bluuebunny/crossref_metadata_2025_split huggingface dataset:
Pengaruh Budget Participation, Asimetri Informasi Dan Budget Emphasis Terhadap Budget Slack Pada PT Wijaya Karya (Persero) Tbk
Authors: Alifah Andi Audy Noor , Sadikin Dikdik Saleh , Budhijana R. Bambang 
Published: February 2025

This research aims to determine the influence of Budget Participation, Information Asymmetry and budget emphasis on budget slack at PT. Wijaya Karya (Persero) Tbk. The independent variables in this research are Budget Participation, Information Asymmetry and budget emphasis. Meanwhile, the dependent variable is budget slack. The analysis technique for this research uses the PLS or Partial Least Square SmartPLS 4 method. The data collection technique uses a Google Form questionnaire to collect the required information. The results of the number of respondents were 73 employees of PT. Wijaya Karya (Persero) Tbk. The results of the analysis show that Budget Participation has a positive effect on budget slack, information asymmetry has no effect on budget slack, Budget emphasis has no effect on budget slack..
Transfer-printed nanophotonic waveguide on an erbium doped crystal towards hybrid photonic quantum devices
Authors: Okajima Taiyu , Ohta Ryuichi , Sato Takumi , Tachizaki Yuma , Xu xuejun , Okamoto Hajime , OTA Yasutomo 
Published: February 2025

Abstract
We report the design, fabrication and optical characterization of silicon nanophotonic waveguides on an erbium doped crystal. The silicon waveguide allows for efficient optical addressing of erbium ions embedded near the crystal surface. We employed the transfer printing method to assemble the heterogeneous photonic structure in a simple pick-and-place manner. We observed coupling of the emission from erbium ions into the waveguide in the telecommunication wavelength band. The developed methodology opens the way to functional hybrid quantum devices mediating between photons, electrons and phonons.
TRANSFORMATION OF ANIMATION CHARACTERS INTO THE GAMING WORLD
Authors: Nuswantoro Fajar 
Published: February 2025

In the gaming industry, the main challenge faced is the complexity of combining information technology science and film-animation art. These technical and artistic gaps often slow down the production process and reduce the amount of output that can be achieved. This research aims to identify simpler and cheaper alternative production methods to increase the quantity of game production without sacrificing quality.

To achieve this goal, a series of hands-on game creation experiments were carried out by researcher. This method is expected to provide an idea of game engine easiness and how helpful a community when the researcher encounter difficulties in making games.

The results of this research show that the use of Godot in game production has a significant impact on production efficiency. This more efficient process has the potential to increase the amount of game production in Indonesia, providing opportunities for the local games industry to develop and compete in the global market. Thus, this research not only contributes to academic knowledge, but also has significant practical implications for the gaming industry. This discovery is expected to encourage more innovation and aesthetics in the application of artificial intelligence in various aspects of game production.

Keywords: efficiency, games, media transfer, godot, animation
Epidermólise Bolhosa: Manejo das Coberturas
Authors: Rodrigues Simone Alves , Silva Ferreira Brisa Emanuelle , Silva Elisa Lima e , Gandra Elen Cristina , Araújo Claudirene Milagres , Neves Társila Lamounier 
Published: February 2025

A Epidermólise Bolhosa é uma doença rara, não contagiosa e sem cura, hereditária causada por mutações em várias proteínas estruturais da pele, de diferentes intensidades que podem dar origem a flictenas em todo o corpo, cuja gravidade dependerá da mutação envolvida na patogenia. Engloba quatro tipos principais: simples, juncional, distrófica e kindler. Este artigo teve por objetivo avaliar o manejo adequado, relacionado ao uso das coberturas nos indivíduos portadores da doença. Para isso, foi realizada uma revisão de toda literatura específica encontrada sobre o tema. Foram consultadas as bases eletrônicas scielo, bireme e Google Academic no período de março e abril de 2021; além de fontes primárias como livros. O material foi selecionado de acordo com as palavras chaves: Epidermólise Bolhosa, causas, tratamento, utilização de coberturas; datados de 2010 a 2021. Os resultados encontrados demostram que, o cuidado dirigido aos pacientes com a doença, independentemente do tipo, é inespecífico, sendo considerado de grande importância o manejo adequado com as lesões cutâneas de acordo com as características. É recomendada uma avaliação rigorosa da equipe multidisciplinar, para analisar o envolvimento cutâneo e extracutâneo, evitando complicações como por exemplo as infecções, garantindo uma melhor qualidade de vida. Conclui-se que o tratamento da Epidermólise Bolhosa deve ter como foco a prevenção das complicações, utilizando coberturas apropriadas para cada evolução das lesões, envolvendo também o atendimento psicológico do paciente e família, para um melhor entendimento da doença resultado assim em um melhor cuidado.
Analysis of the Gap Between the Polri Almatsus Blueprint and Operational Needs in the Meta-Globalization Era
Authors: Prabowo Dikie , Nita Surya , Gani Yopik 
Published: February 2025

This creates new challenges for security institutions, including the Indonesian National Police (Polri), which are required to adjust their strategies, tactics, and special equipment (Almatsus) to address various threats and operational demands in this highly dynamic era. This study aims to analyze the factors causing the gap between the planning of special equipment (Almatsus) by Polri and the needs in the field in facing global challenges, as well as to analyze the impact of the gap between the Almatsus Blueprint and the reality of operational needs on the effectiveness of Polri's performance in maintaining security and order in the era of meta-globalization. This research employs a qualitative research method, using strategic management theory as the analytical lens. The findings reveal that the gap between the planning and needs of Polri’s special equipment (Almatsus) is caused by external factors, such as technological advancements and the dynamics of modern crime, as well as internal factors, including a lack of coordination, limited human resources, and inflexible planning. This results in a mismatch between what is planned and operational realities, negatively impacting Polri's effectiveness in maintaining security, especially in the era of meta-globalization. This gap can decrease operational effectiveness, personnel morale, and institutional image, as well as result in material losses due to inappropriate procurement.
Minute-cadence Observations of the LAMOST Fields with the TMTS. VI. Physical Parameters of Contact Binaries
Authors: Xia Qiqi , Wang Xiaofeng , Li Kai , Gao Xiang , Guo Fangzhou , Lin Jie , Liu Cheng , Mo Jun , Peng Haowei , Liu Qichun , Xi Gaobo , Yan Shengyu , Jiang Xiaojun , Zhang Jicheng , Song Cui-Ying , Shi Jianrong , Ma Xiaoran , Xiang Danfeng , Li Wenxiong 
Published: February 2025

Abstract
With the development of wide-field surveys, a large amount of data on short-period W UMa contact binaries have been obtained. Continuous and uninterrupted light curves as well as high-resolution spectroscopic data are crucial in determining the absolute physical parameters. Targets with both TMTS light curves and LAMOST medium-resolution spectra were selected. The absolute physical parameters were inferred with the W-D code for 10 systems, all of them are W-type shallow or medium contact binaries. The O'Connell effect observed in the light curves can be explained by adding a spot on the primary or secondary component in the models. According to O − C analysis, the orbital periods exhibit a long-term increasing or decreasing trend, among which J0132, J1300, and J1402 show periodic variations that may be attributed to the presence of a third body or magnetic activity cycles. Spectral subtraction analysis revealed that the equivalent width of Hα indicates strong magnetic activity in J0047, J0305, J0638, and J1402. Among the 10 selected binary systems, except for J0132 and J0913, the more massive components are found to be main-sequence stars while the less massive components have evolved off the main sequence. In J0132, both components are in the main sequence, whereas both components of J0913 lie above the terminal-age main sequence. Based on the relationship between orbital angular momentum and total mass for these two systems, as well as their low fill-out factors, it is possible that these two systems are newly formed contact binaries, having recently evolved from the detached configuration.
Disk in the Circumstellar Envelope of Carbon Mira V Cygni
Authors: Safonov Boris S. , Zheltoukhov Sergey G. , Tatarnikov Andrey M. , Strakhov Ivan A. , Shenavrin Victor I. 
Published: February 2025

Abstract
Asymptotic giant branch (AGB) stars are the primary source of dust and complex molecules in the interstellar medium. The determination of outflow parameters is often hindered by the unknown geometry of the circumstellar environment, creating a demand for high-angular resolution observations. We use our near-infrared spectra and photometry of the carbon AGB star V Cyg, along with literature data, to construct its spectral energy distribution over a wide range of wavelengths. The dust envelope responsible for the infrared excess was also resolved in scattered polarized light at angular scales of 50–80 mas using differential speckle polarimetry. We present an interpretation of the thermal and scattered radiation of the dust using models of a spherical dusty outflow (M
dust = 5.3 × 10−7
M
⊙) and an inclined equatorial density enhancement, either in the form of a disk (M
dust = 7.6 × 10−3
M
⊕) or a torus (M
dust = 5.7 × 10−3
M
⊕), which material is concentrated at stellocentric distances less than 25 au. The dust material consists of amorphous carbon and SiC, with 84% of the dust being amorphous carbon. Dust particle radii range from 5 to 950 nm and follow a power law with an exponent of −3.5. Modeling the envelope allowed us to improve the accuracy of stellar luminosity estimations: 21,000L
⊙ and 8300L
⊙ at maximum and minimum brightness, respectively. The relation between the disk and the high water content in the envelope is also discussed.
Solar Variability in the Mg ii h and k Lines
Authors: Sowmya K. , Snow M. , Shapiro A. I. , Krivova N. A. , Chatzistergos T. , Solanki S. K. 
Published: February 2025

Abstract
Solar irradiance and its variations in the ultraviolet (UV) control the photochemistry in Earth's atmosphere and influence Earth's climate. The variability in the Mg ii h and k core-to-wing ratio, also known as the Mg ii index, is highly correlated with the solar UV irradiance variability. Because of this, the Mg ii index is routinely used as a proxy for solar UV irradiance variability, which can help to get insights into the influence of solar UV irradiance variability on Earth's climate. Measurements of the Mg ii index, however, have only been carried out since 1978 and do not cover climate-relevant timescales longer than a few decades. Here we present a model to calculate the Mg ii index and its variability based on the well-established Spectral And Total Irradiance REconstruction (SATIRE) model. We demonstrate that our model calculations yield an excellent agreement with the observed Mg ii index variations, both on the solar activity cycle and on the solar rotation timescales. Using this model, we synthesize the Mg ii index time series on climate-relevant timescales of decades and longer. Here we present the time series of the Mg ii index spanning nearly three centuries.
The Secondary Component of the Extremely Low Mass Ratio Massive Binary HD 165246 Revealed by GHOST
Authors: Rodriguez C. N. , Ansin T. , Ferrero G. A. , Benvenuto O. G. , Gamen R. , Morrell N. I. , Arias J. I. , Higa R. E. , Putkuri C. , Johnston C. , Chiboucas K. , Deibert E. , Hayes C. R. , Heo J.-E. , Jeong M. , Kalari V. , Martioli E. , Placco V. M. , Venn K. A. , Xu S. , Diaz R. , Gomez-Jimenez M. , Ruiz-Carmona R. , Simpson C. , McConnachie A. W. , Pazder J. , Burley G. , Berg T. A. M. , Robertson J. G. , Labrie K. , Thomas-Osip J. 
Published: February 2025

Abstract
In the pursuit of understanding the multiplicity of massive stars, the OWN Survey has undertaken spectroscopic monitoring of hundreds of targets over the past 20 yr. This effort has led to the discovery of new single-lined spectroscopic binaries. Characterizing the unseen companions of these systems is crucial to deriving precise stellar parameters, including the mass of each component, and constraining formation models for massive binary systems. In this paper, we aim to physically and evolutionarily characterize the stellar components of the massive binary HD 165246. We analyzed spectra obtained by the OWN Survey and used Kepler's second mission (K2) photometry, from which we determined the physical parameters of the system. Thanks to the high-resolution capabilities of the new echelle spectrograph Gemini/GHOST, we could directly detect spectral features of the secondary component for the first time. A very low mass ratio for the system is confirmed (q ~ 0.16), making this binary one of the few extremely low mass ratio systems known. The primary star has a mass of M
a = 22 ± 1 M
⊙ and a radius of R
a = 7.0 ± 0.1 R
⊙, while the secondary star has a mass of M
b = 3.4 ± 0.1 M
⊙ and a radius of R
b = 2.22 ± 0.02 R
⊙. Stellar evolution models indicate that the system has undergone approximately two million years of evolution since its formation. Moreover, the secondary star is identified as a pre-main-sequence object, progressing toward the zero-age main sequence. This paper illustrates the power of high-resolution spectrographs such as GHOST in finding much lower mass, previously unseen stellar components of binary star systems.
Toward High-order Solar Corona Simulations: A High-order Hyperbolized Poisson Approach for Magnetic Field Initialization
Authors: Dhib Rayan , Ben Ameur Firas , Sharma Vatsalya , Lani Andrea , Poedts Stefaan 
Published: February 2025

Abstract
Proper initialization of the solar corona magnetic field is important for easing the iterative process of realistic and efficient global magnetohydrodynamics (MHD) simulations. This study introduces a high-order flux reconstruction (FR) framework for solving the Poisson equation, a necessary step for computing a potential-field source-surface (PFSS) to initialize the magnetic field for global solar corona simulations with MHD. By hyperbolizing the elliptic Poisson equation into a set of hyperbolic equations, we develop an efficient and robust high-order PFSS solver. Our contributions include developing a Q2 (i.e., quadratic) geometrical representation using prismatic elements for the computational domain, which enables high-order mesh generation. Such a hyperbolized Poisson solver effectively relaxes magnetic fields extrapolated from solar magnetograms, producing scalar potential fields that align well with theoretical expectations. Extensive verification was conducted on the high-order FR solver for polynomial orders up to P3, achieving fourth-order spatial accuracy. The hyperbolized solver demonstrates comparable accuracy to reference solutions (both analytical and numerical) while offering efficient performance, particularly on coarser meshes, making it competitive with state-of-the-art low-order finite volume solvers, which are mostly used for solar MHD simulations. The described developments are a milestone for enabling high-order global solar corona simulations on 3D unstructured grids.
ASKAP Observations of the Radio Shell in the Composite Supernova Remnant G310.6-1.6
Authors: Jing Wenhui , West Jennifer L. , Sun Xiaohui , Raja Wasim , Li Xianghua , Dang Lingxiao , Zhou Ping , Filipović Miroslav D. , Hopkins Andrew M. , Kothes Roland , Lazarević Sanja , Leahy Denis , Lenc Emil , Ma Yik Ki , Van Eck Cameron L. 
Published: February 2025

Abstract
We report the observations of the radio shell of the supernova remnant (SNR) G310.6–1.6 at 943 MHz from the Evolutionary Map of the Universe (EMU) and the Polarization Sky Survey of the Universe’s Magnetism (POSSUM) surveys by using the Australian Square Kilometre Array Pathfinder (ASKAP). We detect polarized emission from the central pulsar wind nebula (PWN) with rotation measures varying from –696 rad m−2 to –601 rad m−2. We measure the integrated flux density of the shell to be 36.4 ± 2.2 mJy at 943 MHz and derive a spectral index of α
pwn = −0.4 ± 0.1 for the PWN and α
shell = −0.7 ± 0.3 for the SNR shell. From the combined radio and X-ray observations, the object can be identified as a supernova explosion of about 2500 yr ago with an energy of about 1.3 × 1050 erg, suggesting an ejected mass of about 10 M
⊙. The circular radio shell outside the circular hard X-ray shell is unique among Galactic SNRs. We discuss several possible scenarios, including blast wave, reverse shock, and pulsar-fed emission, but find that none of them can fully explain the observed characteristics of the shell. This poses a challenge for understanding the evolution of SNRs. The results of this paper demonstrate the potential of the ASKAP EMU and POSSUM surveys to discover more objects of small angular size and low surface brightness.
A Comprehensive Study of Type I (Thermonuclear) Bursts in the New Transient SRGA J144459.2–604207
Authors: Fu Tao , Li Zhaosheng , Pan Yuanyue , Ji Long , Chen Yupeng , Kuiper Lucien , Galloway Duncan K. , Falanga Maurizio , Xu Renxin , Li Xiaobo , Ge Mingyu , Song L. M. , Zhang Shu , Zhang Shuang-Nan 
Published: February 2025

Abstract
We report an analysis of Insight-HXMT observations of the newly discovered accreting millisecond pulsar SRGA J144459.2–604207. During the outburst, detected in 2024 February by SRG/ART-XC, the broadband persistent spectrum was well fitted by an absorbed Comptonization model. We detected 60 type I X-ray bursts in the Insight-HXMT medium energy (ME) data, and 37 were also detected with the low-energy (LE) telescope. By superimposing the Insight-HXMT/LE/ME/HE light curves of 37 bursts with similar profiles and intensities, we measured a deficit of X-rays in the 40–70 keV energy band. By analyzing the time-resolved X-ray burst spectra, we determine the mean ratio of persistent to burst flux ofα = 71 ± 7. We estimate the average hydrogen mass fraction in the fuel at ignition, as

X

¯

=
0.342
±
0.033

, and constrain the burst fuel composition as X
0 ≲ 0.4. We found that 14 out of 60 X-ray bursts exhibited photospheric expansion, and thus we estimated the distance to the source as 10.03 ± 0.71 kpc. Combined with IXPE observations, the burst recurrence time increased from 1.55 to 8 hr as the local mass accretion rate decreased, which can be described as

Δ

T

rec

∼

m

̇

−
0.91
±
0.02

.
Wild bee diversity of the National Park of the Semois Valley (Belgium)
Authors: Gérard Maxence , Fiordaliso William , Ferrais Louise , Fournier Chloé , Hairault Malo , Lheureux Lise , Rosa Paolo , Ghisbain Guillaume 
Published: February 2025

Wild bees are essential pollinators, yet their decline due to human activities threatens ecosystem stability. Protecting these pollinators requires a detailed understanding of both their diversity and distribution. In Belgium, the recently-established Semois Valley National Park (SVNP) is located in a region with limited bee sampling data and this study aims to identify the habitats most suitable to bees, especially for threatened species.
Over five months, we surveyed 32 sites and collected a total of 1,119 specimens belonging to 120 bee species. Twenty-two of the observed species are listed as threatened in Belgium according to the last Red List published in 2019 for the country, four of them being Critically Endangered. Our findings indicate that mesic grasslands support the highest species diversity, as well as the highest number of threatened species. Our results underscore the need for conservation efforts aimed at maintaining diversity and species richness in this region. Effective biodiversity preservation will require enhanced habitat management and strategies tailored to bee species' ecological requirements.
Anthropophagie dans Western, ciné-poème guadeloupéen de Max Jeanne
Authors: Archimède Maëva 
Published: February 2025

Cet article propose une exploration du recueil Western ciné-poème du poète guadeloupéen Max Jeanne, au regard de sa problématique première : la narration de l’histoire guadeloupéenne. Déjouant le « piège » de l’Histoire (avec un H majuscule), le recueil absorbe divers textes, genres, discours pour les neutraliser ou les mettre à profit. L’entreprise que l’on peut qualifier d’anthropophagique s’analyse au regard des théories de l’intertextualité qui mettent en lumière le rôle des poètes dans l’écriture de l’histoire et le questionnement d’une identité caraïbe.
Inter-examiner repeatability and validity of static retinoscopy
Authors: Hasrod Nabeela 
Published: February 2025

Background: Studies on inter-examiner repeatability of measurements from retinoscopy without cycloplegia are quite limited within and across individuals.Aim: To investigate the inter-examiner repeatability and validity of static retinoscopy to autorefraction in young adults.Setting: The study took place within a South African university.Methods: Convenience, non-random sampling was used to obtain a sample of 68 adult participants, predominantly male (51.5%) of African descent (60.3%). The age range was from 18 years to 25 years with the mean ± standard deviation (s.d.) of 22.5 ± 0.71 years. The right eyes of participants underwent autorefraction, and static retinoscopy was done by two different student examiners. Bland-Altman plots and multivariate analysis were applied to assess inter-examiner repeatability and validity of retinoscopy to autorefraction of sphere, cylinder, spherical equivalent refraction (SER = M), and vector components J0 and J45.Results: Stereo-pair scatter plots for the three refractive samples from both student examiners obtained for the right eye clustered within the same region, which suggested minimal variation in refractive error between the different samples. Bland-Altman plots for mean differences () were less than or equal to one clinical step (0.25 dioptre [D]) for all refractive error variables although 95% Limits of Agreement (LoA) widths were larger for the spherical equivalent coefficients (M).Conclusion: Clinically, inter-examiner retinoscopy is repeatable and comparable to autorefraction as results differed only by approximately 0.25 D.Contribution: This study will be the first in Africa to provide multivariate analysis for inter-examiner repeatability of retinoscopy.