bluuebunny/crossref_metadata_2025_split huggingface dataset:
PENGARUH KOMPENSASI DAN LINGKUNGAN KERJA TERHADAP KEPUASAN KERJA PEGAWAI NEGERI SIPIL MELALUI WORK-LIFE BALANCE
Authors: Sutiara Sutiara , Firman Ahmad , Razak Mashur 
Published: January 2024

Penelitian ini dimaksudkan untuk mengetahui pengaruh kompensasi dan lingkungan kerja terhadap kepuasan kerja pegawai melalui work-life balance, penelitian ini dilaksanakan pada Sekretariat Daerah Kabupaten Sidenreng Rappang dengan mengambil 86 pegawai negeri sipil sebagai sampel penelitian. Penelitian ini menggunakan pendekatan kuantitatif dengan teknik analisis data menggunakan analisis deskriptif dengan bantuan Software SmartPLS 3. Hasil penelitian menunjukkan bahwa kompensasi dan lingkungan kerja berpengaruh positif dan signifikan terhadap work-life balance, kompensasi dan work-life balance berpengaruh positif dan signifikan terhadap kepuasan kerja, lingkungan kerja berpengaruh positif dan tidak signifikan terhadap kepuasan kerja, kompensasi berpengaruh positif dan tidak signifikan terhadap kepuasan kerja melalui work-life balance, lingkungan kerja berpengaruh positif dan signifikan terhadap kepuasan kerja melalui work-life balance. Penelitian ini menghasilkan nilai koefisien determinasi untuk variabel work-life balance sebesar 0.318 berarti variabel work-life balance dapat dijelaskan oleh variabel kompensasi dan lingkungan kerja sebesar 31.8% dan untuk variabel kepuasan kerja diperoleh sebesar 0.466, hal ini berarti variabel kepuasan kerja dapat dijelaskan oleh variabel kompensasi, lingkungan kerja dan work-life balance sebesar 46.6 %.

Kata kunci : Kompensasi, Lingkungan Kerja, Work-Life Balance, Kepuasan Kerja.
The reciprocity of spatial–numerical associations of vocal response codes depends on stimulus mode
Authors: Richter Melanie , Wühr Peter 
Published: January 2024

AbstractIndividuals make faster left responses to small/er numbers and faster right responses to large/r numbers than vice versa. This “spatial–numerical association of response codes” (SNARC) effect represents evidence for an overlap between the cognitive representations of number and space. Theories of the SNARC effect differ in whether they predict bidirectional S-R associations between number and space or not. We investigated the reciprocity of S-R priming effects between number and location in three experiments with vocal responses. In Experiments 1 and 2, participants completed a number–location task, with digits as stimuli and location words as responses, and a location–number task, with physical locations as stimuli and number words as responses. In addition, we varied the S-R mapping in each task. Results revealed a strong SNARC effect in the number–location task, but no reciprocal SNARC effect in the location–number task. In Experiment 3, we replaced physical location stimuli with location words and digit stimuli with number words. Results revealed a regular and a reciprocal SNARC effect of similar size. Reciprocal SNARC effects thus seem to emerge with verbal location stimuli and vocal responses, but not with physical location stimuli and vocal responses. The S-R associations underlying the SNARC effect with vocal responses thus appear bidirectional and symmetrical for some combinations of stimulus and response sets, but not for others. This has implications for theoretical accounts of the SNARC effect which need to explain how stimulus mode affects the emergence of reciprocal but not regular SNARC effects.
The Influence of the Independent Board of Commissioners, Institutional Ownership and Managerial Ownership on Profit Management
Authors: Orbawan Yodi , April Sonni Tri Aries 
Published: January 2024

This research aims to determine the influence of an independent board of commissioners, institutional ownership and managerial ownership on earnings management in various industrial and textile subsectors in 2018-2020. This type of research is quantitative research. The population in this research are various industrial and textile sector companies listed on the Indonesia Stock Exchange in 2018-2020. Sampling used the perposive sampling method. The number of samples is 30. The sampling method uses the perposive sampling method. The number of samples is 30. The data collection method in this research is documentation. Using SPSS 25 data testing. The data analysis techniques used are descriptive statistics, classical assumption tests and T statistical tests. Independent Board of Commissioners has a positive and insignificant effect on earnings quality, institutional ownership has no significant effect on earnings quality, managerial ownership has an insignificant effect on earnings quality. Meanwhile, simultaneously the influence of the independent board of commissioners, institutional ownership and managerial ownership on earnings management has no effect.

Keywords: board of commissioners, institutional ownership, managerial ownership, profit management
Analysis of Financing with Murabahah Agreements
Authors: Setiyati Esti , Waruwu Shinta Nuriah 
Published: January 2024

One of the financial institutions that operates with the sharia concept is the Baytul Ikhtiar Sharia Financing Savings and Loans Cooperative (KSPPS). In terms of legality, KSPPS Baytul Ikhtiar has a legal entity: 518/169/BH/KPTS/KKUKM/2008. Based on the decision of the Minister of Cooperatives and Small and Medium Enterprises of the Republic of Indonesia Number 11/PER/M.KUKM/XII/2017 concerning the Implementation of savings and loan business activities and sharia financing by cooperatives which provides the understanding that KSPPS Baytul Ikhtiar is a cooperative whose business activities are carried out in in the fields of financing, investment and savings according to the profit sharing pattern (syariah). One of the contracts used by KSPPS Baytul Ikhtiar in buying and selling based financing transactions is Murabahah. Murabahah is a sale and purchase contract where the institution acts as the seller and the customer as the buyer. The aim of the research is to determine the implementation of murabahah financing at KSPPS Baytul Ikhtiar. This research method includes a type of field research with a descriptive analytical approach to present the data obtained in the field and then analyze it and reach conclusions. The results of the research show that the implementation of murabahah financing products at KSPPS Baytul Ikhtir is in accordance with sharia principles because they have implemented a murabaha contract although there are still things that must strictly comply with these principles.

Keywords: Murabah Agreement . Financing
‘We’re All Sinners Here’: A Microhistorical Exploration of the Deviance-Identification Nexus
Authors: Sadeghi Yasaman 
Published: January 2024

Extant research shows that deviance as a departure from established norms is influential to innovation and change. However, challenging the embedded assumptions and practices renders deviance subject to heavy stigmatization, compelling the identification of deviance to ensure that deviance can be balanced or controlled for the good of the organization. Yet, this focus often ignores the dynamics between the deviants and their audiences, which also impacts the spread of deviance, since deviance is best understood through actions as well as responses. Because deviance is likely to provoke deep introspection, identification with deviance is an essential, yet underexplored aspect of its spread. This article takes a micro-historical approach to analyze Dogme95, a highly controversial filmmaking movement, where identification with deviance influenced its spread. It elucidates symbolic disruption, straddling identification, and limiting the duration as three stages through which deviance can spread in and around organizations through identification. The article thus contributes to the extant literature by reconciling some theoretical contradictions regarding the spread of deviance despite its negative connotations and provides a novel perspective on the deviance-identification nexus.
Maser Investigation toward Off-Plane Stars (MIOPS): Detection of SiO Masers in the Galactic Thick Disk and Halo
Authors: Yang 杨 Wenjin 文锦 , Wu 吴 Yuanwei 元伟 , Gong 龚 Yan 龑 , Mauron Nicolas , Zhang 张 Bo 波 , Menten Karl M. , Mai 麦 Xiaofeng 晓枫 , Liu 刘 Dejian 德剑 , Li 李 Juan 娟 , Li 李 Jingjing 晶晶 
Published: January 2024

Abstract
Studying stars that are located off the Galactic plane is important for understanding the formation history of the Milky Way. We searched for SiO masers toward off-plane O-rich asymptotic giant branch (AGB) stars from the catalog presented by Mauron et al. in order to shed light on the origins of these objects. A total of 102 stars were observed in the SiO J = 1−0, v = 1 and 2 transitions with the Effelsberg 100 m and Tianma 65 m telescopes. SiO masers were discovered in eight stars, all first detections. The measured maser velocities allow for initial estimates of the host AGB stars’ radial velocities. We find that the radial velocities of three stars (namely G068.881−24.615, G070.384−24.886, and G084.453−21.863) significantly deviate from the values expected from Galactic circular motion. The updated distances and 3D motions indicate that G068.881−24.615 is likely located in the Galactic halo, while G160.648−08.846 is probably located in the Galactic thin disk, and the other six stars are probably part of the Galactic thick disk.
Precision MARS Mass Reconstruction of A2744: Synergizing the Largest Strong-lensing and Densest Weak-lensing Data Sets from JWST
Authors: Cha Sangjun , HyeongHan Kim , Scofield Zachary P. , Joo Hyungjin , Jee M. James 
Published: January 2024

Abstract
We present a new high-resolution free-form mass model of A2744 that combines both weak-lensing (WL) and strong-lensing (SL) data sets from JWST. The SL data set comprises 286 multiple images, presenting the most extensive SL constraint to date for a single cluster. The WL data set, employing photo-z selection, yields a source density of

∼
350

arcmin

−
2

, marking the densest WL constraint ever. The combined mass reconstruction enables the highest-resolution mass map of A2744 within the ∼1.8 Mpc × 1.8 Mpc reconstruction region to date, revealing an isosceles triangular structure with two legs of ∼1 Mpc and a base of ∼0.6 Mpc. Although our algorithm, which is called MAximum-entropy ReconStruction (MARS), is entirely blind to the cluster galaxy distribution, the resulting mass reconstruction traces the brightest cluster galaxies remarkably well. The five strongest mass peaks coincide with the five most luminous cluster galaxies within ≲2″. We do not detect any unusual mass peaks that are not traced by the cluster galaxies, unlike the findings in previous studies. Our mass model shows the smallest scatter of SL multiple images in both source (∼0.″05) and image (∼0.″1) planes, which is lower than in previous studies by a factor of ∼4. Although MARS represents the mass field with an extremely large number of free parameters (∼300,000), it converges to a solution within a few hours because we use a deep-learning technique. We make our mass and magnification maps publicly available.
Gas Morphology of Milky Way–like Galaxies in the TNG50 Simulation: Signals of Twisting and Stretching
Authors: Waters Thomas K. , Peterson Colton , Emami Razieh , Shen Xuejian , Hernquist Lars , Smith Randall , Vogelsberger Mark , Alcock Charles , Tremblay Grant , Liska Matthew , Forbes John C. , Moreno Jorge 
Published: January 2024

Abstract
We present an in-depth analysis of gas morphologies for a sample of 25 Milky Way–like galaxies from the IllustrisTNG TNG50 simulation. We constrain the morphology of cold, warm, hot gas, and gas particles as a whole using a local shell iterative method and explore its observational implications by computing the hard-to-soft X-ray ratio, which ranges between 10−3 and 10−2 in the inner ∼50 kpc of the distribution and 10−5–10−4 at the outer portion of the hot gas distribution. We group galaxies into three main categories: simple, stretched, and twisted. These categories are based on the radial reorientation of the principal axes of the reduced inertia tensor. We find that a vast majority (77%) of the galaxies in our sample exhibit twisting patterns in their radial profiles. Additionally, we present detailed comparisons between (i) the gaseous distributions belonging to individual temperature regimes, (ii) the cold gas distributions and stellar distributions, and (iii) the gaseous distributions and dark matter (DM) halos. We find a strong correlation between the morphological properties of the cold gas and stellar distributions. Furthermore, we find a correlation between gaseous distributions with a DM halo that increases with gas temperature, implying that we may use the warm–hot gaseous morphology as a tracer to probe the DM morphology. Finally, we show gaseous distributions exhibit significantly more prolate morphologies than the stellar distributions and DM halos, which we hypothesize is due to stellar and active galactic nucleus feedback.
Can Emission Measure Distributions Derived from Extreme-ultraviolet Images Accurately Constrain High-temperature Plasma?
Authors: Athiray P. S. , Winebarger Amy R. 
Published: January 2024

Abstract
Measuring the relative amount of high-temperature, low emission measure (EM) plasma is considered to be a smoking-gun observation to constrain the frequency of plasma heating in coronal structures. Often, narrowband, extreme-ultraviolet images, such as those obtained by the Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO), are used to determine the EM distribution, though the sensitivity to high-temperature plasma is limited. Conversely, the soft X-ray wavelength range offers multiple high-temperature diagnostics, including emission lines of N vii, O vii, O viii, Fe xvii, Ne ix, and Mg xi, which can provide tight constraints to the high-temperature plasma in the log T = 6.1–6.7 (∼1–5+ MK) range. The Marshall Grazing Incidence X-ray Spectrometer (MaGIXS), a slitless spectrograph launched on a NASA sounding rocket on 2021 July 30, resolved an X-ray-bright point in multiple emission lines in the soft X-ray wavelength range. Using coordinated observations of the same X-ray-bright point from SDO/AIA, we compare and contrast the EM distributions from the EUV image data, the X-ray spectra, and the combined EUV and X-ray data set. In this paper, we demonstrate that EM distributions from SDO/AIA data alone can overestimate the amount of high-temperature (log T > 6.4) plasma in the solar corona by a factor of 3–15. Furthermore, we present our effort to cross-calibrate Hinode/X-ray Telescope (XRT) response functions by comparing the observed XRT fluxes with the predicted ones from combined MaGIXS-1 + AIA EM analysis.
Tectonics and Seismicity of the Lunar South Polar Region
Authors: Watters T. R. , Schmerr N. C. , Weber R. C. , Johnson C. L. , Speyerer E. J. , Robinson M. S. , Banks M. E. 
Published: January 2024

Abstract
The lunar south pole regions are subjected to global stresses that result in contractional deformation and associated seismicity. This deformation is mainly expressed by lobate thrust fault scarps; examples are globally distributed, including polar regions. One small cluster of lobate scarps falls within the de Gerlache Rim 2 Artemis III candidate landing region. The formation of the largest de Gerlache scarp, less than 60 km from the pole, may have been the source of one of the strongest shallow moonquakes recorded by the Apollo Passive Seismic Network. The scarp is within a probabilistic space of relocated epicenters for this event determined in a previous study. Modeling suggests that a shallow moonquake with an M

w
of ∼5.3 may have formed the lobate thrust fault scarp. We modeled the peak ground acceleration generated by such an event and found that strong to moderate ground shaking is predicted at a distance from the source of at least ∼40 km, while moderate to light shaking may extend beyond ∼50 km. Models of the slope stability in the south polar region predict that most of the steep slopes in Shackleton crater are susceptible to regolith landslides. Light seismic shaking may be all that is necessary to trigger regolith landslides, particularly if the regolith has low cohesion (on the order of ∼0.1 kPa). The potential of strong seismic events from active thrust faults should be considered when preparing and locating permanent outposts and pose a possible hazard to future robotic and human exploration of the south polar region.
Three-Dimensional Ultrasound Imaging of Retinoblastoma and Its Correlation With Pathology
Authors: Ramasubramanian Aparna , Riemann Monique , Brown Alex , Tukan Alyson , Tiwari Nishant , Abruzzo Todd , Goncalves Luis F. 
Published: January 2024

Background and Objective:
Monitoring the response of retinoblastoma to globe-salvaging therapies is based on subjective assessments of changes determined by fundoscopy, ultrasound, and optical coherence tomography. Advances in organ-preserving therapies have increased the need for objective, quantitative estimates of tumor response to treatment. Primary tumor volume is a metric that can be objectively determined as a surrogate measure of treatment response.

Patients and Methods:
We evaluated the correlation of objective, quantitative estimates of tumor volume made with two-dimensional (2D) and three-dimensional (3D) ultrasound with gold standard pathological tumor volumes derived by analysis of enucleation specimens.

Results:

Twelve eyes in 12 patients undergoing primary enucleation were evaluated by 2D and 3D ultrasound during ophthalmic examination under anesthesia prior to enucleation. 2D- and 3D-ultra-sound measurements of tumor volume were both strongly correlated with pathological estimates of tumor volume (
r
= 0.69,
P
= 0.018; and
r
= 0.66,
P
= 0.027, respectively).

Conclusions:
2D- and 3D-ultrasound measurements of retinoblastoma primary tumor volume are highly correlated with pathological estimates. 3D measurements are easy to perform with volumetric probes and consider the irregular morphology of the tumor. Further study should be undertaken to evaluate the performance of these metrics as surrogate markers of tumor response to treatment.

[
Ophthalmic Surg Lasers Imaging Retina
2024;55:136–140.]
Exploring Travel Medicine Perspectives among Primary Care Physicians in Kurnool District: A Comprehensive Study of Knowledge, Attitudes, and Practices
Authors: Satharla Rajesh Raja , Ahad Hindustan Abdul 
Published: January 2024

Abstract

Background and Aim:
The study’s purpose is to improve the quality of care for both local residents and travelers in the Kurnool district by identifying and addressing gaps and barriers. The main objective of the research was to assess the knowledge, attitudes, and practical implementation of travel medicine among primary health-care physicians working in the Kurnool district.

Materials and Methods:
The research utilized a descriptive cross-sectional study design. A total of 397 primary care doctors in the Kurnool area participated. Data were collected through a self-administered questionnaire, which covered sociodemographic factors, travel medicine knowledge, attitudes, and practices.

Results:
The study revealed that a significant portion (around 79.5%) of the participants reported providing travel health advice at some point. The primary source of information on travel medicine for most participants (66%) was the Ministry of Health’s travel guides. However, the study identified a knowledge gap, as 11.4% of individuals were unaware of the origin of typhoid infection. The most common health issues reported during posttrip consultations were diarrhea and respiratory infections.

Conclusion:
The study’s findings suggested that the general practitioners in the Kurnool district had insufficient knowledge, attitudes, and practices concerning travel medicine. This underscores the need for additional education and training in travel medicine to improve traveler health care and reduce the risk of preventable diseases.
Yolk Sac Tumor in Ascitic Fluid – Cytodiagnosis of a Rare Case
Authors: Mehraj Meesa , Aden Durre , Khan Sabina , Ahmad Nehal , Jetley Sujata 
Published: January 2024

Abstract
Yolk sac tumor (YST) is a germ cell tumor of gonads presenting in children and young adults. It is rare to find metastasis of the YST in effusion fluid. We report a case of a YST in a 17-year-old female diagnosed on cytological examination of ascitic fluid and confirmed histologically after resection as YST. This case not only highlights the rare possibility of metastasis of the YST in ascitic fluid cytology but also emphasizes the diagnostic dilemma it causes in diagnosing such cases in body fluids. Detailed clinical history including the age of the patient, along with serum alpha-fetoprotein (AFP) levels is essential to a make a preoperative diagnosis. Histopathology with AFP immunohistochemistry confirms the diagnosis of such lesions.
Comparison of quantification of intraretinal hard exudates between optical coherence tomography en face image versus fundus photography
Authors: Park Donghee , Kim Kyoung Lae , Park Sung Pyo , Kim Yong-Kyu 
Published: January 2024

Purpose:
To compare the quantification of intraretinal hard exudate (HE) using en face optical coherence tomography (OCT) and fundus photography.

Methods:
Consecutive en face images and corresponding fundus photographs from 13 eyes of 10 patients with macular edema associated with diabetic retinopathy or Coats’ disease were analyzed using the machine-learning-based image analysis tool, “ilastik.”

Results:
The overall measured HE area was greater with en face images than with fundus photos (en face: 0.49 ± 0.35 mm2 vs. fundus photo: 0.34 ± 0.34 mm2, P < 0.001). However, there was an excellent correlation between the two measurements (intraclass correlation coefficient [ICC] = 0.844). There was a negative correlation between HE area and central macular thickness (CMT) (r = -0.292, P = 0.001). However, HE area showed a positive correlation with CMT in the previous several months, especially in eyes treated with anti-vascular endothelial growth factor (VEGF) therapy (CMT 3 months before: r = 0.349, P = 0.001; CMT 4 months before: r = 0.287, P = 0.012).

Conclusion:
Intraretinal HE can be reliably quantified from either en face OCT images or fundus photography with the aid of an interactive machine learning–based image analysis tool. HE area changes lagged several months behind CMT changes, especially in eyes treated with anti-VEGF injections.