 + 0.02 . TOI-2416 b is more massive than Jupiter with m = 3.0 − 0.09 + 0.10 M jup , however is significantly smaller with a radius of r = 0.88 − 0.02 + 0.02 , R jup , leading to a high mean density of ρ = 5.4 − 0.3 + 0.3 g cm − 3 . TOI-2524 b is a warm Jupiter near the hot Jupiter transition region, orbiting its star every ∼7.2 days on a circular orbit. It is less massive than Jupiter with a mass of m = 0.64 − 0.04 + 0.04 M jup , and is consistent with an inflated radius of r = 1.00 − 0.03 + 0.02 R jup , leading to a low mean density of ρ = 0.79 − 0.08 + 0.08 g cm − 3 . The newly discovered exoplanets TOI-2373 b, TOI-2416 b, and TOI-2524 b have estimated equilibrium temperatures of 860 − 10 + 10 K, 1080 − 10 + 10 K, and 1100 − 20 + 20 K, respectively, placing them in the sparsely populated transition zone between hot and warm Jupiters. © 2023. The Author(s). Published by the American Astronomical Society.This research has made use of the Exoplanet Follow-up Observation Program website, which is operated by the California Institute of Technology, under contract with the National Aeronautics and Space Administration under the Exoplanet Exploration Program. Resources supporting this work were provided by the NASA High-End Computing (HEC) Program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center for the production of the SPOC data products. We acknowledge the use of public TESS data from pipelines at the TESS Science Office and at the TESS Science Processing Operations Center. This paper includes data collected by the TESS mission, which are publicly available from the Mikulski Archive for Space Telescopes (MAST) operated by the Space Telescope Science Institute (STScI). Funding for the TESS mission is provided by NASA's Science Mission Directorate. This work makes use of observations from the ASTEP telescope. ASTEP benefited from the support of the French and Italian polar agencies IPEV and PNRA in the framework of the Concordia station program, from OCA, INSU, Idex UCAJEDI (ANR- 15-IDEX01), and ESA through the Science Faculty of the European Space Research and Technology Centre (ESTEC). This work made use of tpfplotter by J. Lillo-Box (publicly available in www.github.com/jlillo/tpfplotter), which also made use of the python packages astropy, lightkurve, matplotlib, and numpy. The data used for the analyses presented in this paper can be accessed via 10.17909/zsh5-wq95, 10.17909/edzq-va27, and 10.17909/phhz-qv30. Gaia DR2 data can be accessed via ESA (Gaia Collaboration 2018). The results reported herein benefited from collaborations and/or information exchange within NASA's Nexus for Exoplanet System Science (NExSS) research coordination network sponsored by NASA's Science Mission Directorate under Agreement No. 80NSSC21K0593 for the program "Alien Earths." R.Br. acknowledges support from FONDECYT Project 11200751. A.J., R.Br., F.R., and M.H. acknowledge support from ANID-Millennium Science Initiative-ICN12_009. A.J. acknowledges additional support from FONDECYT project 1210718. T.T. acknowledges support by the DFG Research Unit FOR 2544 "Blue Planets around Red Stars" project No. KU 3625/2-1. T.T. further acknowledges support by the BNSF program "VIHREN-2021" project No. & Kcy;& Pcy;-06-& Dcy;& Vcy;/5. R.Bu. acknowledges the support from DFG under Germany's Excellence Strategy EXC 2181/1-390900948, Exploratory project EP 8.4 (the Heidelberg STRUCTURES Excellence Cluster). T.H. acknowledges support from the European Research Council under the Horizon 2020 Framework Program via the ERC Advanced grant Origins 832428. The postdoctoral fellowship of K.B. is funded by F.R.S.-FNRS grant T.0109.20 and by the Francqui Foundation. This research received funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program (grant agreement No 803193/BEBOP), and from the Science and Technology Facilities Council (STFC; grant No ST/S00193X/1)
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