bluuebunny/crossref_metadata_2025_split huggingface dataset:
El modelo DUA y sus formas de evaluación
Authors: Chuquiguanca Jiménez Celia Carmita , Palacios Argüello Diana Alexandra , Villarreal Silva Ximena Enriqueta , Yánez Taco Daniela Joselyn , Chucho Mayanza Freddy Paul 
Published: September 2023

El Diseño Universal para el Aprendizaje (DUA) establece una serie de principios y pautas relevantes para el desarrollo de currículos que ofrezcan a todos los estudiantes igualdad de oportunidades en el proceso enseñanza-aprendizaje. Estos principios permiten que el modelo tenga una actuación pedagógica que hace posible a través de la puesta en marcha de diversas estrategias, la evaluación de aprendizajes y el logro de las competencias que se desean lograr, de acuerdo la diversidad de aprendizaje de los alumnos. Por esta razón, el presente artículo tiene como objetivo general analizar el modelo DUA y sus formas de evaluación, a fin de poder precisar qué tan bien los alumnos están llevando a cabo los objetivos de aprendizaje en las aulas de clase. La metodología que se utilizó fue de una investigación de tipo descriptiva y como técnica de análisis se usó la revisión documental la cual hizo posible la obtención de recursos claves sobre el tema establecido. Como conclusión, se obtuvo que las formas de evaluación del DUA deben ser entendidas por los docentes no como un fase final, sino como un proceso constante utilizado para conocer el rendimiento académico de los estudiantes.
Looking Racism in the Face at Clemson University
Authors: Fryberger Charissa 
Published: September 2023

This article will outline the rhetorical scaffolding I placed around an experimental assignment in Clemson University’s freshman Composition and Rhetoric classes to help students understand not only the history, but its impact on the experience of the African Americans who study and work on this campus today. The project asked students to do an extensive research project and develop a presentation related to the rhetoric that surrounds the history of African American contributions to the university, using, as a jumping-off place for their research, the extensive archival work of Dr. Rhondda Thomas in her “Call My Name” project. Based on 119 student responses taken at various points in the project, it will attempt to analyze what students learned and how the activities in which they participated affected their understanding of racial relationships and issues. My observations during this experiment have led me to believe that educational projects which encourage students to discover the impacts of racism through real encounters with those who have suffered those impacts (whether historical or living) are valuable ways to combat racism, improve multicultural understanding, and waken students from dominant groups to the roles they can play in changing racist systems and assumptions.
UV-bright Star-forming Clumps and Their Host Galaxies in UVCANDELS at 0.5 ≤ z ≤ 1
Authors: Martin Alec , Guo Yicheng , Wang Xin , Koekemoer Anton M. , Rafelski Marc , Teplitz Harry I. , Windhorst Rogier A. , Alavi Anahita , Grogin Norman A. , Prichard Laura , Sunnquist Ben , Ceverino Daniel , Chartab Nima , Conselice Christopher J. , Dai Y. Sophia , Dekel Avishai , Gardner Jonathan P. , Gawiser Eric , Hathi Nimish P. , Hayes Matthew J. , Jansen Rolf A. , Ji Zhiyuan , Koo David C. , Lucas Ray A. , Mandelker Nir , Mehta Vihang , Mobasher Bahram , Nedkova Kalina V. , Primack Joel , Ravindranath Swara , Robertson Brant E. , Rutkowski Michael J. , Sattari Zahra , Soto Emmaris , Yung L. Y. Aaron 
Published: September 2023

Abstract
Giant star-forming clumps are a prominent feature of star-forming galaxies (SFGs) and contain important clues on galaxy formation and evolution. However, the basic demographics of clumps and their host galaxies remain uncertain. Using the Hubble Space Telescope/Wide Field Camera 3 F275W images from the Ultraviolet Imaging of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey, we detect and analyze giant star-forming clumps in galaxies at 0.5 ≤ z ≤ 1, connecting two epochs when clumps are common (at cosmic high noon, z ∼ 2) and rare (in the local Universe). We construct a clump sample whose rest-frame 1600 Å luminosity is 3 times higher than the most luminous local H ii regions (M
UV ≤ −16 AB). In our sample, 35% ± 3% of low-mass galaxies (log[M
∗/M
⊙] < 10) are clumpy (i.e., containing at least one off-center clump). This fraction changes to 22% ± 3% and 22% ± 4% for intermediate (10 ≤ log[M
∗/M
⊙] ≤ 10.5) and high-mass (log[M
∗/M
⊙] > 10.5) galaxies, in agreement with previous studies. When compared to similar-mass nonclumpy SFGs, low- and intermediate-mass clumpy SFGs tend to have higher star formation rates (SFRs) and bluer rest-frame U − V colors, while high-mass clumpy SFGs tend to be larger than nonclumpy SFGs. However, clumpy and nonclumpy SFGs have similar Sérsic index, indicating a similar underlying density profile. Furthermore, we investigate how the UV luminosity of star-forming regions correlates with the physical properties of host galaxies. On average, more luminous star-forming regions reside in more luminous, smaller, and/or higher specific SFR galaxies and are found closer to their hosts’ galactic centers.
CHANDRA X-Ray Observations of A119: Cold Fronts and a Shock in an Evolved Off-axis Merger
Authors: Watson Courtney B. , Blanton Elizabeth L. , Randall Scott W. , Sarazin Craig L. , Sarkar Arnab , ZuHone John A. , Douglass E. M. 
Published: September 2023

Abstract
We present Chandra X-ray observations of the dynamically complex galaxy cluster A119 (z = 0.044). A119 is host to two narrow-angle-tail (NAT) radio sources (0053-015 and 0053-016), whose tails are oriented parallel to each other, despite orthogonally oriented jet axes. Imaging and spectral analysis reveal X-ray emission elongated along the NE–SW axis, along with the presence of complex structures, including surface brightness discontinuities, which suggest possible merger activity along this axis. From radial profiles of the X-ray surface brightness, temperature, pressure, and density, we identify two surface brightness edges that are found to be cold fronts, possibly associated with large-scale sloshing of intracluster medium gas. We also identify a brightness edge to the S that is found to be a shock front with Mach number M = 1.21 ± 0.11, consistent with a merger shock. In addition, previous optical studies show the alignment of optical substructures along the N–S direction. The elongated X-ray emission, orientations of the NAT tails, and alignment of the optical substructure all suggest recent or ongoing merger activity in the NE–SW direction.
Direct Collapse to Precursors of Supermassive Black Hole Seeds: Radiation-feedback-generated Outflows
Authors: Luo Yang , Shlosman Isaac , Nagamine Kentaro 
Published: September 2023

Abstract
We use high-resolution zoom-in cosmological simulations to model outflow triggered by radiation and thermal drivers around the central mass accumulation during direct collapse within the dark matter (DM) halo. The maximal resolution is 1.3 × 10−5 pc, and no restrictions are put on the geometry of the inflow/outflow. The central mass is considered prior to the formation of the supermassive black hole seed at a redshift of z ∼ 15.9 and can constitute either a supermassive star (SMS) of ∼105
M
⊙ surrounded by a growing accretion disk or a self-gravitating disk. The radiation transfer is modeled using the ray-tracing algorithm. Due to the high accretion rate of ∼1 M
⊙ yr−1 determined by the DM halo, accretion is mildly supercritical, resulting in mildly supercritical luminosity that has only a limited effect on the accretion rate, with a duty cycle of ∼0.9. We observe a fast development of hot cavities, which quickly extend into polar funnels and expand dense shells. Within the funnels, fast winds, ∼103 km s−1, are mass-loaded by the accreting gas. We follow the expanding shells to ∼1 pc, when the shell velocity remains substantially (∼5 times) above the escape speed. The ionization cones formed by the central UV/X-ray completely ionize the cavities. Extrapolating the outflow properties shows that the halo material outside the shell will have difficulty stopping it. We therefore conclude that the expanding wind-driven shell will break out of the central parsec and will reach the halo virial radius. Finally, the anisotropic accretion flow on subparsec scales will attenuate the UV/soft X-rays on the H2. Hence, the formation of funnels and powerful outflows around, e.g., SMSs can have interesting observational corollaries.
Back to Business: SLX 1746–331 after 13 Years of Silence
Authors: Peng Jing-Qiang , Zhang Shu , Wang Peng-Ju , Zhang Shuang-Nan , Kong Ling-Da , Chen Yu-Peng , Shui Qing-Cang , Ji Long , Qu Jin-Lu , Tao Lian , Ge Ming-Yu , Ma Rui-Can , Chang Zhi , Li Jian , Li Zhao-sheng , Yu Zhuo-Li , Yan Zhe , Zhang Peng , Xiao Yun-Xiang , Zhao Shu-Jie 
Published: September 2023

Abstract
The black hole candidate system SLX 1746–331 was back to business in 2023, after a long silence of roughly 13 years. An outburst was observed thoroughly by Insight-HXMT and NICER. The outburst is characterized by spectral dominance of the soft state, where the joint Insight-HXMT and NICER spectral analysis shows the temperature dependence of the disk flux follows

T

in

3.98

, and thus suggests that the inner disk reaches its innermost stable circular orbit during almost the entire outburst. By assuming 0.3 L
Edd for the peak flux and an inclination angle of zero degrees, the lower limit of the compact object hosted in this system is estimated as 3.28 ± 2.14 M
⊙. We also look into the relation between the disk temperature and disk flux for a sample of black hole systems, and by taking the disk temperature derived in the outburst of SLX 1746–331, such a relation results in a mass estimation of 5.2 ± 4.5 M
⊙. Finally, the spin of the compact object is constrained to be larger than 0.8 with the spectral model KERRBB.
The Panchromatic Hubble Andromeda Treasury. XXI. The Legacy Resolved Stellar Photometry Catalog
Authors: Williams Benjamin F. , Durbin Meredith , Lang Dustin , Dalcanton Julianne J. , Dolphin Andrew E. , Smercina Adam , Merica-Jones Petia Yanchulova , Weisz Daniel R. , Bell Eric F. , Gilbert Karoline M. , Girardi Léo , Gordon Karl , Guhathakurta Puragra , Johnson L. Clifton , Lauer Tod R. , Seth Anil , Skillman Evan 
Published: September 2023

Abstract
We present the final legacy version of stellar photometry for the Panchromatic Hubble Andromeda Treasury (PHAT) survey. We have reprocessed all of the Hubble Space Telescope Wide Field Camera 3 and Advanced Camera for Surveys near-ultraviolet (F275W, F336W), optical (F475W, F814W), and near-infrared (F110W, F160W) imaging from the PHAT survey using an improved method that optimized the survey depth and chip-gap coverage by including all overlapping exposures in all bands in the photometry. An additional improvement was gained through the use of charge transfer efficiency (CTE)–corrected input images, which provide more complete star finding as well as more reliable photometry for the NUV bands, which had no CTE correction in the previous version of the PHAT photometry. While this method requires significantly more computing resources and time than earlier versions where the photometry was performed on individual pointings, it results in smaller systematic instrumental completeness variations as demonstrated by cleaner maps in stellar density, and it results in optimal constraints on stellar fluxes in all bands from the survey data. Our resulting catalog has 138 million stars, 18% more than the previous catalog, with lower density regions gaining as much as 40% more stars. The new catalog produces nearly seamless population maps that show relatively well-mixed distributions for populations associated with ages older than 1–2 Gyr and highly structured distributions for the younger populations.
Atmospheric Reconnaissance of TRAPPIST-1 b with JWST/NIRISS: Evidence for Strong Stellar Contamination in the Transmission Spectra
Authors: Lim Olivia , Benneke Björn , Doyon René , MacDonald Ryan J. , Piaulet Caroline , Artigau Étienne , Coulombe Louis-Philippe , Radica Michael , L’Heureux Alexandrine , Albert Loïc , Rackham Benjamin V. , de Wit Julien , Salhi Salma , Roy Pierre-Alexis , Flagg Laura , Fournier-Tondreau Marylou , Taylor Jake , Cook Neil J. , Lafrenière David , Cowan Nicolas B. , Kaltenegger Lisa , Rowe Jason F. , Espinoza Néstor , Dang Lisa , Darveau-Bernier Antoine 
Published: September 2023

Abstract
TRAPPIST-1 is a nearby system of seven Earth-sized, temperate, rocky exoplanets transiting a Jupiter-sized M8.5V star, ideally suited for in-depth atmospheric studies. Each TRAPPIST-1 planet has been observed in transmission both from space and from the ground, confidently rejecting cloud-free, hydrogen-rich atmospheres. Secondary eclipse observations of TRAPPIST-1 b with JWST/MIRI are consistent with little to no atmosphere given the lack of heat redistribution. Here we present the first transmission spectra of TRAPPIST-1 b obtained with JWST/NIRISS over two visits. The two transmission spectra show moderate to strong evidence of contamination from unocculted stellar heterogeneities, which dominates the signal in both visits. The transmission spectrum of the first visit is consistent with unocculted starspots and the second visit exhibits signatures of unocculted faculae. Fitting the stellar contamination and planetary atmosphere either sequentially or simultaneously, we confirm the absence of cloud-free, hydrogen-rich atmospheres, but cannot assess the presence of secondary atmospheres. We find that the uncertainties associated with the lack of stellar model fidelity are one order of magnitude above the observation precision of 89 ppm (combining the two visits). Without affecting the conclusion regarding the atmosphere of TRAPPIST-1 b, this highlights an important caveat for future explorations, which calls for additional observations to characterize stellar heterogeneities empirically and/or theoretical works to improve model fidelity for such cool stars. This need is all the more justified as stellar contamination can affect the search for atmospheres around the outer, cooler TRAPPIST-1 planets for which transmission spectroscopy is currently the most efficient technique.
Libration- and Precession-driven Dissipation in the Fluid Cores of the TRAPPIST-1 Planets
Authors: Bansal Dhananjhay , Christie Hannah S. , Dumberry Mathieu 
Published: September 2023

Abstract
The seven planets orbiting TRAPPIST-1 have sizes and masses similar to Earth and mean densities that suggest that their interior structures are comprised of a fluid iron core and rocky mantle. Here we use idealized analytical models to compute estimates of the viscous dissipation in the fluid cores of the TRAPPIST-1 planets induced by mantle libration and precession. The dissipation induced by the libration at orbital periods is largest for TRAPPIST-1b, of the order of 600 MW, and decreases with orbital distance, to values of 5–500 W for TRAPPIST-1h, depending on its triaxial shape. Extrapolating these results to the larger libration amplitudes expected at longer periods, dissipation may perhaps be as high as 1 TW in TRAPPIST-1b. Orbital precession induces a misalignment between the spin axes of the fluid core and mantle of a planet, the amplitude of which depends on the resonant amplification of its free precession and free core nutation. Assuming Cassini states, we show that the dissipation from this misalignment can reach a few TW for planets e and f. Our dissipation estimates are lower bounds, as we neglect ohmic dissipation, which may dominate if the fluid cores of the TRAPPIST-1 planets sustain magnetic fields. Our results suggest that dissipation induced by precession can be of the same order as tidal dissipation for the outermost planets, may perhaps be sufficient to supply the power to a generate a magnetic field in their liquid cores, and likely played an important role in the evolution of the TRAPPIST-1 system.
Penser la plateforme Uber au prisme de l’épistémologie de la communication organisationnelle
Authors: Parrini-Alemanno Sylvie , El Bourkadi Salma 
Published: September 2023

Nous considérons les plateformes numériques marchandes comme de nouvelles formes organisationnelles, marquées par un organizing managérial et caractérisées par une forte dimension matérielle (par opposition à humaine). Nous observerons les processus info-communicationnels qui régissent la plateforme du transport de personnes VTC (véhicule de transport avec chauffeur) Uber et sa nature sociotechnique, les incidences sur les acteurs humains qui y participent, ses modalités spécifiques de médiation à partir de l’éclairage de deux approches de la communication dite organisationnelle : la Communication Constitutive des Organisations (CCO) et les Approches Communicationnelles des Organisations (ACO). Des entretiens semi-directifs de type récit de vie montrent une hyper-rationalisation par des procès informationnels organisants.
Des sœurs dans la guerre. Poursuivre les activités de soins en Indochine française (1939-1946)
Authors: de Rugy Marie 
Published: September 2023

Si l’historiographie consacrée à la Seconde Guerre mondiale en Indochine est désormais riche, elle n’aborde pas la place des congrégations féminines missionnaires, leur expérience de la guerre et les recompositions de leurs activités durant la période. C’est pour commencer à combler ce manque que cet article, fondé essentiellement sur les archives des Franciscaines Missionnaires de Marie et des Filles de la Charité, se concentre sur les activités de soins des sœurs. Trois périodes apparaissent : jusqu’à l’invasion japonaise du 9 mars 1945, les continuités coloniales l’emportent, alors que la Révolution nationale est appliquée en Indochine ; l’occupation japonaise accroît les pénuries et la nécessité d’y faire face mais, par le statut spécial qui leur est accordé, les sœurs sont moins touchées que la population européenne. C’est surtout la prise du pouvoir du Viêt Minh, après la révolution d’août 1945, qui entraîne les recompositions les plus importantes.
Le secteur spatial européen pris dans une tenaille stratégique
Authors: Wohrer Paul 
Published: September 2023

Le secteur spatial européen traverse une période difficile, marquée par la perte temporaire de ses capacités autonomes d’accès à l’espace, par la forte concurrence américaine et par la transformation du marché des satellites. L’Union européenne est aussi en retard dans le domaine numérique et la valorisation des données spatiales lui échappe largement. Dans ce contexte tendu, où les États-Unis et la Chine investissent massivement, un réveil européen est nécessaire – au risque d’un abandon de souveraineté.
Pacifique Sud : les Îles Salomon entre Pékin et Washington
Authors: Perrot Sophie , Cadenza Academic translations  
Published: September 2023

Alors que les tensions entre les États-Unis et la Chine s’intensifient, les États de la région indopacifique subissent des pressions croissantes pour choisir leur camp. Les États insulaires du Pacifique Sud s’imposent comme une nouvelle arène de confrontation. Un cas exemplaire à cet égard est celui des Îles Salomon, traditionnellement alliées à l’Australie et aux États-Unis, qui ont fait la une de l’actualité internationale en 2022 après avoir signé un pacte de sécurité avec la Chine.
Feasibility of Nurse-led Development of Custom Virtual Reality Experiences for Health Care Interventions
Authors: Sauers Brody , Dyal Brenda W. , Johnson-Mallard Versie , Ezenwa Miriam O. , Halan Shiva , Fillingim Roger B. , Kalyanaraman Sriram , Wilkie Diana J. 
Published: September 2023

Background:
The immersive and interactive nature of virtual reality (VR) renders it a potential pedagogical approach for nursing education. A bottleneck for exploiting VR advantages has been the complexity of creating new experiences; however, recent advances with VR hardware and software enable novice users to create compelling experiences.

Method:
A case study describes an undergraduate nursing student with minimal technical skills using off-the-shelf VR software to create a pain management VR experience.

Results:
Using off-the-shelf hardware and software platforms eliminates the need to work with computer code. The team created a virtual environment and the objects in it through easy manipulation with click-and-drag techniques and by toggling simple settings.

Conclusion:

The insights gained from this case suggest nurse educators can create simple yet powerful VR experiences themselves, which can greatly enhance existing tools for nursing education.

[
J Nurs Educ
. 2024;63(4):261–264.]
Use of Simulation to Integrate Behavioral Health Into Primary Care Nurse Practitioner Programs
Authors: Strauch Kimberly A. , Renz Susan M. , DeMutis Kathleen O. , Sochalski Julie 
Published: September 2023

Background:
Identifying and treating acute and chronic behavioral health conditions is integral to primary care practice, yet primary care nurse practitioner (NP) training models do not meet the demand for integrated behavioral health practices. Simulation offers an effective pedagogical tool for integrating behavioral health training in primary care.

Method:
With support from federal funding and external consultants, new didactic and complementary simulation curricula in integrated behavioral health care were introduced in the primary care and psychiatric mental health NP programs at a school of nursing. Two rounds of this curricular innovation were implemented and evaluated across specialties.

Results:
Ninety-seven students participated in the training and reported enhanced behavioral-health assessment and hand-off skills, greater confidence in applying core content, and improved communication skills.

Conclusion:

Thoughtfully designed simulation offers an important tool for developing integrated behavioral health competencies that will help prepare future primary care clinicians meet the needs of patients and communities.

[
J Nurs Educ
. 2024;63(2):128–133.]
Subcutaneous Bacillus Calmette–Guérin Administration Induces Innate Training in Monocytes in Preweaned Holstein Calves
Authors: Samuel Beulah E R , Maina Teresia W , McGill Jodi L 
Published: September 2023

Abstract
The bacillus Calmette–Guérin (BCG) vaccine, administered to prevent tuberculosis, is a well-studied inducer of trained immunity in human and mouse monocytes. We have previously demonstrated that aerosol BCG administration induces innate training in calves. The current study aimed to determine whether s.c. BCG administration could induce innate training, identify the cell type involved, and determine whether innate training promoted resistance to bovine respiratory syncytial virus (BRSV) infection, a major cause of bovine respiratory disease in preweaned calves. A total of 24 calves were enrolled at 1–3 d of age and blocked by age into two treatment groups (BCG, n = 12; control, n = 12). BCG was given s.c. to preweaned calves. The control calves received PBS. We observed a trained phenotype, demonstrated by enhanced cytokine production in response to in vitro stimulation with LPS (TLR-4 agonist) in PBMCs and CD14+ monocytes from the BCG group 2 wk (IL-1β, p = 0.002) and 4 wk (IL-1β, p = 0.005; IL-6, p = 0.013) after BCG administration, respectively. Calves were experimentally infected via aerosol inoculation with BRSV strain 375 at 5 wk after BCG administration and necropsied on day 8 postinfection. There were no differences in disease manifestation between the treatment groups. Restimulation of bronchoalveolar lavage fluid cells isolated on day 8 after BRSV infection revealed enhanced IL-1β (p = 0.014) and IL-6 (p = 0.010) production by the BCG group compared with controls. In conclusion, results from our study show that s.c. administration of the BCG vaccine can induce trained immunity in bovine monocytes and influence cytokine production in the lung environment after BRSV infection.