bluuebunny/crossref_metadata_2025_split huggingface dataset:
L'Église, les Capétiens et le Languedoc au temps d'Alphonse de Poitiers : autour des enquêtes pontificales sur les crimes imputés à Vézian (OFM), évêque de Rodez (1261-1276)
Authors: Théry Julien 
Published: January 2018

Tres papas sucesivos, Alejandro IV, Urbano IV y Clemente IV, mandaron que se hiciera durante seis años un «procesamiento inquisitorial » (inquisitionis negocium)
contra el obispo de Rodez Vezian. A éste se la acusaba ante la justicia, sin que se aclarara jamás quién le acusaba, de «enormes fechorías » (enormia sinistra) : profanación del oficio divino, simonía, sodomía y «otros numerosos crímenes que ofenden a Dios y escandalizan a los hombres » . Audiencias de testigos se hicieron en Rodez y el obispo tuvo que defenderse con ahinco ante la Curia romana antes de librarse de toda condena. En este artículo se propone una primera aproximación a ese procedamiento bastante bien documentado que hay que colocar en la larga serie, poco conocida, de los procedimientos inquisitoriales impulsados pos los papas en contra de los prelados acusados de abusos durante los siglos XIII y XIV. Teniendo en cuenta la historia agitada del episcopado (1247-1274) y las relaciones de conflicto entre Vezian y la nueva administración condal de Alfonso de Poitiers, en un contexto de gobierno conjunto de Languedoc por la Igleia y los Capetos después de la desposesión reciente de la casa de Saint-Gilles, se sugiere que las diligencias las impulsó el conde. El que se designara como perquisidor, al principio al arzobispo de Narbona, Gui Foucois, un personaje emblemático de la simbiosis entre Iglesia romana y realeza francesa en la región, constituye un elemento importante que apoya esa interpretación. El procesamiento inquisitorial ponía al obispo en situación dificultosa pero estaba destinada a ir para largo como casi todos los procedimientos de ese tipo sin que por otra parte tuvieran necesariamente un día una conclusión precisa. Al aceptar que se hicieran esas diligencias, los papas contenían la irritación de su poderoso aliado capeto satisfaciéndole en parte sin condenar claramente a un prelado fiel a los principios de la teocracia. La justicia inquisitorial sirve aquí de mediación sin que sea dicho explícitamente y sin desentenderse de las formas jurídicas, ni mucho menos. Parece ser un instrumento político muy sutil en su manejo al servicio del gobierno pontificio.
Un théâtre sans acteurs : l'enlèvement de Hanns Martin Schleyer par la Fraction Armée Rouge
Authors: Hamers Jeremy 
Published: January 2018

Le 5 septembre 1977 , un commando de la Fraction Armée Rouge enlève le patron des patrons allemands et ancien SS Hanns Martin Schleyer. Cette prise d'otage constitue le point de départ de l'Automne Allemand, qui se soldera par l'assassinat de l'otage et le suicide des têtes pensantes de la Bande à Baader.
Depuis 1977, l'Automne Allemand fait l'objet de nombreux traitements audiovisuels qui témoignent de la réduction progressive des événements à quelques images emblématiques. Cet article ambitionne d'analyser le rôle central joué par une de ces images, la photo du lieu de l'enlèvement de Hanns Martin Schleyer, un décor sans corps que les médias ne peuvent, nécessairement, filmer qu'après le déroulement de l'événement. Agissant comme un formidable producteur de vide et d'absence, cette photo puise son potentiel dramatique dans une dynamique de la frustration visuelle et de la (re-)charge fantasmatique qu'elle autorise. L'image déclenche ainsi une vaste entreprise de «remplissage» et de réinvestissement sémantique dans laquelle les journaux télévisés, le cinéma documentaire, l'art vidéo, et les représentations produites par les terroristes s'entremêlent inextricablement.
The Longevity of Musical Works for Instruments and Electronic Music in the Digital Era
Authors: Gerzso Andrew 
Published: January 2018

Until the mid-XXth century, classical music relied on a range of stable practices that guaranteed its survival : the written score ; the notion of interpretation ; lutherie instrument making ; oral (in particular) and written teaching traditions ; institutions (conservatories, ensembles, orchestras etc.).
The advent of digital technology in musical creation from the 1970s onwards perturbed this landscape, forcing us to rethink these practices, particularly all those concerning the endurance of the new kinds of works that have emerged over the past thirty years – especially works for traditional and electronic instruments. Furthermore, the digital arts - though scarcely established - were soon in danger through the proliferation and fragility of digital standards and formats (cf. the “ Digital Dark Age” phenomenon). If contemporary music has the ambition to prolong the classical music tradition, it must find the techniques, modalities and practices to ensure its survival despite the instability of digital technology.
“Walls Have Never Held Us Back”: 60 Years of Student Films at the University Babelsberg Konrad Wolf
Authors: Brombach Ilka , Ebbrecht Tobias , Wahl Chris 
Published: January 2018

Owing to its location, the Film University Babelsberg KONRAD WOLF is particularly well suited to reflect audiovisual cultural heritage. It is situated in close proximity to the Babelsberg film studios, which has a tradition of filmmaking that goes back more than a century, and the University, which is the oldest of its kind in Germany, has benefited from the studio’s mythos. With the creation of an endowed professorship for audiovisual heritage in June 2013, as well as the initiation of a new program of study devoted to film heritage (to Filmkulturerbe), the Film University is positioned to assert the importance of securing and maintaining audiovisual heritage. On this basis, a scholarly project (supported by the Deutsche Forschungsgemeinschaft
[DFG]) has been dedicated to studying the university’s filmic heritage. Student films from 60 years of the school’s history, with a particular focus on the films from the GDR era, are being analyzed in the context of film history and in terms of institutional history as well. The research takes stock of how the student films have been archived and transmitted, and it also examines the school’s own narratives about its history. Both film historical and aesthetic readings of selected films are conducted with reference to recent debates about DEFA cinema. In addition to the research project on student films, a number of other initiatives are underway, ones that pay particular attention to questions of preservation and digitization.
Sur la répétition de la préposition en vieux russe et les structures à préposition non initiale dans les langues indo-européennes anciennes
Authors: Le Feuvre Claire 
Published: January 2018

La répétition de la préposition devant les modifieurs du nom dans un SPrep., fréquente en vieux russe et attestée dans d’autres langues slaves, est liée à un ordre des mots marqué, et a de ce fait une fonction pragmatique. C’est un argument en faveur de l’analyse de Borkovskij, qui voyait dans la répétition de la préposition une emphase sur le modifieur, contre l’analyse de Worth (1982) qui y voit un phénomène mécanique (suivi par Klenin 1989, Zaliznjak 1986). on propose d’analyser la répétition de la préposition comme le résultat d’une anticipation de la préposition non initiale dans une structure [ Adj. Prep. N], [ Da Prep. N], ou [ N Prep. Adj.], [ N Prep. Da], très bien attestée dans les langues indo-européennes anciennes : [ Adj. Prep. N] devient [ Prep. Adj. Prep. N], conformément à la règle synchronique qui veut que la préposition soit en première position du SPrep. ; parallèlement, [ N Prep. Adj.] devient [ Prep. N Prep. Adj.]. L’ancienne préposition régissante, proclitique, qui fait corps avec N dans [ Adj. Prep. N], avec Adj. dans [ N Prep. Adj.], est conservée à sa place ancienne. Le développement symétrique est bien attesté en grec et en sabellique pour des postpositions, [ Adj. Postp N] devenant [ Adj. Postp. N Postp.] (grec homérique hon de domon de «vers sa maison » , réfection de * hon de domon, litt. sa-vers maison ; sudpicénien
esmen vepeten «dans cette pierre » , litt. «cette-dans pierre-dans » , ancien [ Da Postp. N]). La structure [ Adj. Prep. N] ou [ N Prep. Adj.] avec extraposition d’un constituant correspondait en effet à une mise en relief de ce dernier, et la structure héritière avec préposition répétée continue cette même fonction. Le vieux russe a éliminé la structure [ Prep. Adj. Prep. N], attestée en vieux slave et connue des byliny,
au profit de [ Prep. N Prep. Adj.], structure marquée en face de la structure non marquée [ Prep. Adj. N], parce que la mise en relief de l’adjectif est normalement assurée en russe par sa postposition. Les textes montrent une tendance à la grammaticalisation de ce tour aux dépens de sa valeur énonciative, notamment avec une apposition. Cette même structure se rencontre quand l’expansion de N est un complément de nom au génitif : elle a la même origine et remonte à [ NCt Prep. N], remodelé en [ Prep. NCt Prep. N], elle accompagne aussi un ordre des mots marqué avec complément de nom antéposé, mais elle semble avoir acquis dans ce cas spécifique une fonction syntaxique de désambiguïsation et de marque du régime disjoint de la préposition.
"Взятие редута": Мериме и Лермонтов ["L’Enlèvement de la Redoute" : Mérimée et Lermontov]
Authors: Nikolaeva Tatiana Mikhailovna 
Published: January 2018

В русском лермонтоведении принято было считать, что стихотворение Лермон-това «Бородино » (1837) было переработкой его раннего стихотворения «Поле Бородина » (1830). Однако анализ текстов обоих стихотворений Лермонтова и сравнение «Бородино » с очерком Проспера Мериме l’Enlèvement de la redoute,
проведенный автором статьи, показал, что текст «Бородино » гораздо ближе к тексту П. Мериме по текстуальным показателям, чем к раннему стихотворению Лермонтова. Т. Николаева предполагает, что Лермонтов ознакомился в период с 1830 по 1837 год с новеллой Проспера Мериме.
L’image de Napoléon dans la culture populaire russe au XIXe siècle
Authors: Tchoudinov Alexandre V. 
Published: January 2018

Образ Наполеона в народной культуре России XIX века
В российском фольклоре XIX века образ иностранного неприятеля прошлых времен
– шла ли речь о татарах, поляках, турках или французах в целом – изображался в соответствии с традиционным архетипом : иноземный враг – всегда свирепый разбой-ник и губитель веры православной. Этни-ческие черты этого образа были размы-тыми : в разных версиях одного и того же сочинения татары легко могли заменяться поляками, турки – французами, и всё это без ущерба для сути текста. Не приходится говорить и о какой-либо персонификации подобного образа, за единственным, од-нако, исключением, каковым был образ Наполеона. Проведенные на исходе XIX в. этнографические исследования показали, что из всех зарубежных исторических дея-телей только Наполеона крестьяне знали практически по всей России, причем, одобряя разгром его Великой армии в
1812 году, к самому французскому импе-ратору относились с долей сочувствия. Ис-следовав эволюцию этого образа в народ- ной культуре России на протяжении XIX в., автор статьи пришел к выводу, что подоб-ная противоречивость, очевидно, была свя-зана с бытованием среди русского народа в некоторые периоды истории легенды о Наполеоне как возможном освободителе крепостных людей от неволи.
An Investigation of the Ranges of Validity of Asteroid Thermal Models for Near-Earth Asteroid Observations
Authors: Mommert M. , Jedicke R. , Trilling D. E. 
Published: January 2018

Abstract
The majority of known asteroid diameters are derived from thermal-infrared observations. Diameters are derived using asteroid thermal models that approximate their surface temperature distributions and compare the measured thermal-infrared flux with model-dependent predictions. The most commonly used thermal model is the Near-Earth Asteroid Thermal Model (NEATM), which is usually perceived as superior to other models like the Fast-Rotating Model (FRM). We investigate the applicability of the NEATM and the FRM to thermal-infrared observations of Near-Earth Objects using synthetic asteroids with properties based on the real Near-Earth Asteroid (NEA) population. We find the NEATM to provide more accurate diameters and albedos than the FRM in most cases, with a few exceptions. The modeling results are barely affected by the physical properties of the objects, but we find a large impact of the solar phase angle on the modeling results. We conclude that the NEATM provides statistically more robust diameter estimates for NEAs observed at solar phase angles less than ∼65°, while the FRM provides more robust diameter estimates for solar phase angles greater than ∼65°. We estimate that <5% of all NEA diameters and albedos derived up to date are affected by systematic effects that are of the same order of magnitude as the typical thermal model uncertainties. We provide statistical correction functions for diameters and albedos derived using the NEATM and FRM as a function of solar phase angle.
Exploring the Chemical Composition and Double Horizontal Branch of the Bulge Globular Cluster NGC 6569
Authors: Johnson Christian I. , Rich R. Michael , Caldwell Nelson , Mateo Mario , Bailey John I. , Olszewski Edward W. , Walker Matthew G. 
Published: January 2018

Abstract
Photometric and spectroscopic analyses have shown that the Galactic bulge cluster Terzan 5 hosts several populations with different metallicities and ages that manifest as a double red horizontal branch (HB). A recent investigation of the massive bulge cluster NGC 6569 revealed a similar, though less extended, HB luminosity split, but little is known about the cluster’s detailed chemical composition. Therefore, we have used high-resolution spectra from the Magellan–M2FS and VLT–FLAMES spectrographs to investigate the chemical compositions and radial velocity distributions of red giant branch and HB stars in NGC 6569. We found the cluster to have a mean heliocentric radial velocity of −48.8 km s−1 (σ = 5.3 km s−1; 148 stars) and

dex (19 stars), but the cluster’s 0.05 dex [Fe/H] dispersion precludes a significant metallicity spread. NGC 6569 exhibits light- and heavy-element distributions that are common among old bulge/inner Galaxy globular clusters, including clear (anti)correlations between [O/Fe], [Na/Fe], and [Al/Fe]. The light-element data suggest that NGC 6569 may be composed of at least two distinct populations, and the cluster’s low

dex indicates significant pollution with r-process material. We confirm that both HBs contain cluster members, but metallicity and light-element variations are largely ruled out as sources for the luminosity difference. However, He mass fraction differences as small as ΔY ∼ 0.02 cannot be ruled out and may be sufficient to reproduce the double HB.
Stellar Spin–Orbit Alignment for Kepler-9, a Multi-transiting Planetary System with Two Outer Planets Near 2:1 Resonance
Authors: Wang Songhu , Addison Brett , Fischer Debra A. , Brewer John M. , Isaacson Howard , Howard Andrew W. , Laughlin Gregory 
Published: January 2018

Abstract
We present spectroscopic measurements of the Rossiter–McLaughlin effect for the planet b of the Kepler-9 multi-transiting planetary system. The resulting sky-projected spin–orbit angle is λ = −13° ± 16°, which favors an aligned system and strongly disfavors highly misaligned, polar, and retrograde orbits. Including Kepler-9, there are now a total of four Rossiter–McLaughlin effect measurements for multiplanet systems, all of which are consistent with spin–orbit alignment.
ALMA 26 arcmin2 Survey of GOODS-S at One-millimeter (ASAGAO): X-Ray AGN Properties of Millimeter-selected Galaxies
Authors: Ueda Y. , Hatsukade B. , Kohno K. , Yamaguchi Y. , Tamura Y. , Umehata H. , Akiyama M. , Ao Y. , Aretxaga I. , Caputi K. , Dunlop J. S. , Espada D. , Fujimoto S. , Hayatsu N. H. , Imanishi M. , Inoue A. K. , Ivison R. J. , Kodama T. , Lee M. M. , Matsuoka K. , Miyaji T. , Morokuma-Matsui K. , Nagao T. , Nakanishi K. , Nyland K. , Ohta K. , Ouchi M. , Rujopakarn W. , Saito T. , Tadaki K. , Tanaka I. , Taniguchi Y. , Wang T. , Wang W.-H. , Yoshimura Y. , Yun M. S. 
Published: January 2018

Abstract
We investigate the X-ray active galactic nucleus (AGN) properties of millimeter galaxies in the Great Observatories Origins Deep Survey South (GOODS-S) field detected with the Atacama Large Millimeter/submillimeter Array (ALMA), by utilizing the Chandra 7-Ms data, the deepest X-ray survey to date. Our millimeter galaxy sample comes from the ASAGAO survey covering 26 arcmin2 (12 sources at a 1.2 mm flux-density limit of

mJy), supplemented by the deeper but narrower 1.3 mm survey of a part of the ASAGAO field by Dunlop et al. Ofthe 25 total millimeter galaxies, 14 have Chandra counterparts. The observed AGN fractions at

are found to be

% and

% for the ultra-luminous and luminous infrared galaxies with log

/

= 12–12.8 and log

/

= 11.5–12, respectively. The majority (∼2/3) of the ALMA and/or Herschel detected X-ray AGNs at z = 1.5−3 appear to be star-formation-dominant populations, having

/

ratios smaller than the “simultaneous evolution” value expected from the local black-hole-mass-to-stellar-mass (

–M
*) relation. On the basis of the

and stellar mass relation, we infer that a large fraction of star-forming galaxies at

have black hole masses that are smaller than those expected from the local

–M
* relation. This contrasts previous reports on luminous AGNs at the same redshifts detected in wider and shallower surveys, which are subject to selection biases against lower luminosity AGNs. Our results are consistent with an evolutionary scenario in which star formation occurs first, and an AGN-dominant phase follows later, in objects that finally evolve into galaxies with classical bulges.
Limits on the Lorentz Invariance Violation from UHECR Astrophysics
Authors: Guedes Lang Rodrigo , Martínez-Huerta Humberto , de Souza Vitor 
Published: January 2018

Abstract
In this paper, the Lorentz invariance violation (LIV) is introduced in the calculations of photon propagation in the universe. LIV is considered in the photon sector, and the mean-free path of the

interaction is calculated. The corresponding photon horizon, including LIV effects, is used to predict major changes in the propagation of photons with energy above 1018 eV. The flux of GZK photons on Earth, considering LIV, is calculated for several source models of ultra-high-energy cosmic rays (UHECRs). The predicted flux of GZK gamma-rays is compared to the new upper limits on the photon flux obtained by the Pierre Auger Observatory in order to impose upper limits on the LIV coefficients of order n = 0, 1, and 2. The limits on the LIV coefficients derived here are more realistic than previous works and in some cases more restrictive. The analysis resulted in LIV upper limits in the photon sector of

,

, and

in the astrophysical scenario, which best describes UHECR data.
Time-dependent Electron Acceleration in Pulsar Wind Termination Shocks: Application to the 2011 April Crab Nebula Gamma-Ray Flare
Authors: Kroon John J. , Becker Peter A. , Finke Justin D. 
Published: January 2018

Abstract
The γ-ray flares from the Crab Nebula observed by AGILE and Fermi-LAT between 2007 and 2013 reached GeV photon energies and lasted several days. The strongest emission, observed during the 2011 April “superflare”, exceeded the quiescent level by more than an order of magnitude. These observations challenge the standard models for particle acceleration in pulsar wind nebulae, because the radiating electrons have energies exceeding the classical radiation-reaction limit for synchrotron emission. Particle-in-cell simulations have suggested that the classical synchrotron limit can be exceeded if the electrons also experience electrostatic acceleration due to shock-driven magnetic reconnection. In this paper, we revisit the problem using an analytic approach based on solving a fully time-dependent electron transport equation describing the electrostatic acceleration, synchrotron losses, and escape experienced by electrons in a magnetically confined plasma “blob” as it encounters and passes through the pulsar wind termination shock. We show that our model can reproduce the γ-ray spectra observed during the rising and decaying phases of each of the two sub-flare components of the 2011 April superflare. We integrate the spectrum for photon energies

MeV to obtain the light curve for the event, which also agrees with the observations. We find that strong electrostatic acceleration occurs on both sides of the termination shock, driven by magnetic reconnection. We also find that the dominant mode of particle escape changes from diffusive escape to advective escape as the blob passes through the shock.
Inverse Compton Scattered Merger-nova: Late X-Ray Counterpart of Gravitational-wave Signals from NS–NS/BH Mergers
Authors: Ai Shunke , Gao He 
Published: January 2018

Abstract
The recent observations of GW170817 and its electromagnetic (EM) counterparts show that double neutron star mergers could lead to rich and bright EM emissions. Recent numerical simulations suggest that neutron star and neutron star/black hole (NS–NS/BH) mergers would leave behind a central remnant surrounded by a mildly isotropic ejecta. The central remnant could launch a collimated jet and when the jet propagates through the ejecta, a mildly relativistic cocoon would be formed and the interaction between the cocoon and the ambient medium would accelerate electrons via external shock in a wide angle, so that the merger-nova photons (i.e., thermal emission from the ejecta) would be scattered into higher frequency via an inverse Compton (IC) process when they propagate through the cocoon shocked region. We find that the IC scattered component peaks at the X-ray band and it will reach its peak luminosity on the order of days (simultaneously with the merger-nova emission). With current X-ray detectors, such a late X-ray component could be detected out to 200 Mpc, depending on the merger remnant properties. It could serve as an important electromagnetic counterpart of gravitational-wave signals from NS–NS/BH mergers. Nevertheless, simultaneous detection of such a late X-ray signal and the merger-nova signal could shed light on the cocoon properties and the concrete structure of the jet.
An Efficient Statistical Method to Compute Molecular Collisional Rate Coefficients
Authors: Loreau Jérôme , Lique François , Faure Alexandre 
Published: January 2018

Abstract
Our knowledge about the “cold” universe often relies on molecular spectra. A general property of such spectra is that the energy level populations are rarely at local thermodynamic equilibrium. Solving the radiative transfer thus requires the availability of collisional rate coefficients with the main colliding partners over the temperature range ∼10–1000 K. These rate coefficients are notoriously difficult to measure and expensive to compute. In particular, very few reliable collisional data exist for inelastic collisions involving reactive radicals or ions. In this Letter, we explore the use of a fast quantum statistical method to determine molecular collisional excitation rate coefficients. The method is benchmarked against accurate (but costly) rigid-rotor close-coupling calculations. For collisions proceeding through the formation of a strongly bound complex, the method is found to be highly satisfactory up to room temperature. Its accuracy decreases with decreasing potential well depth and with increasing temperature, as expected. This new method opens the way to the determination of accurate inelastic collisional data involving key reactive species such as

, H2O+, and H3O+ for which exact quantum calculations are currently not feasible.