bluuebunny/crossref_metadata_2025_split huggingface dataset:
Autoeficacia y el desarrollo del pensamiento crítico en estudiantes de educación superior pertenecientes a una universidad de Lima metropolitana. 2023
Authors: Alva Miguel Walter Hugo , Wong Fajardo Emma Margarita , Zúñiga Reynoso Carlos 
Published: August 2024

Resumen

Se llevó a cabo una investigación cuyo objetivo esencial fue determinar la relación existente entre la autoeficacia y el pensamiento crítico en estudiantes de Educación Superior de una Universidad de Lima Metropolitana. Con este fin, se aplicó a una muestra de 50 alumnos de Educación Superior dos instrumentos de evaluación psicológica elaborados con tales propósitos: Inventario de Expectativas de Autoeficacia Académica de Barraza (2010) y la Encuesta de Capacidad de Pensamiento Crítico de Córdova (2021). Ambos instrumentos contaban con la debida validez y confiabilidad comprobada para nuestro medio. Estos instrumentos se aplicaron a una muestra seleccionada mediante muestreo no-probabilístico, de tipo criterial u opinático. Metodológicamente, se trató de una investigación descriptiva explicativa de nivel correlacional, con enfoque cuantitativo, de diseño no-experimental, de corte transversal, que aplicó la estadística paramétrica (Correlación Producto – Momento de Pearson) porque así lo estableció la Prueba de Kolmogorov – Smirnorv, para determinar la normalidad o no de las puntuaciones recabadas. El procedimiento estadístico corrió a cargo del Programa Excel 365 y del Programa SPSS Versión 25 para Windows y permitió comprobar las hipótesis planteadas, en el sentido que existía una relación directa y significativa (p= 0.001) entre las variables consideradas. En tal sentido se plantearon las conclusiones y las respectivas recomendaciones. Se elaboraron y presentaron complementariamente, las respectivas tablas y gráficos estadísticos.

Palabras clave: Autoeficacia, Desarrollo del Pensamiento Crítico, Educación Superior.
Editorial Note
Authors: Warren David 
Published: August 2024

Volume 41 Issue 2 of the American Journal of Islam and Society comprises four main research articles, each of which engages themes of Muslim collectiv­ity, community, and umma from different vantage points. The first article is Rezart Beka’s contribution, “The Reconceptualization of the Umma and Ummatic Actions in Abdullah Bin Bayyah’s Discourse.” The second article is titled “An Egyptian Ethicist: Muḥammad ʿAbd Allāh Drāz (1894-1958) and His Qurʾān-Based Moral Theory” by Ossama Abdelgawwad. The third research article for this issue is “The Other Legitimate Game in Town? Understanding Public Support for the Caliphate in the Islamic World”, a co-au­thored study by Mujtaba A. Isani, Daniel Silverman, and Joseph J. Kaminski. The fourth and final research article in this issue is Ashwak Hauter’s, “The Reparative Work of the Imagination: Yemen, ‘Afiya, and Politics of the Umma”.

This issue of the American Journal of Islam and Society also includes a number of insightful book reviews, including editor Ovamir Anjum’s review essay engaging Joel Hayward’s recent work The Warrior Prophet: Muhammad and War and Celene Ibrahim’s author response to a review authored in a previous issue on her book, Women and Gender in the Qur’an.
Pronomina Bahasa Melayu Dalam Naskah Drama Puteri Lindung Bulan Karya Dasri Al Mubary dan Kawan-Kawan
Authors: Hidayati Intan , Morelent Yetty , Naini Ineng , Syofiani Syofiani 
Published: August 2024

Tujuan penelitian ini adalah untuk mengetahui dan mendeskripsikan pronomina bahasa Melayu yang terdapat dalam naskah drama Puteri Lindung Bulan karya Dasri Al Mubary dan kawan-kawan. Teori yang digunakan adalah teori yang dikemukakan oleh Alwi, dkk (2010). Jenis penelitian ini adalah penelitian kualitatif dengan metode deskriptif. Teknik pengumpulan data penelitian ini yaitu: teknik dokumentasi, dan teknik hermeneutik (baca, catat, dan simpulkan). Teknik analisis data penelitian ini yaitu: reduksi data, penyajian data, dan penarikan kesimpulan. Hasil penelitian mengindikasikan bahwa di dalam naskah drama Puteri Lindung Bulan karya Dasri Al Mubary dan kawan-kawan digunakan Pronomina persona pertama tunggal yaitu [hambə], [bəta], [ananda]. Pronomina persona pertama jamak [kite]. Pronomina persona kedua tunggal [əngkau], [awak], [tuan], [datuk], [əncik], [kandə], [dində], [baginda], [ananda], [ayahandə]. Pronomina persona ketiga tunggal [Nyə], [diə], [bəliau], [əncik], [dində], [ayahandə], [puan]. Pronomina persona ketiga jamak [mərekə]. Pronomina Penunjuk Umum [ni] dan [tu]. Pronomina Penunjuk tempat [kəmari], [sini], dan [sanə]. Pronomina Penanya [siapə], [apə], [bagaimanə], [manə], [məngapə], dan [bərapə].
Pengaruh Green Motive Terhadap Green Product Innovation Performance pada IKM Batik Ramah Lingkungan di Jawa Timur
Authors: Rahayu Rahayu , Armin Rini , Heru Dwihandoko Toto 
Published: August 2024

Studi empiris ini menguji hipotesis menggunakan survei kuesioner untuk mengeksplorasi pengaruh positif green motive terhadap green product innovation performance pada IKM batik ramah lingkungan di Jawa Timur. Studi ini mengkaji motif instrumental, relasional, dan moral serta mengungkapkan bahwa motif instrumental merupakan pendorong kuat dibandingkan motif moral, sedangkan motif relasional tidak berpengaruh signifikan. Kondisi ini terjadi karena IKM memiliki kepedulian terhadap lingkungan yang cukup tinggi tanpa disupport pemangku kepentingan. Studi ini juga menentukan bahwa motif moral mempunyai pengaruh positif terhadap kinerja inovasi produk ramah lingkungan. Studi ini menyarankan agar IKM batik ramah lingkungan harus tetap menumbuhkembangkan green product agar bisnis yang dijalankan dapat berkelanjutan diimbangi dengan keberlanjutan lingkungan.
Peran E-Commerce Dan Gaya Hidup Dalam Menentukan Perilaku Konsumen
Authors: Moehadi  , Hartiningsih Astuti  , Siti Alfiyana  , Kiswati Dewi Kartika  
Published: August 2024

Consumer behavior is all activities and psychology that motivate these activities before buying, purchasing products and services, using, consuming, after doing these things or evaluation activities. The factors that influence consumer behavior are mainly cultural factors, which include culture, subculture and social class. Two social factors are reference group, family, role, and status. Three personal factors consisting of age and stage, financial situation, work, lifestyle and personality. And finally, psychological factors include motivation, perception, knowledge, beliefs and attitudes. This research aims to analyze consumer behavior. Consumer behavior in this research is thought to be influenced by e-commerce and lifestyle. This research method was carried out using a descriptive quantitative analysis approach with primary data measured using a Likert scale. The research was conducted in the Bojonegoro University environment. This research was conducted on students of the economics faculty at Bojonegoro University. The sampling technique is based on a representative sample size, namely between 50-100 samples. Data analysis was carried out using several stages, namely testing data instruments, classical assumptions and multiple linear regression analysis. Based on the results of partial data analysis, e-commerce and lifestyle have a significant positive influence on consumer behavior. Meanwhile, e-commerce and lifestyle simultaneously influence consumer behavior. Then based on the R2 value of 0.888, it shows that e-commerce and lifestyle contribute to influencing consumer behavior by 88.8%.

Keywords: E-commerce, Lifestyle, Consumer Behavior
Timbral brightness perception investigated through multimodal interference
Authors: Saitis Charalampos , Wallmark Zachary 
Published: August 2024

AbstractBrightness is among the most studied aspects of timbre perception. Psychoacoustically, sounds described as “bright” versus “dark” typically exhibit a high versus low frequency emphasis in the spectrum. However, relatively little is known about the neurocognitive mechanisms that facilitate these metaphors we listen with. Do they originate in universal magnitude representations common to more than one sensory modality? Triangulating three different interaction paradigms, we investigated using speeded classification whether intramodal, crossmodal, and amodal interference occurs when timbral brightness, as modeled by the centroid of the spectral envelope, and pitch height/visual brightness/numerical value processing are semantically congruent and incongruent. In four online experiments varying in priming strategy, onset timing, and response deadline, 189 total participants were presented with a baseline stimulus (a pitch, gray square, or numeral) then asked to quickly identify a target stimulus that is higher/lower, brighter/darker, or greater/less than the baseline after being primed with a bright or dark synthetic harmonic tone. Results suggest that timbral brightness modulates the perception of pitch and possibly visual brightness, but not numerical value. Semantically incongruent pitch height-timbral brightness shifts produced significantly slower reaction time (RT) and higher error compared to congruent pairs. In the visual task, incongruent pairings of gray squares and tones elicited slower RTs than congruent pairings (in two experiments). No interference was observed in the number comparison task. These findings shed light on the embodied and multimodal nature of experiencing timbre.
The Impact of Third Party Funds, Loan To Deposit Ratio And Capital Adequacy Ratio On Return On Assets
Authors: Arif Bahtiar , Priono Putriasyahwa Nurezky , Suardy Weman , Azhar Zul 
Published: August 2024

This research aims to determine whether Third Party Funds, Loan to Deposit Ratio, and Capital Adequacy Ratio have a partial and simultaneous effect on Return On Assets. The population in this research is banks registered on the Indonesia Stock Exchange for the period 2018 - 2022, totaling 45 banks, then the sample was determined using the Purposive Sampling method so that a sample of 7 banks was obtained. The analytical methods used are the classical assumption test, multiple linear regression analysis test, t test, f test, and coefficient of determination test. Data testing was carried out using IBM SPSS Statistics 27 Software. The results of this research show that: 1) Third Party Funds partially have a significant effect on Return on Assets. If Third Party Funds experience an increase, this will be followed by an increase in Return On Assets. 2) Loan to Deposit Ratio partially has a significant effect on Return on Assets. A high LDR ratio can cause banks to earn greater profits as loans increase. 3) Capital Adequacy Ratio partially has a significant effect on Return on Assets. A high CAR indicates that the bank has sufficient capital to cover risks that may arise from its operational activities. 4) Third Party Funds, Loan to Deposit Ratio and Capital Adequacy Ratio simultaneously have a significant effect on Return On Assets with a coefficient of determination of 52.2%.

Keywords: Third Party Funds, Loan to Deposit Ratio, Capital Adequacy Ratio, Return On Assets
Mixed Convection Boundary Layer Flow on A Vertical Flat Plate in Al203-Ag/Water Hybrid Nanofluid with Viscous Dissipation Effects
Authors: Elfiano Eddy , Nik Ibrahim Nik Mohd Izual , Mohamed Muhammad Khairul Anuar 
Published: August 2024

The present research examined the mixed convection boundary layer flow and heat transfer of hybrid nanofluid on a vertical flat plate with various volume concentrations and viscous dissipation effects. The governing non-linear partial differential equations are first transformed to a system of ordinary differential equations through the use of a similarity transformation. Subsequently, these equations are solved numerically using the Runge-Kutta-Fehlberg (RKF45) method in MAPLE. The numerical solution is computed for the temperature profiles, velocity profiles, reduced Nusselt number and reduced skin friction coefficient. The characteristics of flow and heat transfer for the Eckert number, the mixed convection parameter, and the hybrid nanoparticles volume fraction are analyzed and discussed. The velocity profiles are not influenced by the various values of and in specific cases, the - water-based hybrid nanofluid examined in this study achieves comparable results to the -water-based nanofluid.
NotPlaNET: Removing False Positives from Planet Hunters TESS with Machine Learning
Authors: Tardugno Poleo Valentina , Eisner Nora , Hogg David W. 
Published: August 2024

Abstract
Differentiating between real transit events and false-positive signals in photometric time-series data is a bottleneck in the identification of transiting exoplanets, particularly long-period planets. This differentiation typically requires visual inspection of a large number of transit-like signals to rule out instrumental and astrophysical false positives that mimic planetary transit signals. We build a one-dimensional convolutional neural network (CNN) to separate eclipsing binaries and other false positives from potential planet candidates, reducing the number of light curves that require human vetting. Our CNN is trained using the TESS light curves that were identified by Planet Hunters citizen scientists as likely containing a transit. We also include the background flux and centroid information. The light curves are visually inspected and labeled by project scientists and are minimally preprocessed, with only normalization and data augmentation taking place before training. The median percentage of contaminants flagged across the test sectors is 18% with a maximum of 37% and a minimum of 10%. Our model keeps 100% of the planets for 16 of the 18 test sectors, while incorrectly flagging one planet candidate (0.3%) for one sector and two (0.6%) for the remaining sector. Our method shows potential to reduce the number of light curves requiring manual vetting by up to a third with minimal misclassification of planet candidates.
The Nature of X-Rays from Young Stellar Objects in the Orion Nebula Cluster—A Chandra HETGS Legacy Project
Authors: Schulz Norbert S. , Huenemoerder David P. , Principe David A. , Gagne Marc , Günther Hans Moritz , Kastner Joel , Nichols Joy , Pollock Andrew , Preibisch Thomas , Testa Paola , Reale Fabio , Favata Fabio , Canizares Claude R. 
Published: August 2024

Abstract
The Orion Nebula Cluster (ONC) is the closest site of very young (∼1 Myr) massive star formation The ONC hosts more than 1600 young and X-ray bright stars with masses ranging from ∼0.1–35 M
⊙. The Chandra HETGS Orion Legacy Project observed the ONC with the Chandra High Energy Transmission Grating Spectrometer (HETGS) for 2.1 Ms. We describe the spectral extraction and cleaning processes necessary to separate overlapping spectra. We obtained 36 high-resolution spectra, which include a high-brilliance X-ray spectrum of θ
1 Ori C with over 100 highly significant X-ray lines. The lines show Doppler broadening between 300 and 400 km s−1. Higher spectral diffraction orders allow us to resolve line components of high Z He-like triplets in θ
1 Ori C with unprecedented spectral resolution. Long-term light curves spanning ∼20 yr show all stars to be highly variable, including the massive stars. Spectral fitting with thermal coronal emission line models reveals that most sources show column densities of up to a few times 1022 cm−2 and high coronal temperatures of 10–90 MK. We observe a bifurcation of the high-temperature component where some stars show a high component of 40 MK, while others show above 60 MK, indicating heavy flaring activity. Some lines are resolved with Doppler broadening above our threshold of ∼200 km s−1, up to 500 km s−1. This data set represents the largest collection of HETGS high-resolution X-ray spectra from young pre-main-sequence stars in a single star-forming region to date.
A Multiwavelength Survey of Nearby M Dwarfs: Optical and Near-ultraviolet Flares and Activity with Contemporaneous TESS, Kepler/K2, Swift, and HST Observations
Authors: Paudel Rishi R. , Barclay Thomas , Youngblood Allison , Quintana Elisa V. , Schlieder Joshua E. , Vega Laura D. , Gilbert Emily A. , Osten Rachel A. , Peacock Sarah , Tristan Isaiah I. , Feliz Dax L. , Boyd Patricia T. , Davenport James R. A. , Huber Daniel , Kowalski Adam F. , Monsue Teresa , Silverstein Michele L. 
Published: August 2024

Abstract
We present a comprehensive multiwavelength investigation into flares and activity in nearby M dwarf stars. We leverage the most extensive contemporaneous data set obtained through the Transiting Exoplanet Sky Survey, Kepler/K2, the Neil Gehrels Swift Observatory, and the Hubble Space Telescope, spanning the optical and near-ultraviolet (NUV) regimes. In total, we observed 213 NUV flares on 24 nearby M dwarfs, with ∼27% of them having detected optical counterparts, and found that all optical flares had NUV counterparts. We explore NUV/optical energy fractionation in M dwarf flares. Our findings reveal a slight decrease in the ratio of optical to NUV energies with increasing NUV energies, a trend in agreement with prior investigations on G–K stars’ flares at higher energies. Our analysis yields an average NUV fraction of flaring time for M0–M3 dwarfs of 2.1%, while for M4–M6 dwarfs it is 5%. We present an empirical relationship between NUV and optical flare energies and compare to predictions from radiative hydrodynamic and blackbody models. We conducted a comparison of the flare frequency distribution (FFDs) of NUV and optical flares, revealing that the FFDs of both NUV and optical flares exhibit comparable slopes across all spectral subtypes. NUV flares on stars affect the atmospheric chemistry, the radiation environment, and the overall potential to sustain life on any exoplanets they host. We find that early and mid-M dwarfs (M0–M5) have the potential to generate NUV flares capable of initiating abiogenesis.
Microphysics of Particle Reflection in Weibel-mediated Shocks
Authors: Parsons Jasmine , Spitkovsky Anatoly , Vanthieghem Arno 
Published: August 2024

Abstract
Particle-in-cell (PIC) simulations have shown that relativistic collisionless shocks mediated by the Weibel instability accelerate ∼1% of incoming particles, while the majority are transmitted through the shock and become thermalized. The microphysical processes that determine whether an incoming particle will be transmitted or reflected are poorly understood. We study the microphysics of particle reflection in Weibel-mediated shocks by tracking a shell of test particles in a PIC simulation of a shock in pair plasma. We find that electrons in positron-dominated filaments and positrons in electron-dominated filaments efficiently reflect off of strong magnetic structures at the shock. To participate in diffusive shock acceleration, however, these reflected particles headed toward the upstream must avoid getting advected downstream. This is enabled by incoming filaments, which trap reflected particles carrying the same sign of current as the filaments. The final injection efficiency on the order of ∼1% thus results from the effectiveness of the initial reflection at the shock and the reflected particles’ probability of survival in the upstream postreflection. We develop a model that predicts the fraction of high-energy particles as a function of the properties of Weibel filamentation.
The Incompressible Magnetohydrodynamic Energy Cascade Rate Upstream of Mars: Effects of the Total Energy and the Cross-helicity on Solar Wind Turbulence
Authors: Romanelli Norberto , Andrés Nahuel , DiBraccio Gina A. , Verniero Jaye L. , Gruesbeck Jacob R. , Szabo Adam , Espley Jared R. , Halekas Jasper S. 
Published: August 2024

Abstract
Solar wind turbulence is a dynamical phenomenon that evolves with heliocentric distance. Orbiting Mars since 2014 September, Mars Atmosphere and Volatile EvolutioN offers a unique opportunity to explore some of its main properties beyond ∼1.38 au. Here, we analyze solar wind turbulence upstream of Mars' bow shock, utilizing more than 5 years of magnetic field and plasma measurements. This analysis is based on two complementary methodologies: (1) the computation of magnetohydrodynamic (MHD) invariants characterizing incompressible fluctuations; (2) the estimation of the incompressible energy cascade rate at MHD scales (i.e., 〈ε

T
〉MHD). Our results show the solar wind incompressible fluctuations are primarily in a magnetically dominated regime, with the component traveling away from the Sun having a higher median pseudoenergy. Moreover, turbulent fluctuations have a total energy per mass of up to ∼ 300 km2 s−2, a range smaller than reported at 1 au. For these conditions, we determine the probability distribution function of 〈ε

T
〉MHD ranges mainly between ∼ −1 × 10−16 and ∼1 × 10−16 J m−3 s −1, with a median equal to −1.8 × 10−18 J m−3
s −1, suggesting back transfer of energy. Our results also suggest that ∣〈ε

T
〉MHD∣ is correlated with the total energy per mass of fluctuations and that the median of 〈ε

T
〉MHD does not vary significantly with the cross-helicity. We find, however, that the medians of the inward and outward pseudoenergy cascade rates vary with the solar wind cross-helicity. Finally, we discuss these results and their implications for future studies that can provide further insight into the factors affecting the solar wind energy transfer rate.
On the Origin of Solar Hemispheric Helicity Rules: Rise of 3D Magnetic Flux Concentrations through a Background Magnetic Field
Authors: Manek Bhishek , Brummell Nicholas 
Published: August 2024

Abstract
Sunspots and active regions observed on the solar surface are widely believed to be manifestations of compact predominantly toroidal magnetic field structures (“flux tubes”) that emerge by magnetic buoyancy from the deeper interior of the Sun. Much work has examined the evolution of such magnetic structures, typically considering them as idealized isolated magnetic entities and not as more realistic magnetic concentrations in a volume-filling background magnetic field. Here, we report results that explore the buoyant rise dynamics of magnetic concentrations in a volume-filling field in the full three dimensions. Earlier 2.5D work in this series established the remarkable fact that the twist orientation of a flux concentration relative to the background field affected its likelihood to rise and emerge, regardless of whether the buoyant rise took place in the absence or presence of convection. The contrasting dynamics between structures with differing orientations lead to a selection mechanism that reproduces characteristics of the “solar hemispheric helicity rule(s)” observations strikingly well. Here, we show that this two-dimensional selection mechanism persists in the face of the added complexity of three-dimensional dynamics. Arching of the magnetic structure in the third dimension, as might be expected in the solar application, is introduced. The role of tension force leading to this selection mechanism is elucidated and subtle differences that arise due to the three-dimensional geometry are discussed.