bluuebunny/crossref_metadata_2025_split huggingface dataset:
Hubungan Pemberdayaan Suami dan Keluarga dengan Kepatuhan Melaksanakan ANC Pada Ibu Hamil di Puskesmas Pasar Rebo
Authors: Utami Febi Puji , Chadaryanti Diyah 
Published: January 2025

Background : Pregnancy is a very meaningful experience for women. Examination and supervision of pregnant women really needs to be carried out regularly. This aims to prepare the mother and child as optimally as possible physically and mentally during pregnancy, childbirth and postpartum so that a healthy mother and child are obtained. For pregnant women who have never been pregnant or given birth before (primigravida), pregnancy or childbirth is something foreign to them. This is because it is something new he has experienced. Family support, especially husbands, greatly influences antenatal care (ANC) visits for primigravida mothers. Family support is able to motivate primigravida mothers to visit antenatal care. Antenatal care is a pregnancy examination carried out on pregnant women during their pregnancy to prevent complications during pregnancy and to prepare for a healthy birth.Objective : This study aims to determine whether there is a relationship between husband and family empowerment and compliance with antenatal care (ANC) for pregnant women in the Pasar Rebo Health Center working area.Methods: This research used an analytical research design with a cross sectional approach which was carried out at the Air Salobar Community Health Center with a sample size of Â 32 respondents. Data collection was carried out using questionnaires and observation sheets. From the Chi Square statistical test.Results: The results of this study indicate that there is a significant relationship between husband's support and compliance with ANC visits (p = 0.003).Conclusions and suggestions: The conclusion of this research is that there is a significant relationship between family support and compliance with ANC visits for pregnant women at the Pasar Rebo Health Center. This research is expected to provide information and understanding to pregnant women, husbands and community health center midwives about the relationship between family support and compliance with antenatal care (ANC) in pregnant women.Recommendation: In further research, it is hoped that research can be developed even betterÂ Keywords: Â Family Support, Compliance in Antenatal Care Visit
The English Competencies of Tourism High School Students
Authors: Nurika Intan Fajrian , Engelbrecht Natasha , Zemieche Amina 
Published: January 2025

Purpose of the study: This study was designed to investigate what are the competencies of tourism high school students in DKI Jakarta.
Methodology: There were 420 students of 21 tourism high schools in DKI Jakarta that participated in this study. Theoretical (study of theoretical literature and sources) and empirical methods of the research data obtaining methods (students and teachers’ interviews, teachers and students questionnaire, and unstructured observation) and also both qualitative and quantitative data processing method were used in this study.
Main Findings: The result showed that the most needed skill to work in tourism industries is speaking skill. Students were expected to have good oral communication since it was useful when they had a job training program in real industry. They need more vocabularies which are in tourism terminology. However, the result of teachers’ instruments indicated more than 75% English teachers focus on national examination which is mean that students learned more in reading rather than speaking. Teachers also followed a curriculum which is provided for all major of vocational high school. The curriculum compilers were not develop curriculum for each major. It means that the curriculum itself was in general ideas. The teachers should select and develop the appropriate materials for students’ major.
Novelty/Originality of this study: It can be concluded that the tourism high school students need good oral communication by improving speaking and also listening skill to achieve both learning objective stated in Regulation Number 22 year 2006 and industry needs.
Diffuse Ionized Gas in the Anticenter of the Milky Way
Authors: Wen Shiming , Zhang Wei , Ma Lin , Zhao Yunning , Lam Man I. , Wu Chaojian , Ren Juanjuan , Chen Jianjun , Wu Yuzhong , Hu Guozhen , Hou Yonghui , Zhao Yongheng , Wu Hong 
Published: January 2025

Abstract
Using data from the Large Area Multi-Object fiber Spectroscopic Telescope Medium-Resolution Spectroscopic Survey of Nebulae, we create a sample of 17,821 diffuse ionized gas spectra in the anticenter region of the Milky Way by excluding fibers in the directions of H ii regions and supernova remnants. We then analyze the radial and vertical distributions of three line ratios ([N ii]/Hα, [S ii]/Hα, and [S ii]/[N ii]), as well as the oxygen abundance. [N ii]/Hα and [S ii]/Hα do not exhibit a consistent, monotonic decrease with increasing Galactocentric distance (R
gal). Instead, they show enhancement within the interarm region, positioned between the Local Arm and the Perseus Arm. [S ii]/[N ii] has a radial gradient of 0.1415 ± 0.0646 kpc−1 for the inner disk (8.34 < R
gal < 9.65 kpc) and remains nearly flat for the outer disk (R
gal > 9.65 kpc). In the vertical direction, [N ii]/Hα, [S ii]/Hα, and [S ii]/[N ii] increase with increasing Galactic disk height (∣z∣) in both southern and northern disks. Based on the N2S2Hα method, which combines [S ii]/[N ii] and [N ii]/Hα, we estimate the oxygen abundance. The oxygen abundance exhibits a consistent radial gradient with R
gal, featuring a slope of −0.0559 ± 0.0209 dex kpc−1 for the inner disk and a similar slope of −0.0429 ± 0.0599 dex kpc−1 for the outer disk. A single linear fitting to the entire disk yields a slope of −0.0317 ± 0.0124 dex kpc−1. In the vertical direction, the oxygen abundance decreases with increasing ∣z∣ in both southern and northern disks.
True Mass and Atmospheric Composition of the Nontransiting Hot Jupiter HD 143105 b
Authors: Finnerty Luke , Xin Yinzi , Xuan Jerry W. , Inglis Julie , Fitzgerald Michael P. , Agrawal Shubh , Baker Ashley , Bartos Randall , Blake Geoffrey A. , Calvin Benjamin , Cetre Sylvain , Delorme Jacques-Robert , Doppmann Greg , Echeverri Daniel , Horstman Katelyn , Hsu Chih-Chun , Jovanovic Nemanja , Liberman Joshua , López Ronald A. , Martin Emily C. , Mawet Dimitri , Morris Evan , Pezzato-Rovner Jacklyn , Ruffio Jean-Baptiste , Sappey Ben , Schofield Tobias , Skemer Andrew , Venenciano Taylor , Wallace J. Kent , Wallack Nicole L. , Wang 王 Jason J. 劲飞 , Wang 王 Ji 吉 
Published: January 2025

Abstract
We present Keck/KPIC Phase II K-band observations of the nontransiting hot Jupiter HD 143105 b. Using a cross-correlation approach, we make the first detection of the planetary atmosphere at

K
p

=
18

5

−
13

+
11

km s−1 and an inferior conjunction time 2.5 hr before the previously published ephemeris. The retrieved K
p value, in combination with the orbital period, mass of the host star, and lack of transit detection, give an orbital inclination of

7

8

−
12

∘
+
2

and a true planet mass of 1.23 ± 0.10 M
J. While the equilibrium temperature of HD 143105 b is in the transition regime between noninverted and inverted atmospheres, our analysis strongly prefers a noninverted atmosphere. Retrieval analysis indicates the atmosphere of HD 143105 b is cloud free to approximately 1 bar and dominated by H2O absorption (

logH
2

O
MMR

=
−
3
.

9

−
0.5

+
0.8

), placing only an upper limit on the CO abundance (

logCO
MMR

<
−
3.7

at 95% confidence). We place no constraints on the abundances of Fe, Mg, or 13CO. From these abundances, we place an upper limit on the carbon-to-oxygen ratio for HD 143105 b, C/O < 0.2 at 95% confidence, and find the atmospheric metallicity is approximately 0.1 × solar. The low metallicity may be responsible for the lack of a thermal inversion, which at the temperature of HD 143105 b would likely require significant opacity from TiO and/or VO. With these results, HD 143105 b joins the small number of nontransiting hot Jupiters with detected atmospheres.
COOL-LAMPS. VII. Quantifying Strong-lens Scaling Relations with 177 Cluster-scale Strong Gravitational Lenses in DECaLS
Authors: Mork Simon D. , Gladders Michael D. , Khullar Gourav , Sharon Keren , Chicoine Nathalie , Cloonan Aidan P. , Dahle Håkon , Garza Diego , Glusman Rowen , Gozman Katya , Horwath Gabriela , Levine Benjamin C. , Liang Olina , Mahronic Daniel , Manwadkar Viraj , Martinez Michael N. , Masegian Alexandra , Matthews Acuña Owen S. , Merz Kaiya , Pan Yue , Sanchez Jorge A. , Sierra Isaac , Kavin Stein Daniel J. , Sukay Ezra , Tamargo-Arizmendi Marcos , Tavangar Kiyan , Tu Ruoyang , Wagner Grace , Zaborowski Erik A. , Zhang Yunchong ,   (COOL-LAMPS Collaboration)
Published: January 2025

Abstract
We estimate the Einstein-radius-enclosed total mass for 177 cluster-scale strong gravitational lenses identified by the ChicagO Optically selected Lenses Located At the Margins of Public Surveys (COOL-LAMPS) collaboration with lens redshifts ranging from 0.2 ⪅ z ⪅ 1.0 using the brightest-cluster-galaxy (BCG) redshift and an observable proxy for the Einstein radius. We constrain the Einstein-radius-enclosed luminosity and stellar mass by fitting parametric spectral energy distributions to aperture photometry from the Dark Energy Camera Legacy Survey (DECaLS) in the g-, r-, and z-band Dark Energy Camera filters. We find that the BCG redshift, enclosed total mass, and enclosed luminosity are strongly correlated and well described by a planar relationship in 3D space. We find that the enclosed total mass and stellar mass are correlated with a logarithmic slope of

0.50

0

−
0.031

+
0.029

, and the enclosed total mass and stellar-to-total mass fraction are correlated with a logarithmic slope of

−
0.49

5

−
0.033

+
0.032

. In tandem with the small radii within which these slopes are constrained, this may suggest invariance in baryon conversion efficiency and feedback strength as a function of cluster-centric radii in galaxy clusters. Additionally, the correlations described here should have utility in ranking strong-lensing candidates in upcoming imaging surveys—such as Rubin/Legacy Survey of Space and Time—in which an algorithmic treatment of strong lenses will be needed due to the sheer volume of data these surveys will produce.
Discrepancies between JWST Observations and Simulations of Quenched Massive Galaxies at z > 3: A Comparative Study with IllustrisTNG and ASTRID
Authors: Weller Emma Jane , Pacucci Fabio , Ni Yueying , Hernquist Lars , Park Minjung 
Published: January 2025

Abstract
Recent JWST observations have uncovered an unexpectedly large population of massive quiescent galaxies at z > 3. Using the cosmological simulations IllustrisTNG and ASTRID, we identify analogous galaxies and investigate their abundance, formation, quenching mechanisms, and post-quenching evolution for stellar masses

9.5
<

log
10

(

M
⋆

/

M
⊙

)
<
12

. We apply three different quenching definitions and find that both simulations significantly underestimate the comoving number density of quenched massive galaxies at z ≳ 3 compared to JWST observations by up to ∼2 dex. In both simulations, the high-z quenched massive galaxies often host overmassive central black holes above the local M
BH–M
⋆ relation, implying that AGN feedback is key in quenching galaxies in the early Universe. The typical quenching timescales for these galaxies are ∼200–600 Myr. IllustrisTNG primarily employs AGN kinetic feedback, while ASTRID relies on AGN thermal feedback at z > 2.3, which is less effective and has a longer quenching timescale. Although these simulations differ in many aspects, making a direct comparison challenging, our findings suggest the need for improved physical models of AGN feedback in galaxy formation simulations. At lower stellar masses, the quenched galaxies have denser local environments than the star-forming galaxies, suggesting that environmental quenching helps quench less-massive galaxies. We also study the post-quenching evolution of the high-z massive quiescent galaxies and find that many experience subsequent reactivation of star formation, evolving into primary progenitors of z = 0 brightest cluster galaxies.
Electron Acceleration by Multiple Fast Fermi Reflections at Earth’s Bow Shock
Authors: Liu Y. Y. , Cao J. B. , Liu C. M. , Song Y. T. , Hu D. K. 
Published: January 2025

Abstract
The generation of energetic particles in the Universe is an important topic in astrophysical and space physics. Although the diffusive shock acceleration has been acknowledged to play an essential role in particle acceleration, the injection problem has not been well resolved yet. Using measurements from the Magnetospheric Multiscale spacecraft, we report unexpected spiky enhancements of energetic electron flux in the upstream region of the Earth’s bow shock. Such enhancements are then demonstrated to result from the accelerated electron population by shock reflection. Meanwhile, the magnetic field exhibits no variations except an increase in radius of curvature. Based on the results above, we uncover the underlying acceleration scenario. When the interplanetary magnetic field with a proper curvature approaches the bow shock, the two ends of a magnetic field line may touch the shock front earlier than its middle part. Magnetic mirror points form at the two field-line-shock intersections. The solar wind electrons are therefore trapped and bounce between two mirror points. Eventually, these electrons undergo fast Fermi reflection several times and gain substantial energies. The spacecraft observation of accelerated electrons is reproduced with a numerical method based on the reflection model. Such an acceleration process may be a potential solution to the injection problem.
Hot Jupiters Are Asynchronous Rotators
Authors: Wazny Marek , Menou Kristen 
Published: January 2025

Abstract
Hot Jupiters are typically assumed to be synchronously rotating, from tidal locking. Their thermally driven atmospheric winds experience Lorentz drag on the planetary magnetic field anchored at depth. We find that the magnetic torque does not integrate to zero over the entire atmosphere. The resulting angular momentum feedback on the bulk interior can thus drive the planet away from synchronous rotation. Using a toy tidal–ohmic model and atmospheric general circulation model outputs for HD189733b, HD209458b, and Kepler7b, we establish that off-synchronous rotation can be substantial at tidal–ohmic equilibrium for sufficiently hot and/or magnetized hot Jupiters. Potential consequences of asynchronous rotation for hot Jupiter phenomenology motivate follow-up work on the tidal–ohmic scenario with approaches that go beyond our toy model.
IgG-Mediated Food Intolerance in a Patient with Allergic Symptoms, Acne and Obesity - Effect of Elimination Diet
Authors: Andjelković Marija , Vojvodić Aleksandra , Dikić Nenad 
Published: January 2025

BACKGROUND: Although the association of food-specific IgG with the development and progression of specific diseases has been shown by many studies, strong correlations are still under question. Are these antibodies a normal immune response to foods, or is the pathogenetic mechanism triggered in another way? Why do elimination diets improve, in many studies, different diseases at different ages?
CASE PRESENTATION: We will present the case of a patient who experienced significant improvement in allergic symptoms and reduced body weight by implementing an elimination diet. Type III hypersensitivity reactions are associated with IgG antibodies. They are considered to be normal reactions to food antigens. They are absorbed into the bloodstream in small amounts. However, immediately after a meal, antibodies and food antigen complexes bound to specific IgG circulate in the serum, rapidly cleared by a healthy immune system, specifically the reticuloendothelial system. If large amounts of antibodies are produced and immune complexes are deposited in the blood vessels of various organs and organ systems, various manifestations may occur.
CONCLUSION: This is a new field of medicine. Further research, better-standardized tests, and much more extensive studies are needed to prove how to utilize the IgG antibody-based elimination diet properly.
Sobre la presencia de Oxybasis rubra (Amaranthaceae) en Cerdeña, con notas sobre Chenopodium blitoides y C. humile
Authors: Iamonico Duilio , Mereu Giuliano 
Published: January 2025

Como parte de los estudios en curso del género Chenopodium s. l., se descubrieron 20 poblaciones de Oxybasis rubra var. rubra en Cerdeña, representando una confirmación de este taxon para la flora de la isla. De hecho, según la literatura, O. rubra fue indicada de manera diferente en Cerdeña a lo largo del tiempo como presente, dudosa o ausente. Se dan caracteres morfológicos, así como datos ecológicos y corológicos. Se proporcionan notas nomenclaturales sobre los nombres C. blitoides and C. humile, y se proponen neotipificaciones utilizando especímenes conservados, respectivamente, en los herbarios BR y K.
Navigating Noise: A Stratified Model for Scholarly Digital Editions of Arabic Manuscripts in Hebrew Script
Authors: Lanza Valentina B. 
Published: January 2025

Cet article examine le rôle des éditions numériques savantes dans le développement de la recherche textuelle, en se focalisant sur le judéo-arabe, une variété linguistique unique utilisant l’alphabet hébreu pour représenter l’arabe. Nous proposons un modèle stratifié pour les éditions numériques savantes, visant à gérer les complexités orthographiques du judéo-arabe, notamment la transcription, la conversion de l’écriture, la normalisation et l’intégration des métadonnées. L’étude souligne l’importance cruciale de la gestion du « bruit » dans l’édition des textes, particulièrement lors de l’acquisition des données, où toute distorsion ou omission d’éléments orthographiques peut compromettre l’intégrité scientifique. Une étude de cas portant sur un manuscrit médiéval en judéo-arabe illustre l’application de ce modèle, en montrant comment il préserve l’intégrité textuelle tout en enrichissant l’analyse scientifique. Cette méthodologie aborde non seulement les défis spécifiques au judéo-arabe, mais elle est également adaptable à d’autres systèmes allographiques.
Transcription automatique des interactions verbales. Limites observées et perspectives envisagées à partir d’un corpus de consultations médicales
Authors: Bertin Thomas , Quellec Gwenolé 
Published: January 2025

Les applications de transcription automatique de l’audio vers un texte écrit (par ex. Whisper) ont fait de fulgurants progrès ces dernières années. Cependant, généralement destinées à produire des textes conformes aux normes de l’écrit, elles tendent à gommer toute marque de l’oralité (ex. : répétitions, pauses dans le flot de paroles, phatiques comme euh…). Ainsi, même si elles laissent envisager des bénéfices importants en temps de travail comme en fidélité de transcription, elles restent globalement inadaptées pour les chercheurs analysant des interactions verbales. À partir d’un échantillon de transcriptions de consultations pré-opératoires en vue d’une intervention de neurochirurgie en conditions éveillées (recherche en cours), l’étude se donne trois objectifs : (i) recenser les difficultés que pose une application comme Whisper du point de vue d’un interactionniste de la parole ; (ii) expliciter l’origine de ces difficultés ; (iii) proposer des pistes pour les surmonter.
Quelle solution pour améliorer les performances de la reconnaissance d’entités nommées sur des données bruitées, corriger l’entrée ou filtrer la sortie ?
Authors: Petkovic Ljudmila , Koudoro-Parfait Caroline , Desmarest Marie-Sophie , Lejeune Gaël 
Published: January 2025

Cet article présente les résultats d’un travail de recherche qui vise à déterminer si la correction de l’OCR, en amont, permet d’améliorer significativement les résultats de la tâche de la Reconnaissance d’Entités Nommées (REN). Les expériences ont été appliquées aux corpus ELTeC et Très Grande Bibliothèque (TGB). Notre objectif est d’établir (i) une typologie des contaminations d’OCR issues des outils Kraken et Tesseract et (ii) une typologie des erreurs de la correction automatique produite par l’outil JamSpell. Dans le cadre de notre évaluation, nous étudions les intersections entre les EN détectées par l’outil spaCy dans les textes de référence et les deux versions d’OCR d’une part, et d’autre part la mesure cosinus utilisée pour calculer la distance textuelle entre ces versions. Nos résultats montrent que la correction automatique introduit des biais dans les données textuelles et que le filtrage des entités en sortie semble être une piste plus prometteuse. Enfin, nous constatons que les EN incorrectes sont massivement des entités courtes et hapax en corpus, ainsi que la longueur des entités et la fréquence documentaire sont les critères discriminatoires pour exclure des EN candidates avec une précision de plus de 98 %.
Élaboration de corpus pour l’enseignement de la grammaire : le corpus du jeu PP L’archer de Alloprof
Authors: Gauvin Isabelle , Leblanc Samuel , Martineau Marion Deslandes , Tanguay Marc-Antoine 
Published: January 2025

Les corpus en didactique de la grammaire sont peu étudiés, alors qu’ils apparaissent centraux pour soutenir l’enseignement et, surtout, l’apprentissage de notions grammaticales. Après avoir clarifié leur rôle dans l’enseignement et dégagé les caractéristiques d’un corpus bien construit, nous analysons le corpus du populaire jeu numérique PP L’archer de la plateforme Alloprof. Nous constatons qu’il comporte un nombre limité de phrases et qu’elles manquent de diversité dans leur construction. Nous discutons de la pertinence de nos constats pour l’amélioration de la version du jeu en ligne et, plus largement, pour l’amélioration des corpus grammaticaux présentés aux élèves.
Three brothers in biology: bugs, birds, books, conservation, and politics
Authors: Cannings Robert A. , Cannings Sydney G. , Cannings Richard J. 
Published: January 2025

Abstract
Three Cannings brothers describe their intertwined but separate careers in Canadian biology: Rob as an entomologist, Syd as an entomologist and conservation biologist, and Dick as an ornithologist and politician. They emphasise the influence on their lives of the British Columbia’s Okanagan Valley where they grew up, the naturalist family in which they were raised, and the mentors who inspired them in their work. Bird study and nature interpretation in BC Parks were early enthusiasms and influences. Biological research, museum work, nature conservation, public education, and writing have dominated their careers. In Dick’s case, his public life has culminated in a decade of Canadian federal politics as a member of Parliament.

This article is modified from the closing plenary address presented at Entomology 2022, the joint annual meeting of the Entomological Society of America, the Entomological Society of Canada, and the Entomological Society of British Columbia, in Vancouver, British Columbia, Canada, 16 November 2022. The presentation also acted as the 2022 Heritage Lecture of the Entomological Society of Canada.