bluuebunny/crossref_metadata_2025_split huggingface dataset:
Identifikasi Aspek Elemen Desain Pada Gim A Space for the Unbound
Authors: Ika Resmika Andelina  , Eko Prasetyo Martinus , Theresia Sherly 
Published: October 2024

Seiring perkembangan teknologi, kini bentuk dan jenis media hiburan sudah beragam, antara lain, film, gim, film animasi, buku, dan sebagainya. Gim adalah salah satu media hiburan yang sudah sangat dikenal dan beradar masif di masyarakat, dengan banyaknya kategori yang ada. Salah satu gim yang berhasil menggaet banyak perhatian dan respon positif adalah A Space for the Unbound, yang dikembangkan dan diproduksi oleh Mojiken Studio & Toge Production dari Indonesia. Gim ini berhasil menyabet banyak penghargaan internasional dengan menggunakan gaya visual pixel art, disertai pemilihan setting negara Indonesia pada era tahun 90-an. Begitu banyak elemen di dalam gim ini yang menarik perhatian para konsumen, salah satunya adalah setting negara Indonesia yang disertai berbagai karakter yang relatable, latar belakang cerita yang menarik, gimplay yang mudah dimengerti dan berbagai elemen lainnya. Elemen-elemen inilah yang menarik untuk dibedah lebih lanjut lebih mendalam untuk mengetahui elemen desain apa saja yang memiliki pengaruh besar terhadap kesuksesan A Space for the Unbound. Analisis dilakukan secara kualitatif deskriptif untuk semua elemen desain yang akan ditemukan dalam gim. Penguraian elemen-elemen desain visual dibedah dengan pendekatan mimesis milik Plato, yang kemudian diperdalam oleh pendekatan karakter Holistik milik Mounsey untuk menelaah elemen lain di belakang penciptaan sebuah karakter, seperti cerita dan sifat karakter serta penerimaan oleh konsumen.
Rescate y Fomento de las Expresiones Culturales de la Parroquia Quiroga, Cantón Cotacachi, Provincia de Imbabura, Mediante la Confección y Exposición del Traje Típico del Chagra Quirogueño
Authors: Vaca Gómez Diego Marconi , Ruiz Ruiz Edison Santiago , Echeverría Núñez Andrés Danilo 
Published: October 2024

La elaboración del traje típico del “Chagra quirogueño” se desarrolló baja la investigación cualitativa en donde se ha recurrido a las memorias colectivas el cual reconstruye un pasado significativo que se hace desde el presente, una tradición que desde hace 27 años viene potenciándose y arraigándose más y más en los quirogueños, el objetivo de este trabajo de investigación es representar el traje típico del “Chagra quirogueño”, mediante la confección del traje típico y sus accesorios, el mismo que a través de su exhibición fomentará el rescate de la transmisión cultural de Quiroga. El trabajo se llevó a cabo en tres fases: la etapa 1 se refiere a la recopilación de la información con la participación de los estudiantes del ISU Cotacachi, la fase 2 comprende la elaboración del diseño y prototipado del traje, se desarrolla principalmente, el diseño plano, el patronaje, el ensamble, y las fichas técnicas del control de calidad y la fase 3 se refiere a la revisión de la elaboración del traje detallado en la etapa 2 y la exposición de los resultados finales del traje típico en estudio. . Finalmente, la elaboración del traje típico del “Chagra quirogueño” constituye una alternativa para fomentar el rescate de las tradiciones de la parroquia de Quiroga del cantón Cotacachi, y fortalecieron en los estudiantes sus habilidades de investigación y las destrezas técnicas que conlleva las actividades de la confección textil, al intervenir directamente en las diferentes etapas de conlleva el desarrollo del presente trabajo.
Intención de los Estudiantes de Ingeniería por Desarrollar Emprendimientos Sustentables
Authors: Montero Hernández Adriana , Espinosa Espíndola Mónica Teresa , Ruíz González Martha Angélica , Méndez Adolfo Maceda , Calderón Yannet Paz 
Published: October 2024

Los emprendimientos sustentables constituyen una alternativa de autoempleo y promueven el uso responsable de los recursos. El objetivo de esta investigación es analizar la intención de los estudiantes de carreras de ingeniería próximos a egresar de la Universidad Tecnológica de la Mixteca (UTM), situada al sur de México, por llevar a cabo emprendimientos sustentables. La investigación es mixta, con un alcance exploratorio descriptivo, en el que se busca identificar los elementos que han contribuido a desarrollar la intención de los estudiantes por el emprendimiento sustentable, o bien aquellos aspectos que se pueden fortalecer. Se utilizó investigación documental, se realizaron entrevistas a los jefes de carrera de las ingenierías consideradas y se aplicó una encuesta a una muestra estadísticamente representativa de estudiantes próximos a egresar de las carreras de ingeniería de la UTM. Entre los principales resultados se encontró que 82% de los estudiantes ha tenido ideas de negocios durante sus estudios, 77% considera al emprendimiento como una alternativa al terminar su carrera, el 90% tiene interés en solucionar alguna problemática detectada en su comunidad y el 75% no emprendería si su proyecto implica la utilización de grandes cantidades de algún recurso natural.
Discovery of MgS and NaS in the Interstellar Medium and Tentative Detection of CaO
Authors: Rey-Montejo Marta , Jiménez-Serra Izaskun , Martín-Pintado Jesús , Rivilla Víctor M. , Megías Andrés , San Andrés David , Sanz-Novo Miguel , Colzi Laura , Zeng Shaoshan , López-Gallifa Álvaro , Martínez-Henares Antonio , Martín Sergio , Tercero Belén , de Vicente Pablo , Requena-Torres Miguel 
Published: October 2024

Abstract
We report the first detection of the metal-bearing molecules sodium sulfide and magnesium sulfide and the tentative detection of calcium monoxide in the interstellar medium toward the Galactic center molecular cloud G+0.693-0.027. The derived column densities are (5.0 ± 1.1) × 1010 cm−2, (6.0 ± 0.6) × 1010 cm−2, and (2.0 ± 0.5) × 1010 cm−2, respectively. This translates into fractional abundances with respect to H2 of (3.7 ± 1.0) × 10−13, (4.4 ± 0.8) × 10−13, and (1.5 ± 0.4) × 10−13, respectively. We have also searched for other Na-, Mg-, and Ca-bearing species toward this source but none of them have been detected and thus we provide upper limits for their abundances. We discuss the possible chemical routes involved in the formation of these molecules containing metals under interstellar conditions. Finally, we compare the ratio between sulfur-bearing and oxygen-bearing molecules with and without metals, finding that metal-bearing sulfur molecules are much more abundant than metal-bearing oxygen ones, in contrast with the general trend found in the ratios between other nonmetal-oxygen- and sulfur-bearing molecules. This further strengthens the idea that sulfur may be a little depleted in G+0.693-0.027 as a result of the low-velocity shocks present in this source sputtering large amounts of material from dust grains.
Distorted Magnetic Flux Ropes within Interplanetary Coronal Mass Ejections
Authors: Weiss Andreas J. , Nieves-Chinchilla Teresa , Möstl Christian 
Published: October 2024

Abstract
Magnetic flux ropes (MFRs) at the center of interplanetary coronal mass ejections (ICMEs) are often characterized as simplistic cylindrical or toroidal tubes with field lines that twist around the cylinder or torus axis. Recent multipoint observations suggest that the overall geometry of these large-scale structures may be significantly more complex. As such, contemporary modeling approaches are likely insufficient to properly understand the global structure of any ICME. In an attempt to rectify this issue, we have developed a novel flux rope modeling approach that allows for the description of arbitrary distortions of the flux rope cross section or deformation of the magnetic axis. The resulting distorted MFR model is a fully analytic model that can be used to describe a complex geometry and is numerically efficient enough to be used for event reconstructions. To demonstrate the usefulness of our approach, we focus on a specific implementation of our model and apply it to an ICME event that was observed in situ on 2023 April 23 at the L1 point by the Wind spacecraft and also by the STEREO-A spacecraft, which was 10.°2 further east and 0.°9 south in heliographic coordinates. We demonstrate that our model can accurately reconstruct each observation individually and also gives a fair reconstruction of both events simultaneously using a multipoint reconstruction algorithm, which results in a geometry that is inconsistent with a cylindrical or toroidal approximation.
A Model for Flux Rope Formation and Disconnection in Pseudostreamer Coronal Mass Ejections
Authors: Wyper P. F. , Lynch B. J. , DeVore C. R. , Kumar P. , Antiochos S. K. , Daldorff L. K. S. 
Published: October 2024

Abstract
Coronal mass ejections (CMEs) from pseudostreamers represent a significant fraction of large-scale eruptions from the Sun. In some cases, these CMEs take a narrow jet-like form reminiscent of coronal jets; in others, they have a much broader fan-shaped morphology like CMEs from helmet streamers. We present results from a magnetohydrodynamic simulation of a broad pseudostreamer CME. The early evolution of the eruption is initiated through a combination of breakout interchange reconnection at the overlying null point and ideal instability of the flux rope that forms within the pseudostreamer. This stage is characterized by a rolling motion and deflection of the flux rope toward the breakout current layer. The stretching out of the strapping field forms a flare current sheet below the flux rope; reconnection onset there forms low-lying flare arcade loops and the two-ribbon flare footprint. Once the CME flux rope breaches the rising breakout current layer, interchange reconnection with the external open field disconnects one leg from the Sun. This induces a whip-like rotation of the flux rope, generating the unstructured fan shape characteristic of pseudostreamer CMEs. Interchange reconnection behind the CME releases torsional Alfvén waves and bursty dense outflows into the solar wind. Our results demonstrate that pseudostreamer CMEs follow the same overall magnetic evolution as coronal jets, although they present different morphologies of their ejecta. We conclude that pseudostreamer CMEs should be considered a class of eruptions that are distinct from helmet-streamer CMEs, in agreement with previous observational studies.
Detecting Detached Black Hole Binaries through Photometric Variability
Authors: Chawla Chirag , Chatterjee Sourav , Shah Neev , Breivik Katelyn 
Published: October 2024

Abstract
Understanding the connection between the properties of black holes (BHs) and their progenitors is interesting in many branches of astrophysics. Discovering BHs in detached orbits with luminous companions (LCs) promises to help establish this connection since the LC and BH progenitor are expected to have the same metallicity and formation time. We explore the possibility of detecting BH–LC binaries in detached orbits using photometric variations of the LC flux, induced by tidal ellipsoidal variation, relativistic beaming, and self-lensing. We create realistic present-day populations of detached BH–LC binaries in the Milky Way (MW) using binary population synthesis where we adopt observationally motivated initial stellar and binary properties, star formation history, and the present-day distribution of these sources in the MW based on detailed cosmological simulations. We test detectability of these sources via photometric variability by Gaia and TESS missions by incorporating their respective detailed detection biases as well as interstellar extinction. We find that Gaia is expected to resolve ∼300–1000 (∼700–1500) detached BH–LC binaries with signal-to-noise ratio (SNR) ≥ 10 (1) depending on the photometric precision and details of supernova physics. Similarly, the number of resolved BH–LC binaries with TESS is ∼50–200 (∼140–350). We find that

136

−
15

+
15

BH–LC binaries would be common between Gaia and TESS. Moreover, ∼60–70 (∼50–200) BH–LC binaries identifiable using photometry with SNR ≥ 10 may also be resolved using Gaia’s radial velocity (astrometry).
Photonuclear Reaction Rates of 157,159Ho and 163,165Tm and Their Impact in the γ-process
Authors: Cheng Hao , Sun Bao-Hua , Zhu Li-Hua , Kusakabe Motohiko , Luo Yudong , Kajino Toshitaka , Wang Chang-Jian , Yao Xing-Qun , He Chuang-Ye , Liu Fu-Long , Guo Bing 
Published: October 2024

Abstract
Reliable photonuclear reaction rates in stellar conditions are essential for understanding the origin of the heavy stable neutron-deficient isotopes between 74Se and 196Hg, i.e., p-nuclei. However, many reaction rates of relevance still have to rely on the Hauser–Feshbach (HF) model due to the rarity of experimental progress. One such case is in the mass range of 160 for Dy, Er, Ho, and Tm isotopes. In this work we attempt to constrain the HF model in the TALYS package by reproducing the available experimental data on 160Dy(p, γ)161Ho and 162Er(p, γ)163Tm in the A ∼ 160 mass region, and examine the effects of level density, gamma strength function, and the optical model potential. The constrained model then allows us to calculate the reaction rates of 157,159Ho(γ, p) and 163,165Tm(γ, p) for the γ-process nucleosynthesis in a carbon-deflagration model for Type Ia supernovae. Our recommended rates differ from the JINA REACLIB by more than one order of magnitude in the temperature range 2–3 GK. This results in changes in the final abundance of p-nuclei in the A ∼ 160 mass range by −5.5% to 3% from those with JINA, which means that the uncertainty of (γ, p) reactions is not predominant for the synthesis of these nuclei.
Hedgehog: An Isolated Quiescent Dwarf Galaxy at 2.4 Mpc
Authors: Li 李 Jiaxuan 嘉轩 , Greene Jenny E. , Carlsten Scott G. , Danieli Shany 
Published: October 2024

Abstract
It is well known that almost all isolated dwarf galaxies are actively forming stars. We report the discovery of dw1322m2053 (nicknamed Hedgehog), an isolated quiescent dwarf galaxy at a distance of 2.40 ± 0.15 Mpc with a stellar mass of M
⋆ ≈ 105.8
M
⊙. The distance is measured using surface brightness fluctuations with both Legacy Surveys and deep Magellan/IMACS imaging data. Hedgehog is 1.7 Mpc from the nearest galaxy group, Centaurus A, and has no neighboring galaxies within 1 Mpc, making it one of the most isolated quiescent dwarf galaxies at this stellar mass. It has a red optical color and early-type morphology and shows no UV emission. This indicates that Hedgehog has an old stellar population and no ongoing star formation. Compared with other quiescent dwarfs in the Local Group and Local Volume, Hedgehog appears smaller in size for its luminosity but is consistent with the mass–size relations. Hedgehog might be a backsplash galaxy from the Centaurus A group, but it could also have been quenched in the field by ram pressure stripping in the cosmic web, reionization, or internal processes such as supernova and stellar feedback. Future observations are needed to fully unveil its formation, history, and quenching mechanisms.
A New Detailed Global Map of Lunar Light Plains
Authors: Giuri Barbara , van der Bogert Carolyn H. , Hiesinger Harald , Schmedemann Nico 
Published: October 2024

Abstract
Lunar light plains (LPs) are globally distributed, smooth and flat geologic units occurring in crater floors and topographic lows, similar in morphology to mare basalts, but with moderate to high albedo. Despite numerous studies investigating LPs, their emplacement mechanism(s), ages, and origins remain highly debated. To aid in deciphering their origin(s), we produced a new independent global map of the extent of the LPs. Thus, we (1) evaluated the morphological and compositional definitions of LP; (2) tested the reproducibility of previous work; and (3) extended the previously mapped extents of LPs. We find morphological similarities between near- and farside LPs with regional variations in albedo and FeO contents. We were able to reproduce the majority of previous LP maps, with some notable exceptions. We find ∼13% of the lunar surface is covered by LPs, which is slightly higher than previous studies, likely due to our inclusion of smaller deposits. Overall, the distribution of LPs on the nearside appears to be denser around mare regions and exhibits more widely varying degrees of smoothness, size, albedo, and FeO contents compared to the farside highlands. In contrast, on the farside, we find a large number of LPs with similar morphologies and FeO contents, in ray-like patterns likely related to the Orientale impact event. Beyond Orientale’s influence, the occurrences of LPs are of lower albedo and FeO contents are fewer and sparser, with similar morphologies to the nearside deposits. Thus, our study indicates that an impact-related origin for the majority of LP deposits is most likely.
Inconsistencies in Simple Thermal Model Results for Near-Earth Asteroids between Infrared Telescope Facility SpeX and NEOWISE Data
Authors: Myers Samuel A. , Howell Ellen S. , Magri Christopher , Vervack Ronald J. , Fernández Yanga R. , Hinkle Mary L. , Marshall Sean E. 
Published: October 2024

Abstract
Understanding the properties of near-Earth asteroids (NEAs) is key for many aspects of planetary science, particularly planetary defense. Our current knowledge of NEA sizes and regolith properties is heavily dependent on simple thermal models. These models are often used to analyze data from missions such as NEOWISE because they are well suited to deal with large volumes of data. However, simple model results based on NEOWISE data may be inconsistent with results based on other types of observation in some cases. In this work, we seek to better understand these potential inconsistencies, as well as the situations for which they are most prevalent. We do this by comparing simple model results based on Infrared Telescope Facility SpeX data to similar results based on NEOWISE data. This is carried out for six NEAs that represent a range of spectral types, shapes, and rotation states. We find that models based on SpeX and NEOWISE data for these six objects are inconsistent in some cases, even though the SpeX results are consistent with other methods and observations. We find that objects observed at fainter magnitudes and objects with more primitive compositions are more likely to produce inconsistent fits. These results highlight the importance of better understanding the limitations of simple models as applied to large survey data sets like NEOWISE. This is particularly true as we move into an era where our understanding of the NEA population will be dominated by future large surveys such as NEO Surveyor.
Implantation et architecture de l’abbaye cistercienne de Bon-Repos : un programme de recherche interdisciplinaire
Authors: Dubois Adrien , Vincent Jean-Baptiste 
Published: October 2024

Dans le cadre d’un réaménagement du site de l’abbaye de Bon-Repos, plusieurs investigations de terrain, sans altération du sous-sol (levé microtopographique, étude des élévations à partir d’une modélisation photogrammétrique des maçonneries, prospection radar du sous-sol), ont été menées et croisées avec les sources textuelles et iconographiques en vue de proposer, par une lecture régressive, une restitution de l’abbaye médiévale que les travaux de l’époque moderne ont fait quasiment disparaître. L’étude amène à relativiser la notion de « modèle », souvent évoquée pour ces établissements lorsque l’on en ignore la configuration primitive, notion qui passe sous silence les enjeux techniques. Il s’agit ici au contraire de tenter de comprendre la configuration des lieux au xiie siècle, ses atouts, mais aussi les moyens mis en œuvre pour s’adapter à ses inconvénients. Ce type de monographie apparaît en effet comme un préalable indispensable à toute modélisation et sans doute même à toute fouille archéologique.
L’huître ou le maërl ? Le dilemme de la Marine face aux convoitises de la société d’agriculture de Brest (1840-1849)
Authors: Bosseboeuf Lucas 
Published: October 2024

Au début des années 1840, la Marine déplore l’appauvrissement des bancs d’huîtres plates (Ostrea edulis) de la rade de Brest. Cette activité très rémunératrice et prisée des pêcheurs renfloue indirectement le nombre d’inscrits maritimes. La Marine, qui se doit de ménager cette ressource, charge un enquêteur de sillonner la rade pour en rechercher les causes. Rapidement, le dragage du maërl (Lithothamnium corallioides, Phymatholiton calcareum et Lithophyllum fasciculatum) est accusé de détériorer les fonds d’huîtres et son exploitation devient interdite. Or, à cette même période, la société d’agriculture de Brest encourage l’usage de cette algue pour amender les terres « incultes » du centre Bretagne. Un bras de fer s’opère entre la Marine et la société d’agriculture de Brest. Leurs intérêts convergents et divergents incitent le ministre de la Marine à former une commission mixte en 1847. Celle-ci est chargée d’évaluer les répercussions de l’exploitation des amendements marins sur l’état de santé des huîtres plates. Au terme de cette enquête, la négociation aboutit à un résultat jugé d’intérêt général. La Marine s’est enfin dotée d’un règlement des pêches, tandis que la société d’agriculture est à nouveau autorisée à exploiter le maërl et le goémon rouge. Pour autant, cette issue est-elle réellement favorable à toutes les parties ?
Structure thématique du paragraphe dans les productions d’apprenants sinophones de français langue seconde
Authors: Aleksandrova Tatiana 
Published: October 2024

Cet article porte sur l’organisation thématique des paragraphes rédigés par des apprenants sinophones de niveau B2 en français langue seconde (L2) dans le cadre de la production d’un essai argumenté. Rédiger un texte en L2 est une tâche complexe nécessitant de nombreuses compétences : linguistiques, rhétoriques et pragmatiques. Des travaux précédents attestent les difficultés persistantes d’apprenants de L2 à l’écrit. Les résultats de cette étude montrent que les apprenants sinophones partagent un certain nombre de stratégies propres aux francophones natifs, à savoir les formes particulières de progression thématique qui sont mises en œuvre pour relier les propositions. Des écarts sont par ailleurs observables : 1) les paragraphes des apprenants sont systématiquement plus courts que ceux des francophones et comportent moins de progressions linéaires préférant la progression à thème constant ; 2) les ruptures thématiques sont également plus fréquentes dans leurs productions. En ce qui concerne les moyens linguistiques, nous relevons certaines différences au niveau des reprises anaphoriques. Une différence pragmatique en lien avec le registre de langue est également observée. Notre analyse thématique et linguistique des productions permet de mieux comprendre les spécificités d’organisation du paragraphe dans les productions des apprenants sinophones.
Les écrivaines de La Grande librairie : des invitées de deuxième ligne ?
Authors: Pons Desoutter Martine , Rossato Solange , Zampa Virginie 
Published: October 2024

Pour cet article, nous nous sommes intéressées à la place des autrices dans une émission de télévision littéraire très suivie sur une chaine du service public français. Notre analyse porte sur les temps de parole, les thématiques des émissions, la répartition sexuée des invité·e·s et les processus langagiers mis en œuvre. Elle révèle que la parité et l’équité entre les sexes ne vont pas de soi. En effet, elle montre que le choix des invités, le déroulé des échanges comme les adresses ainsi que certains éléments langagiers de l’animateur contribuent à minorer la place des autrices.