bluuebunny/crossref_metadata_2025_split huggingface dataset:
BAYANI EPISTEMOLOGIES IN MODERN INDONESIA: The Contribution of Al Washliyah Ulama to Quranic Exegesis Studies
Authors: Ja'far Ja'far , Iqbal Muhammad 
Published: July 2023

<p><strong>Abstrak</strong>: Studi tentang peran organisasi Islam di Indonesia dalam kajian tafsir belum banyak dilakukan para peneliti. Padahal, kajian ini menarik dilakukan mengingat pengaruh eksistensi organisasi Islam terhadap seluruh aspek kehidupan Muslim di Indonesia. Al Washliyah merupakan organisasi Islam terbesar ketiga di Indonesia yang sangat jarang diteliti para ahli, termasuk perannya dalam pelestarian dan pengembangan kajian tafsir Alquran di Indonesia. Studi ini merupakan studi kepustakaan dengan menggunakan pendekatan sejarah. Topik penelitian dianalisis dengan teori Max Weber tentang tindakan sosial dan dominasi kekuasaan. Studi ini mengajukan temuan bahwa Al Washliyah mengajarkan sejumlah kitab tafsir Alquran di madrasah-madrasahnya; menerbitkan artikel terkait Alquran dan tafsirnya pada majalah resminya, <em>Medan Islam </em>(juga <em>Dewan Islam</em>)<em>;</em> dan ulama-ulamanya juga menghasilkan sejumlah karya dalam bidang Alquran dan tafsir. Kepatuhan Al Washliyah terhadap akidah Ahl al-Sunnah wa al-Jamâ‘ah (Sunni) dan mazhab fikih Syafi‘iyah juga membuat organisasi ini abai terhadap literatur tafsir dari mazhab lainnya. Studi ini berkontribusi terhadap penguatan literatur tentang kajian tafsir di Indonesia.</p><p><strong>Kata Kunci</strong>: tafsir Alquran, Al Washliyah, madrasah, majalah Islam, ulama</p><p><strong>Abstract: </strong>The contribution of Islamic organizations in Quranic exegesis (<em>tafsîr</em>) in Indonesia has been largely overlooked by researchers. However, this study aims to explore this topic due to the significant influence of Islamic organizations on various aspects of Muslim life in the country. One such organization is Al Washliyah, the third largest Islamic organization in Indonesia, which has received limited attention from experts in terms of its contribution to the preservation and development of Quranic exegesis. This literature-based research adopts a historical approach, and the research topic is analyzed through Max Weber’s theories of social action and dominance of power. This study argues that Al Washliyah ulama have taught various books on Quranic exegesis in its madrasas, published articles on the Quran and its tafsir in its official magazine <em>Medan Islam</em> (also <em>Dewan Islam</em>), and its ulama have produced several works in the field of Quranic exegesis. Moreover, due to its adherence to the Ahl al-Sunnah wa al-Jamâ‘ah (Sunni) creed and the Shâfi‘iyah school of jurisprudence, Al Washliyah tends to disregard Quranic exegesis literature from other schools. This study, of course, contributes to the strengthening of literature on Quranic studies in modern Indonesia.</p><p><strong>Keywords</strong>: Quranic exegesis, Al Washliyah, madrasas, Islamic magazine, ulama</p>
Efecto de densidad de siembra en la producción de frijoles nativos
Authors: Monge Perez José Eladio , Oreamuno-Fonseca Patricia , Loría-Coto Michelle 
Published: July 2023

Objetivos: se evaluó el efecto de dos densidades de siembra (125,000 y 714,000 semillas/ha), sobre el rendimiento de seis variedades nativas de frijol (Phaseolus vulgaris L.): Mantequilla, Nica, Revuelto, Sesenteno, Turrialba y Vaina Blanca. Metodología: la siembra se realizó en Matambuguito, Nicoya, Guanacaste, Costa Rica, en un suelo con pendiente, y con bajo uso de insumos. Resultados: la densidad de siembra no tuvo un efecto significativo sobre la producción de grano, pero sí se presentaron diferencias significativas entre los frijoles nativos; Sesenteno obtuvo un mayor rendimiento (329.38kg/ha), en comparación con Turrialba y Vaina Blanca (137.19kg/ha). Conclusiones: este es el primer informe publicado sobre el efecto de la densidad de siembra sobre el rendimiento, en variedades nativas de frijol de Costa Rica.
Can minority shareholders’ “hand-voting” promote green innovation of Enterprises—Empirical evidence from Chinese listed companies
Authors: Shi Xiaofei , Xu Wenxin , Cao Xuefen , Hou Yangshi 
Published: July 2023

China’s listed companies have serious Principal-agent problem of the second kind. Large shareholders have violated the rights and interests of minority shareholders in an endless stream of cases. However, the voice of encouraging minority shareholders to actively participate in enterprise decision-making is growing day-by-day. However, there is no consensus on whether the enthusiasm of minority shareholders in decision-making can have a positive impact on enterprises. Therefore, this article takes China’s A-share listed companies from 2016 to 2020 as the research sample, and from the perspective of green innovation, discusses whether the minority shareholders’ active participation in enterprise decision-making can improve the level of green innovation of enterprises. The study found that the minority shareholders’ active participation in enterprise decision-making can improve the level of green innovation. Moreover, the minority shareholders’ “hand voting” improves the green innovation level of enterprises by influencing the media attention; A higher level of legal environment is conducive to strengthening the role of minority shareholders’ participation in the shareholders’ meeting in green innovation. Based on the property right nature, regional and industrial level, further research found that the minority share-holders’ role in improving green innovation capacity is more significant in non-state-owned enterprises, eastern regions and heavy pollution industries. The research results show that minority shareholders, as an important force to monitor the senior executives’ behavior and enhance corporate value, actively participate in corporate decision-making, can not only improve corporate governance, but also benefit the sustainable development of enterprises.
Outcome of capacity building in mental health for well-being volunteers
Authors: Yaresheemi Shivanand , Elangovan Aravind Raj , Jangam Kavita , Doraiswamy Padmavathy , Sharma Manoj Kumar , Chandra Prabha S. 
Published: July 2023

IntroductionVolunteering is any activity in which time is given to assist another individual, group, or organization. It assists people who want to get involved in philanthropic programs that help volunteers develop awareness and lead healthier personal and social lives. Several volunteers have received specialized training in the fields in which they volunteer, such as health, mental health, education, or emergency rescue. Volunteers are rendering intervention in different areas in mental health. They are providing psychosocial support to the individuals, groups, community, promoting mental health through conducting various mental health awareness programs in the community. There is a growing concern about mental health in India due to the inaccessibility of services. The National Institute of Mental Health and Neuro Sciences (NIMHANS) being a premier institute for mental health, is devising innovative approaches to mental health care to reach the unreachable. One such initiative was to build the capacity of volunteers in the community who are interested in working for the cause of mental health.MethodsThe objective of this study was to evaluate the outcome of the well-being volunteer program. This study used a descriptive cross-sectional research design, wherein all the 136 trained well-being volunteers (WBVs) were included as the study sample. The data was collected from the volunteers who attended the WBV program, which was initiated by NIMHANS Centre for Well-being (NCWB) and the Department of Psychiatric Social Work NIMHANS. A questionnaire on the outcome of the Well Being Volunteers program was developed for the study, and the Volunteer Motivation Inventory scale was used to collect the data from the WBVs. SPSS software was used to analyze the data. Ethical clearance was sought from the Institute Ethics Committee of NIMHANS.ResultsThe WBV program enhanced volunteers’ knowledge of mental health and benefited the volunteers in their personal and social life. They were also able to implement a satisfactory level of mental health-related volunteer activities in the community.ConclusionResults of present study and the available literature suggest that engaging in voluntary services improves mental health knowledge. WBV program has provided opportunity to Volunteers to participate in mental health delivery system at different levels.
IMPLEMENTASI STIMULASI KOGNITIF (GERAKAN SENAM OTAK) DALAM MENURUNKAN TINGKAT DEMENSIA LANSIA
Authors: Hasnah Kholifah , Sakitri Ganik 
Published: July 2023

Demensia menjadi sindrom terjadinya penurunan kognitif yang ditandai dengan perubahan perilaku. Demensia apabila tidak ditangani akan mengakibatkan terjadinya gangguan fungsi intelektual dan gangguan dalam aktivitas sehari-hari. Salah satu implementasi yang dapat diberikan pada penderita demensia adalah dengan melakukan gerakan senam otak. Tujuan dari penelitian ini adalah mengetahui penurunan tingkat demensia setelah diberikan implementasi gerakan senam otak pada lansia. Metode yang digunakan pada penelitian ini adalah quasy eksperimental dengan one group pretest and posttest design. Jumlah subjek dalam penelitian ini adalah 20 lansia yang akan diberikan implementasi gerakan senam otak dan diukur tingkat demensia dengan kuisioner Mini Mental State Examination sebelum dan sesudah diberikan implementasi gerakan senam otak.
Hasil analisa menunjukkan bahwa ada penurunan kategori demensia dari demensia sedang ke demensia ringan dengan selisih nilai rata rata sebesar 2,3 pada nilai pre test dan post test. Kesimpulan Implementasi gerakan senam otak dapat menurunkan tingkat demensia dari demensia sedang ke demensia rendah. Saran perlu adanya penelitian selanjutnya yang berkaitan dengan penyakit degenerative pada lansia
Dementia is a syndrome of cognitive decline characterized by changes in behavior. Dementia if left untreated will result in impaired intellectual function and disruption in daily activities. One of the implementations that can be given to people with dementia is to do brain gymnastic movements. The purpose of this study was to determine the decrease in the level of dementia after being given the implementation of brain gymnastic movements in the elderly. The method used in this research is quasy experimental with one group pretest and posttest design. The number of subjects in this study were 20 elderly who would be given the implementation of brain gymnastic movements and measured their level of dementia with the Mini Mental State Examination questionnaire before and after being given the implementation of brain gymnastic movements.
The results of the analysis showed that there was a decrease in the category of dementia from moderate to mild dementia with a difference in the average score of 2.3 in the pre-test and post-test scores. Conclusion Implementation of brain gymnastic movements can reduce the level of dementia from moderate to low dementia. Suggestions need further research related to degenerative diseases in the elderly
PERILAKU MASYARAKAT DALAM PENCEGAHAN PENULARAN SCHISTOSOMIASIS DI DESA MEKAR SARI KABUPATEN POSO
Authors: Kadek Wartana I , Gustini Gustini , Lilian Mua Estelle , Mornalita Kolupe Veni , A. Sekeon Robi 
Published: July 2023

Masih tingginya angka kejadian schistosomiasis pada keong (2,56%) di Sulawesi Tengah dapat meningkatkan risiko terjadinya penularan pada manusia. Penurunan kasus infeksi schistosomiasis pada manusia dapat dilakukan dengan melibatkan masyarakat masyarakat dalam program pencegahan schistosomiasis yang dapat mengarah pada peningkatan perilaku dan kesadaran tentang pencegahan penyakit schistosomiasis. Penelitian ini menggunakan desain kuantitatif dengan pendekatan cross sectional yang mengambil lokasi penelitian di Desa Mekar Sari Kabupaten Poso. Populasi penelitian berjumlah 369 Kepala Keluarga (KK) dengan jumlah sampel sebanyak 80 KK yang diambil secara proportional random sampling. Alat pengumpulan data menggunakan kuesioner. Data dianalisis secara univariat dan bivariat dengan menggunakan uji chi-square dengan tingkat kepercayaan 95%. Hasil penelitian menunjukkan bahwa 72,9% responden memiliki pengetahuan yang tinggi, 58,8% responden memiliki sikap yang positif, serta 65% responden memiliki perilaku yang baik dalam pencegahan penularan schistosomiasis. Hasi uji chi-square didapatkan nilai p untuk pengetahuan sebesar 0,027 dan untuk sikap sebesar 0,005 (p value < 0,05), sehingga dapat disimpulkan pengetahuan dan sikap secara signifikan berhubungan dengan perilaku pencegahan penularan schistosomiasis di Desa Mekar Sari Kabupaten Poso.
Kata Kunci: Pengetahuan, Sikap, Perilaku, Schistosomiasis
Robust Field-level Likelihood-free Inference with Galaxies
Authors: de Santi Natalí S. M. , Shao Helen , Villaescusa-Navarro Francisco , Abramo L. Raul , Teyssier Romain , Villanueva-Domingo Pablo , Ni Yueying , Anglés-Alcázar Daniel , Genel Shy , Hernández-Martínez Elena , Steinwandel Ulrich P. , Lovell Christopher C. , Dolag Klaus , Castro Tiago , Vogelsberger Mark 
Published: July 2023

Abstract
We train graph neural networks to perform field-level likelihood-free inference using galaxy catalogs from state-of-the-art hydrodynamic simulations of the CAMELS project. Our models are rotational, translational, and permutation invariant and do not impose any cut on scale. From galaxy catalogs that only contain 3D positions and radial velocities of ∼1000 galaxies in tiny

(
25

h

−
1

Mpc
)

3

volumes our models can infer the value of Ωm with approximately 12% precision. More importantly, by testing the models on galaxy catalogs from thousands of hydrodynamic simulations, each having a different efficiency of supernova and active galactic nucleus feedback, run with five different codes and subgrid models—IllustrisTNG, SIMBA, Astrid, Magneticum, SWIFT-EAGLE—we find that our models are robust to changes in astrophysics, subgrid physics, and subhalo/galaxy finder. Furthermore, we test our models on 1024 simulations that cover a vast region in parameter space—variations in five cosmological and 23 astrophysical parameters—finding that the model extrapolates really well. Our results indicate that the key to building a robust model is the use of both galaxy positions and velocities, suggesting that the network has likely learned an underlying physical relation that does not depend on galaxy formation and is valid on scales larger than ∼10 h
−1 kpc.
Massive Hypervelocity Runaway Stars in the Large Magellanic Cloud
Authors: Lin Zehao , Xu Ye , Hao Chaojie , Li Yingjie , Liu Dejian , Bian Shuaibo 
Published: July 2023

Abstract
Since the hypervelocity stars were discovered in the Milky Way, various mechanisms have been proposed to explain these runaway stars. Up to now, however, the dominant ejected mechanism of hypervelocity stars is still unclear. As the largest and closest face-on satellite galaxy of the Milky Way, the Large Magellanic Cloud (LMC) serves as a good target, allowing us to study this issue. Based on the high-precision astrometric parameters provided by Gaia Data Release 3, we researched the proper motions of 3119 massive O–B2-type stars in the LMC and identified 98 (∼3%) as having the ability to escape from the LMC, with more than 50% confidence. Furthermore, by investigating the characteristics of the identified massive stars and adopting a regression analysis, we find that the dynamic ejection scenario might be the dominant mechanism of the massive hypervelocity runaway stars in the LMC.
Modeling of Thermal Emission from ULX Pulsar Swift J0243.6+6124 with General Relativistic Radiation MHD Simulations
Authors: Inoue Akihiro , Ohsuga Ken , Takahashi Hiroyuki R. , Asahina Yuta 
Published: July 2023

Abstract
We perform general relativistic radiation magnetohydrodynamics simulations of super-Eddington accretion flows around a neutron star with a dipole magnetic field for modeling the Galactic ultraluminous X-ray source exhibiting X-ray pulsations, Swift J0243.6+6124. Our simulations show the accretion columns near the magnetic poles, the accretion disk outside the magnetosphere, and the outflows from the disk. It is revealed that the effectively optically thick outflows, consistent with the observed thermal emission at ∼107 K, are generated if the mass accretion rate is much higher than the Eddington rate

M

̇

Edd

and the magnetospheric radius is smaller than the spherization radius. In order to explain the blackbody radius (∼100–500 km) without contradicting the reported spin period (9.8 s) and spin-up rate (

P

̇

=
−
2.22
×

10

−
8

s

s

−
1

), a mass accretion rate of

(
200
–
1200
)

M

̇

Edd

is required. Since the thermal emission was detected in two observations with

P

̇

of −2.22 × 10−8 s s−1 and −1.75 × 10−8 s s−1 but not in another with

P

̇

=
−
6.8
×

10

−
9

s

s

−
1

, the surface magnetic field strength of the neutron star in Swift J0243.6+6124 is estimated to be between 3 × 1011 G and 4 × 1012 G. From this restricted range of magnetic field strength, the accretion rate would be

(
200
–
500
)

M

̇

Edd

when the thermal emission appears and

(
60
–
100
)

M

̇

Edd

when it is not detected. Our results support the hypothesis that the super-Eddington phase in the 2017–2018 giant outburst of Swift J0243.6+6124 is powered by highly super-Eddington accretion flows onto a magnetized neutron star.
Three-dimensional Particle-in-cell Simulations of the Solar Wind Interaction with Asteroid 2016 HO3
Authors: Xie Lianghai , Li Lei , Wang Jindong , Zhang Yiteng , Zhou Bin , Feng Yongyong 
Published: July 2023

Abstract
The recently discovered asteroid 2016 HO3 is the most stable quasi-satellite of our Earth. Several missions to 2016 HO3 have been proposed, including the Tianwen-2 mission of China. Here we study the solar wind interaction with 2016 HO3 with three-dimensional particle-in-cell simulations. It is found that the sunlit surface can be positively charged to more than +10 V, and the shadowed surface is negatively charged to lower than −30 V. The typical electric field on the sunlit surface is about 2 V m−1 but can increase up to 20 V m−1 near the terminator. There is a plasma wake behind 2016 HO3 with a reduced plasma density. Normally, the ion density can be reduced to about 0.3 of the solar wind density at 100 m downstream from 2016 HO3, and the plasma wake is confined by a Mach cone with a cone angle of about 6.°5. In addition, we find that both the solar wind parameters and the secondary electron emission can affect the surface charging, which, in return, changes the wake structure.
Cluster-counterpart Voids: Void Identification from Galaxy Density Field
Authors: Shim Junsup , Park Changbom , Kim Juhan , Hong 홍 Sungwook E. 성욱 
Published: July 2023

Abstract
We identify cosmic voids from galaxy density fields under the theory of void–cluster correspondence. We extend the previous novel void-identification method developed for the matter density field to the galaxy density field for practical applications. From cosmological N-body simulations, we construct galaxy number- and mass-weighted density fields to identify cosmic voids that are counterparts of galaxy clusters of a specific mass. The parameters for the cluster-counterpart void identification such as Gaussian smoothing scale, density threshold, and core volume fraction are found for galaxy density fields. We achieve about 60%–67% of completeness and reliability for identifying the voids of corresponding cluster mass above 3 × 1014
h
−1
M
⊙ from a galaxy sample with the mean number density,

n

¯

=
4.4
×

10

−
3

(

h

−
1

Mpc
)

−
3

. When the mean density is increased to

n

¯

=

10

−
2

(

h

−
1

Mpc
)

−
3

, the detection rate is enhanced by ∼2%–7% depending on the mass scale of voids. We find that the detectability is insensitive to the density weighting scheme applied to generate the density field. Our result demonstrates that we can apply this method to the galaxy redshift survey data to identify cosmic voids corresponding statistically to the galaxy clusters in a given mass range.
Deep Einstein@Home All-sky Search for Continuous Gravitational Waves in LIGO O3 Public Data
Authors: Steltner B. , Papa M. A. , Eggenstein H.-B. , Prix R. , Bensch M. , Allen B. , Machenschalk B. 
Published: July 2023

Abstract
We present the results of an all-sky search for continuous gravitational waves in the public LIGO O3 data. The search covers signal frequencies 20.0 Hz ≤ f ≤ 800.0 Hz and a spin-down range down to −2.6 × 10−9 Hz s−1, motivated by detectability studies on synthetic populations of Galactic neutron stars. This search is the most sensitive all-sky search to date in this frequency/spin-down region. The initial search was performed using the first half of the public LIGO O3 data (O3a), utilizing graphical processing units provided in equal parts by the volunteers of the Einstein@Home computing project and by the ATLAS cluster. After a hierarchical follow-up in seven stages, 12 candidates remain. Six are discarded at the eighth stage, by using the remaining O3 LIGO data (O3b). The surviving six can be ascribed to continuous-wave fake signals present in the LIGO data for validation purposes. We recover these fake signals with very high accuracy with our last stage search, which coherently combines all O3 data. Based on our results, we set upper limits on the gravitational-wave amplitude h
0 and translate these into upper limits on the neutron star ellipticity and on the r-mode amplitude. The most stringent upper limits are at 203 Hz, with h
0 = 8.1 × 10−26 at the 90% confidence level. Our results exclude isolated neutron stars rotating faster than 5 ms with ellipticities greater than

5
×

10

−
8

d

100

pc

within a distance d from Earth and r-mode amplitudes

α
≥

10

−
5

d

100

pc

for neutron stars spinning faster than 150 Hz.
Optical and Near-infrared Continuum Emission Region Size Measurements in the Lensed Quasar FBQ J0951+2635
Authors: Rivera Angelica B. , Morgan Christopher W. , Florence Steven M. , Dahm Scott E. , Vrba Frederick J. , Tilleman Trudy M. , Cornachione Matthew A. , Falco Emilio E. 
Published: July 2023

Abstract
We present 10 seasons of Sloan Digital Sky Survey r-band monitoring observations and five seasons of H-band observations of the two-image system FBQ J0951+2635 from the Kaj Strand Astrometric Reflector at the United States Naval Observatory, Flagstaff Station. We supplement our light curves with six seasons of monitoring data from the literature to yield a 10 + 6 season combined data set, which we analyzed with our Monte Carlo microlensing analysis routine to generate constraints on the structure of this system’s continuum emission source and the properties of the lens galaxy. Complementing our optical light curves with the five-season near-infrared light curves, we ran a joint Monte Carlo analysis to measure the size of the continuum emission region at both wavelengths, yielding log(r
1/2 cm−1) =

16.24

−
0.36

+
0.33

in the r band and

17.04

−
0.30

+
0.26

in the H band at rest wavelengths of 2744 and 7254 Å, respectively, correcting for an assumed inclination angle of 60°. Modeling the accretion disk temperature profile as a power law T(r) ∝ r
−β
, we successfully constrain the slope for FBQ J0951+2635 to

β
=

0.50

−
0.18

+
0.50

, shallower than, but nominally consistent with, the predictions of standard thin-disk theory, β = 0.75.