bluuebunny/crossref_metadata_2025_split huggingface dataset:
Pelatihan Internet Marketing Bagi Siswa/I SMK KARYA MUDA
Authors: Effendi Muhammad Ridwan , . Danarti Hariani 
Published: September 2024

ABSTRACTÂ Karya Muda Vocational School is a tourism vocational school located in the city of Depok. Graduate of. The background to this Community Service activity is that based on the results of the preliminary interviews that have been conducted, it is important to prepare students who have the abilities and skills to be ready to enter the competitive world of work so as to support the fulfillment of these competencies. However, the school is faced with the problem of limited knowledge and understanding of the latest internet marketing as a provision for finding work and independent entrepreneurship among students. Based on the above, this activity aims to provide information to vocational school students/students regarding easy and practical ways to apply internet marketing which can provide students with basic knowledge and skills as provisions for finding work and entrepreneurship. The targets of this service activity are students of Karya Muda Vocational School, Depok, West Java.The method used in this activity is a training/counseling method which includes basic internet marketing training carried out by students as preparation for finding work as well as taking advantage of business opportunities by utilizing information technology. Opportunities in the Digital Marketing sector include reducing numbers unemployment among teenagers and opening up wider opportunities and employment opportunities for teenagers/school age.Â Keywords: Community Service, Digital Marketing, Online Business.
Rancang Bangun Aplikasi Rekrutmen Programmer pada PT. Reka Daya Talenta
Authors: Julfia Fenty Tristanti , Untoro Arie Bayu , Gustiawan Handa , Widodo Yohanes Bowo 
Published: September 2024

Perusahaan PT. Reka Daya Talenta yang bergerak dalam bidang pelatihan dan outsourcing programmer. Perusahaan masih menggunakan sistem manual dalam pengolahan sumber daya manusianya. Dalam proses rekrutmen, pendaftar mendatangi perusahaan dan mengisi formulir pendaftaran dan menunggu pemanggilan interview dari pihak perusahaan. Untuk mempermudah proses pengolahan data rekrutmen, diperlukan sebuah aplikasi khusus berbasis android yang digunakan untuk memudahkan kandidat mendaftarkan diri serta memudahkan pengelolaan data informasi pendaftar sehingga waktu dan kinerja menjadi lebih efektif dan terkontrol. Pengembangan aplikasi bertujuan untuk dapat mempermudah proses mengupdate suatu data sehingga diperoleh informasi yang lebih akurat dan lebih tepat waktu. Metode penelitian ini menggunakan metode R&D (Research and Development) yang mana R&D itu sendiri merupakan metode penelitian yang digunakan untuk menghasilkan produk tertentu dan menguji keefektifan produk tersebut. Metode Pengembangan Sistem menggunakan Metode SDLC (System Development Life Cycle) sedangkan model yang digunakan adalah Waterfall. Sistem ini dibuat dengan menggunakan bahasa Java dan menggunakan database SQL Server. Berdasarkan penelitian yang telah dilakukan, perancangan sistem Informasi Rekrutmen pada PT. Reka Daya Talenta dapat memberikan solusi terhadap permasalahan yang dihadapi dalam proses pengolahan data pendaftaran agar lebih cepat, mudah, dan aman. Kendala dalam proses pendaftaran dan pengelolaan data secara manual yaitu terhambatnya kinerja perusahaan dan besarnya risiko kehilangan atau kerusakan data, dapat diatasi dengan dioperasikannya aplikasi yang telah dikembangkan. Dengan adanya sistem informasi yang sudah terkomputerisasi, mempermudah dalam pendaftaran pelamar dan pengelolaan data.
Mergers and Disintegrations: Political Party Alliance Building in Kenya Between 2002 to 2022
Authors: Kalimi Nduu Bernice , Wekesa Peter Wafula , Mwangi Susan Owino 
Published: September 2024

This study explores the dynamics of political party alliance building in Kenya between 2002 to 2022 following the dissolution of the Kenya African National Union (KANU) as the dominant political entity. Employing a qualitative methodology, the research relies on interviews to gather primary data, providing an in-depth analysis of coalition formation and disbandment patterns in the post-KANU era. The study argues that since 2002, each general election in Kenya has witnessed the emergence of new political parties and alliances, formed primarily to secure electoral victories. However, these coalitions are often short-lived, dissolving soon after elections due to internal disputes, personal ambitions, policy differences, and perceptions of betrayal among members. The paper also contends that political alliances in Kenya are largely transient, driven by immediate electoral goals rather than enduring ideological commitments. The fluid nature of these coalitions indicates that alliances are sustained only as long as they serve the interests of their members. Internal conflicts and personal interests frequently lead to fragmentation, prompting the formation of new alliances aimed at better fulfilling individual ambitions and ensuring political success. This continual cycle of coalition formation and dissolution underscores the dynamic and often unstable nature of Kenyan politics, where alliances survive only until ideological differences and personal interests lead to their disintegration
Pengaruh Problem Solving terhadap Berpikir Kreatif di Moderasi Self-Regulated Learning
Authors: Oktariani Mutiya 
Published: September 2024

One of the essential elements of education for the twenty-first century that students must possess and develop is creative thinking. The purpose of this study was to ascertain how problem-solving techniques and self-regulated learning strategies combine to influence the capacity for creative thought. This study used a 2x3 factorial design and was quasi-experimental in nature. Questionnaires on self-regulated learning and tests of creative thinking were used to gather the data. Two-way ANOVA was used to analyze the data in SPSS Version 25. Based on the research that has been conducted argue that the effect of interaction between proble solving and self-regulated learning on creative thinking skill obtained F count value 13,763 with P = 0,000 < 0,05 it means that was and effect of the interaction between problem solving and self-regulated learning on creative thinking skill. Based on the result it was concluded that very effective in increasing creative thinking skill used problem solving and self-regulated learning.
The brief mind wandering three-factor scale (BMW-3)
Authors: Schubert Anna-Lena , Frischkorn Gidon T. , Sadus Kathrin , Welhaf Matthew S. , Kane Michael J. , Rummel Jan 
Published: September 2024

AbstractIn recent years, researchers from different fields have become increasingly interested in measuring individual differences in mind wandering as a psychological trait. Although there are several questionnaires that allow for an assessment of people’s perceptions of their mind wandering experiences, they either define mind wandering in a very broad sense or do not sufficiently separate different aspects of mind wandering. Here, we introduce the Brief Mind Wandering Three-Factor Scale (BMW-3), a 12-item questionnaire available in German and English. The BMW-3 conceptualizes mind wandering as task-unrelated thought and measures three dimensions of mind wandering: unintentional mind wandering, intentional mind wandering, and meta-awareness of mind wandering. Based on results from 1038 participants (823 German speakers, 215 English speakers), we found support for the proposed three-factorial structure of mind wandering and for scalar measurement invariance of the German and English versions. All subscales showed good internal consistencies and moderate to high test–retest correlations and thus provide an effective assessment of individual differences in mind wandering. Moreover, the BMW-3 showed good convergent validity when compared to existing retrospective measures of mind wandering and mindfulness and was related to conscientiousness, emotional stability, and openness as well as self-reported attentional control. Lastly, it predicted the propensity for mind wandering inside and outside the lab (as assessed by in-the-moment experience sampling), the frequency of experiencing depressive symptoms, and the use of functional and dysfunctional emotion regulation strategies. All in all, the BMW-3 provides a brief, reliable, and valid assessment of mind wandering for basic and clinical research.
Impact of Consumer Motivation and Behavior on Social Instagram Media Platforms Somethinc Skincare Purchases
Authors: Natalia Ros , Sutawidjaya Ahmad Hidayat 
Published: September 2024

In the current digital era, sosial media has become a highly influential platform in the consumer decision-making process, especially in the beauty industry. Instagram, as one of the leading sosial media platforms, plays a significant role in shaping consumer preferences and behaviors related to skincare products. This study aims to examine the impact of consumer motivation and behavior on the purchase of Somethinc skincare products on the Instagram sosial media platform. This research employs a quantitative approach with an explanatory method. The sampling technique used is Non-Probability Sampling with Purposive Sampling, involving a sample size of 100 individuals. The results of the study indicate that intrinsic motivation has a positive influence on purchase decisions, extrinsic motivation also has a positive influence on purchase decisions, and knowledge about the product positively and significantly affects the purchase of Somethinc skincare. However, the attitude toward the product does not have a positive and significant impact on the purchase of Somethinc skincare.
Keywords: Motivation, Consumer Behavior, Purchase, Instagram Sosial Media Platform.
Volatile Elements Characterized by MarSCoDe in Materials at Zhurong Landing Site
Authors: Zhang Yizhong , Ren Xin , Chen Zhaopeng , Luo Yuxuan , Chen Wangli , Liu Jianjun , Liu Xiangfeng , Zhang Zhenqiang , Xu Weiming , Shu Rong , Li Chunlai 
Published: September 2024

Abstract
The study of volatile elements on the Martian surface is a critical way to explore the geological evolution history of Mars. Volatile elements such as hydrogen (H), sulfur (S), and chlorine (Cl) on the Martian surface act as proxies for the potential aqueous or atmospheric environments that formed their corresponding phases. In this work, data collected from the Laser Induced Breakdown Spectroscopy and the Short Wave Infrared Spectroscopy of the Mars Surface Composition Detection onboard the Zhurong rover are employed to analyze the volatile elements (H, S, Cl) and their carriers in materials throughout the landing site. We found that S primarily concentrates in gypsum and other sulfates, and the carriers of H include hydrous mineral combinations such as gypsum, hydrated silica, and ferrihydrite. These altered minerals are probably the products of acid weathering processes, which may have occurred mostly during the relatively humid period of the Zhurong landing site since Amazonian.
JWST NIRSpec Spectroscopy of the Triply Lensed z = 10.17 Galaxy MACS0647–JD
Authors: Hsiao Tiger Yu-Yang , Abdurro’uf  , Coe Dan , Larson Rebecca L. , Jung Intae , Mingozzi Matilde , Dayal Pratika , Kumari Nimisha , Kokorev Vasily , Vikaeus Anton , Brammer Gabriel , Furtak Lukas J. , Adamo Angela , Andrade-Santos Felipe , Antwi-Danso Jacqueline , Bradač Maruša , Bradley Larry D. , Broadhurst Tom , Carnall Adam C. , Conselice Christopher J. , Diego Jose M. , Donahue Megan , Eldridge Jan J. , Fujimoto Seiji , Henry Alaina , Hernandez Svea , Hutchison Taylor A. , James Bethan L. , Norman Colin , Park Hyunbae , Pirzkal Norbert , Postman Marc , Ricotti Massimo , Rigby Jane R. , Vanzella Eros , Welch Brian , Wilkins Stephen M. , Windhorst Rogier A. , Xu Xinfeng , Zackrisson Erik , Zitrin Adi 
Published: September 2024

Abstract
We present JWST/NIRSpec prism spectroscopy of MACS0647−JD, a triply lensed z ∼ 11 candidate discovered in Hubble Space Telescope imaging and spatially resolved by JWST imaging into two components, A and B. Spectroscopy of component A yields a spectroscopic redshift z = 10.17 based on seven detected emission lines: C iii] λ
λ1907, 1909, [O ii] λ3727, [Ne iii] λ3869, [Ne iii] λ3968, Hδ
λ4101, Hγ
λ4340, and [O iii] λ4363. These are the second-most distant detections of these emission lines to date, in a galaxy observed just 460 million years after the Big Bang. Based on observed and extrapolated line flux ratios we derive a gas-phase metallicity 12 + log(O/H) ∼ 7.5–8.0, or Z ∼ (0.06–0.2) Z
⊙, ionization parameter

log
(
U
)

= −1.9 ± 0.2, and an ionizing photon production efficiency

log
(

ξ

ion

)
=
25.2
±
0.2

erg−1 Hz. The spectrum has a softened Lyα break, evidence for a strong Lyα damping wing. The Lyα damping wing also suppresses the F150W photometry, explaining the slightly overestimated photometric redshift z = 10.6 ± 0.3. MACS0647−JD has a stellar mass log(M/M
⊙) = 8.1 ± 0.3, including ∼6 × 107
M
⊙ in component A, most of which formed recently (within ∼20 Myr) with a star formation rate ∼ 2 ± 1 M
⊙ yr−1, all within an effective radius 70 ± 24 pc. Spectroscopy of a fainter companion galaxy C separated by a distance of ∼ 3 kpc reveals a Lyman break consistent with z ∼ 10.17. MACS0647−JD is likely the most distant galaxy merger known.
Kappa-tail Technique: Modeling and Application to Solar Energetic Particles Observed by Parker Solar Probe
Authors: Livadiotis G. , Cummings A. T. , Cuesta M. E. , Bandyopadhyay R. , Farooki H. A. , Khoo L. Y. , McComas D. J. , Rankin J. S. , Sharma T. , Shen M. M. , Cohen C. M. S. , Muro G. D. , Xu Z. 
Published: September 2024

Abstract
We develop the kappa-tail fitting technique, which analyzes observations of power-law tails of distributions and energy flux spectra, and connects them to theoretical modeling of kappa distributions, to determine the thermodynamics of the examined space plasma. In particular, we (i) construct the associated mathematical formulation; (ii) prove its decisive lead for determining whether the observed power-law is associated with kappa distributions; and (iii) provide a validation of the technique using pseudo-observations of typical input plasma parameters. Then, we apply this technique to a case study by determining the thermodynamics of solar energetic particle (SEP) protons, for an SEP event observed on 2021 April 17, by the Parker Solar Probe (PSP)/Integrated Science Investigation of the Sun instrument suite on board PSP. The results show SEP temperatures and densities of the order of ∼1 MeV and ∼5 × 10−7 cm−3, respectively.
Influence of Black Hole Kick Velocity on Microlensing Distributions
Authors: Koshimoto Naoki , Kawanaka Norita , Tsuna Daichi 
Published: September 2024

Abstract
The natal kick velocity distribution for black holes (BHs) is unknown regardless of its importance for understanding the BH formation process. Gravitational microlensing is a unique tool for studying the distribution of BHs in our Galaxy, and the first isolated stellar-mass BH event, OGLE-2011-BLG-0462/MOA-2011-BLG-191 (OB110462), was recently identified by astrometric microlensing. This study investigates how the natal kick velocity for Galactic BHs affects the microlensing event rate distribution. We consider a Maxwell distribution with various average kick velocities, as well as the consequent variation of the spatial distribution of BHs. We find that the event rate for the BH lenses toward the Galactic bulge decreases as v
avg increases, mainly due to the scale height inflation. We focus on the unique microlensing parameters measured for OB110462, with microlens parallax π
E larger than 0.06 for its long timescale of t
E > 200 days. We calculate the expected number of BH events occurring with parameters similar to OB110462 during the OGLE-IV survey by Mróz et al. and compare it with the actual number that occurred, at least one. Our fiducial model predicts 0.52, 0.38, 0.18, 0.042, and 4.0 × 10−3 events occurring for v
avg = 25, 50, 100, 200, and 400 km s−1, respectively, which suggests that the average kick velocity is likely to be v
avg ≲ 100 km s−1. The expected number smaller than unity even at maximum might indicate our luck in finding OB110462, which can be tested with future surveys by, e.g., the Roman Space Telescope.
The Carousel Lens: A Well-modeled Strong Lens with Multiple Sources Spectroscopically Confirmed by VLT/MUSE
Authors: Sheu William , Cikota Aleksandar , Huang Xiaosheng , Glazebrook Karl , Storfer Christopher , Agarwal Shrihan , Schlegel David J. , Suzuki Nao , Barone Tania M. , Bian Fuyan , Jeltema Tesla , Jones Tucker , Kacprzak Glenn G. , O’Donnell Jackson H. , G. C. Keerthi Vasan 
Published: September 2024

Abstract
Over the past few years alone, the lensing community has discovered thousands of strong lens candidates, and spectroscopically confirmed hundreds of them. In this time of abundance, it becomes pragmatic to focus our time and resources on the few extraordinary systems, in order to most efficiently study the Universe. In this paper, we present such a system: DESI-090.9854-35.9683, a cluster-scale lens at z
l = 0.49, with seven observed lensed sources around the core, and additional lensed sources further out in the cluster. From the number and the textbook configuration of the lensed images, a tight constraint on the mass potential of the lens is possible. This would allow for detailed analysis on the dark and luminous matter content within galaxy clusters, as well as a probe into dark energy and high-redshift galaxies. We present our spatially resolved kinematic measurements of this system from the Very Large Telescope Multi Unit Spectroscopic Explorer, which confirm five of these source galaxies (in ascending order, at z
s = 0.962, 0.962, 1.166, 1.432, and 1.432). With previous Hubble Space Telescope imaging in the F140W and F200LP bands, we also present a simple flux-based lens model consisting of two power-law profiles that, for a cluster lens, well models the five lensed arc families with redshifts. We determine the mass to be M(< θ
E) = 4.78 × 1013
M
⊙ for the primary mass potential. From the model, we extrapolate the redshift of one of the two source galaxies not yet spectroscopically confirmed to be at

z

s

=

4.52

−
0.71

+
1.03

.
Study Assessing Use of Mood Stabilizers (Sodium Valproate and Oxcarbazepine) as an Augmentation Strategy in Patients of Treatment-resistant Depression
Authors: Chugh Priya , Mahapatro Fiona 
Published: September 2024

Abstract

Background:
Treatment-resistant depression (TRD) is a major challenge, with a significant proportion of patients failing to achieve remission with initial antidepressant treatment. As per literature, augmentation strategies using nonantidepressant agents have been explored to overcome partial or lack of response. This study aimed to determine the efficacy of adding mood stabilizers, sodium valproate, and oxcarbazepine as augmenting agents in patients with TRD.

Methodology:
This prospective and observational study recruited 106 patients with TRD from a tertiary care center in Navi Mumbai, India. Patients were augmented with either sodium valproate (n = 53) or oxcarbazepine (n = 53) in addition to their ongoing antidepressant and anti-anxiety medications. The Hamilton Depression Rating Scale (HAM-D) and Hamilton Anxiety Rating Scale (HAM-A) were administered at baseline, at 2 weeks, and at 4 weeks after augmentation. Treatment response was documented, and results were statistically analyzed.

Results:
Both augmentation groups showed significant improvements in HAM-D and HAM-A scores at 2 and 4 weeks compared to baseline (P < 0.001). However, the sodium valproate group demonstrated superior efficacy, with a greater reduction in HAM-D scores as compared to the oxcarbazepine group at 2 weeks (25.60 vs. 21.98, P = 0.001) and 4 weeks (34.06 vs. 30.64, P = 0.001).

Conclusion:
The addition of mood stabilizers, sodium valproate, and oxcarbazepine, as augmentation agents led to significant improvement in patients with TRD. Sodium valproate exhibited superior efficacy as compared to oxcarbazepine, suggesting its potential as a valuable augmentation strategy in the management of TRD.
Cardiometabolic Crossroads: Obesity, Sleep-Disordered Breathing, and Epicardial Adipose Tissue in Heart Failure with Preserved Ejection Fraction – A Mini-Review
Authors: Cacciapuoti Fulvio , Mauro Ciro , Capone Valentina , Sasso Angelo , Tarquinio Luca Gaetano , Cacciapuoti Federico 
Published: September 2024

Abstarct
Obesity, a multifaceted metabolic disorder, stands out as a significant risk factor in the development of heart failure with preserved ejection fraction (HFpEF). Its involvement in HFpEF pathogenesis encompasses a complex interplay with adipose tissue, particularly epicardial adipose tissue (EAT), and the effects of sleep-disordered breathing (SDB). Understanding these intricate relationships is pivotal for devising targeted therapeutic approaches to alleviate the burden of HFpEF in individuals with obesity. EAT assumes a central role in linking obesity to HFpEF. As it expands in the context of obesity, EAT contributes to systemic inflammation and insulin resistance, fostering an environment conducive to cardiac remodeling and dysfunction. Furthermore, SDB, prevalent comorbidity in the obese population, emerges as a significant mediator in HFpEF pathogenesis through various mechanisms. The convergence of obesity, EAT expansion, and SDB creates a synergistic effect, heightening the risk of HFpEF development. On the pharmaceutical front, ongoing investigations explore novel strategies targeting inflammation, oxidative stress, and metabolic pathways associated with obesity. These include the potential roles of sodium-glucose cotransporter 2 inhibitors and glucagon-like peptide-1 receptor agonists, offering innovative therapeutic avenues for managing HFpEF in individuals with obesity. In addition, lifestyle modifications such as weight management and interventions addressing SDB and EAT reduction emerge as promising approaches for preventing and managing HFpEF in the obese population. These interventions hold the potential to mitigate obesity-related cardiac risks and improve HFpEF outcomes.