bluuebunny/crossref_metadata_2025_split huggingface dataset:
Pengaruh Mental Toughness dan Employee Experience Terhadap Organizational Commitment Dengan Psychological Well-Being Sebagai Mediator Pada Karyawan Generasi Z di Jakarta
Authors: Rumindang Simanjuntak Fitrinita , Emilisa Netania , Puspa Tiara 
Published: December 2023

Organizational commitment is an important factor for companies in improving their productivity and performance. However, there are stereotypes related to the commitment of Generation Z employees who are new to the workplace, namely, a tendency to be disloyal and a low commitment to the organization. The study aims to analyse the impact of Mental Toughness and Employee Experience on Organizational Commitment with Psychological Well-Being as Mediator on Generation Z Employees in Jakarta. Generation Z is the generation of professionals born between 1997 and 2005 who have recently entered the world of work. This research uses analytical techniques with quantitative methods with a survey approach. A sample of 125 Generation Z employees at a start-up company in Jakarta. The research data was collected using a Likert-scale questionnaire that had 25 statement items that included four variables: mental toughness, employee experience, psychological well-being, and organizational commitment. Hypothesis testing uses SEM (Structural Equation Modelling) as well as SPSS and AMOS software to process data. The results of the study show that Mental toughness has a positive influence on Psychological well-being, Employee experience has a positively influenced psychological wellness, Psychological wellness has a negative influence upon Organizational commitment, and Psychological welfare has a mediating influence between mental toughness and Organizational engagement and the absence of Psychological Well-Being as a mediation between employee experience and Organizational commitment.
Inhibition Test of Ethanol from Extract Mangosteen Leaves (Garcinia mangostana L.) as an Acne Antibacterial
Authors: Ginting Junius Gian , Br. Singarimbun Nurbaiti , Daeli Mestika Clemesiya Yulianti , Simanjuntak Helen Anjelina , Purba Hermawan , Br. Barus Lydia , Zega Defcato Firmawati 
Published: December 2023

A prevalent global infection that manifests frequently in Indonesia. An example of an infectious disease that is commonly encountered during adolescence is acne (Acne vulgaris). Antibiotics can be used to treat acne; however, their misuse can lead to the development of resistance; therefore, we are searching for inexpensive, readily available alternatives that are also secure. Mangosteen leaves (Garcinia mangostana L.)Â are one alternative to synthetic ingredients when it comes to the treatment of acne. Mangosteen leaves comprise xanthone derivative compounds that exhibit significant biological activity, including antioxidant, antibacterial, and antimicrobial properties. Therefore, this this study aimed to ascertain the inhibitory power of an ethanol extract derived from mangosteen leaves in order to determine its antibacterial activity against Staphylococcus epidermidis bacteria. Additionally, the compound content of the ethanol extract of mangosteen leaves was determined. The inhibition test was conducted by utilizing the paper disc technique, while the extraction method employed the maceration method. As indicated by the phytochemical screening test results, simplicia and ethanol extract of mangosteen leaves were found to contain steroids/triterpenoids, alkaloids, flavonoids, saponins, and tannins. The inhibition test outcomes against Staphylococcus epidermidis bacteria revealed the following: a diameter of 3.3 mm for bacteria at a concentration of 20%, 9.4 mm for bacteria at 40%, 10.4 mm for bacteria at 60%, 12.9 mm for bacteria at 80%, and 13.2 mm for bacteria at 100%
Peran Subbagian Advokasi Dan Dokumentasi Hukum Sekertariat Jenderal Dalam Penyelesaian Sengketa MPR RI
Authors: Hafizd Jefik Zulfikar , Harahap Viviyen Jensifa 
Published: December 2023

This journal is motivated by the idea that the role of advocacy in dispute resolution is needed as an advocate who acts as an advisor or defender of cases in court. As one of the people's representative bodies or the legislature of the People's Consultative Assembly consisting of members of the People's Representative Council and Regional Representative Councils elected through general elections, it is certainly not spared from the many disputes or cases submitted by the community who are increasingly critical of existing policies to the court. In dispute resolution, the People's Consultative Assembly requires the role of the legal section, especially the advocacy subdivision and legal documentation to carry out its duties and functions as an advocate. Which plays a role in providing Exepsies, Duplik, Replications, Submitting evidence against claims by legal entities in court to obtain a decision with permanent legal force.
KEARIFAN LOKAL, MODAL SOSIAL DAN PEMBANGUNAN BERKELANJUTAN
Authors: Sagajoka Estherlina , Fatima Imaculata 
Published: December 2023

This Research aims to examine and determine the relationship between local wisdom, social capital and sustainable development. The data and information used in writing this article comes from literature studies nd literature reviews of vrious writings and documents relevant to local wisdom, social capital and sustainable development. Both offline library documents written online.
The result of the study show that the relationship between local wisdom (IndigenousKnoledge) and social capital with sustainable development is that local wisdom is the knowledge of local people wwho hve lived in place for a long time, base on values developed from generation. Social capitl is wwht llows local communities to survive and develop sustainably base on local wisdom, Where community knowledge in certain Fields (Economic Activities, Social activities and environmental adaption) is beneficial for the surrounding environment whilw maintaining environmental sustainability, and has been carried out for generations. From generations to generation. Knowledge of costoms and social capital are important factors that have a significant impact on community economic growth and sustainable development. Although formal reseach on Indigenous Konwledge and social capital is still scarce and currently under development, several preliminary studies on mutual cooperation and wwork institutions are very helpful for rural communities, at leas opening wider opportunities as the main benchmark for more intensive and in-depth reseach on working practices and mechanisms as well as the sustainability of lokal wisdom and social capital in Indonesia, especially in rural areas.
Cognitive control and meta-control in dual-task coordination
Authors: Strobach Tilo 
Published: December 2023

AbstractWhen two tasks are presented simultaneously or in close succession, such as in the overlapping task paradigm of the psychological refractory period, dual-task performance on those tasks is usually impaired compared with separate single-task performance. Numerous theories explain these emerging dual-task costs in terms of the existence of capacity limitations in the constituent component tasks. The current paper proposes active dual-task coordination processes that work on the scheduling of these capacity-limited processes. Further, there are recent findings that point to a meta-cognitive control level in addition to these active coordination processes. This additional level’s responsibility is to adjust the dual-task coordination of capacity-limited stages (i.e., coordination adjustment). I review evidence focusing on the existence of dual-task coordination processes and processes of coordination adjustment. The remainder of the paper elaborates on preliminary findings and points to the separability of these sets of processes, which is a key assumption of the framework of dual-task coordination adjustment.
Dimming the Lights: 2D Simulations of Deflagrations of Hybrid C/O/Ne White Dwarfs Using FLASH
Authors: Feldman Catherine , Gutierrez Nathanael , Eisenberg Ellis , Willcox Donald E. , Townsley Dean M. , Calder Alan C. 
Published: December 2023

Abstract
The dimmest and most numerous outlier of the Type Ia supernova population, the Type Iax event, is increasingly being found in the results of observational campaigns. There is currently no single accepted model to describe these events. This 2D study explores the viability of modeling Type Iax events as a hybrid C/O/Ne white dwarf progenitor undergoing a deflagration using the multiphysics software FLASH. This hybrid was created using the stellar evolution code MESA, and its C-depleted core and mixed structure have demonstrated lower yields than traditional C/O progenitors in previous deflagration-to-detonation studies. To generate a sample, 30 “realizations” of this simulation were performed, the only difference being the shape of the initial match head used to start the deflagration. Consistent with earlier work, these realizations produce the familiar hot dense bound remnant surrounded by sparse ejecta. Our results indicate that the majority of the star remains unburned (∼70%) and bound (>90%). Our realizations produce total ejecta yields on the order of 10−2–10−1
M
☉, ejected 56Ni yields on the order of 10−4–10−2
M
☉, and ejecta kinetic energies on the order of 1048–1049 erg. Compared to yields inferred from recent observations of the dimmest Type Iax events—SN 2007qd, SN 2008ha, SN 2010ae, SN 2019gsc, SN 2019muj, SN 2020kyg, and SN 2021fcg—our simulation produces comparable 56Ni yields but too-small total yields and kinetic energies. Reignition of the remnant is also seen in some realizations.
High-sensitivity Beamformed Observations of the Crab Pulsar's Radio Emission
Authors: Lin Rebecca , van Kerkwijk Marten H. 
Published: December 2023

Abstract
We analyzed four epochs of beamformed European VLBI Network data of the Crab Pulsar at 1658.49 MHz. With the high sensitivity resulting from resolving out the Crab Nebula, we are able to detect even the faint high-frequency components in the folded profile. We also detect a total of 65,951 giant pulses, which we use to investigate the rates, fluence, phase, and arrival time distributions. We find that for the main pulse component, our giant pulses represent about 80% of the total flux. This suggests we have a nearly complete giant pulse energy distribution, although it is not obvious how the observed distribution could be extended to cover the remaining 20% of the flux without invoking large numbers of faint bursts for every rotation. Looking at the difference in arrival time between subsequent bursts in single rotations, we confirm that the likelihood of finding giant pulses close to each other is increased beyond that expected for randomly occurring bursts—some giant pulses consist of causally related microbursts, with typical separations of ∼30 μs—but also find evidence that at separations ≳100 μs the likelihood of finding another giant pulse is suppressed. In addition, our high sensitivity enabled us to detect weak echo features in the brightest pulses (at ∼0.4% of the peak giant pulse flux), which are delayed by up to ∼300 μs.
Scale Invariance in Gamma-Ray Flares of the Sun and 3C 454.3
Authors: Peng Fang-Kun , Wei Jun-Jie , Wang Hai-Qin 
Published: December 2023

Abstract
Using the gamma-ray flare samples of the Sun and 3C 454.3 observed by the Fermi telescope, we investigate the statistical properties of sizes including fluence (energy), peak flux (luminosity), duration time, and waiting time in this work. We find that the cumulative distribution of the fluctuations of these sizes follow well the Tsallis q-Gaussian function. The obtained q values from q-Gaussian distribution remain stable around 2 without any significant change, implying that there is a scale invariance structure in gamma-ray flares of the Sun and 3C 454.3. This scale invariance characteristics of the Sun and 3C 454.3 indicated by q values are also comparable to those of earthquakes, soft gamma repeaters, fast radio burst (FRB 20121102), and X-ray flares of gamma-ray bursts. On top of that, we verify the relationship between q values and the power-law indices α from the size frequency distributions, which is expressed as q = (α + 2)/α. These statistical findings could be well explained within the physical framework of a self-organizing criticality system.
Explaining the Chemical Inventory of Orion KL through Machine Learning
Authors: Scolati Haley N. , Remijan Anthony J. , Herbst Eric , McGuire Brett A. , Lee Kin Long Kelvin 
Published: December 2023

Abstract
The interplay of the chemistry and physics that exists within astrochemically relevant sources can only be fully appreciated if we can gain a holistic understanding of their chemical inventories. Previous work by Lee et al. demonstrated the capabilities of simple regression models to reproduce the abundances of the chemical inventory of the Taurus Molecular Cloud 1 (TMC-1), as well as to provide abundance predictions for new candidate molecules. It remains to be seen, however, to what degree TMC-1 is a “unicorn” in astrochemistry, where the simplicity of its chemistry and physics readily facilitates characterization with simple machine learning models. Here we present an extension in chemical complexity to a heavily studied high-mass star-forming region: the Orion Kleinmann–Low (Orion KL) nebula. Unlike TMC-1, Orion KL is composed of several structurally distinct environments that differ chemically and kinematically, wherein the column densities of molecules between these components can have nonlinear correlations that cause the unexpected appearance or even lack of likely species in various environments. This proof-of-concept study used similar regression models sampled by Lee et al. to accurately reproduce the column densities from the XCLASS fitting program presented by Crockett et al.
The Close AGN Reference Survey (CARS): An Interplay between Radio Jets and AGN Radiation in the Radio-quiet AGN HE0040-1105
Authors: Singha M. , Winkel N. , Vaddi S. , Perez Torres M. , Gaspari M. , Smirnova-Pinchukova I. , O’Dea C. P. , Combes F. , Omoruyi Osase , Rose T. , McElroy R. , Husemann B. , Davis T. A. , Baum S. A. , Lawlor-Forsyth C. , Neumann J. , Tremblay G. R. 
Published: December 2023

Abstract
We present a case study of HE 0040-1105, an unobscured radio-quiet active galactic nucleus (AGN) at a high accretion rate of λ
Edd = 0.19 ± 0.04. This particular AGN hosts an ionized gas outflow with the largest spatial offset from its nucleus compared to all other AGNs in the Close AGN Reference Survey. By combining multiwavelength observations from the Very Large Telescope/MUSE, Hubble Space Telescope/Wide Field Camera 3, Very Large Array, and European VLBI Network, we probe the ionization conditions, gas kinematics, and radio emission from host galaxy scales to the central few parsecs. We detect four kinematically distinct components, one of which is a spatially unresolved AGN-driven outflow located within the central 500 pc, where it locally dominates the interstellar medium conditions. Its velocity is too low to escape the host galaxy’s gravitational potential, and may be re-accreted onto the central black hole via chaotic cold accretion. We detect compact radio emission in HE 0040-1105 within the region covered by the outflow, varying on a timescale of ∼20 yr. We show that neither AGN coronal emission nor star formation processes wholly explain the radio morphology/spectrum. The spatial alignment between the outflowing ionized gas and the radio continuum emission on 100 pc scales is consistent with a weak jet morphology rather than diffuse radio emission produced by AGN winds. >90% of the outflowing ionized gas emission originates from the central 100 pc, within which the ionizing luminosity of the outflow is comparable to the mechanical power of the radio jet. Although radio jets might primarily drive the outflow in HE 0040-1105, radiation pressure from the AGN may contribute to this process.
Probing the Galactic Diffuse Continuum Emission with COSI
Authors: Karwin Christopher M. , Siegert Thomas , Beechert Jacqueline , Tomsick John A. , Porter Troy A. , Negro Michela , Kierans Carolyn , Ajello Marco , Martinez-Castellanos Israel , Shih Albert , Zoglauer Andreas , Boggs Steven E. ,   (for the COSI Collaboration)
Published: December 2023

Abstract
In 2016, the Compton Spectrometer and Imager (COSI) had a successful 46 day flight on board NASA’s Super Pressure Balloon platform. In this work, we report measurements of the Galactic diffuse continuum emission (GDCE) observed toward the inner Galaxy during the flight, which in the COSI energy band (0.2–5 MeV) is primarily generated from inverse Compton radiation. Within uncertainties, we find overall good agreement with previous measurements from INTEGRAL/SPI and COMPTEL. Based on these initial findings, we discuss the potential for further probing the GDCE with the 2016 COSI balloon data, as well as prospects for the upcoming satellite mission.
Direct Statistical Constraints on the Natal Kick Velocity of a Black Hole in an X-Ray Quiet Binary
Authors: Banagiri Sharan , Doctor Zoheyr , Kalogera Vicky , Kimball Chase , Andrews Jeff J. 
Published: December 2023

Abstract
In recent years, a handful of “dark” binaries have been discovered with a nonluminous compact object. Astrometry and radial velocity measurements of the bright companion allow us to measure the post-supernova orbital elements of such a binary. In this paper, we develop a statistical formalism to use such measurements to infer the pre-supernova orbital elements, and the natal kick imparted by the supernova (SN). We apply this formalism to the recent discovery of an X-ray quiet binary with a black hole, VFTS 243, in the Large Magellanic Cloud. Assuming an isotropic, Maxwellian distribution on natal kicks and using broad agnostic mass priors, we find that kick velocity can be constrained to V

k
< 72 km s−1 at 90% confidence. We find that a Blaauw kick cannot be ruled out, and that at least about 0.6M
⊙ was lost during the supernova with 90% confidence. The pre-SN orbital separation is found to be robustly constrained to be around 0.3 au.
NuSTAR Hard X-Ray Monitoring of Gravitationally Lensed Quasar RX J1131–1231
Authors: DeFrancesco Cora A. , Dai Xinyu , Mitchell Mark , Zoghbi Abderahmen , Morgan Christopher W. 
Published: December 2023

Abstract
The X-ray emission from active galactic nuclei is believed to come from a combination of inverse Compton scattering of photons from the accretion disk and reprocessing of the direct X-ray emission by reflection. We present hard (10–80 keV) and soft (0.5–8 keV) X-ray monitoring of a gravitationally lensed quasar RX J1131−1231 (hereafter RXJ1131) with NuSTAR, Swift, and XMM-Newton between 2016 June 10 and 2020 November 30. Comparing the amplitude of quasar microlensing variability at the hard and soft bands allows a size comparison, where larger sources lead to smaller microlensing variability. During the period between 2018 June 6 and 2020 November 30, where both the hard and soft light curves are available, the hard and soft bands varied by factors of 3.7 and 5.5, respectively, with rms variability of 0.40 ± 0.05 and 0.57 ± 0.02. Both the variability amplitude and rms are moderately smaller for the hard X-ray emission, indicating that the hard X-ray emission is moderately larger than the soft X-ray emission region. We found the reflection fraction from seven joint hard and soft X-ray monitoring epochs is effectively consistent with a constant with low significance variability. After decomposing the total X-ray flux into direct and reprocessed components, we find a smaller variability amplitude for the reprocessed flux compared to the direct emission. The power-law cutoff energy is constrained at

96

−
24

+
47

keV, which positions the system in the allowable parameter space due to the pair production limit.
Calibration of the Timing Performance of GECAM-C
Authors: Xiao Shuo , Liu Ya-Qing , Gong Ke , An Zheng-Hua , Xiong Shao-Lin , Li Xin-Qiao , Wen Xiang-Yang , Peng Wen-Xi , Zhang Da-Li , Tuo You-Li , Zheng Shi-Jie , Song Li-Ming , Wang Ping , Zhao Xiao-Yun , Huang Yue , Ma Xiang , Liu Xiao-Jing , Qiao Rui , Xu Yan-Bing , Yang Sheng , Zhang Fan , Wang Yue , Zhang Yan-Qiu , Xue Wang-Chen , Liu Jia-Cong , Zheng Chao , Wang Chen-Wei , Tan Wen-Jun , Cai Ce , Yi Qi-Bin , Zhang Peng , Luo Xi-Hong , Yang Jiao-Jiao , Zhi Qi-Jun , Dong Ai-Jun , Dang Shi-Jun , Shang Lun-Hua , Zhang Shuang-Nan 
Published: December 2023

Abstract
As a new member of the Gravitational-wave high-energy Electromagnetic Counterpart All-sky Monitor (GECAM) after GECAM-A and GECAM-B, GECAM-C (originally called HEBS), which was launched on board the SATech-01 satellite on 2022 July 27, aims to monitor and localize X-ray and gamma-ray transients from ∼6 keV to 6 MeV. GECAM-C utilizes a similar design to GECAM but operates in a more complex orbital environment. In this work, we utilize the secondary particles simultaneously produced by the cosmic-ray events on orbit and recorded by multiple detectors to calibrate the relative timing accuracy between all detectors of GECAM-C. We find the result is 0.1 μs, which is the highest time resolution among all GRB detectors ever flown and very helpful in timing analyses such as minimum variable timescale and spectral lags, as well as in time delay localization. Besides this, we calibrate the absolute time accuracy using the one-year Crab Pulsar data observed by GECAM-C and Fermi’s Gamma-ray Burst Monitor, as well as GECAM-C and GECAM-B. The results are 2.02 ± 2.26 μs and 5.82 ± 3.59 μs, respectively. Finally, we investigate the spectral lag between the different energy bands of the Crab Pulsar observed by GECAM and the Gamma-ray Burst Monitor, which is ∼ −0.2 μs keV−1.
Coronal Loop Detection Using Multiscale Convolutional Neural Networks
Authors: Wang Yunzhi , Liang Bo , Feng Song 
Published: December 2023

Abstract
Solar magnetic fields play an important role in many solar activities, such as the solar wind, coronal mass ejections, and coronal oscillation. Coronal loops are curvilinear structures in the solar atmosphere and are closely related to coronal magnetic fields, so the study of their structure is very important. However, it is difficult to identify coronal loops accurately because of the complexity of their features. Therefore, we propose a two-stage detection method, using multiscale convolutional neural networks, to identify coronal loops. The regions including initial coronal loops are first marked by a improved Res-UNet model. The loop structures in the region are then detected using a improved dense extreme inception network for edge detection model. We selected the coronal images observed by the Transition and Coronal Explorer and the Atmospheric Imaging Assembly of the Solar Dynamics Observatory in the 171 Å channel to illustrate the detection processing. Meanwhile, we also compared the accuracy of our method to others. The results demonstrate that our proposed method has a high recognition rate and good robustness over previous identification methods and can be used to study the physical characteristics of coronal loops.
The Jets and the Neutron Star Kick Velocity of the Supernova Remnant CTB 1
Authors: Bear Ealeal , Soker Noam 
Published: December 2023

Abstract
We identify jet-shaped morphology in the core-collapse supernova remnant (SNR) CTB 1 that includes two opposite structural features. We identify these as the imprints of a pair of jets that were among the last jets to explode the massive stellar progenitor of CTB 1. We find the projected angle between the jets’ axis and the direction of the pulsar velocity, which is the neutron star natal kick, to be α = 78°. We tentatively identify possible signatures of a second pair of opposite jets along a different direction. If this identification holds, SNR CTB 1 has a point-symmetric structure. The morphology and large angle of the jets’ axis to kick velocity are expected in the jittering jets explosion mechanism of core-collapse supernovae.