bluuebunny/crossref_metadata_2025_split huggingface dataset:
Analysis of Patient Safety Culture at Semen Padang Hospital Indonesia
Authors: Ladyventini Yona , Isniati  , Wihardi Triman  
Published: July 2023

Background: Hospitals have a role and function to provide integrated health services for patients as consumers of health services. When providing services to patients, hospitals must pay attention to quality and safety. This study aimed to find out the patient safety culture that has been built at Semen Padang Hospital in 2022.
Methods: This study uses an approach mixed methods research with a design sequential explanatory, namely research that uses a combination of quantitative and qualitative methods simultaneously (quantitative-qualitative). The subjects of this study were employees of Semen Padang Hospital, with as many as 81 respondents for quantitative data and 11 respondents for qualitative data. Measurement of patient safety culture using the MaPSaF instrument (Manchester patient safety framework) in the form of filling out the MaPSCAT questionnaire (Manchester patient safety culture assessment tool). This questionnaire consists of 10 dimensions with a total of 24 questions and is equipped with in-depth interview data.
Results: Data collection was carried out using the MaPSCAT instrument on 10 dimensions of patient safety culture, 6 dominant dimensions were at the proactive level, namely the dimension of overall commitment to continuous improvement (1st dimension), the dimension of system error and individual responsibility (3rd dimension), the dimension of incident evaluation and best practices (5th dimension), effective learning and change (6th dimension), communication about patient safety issues (7th dimension) and staff education and training dimension (9th dimension).
Conclusion: The safety culture at Semen Padang Hospital is generally at a proactive level. This indicates that the hospital places priority on improving patient safety and is carried out on an ongoing basis. A system that is integrated and comprehensive has a wide scale, involved stakeholders, and an evidence-based approach.
PENTINGNYA PENYUSUNAN LAPORAN KEUANGAN UNTUK PENILAIAN KINERJA USAHA UMKM DI RW.08 KELURAHAN KAYU PUTIH, PULO GADUNG, JAKARTA TIMUR
Authors: Hartanti Rina , Sipayung Emma Saur Nauli , Hermi Hermi 
Published: July 2023

The success of MSME (Micro, Small and Medium Entities) entrepreneurs in dealing with the impact of the economic crisis either in 1998 or in 2008/2009 is of course inseparable from the commitment of MSME entrepreneurs themselves to continue to improve the performance of their MSME businesses. Assessment of MSME business performance is very important for MSME entrepreneurs in making strategic business decisions correctly and correctly. The right and correct decision can increase the progress of the MSME business, but on the contrary, wrong decision making can pose a risk of failure of the MSME business.So that the decisions taken by MSME entrepreneurs are not wrong, it is necessary to analyze the performance of their MSME businesses. The information needed in analyzing the business performance of MSMEs can be seen in the financial reports prepared by these MSMEs. In practice there are still many MSME entrepreneurs who still think that the preparation of these financial reports is not very important, so that in the end these MSME entrepreneurs cannot analyze their business performance in real terms. For this reason, The Accounting Study Program, Economics and Business Faculty, Trisakti University in collaboration with The Management of Rukun Warga (RW) 08, Kayu Putih Village, Pulo Gadung District, in East Jakarta, held a Community Service (PKM) Program by providing training to MSME entrepreneurs in Rukun Warga (RW) 08, Kayu Putih Village, Pulo Gadung District, East Jakarta, so that these MSMEs can understand and understand the importance of compiling Financial Reports for MSMEs in accordance with applicable Financial Accounting Standards in analyzing real financial performance. The results after the implementation of the PKM were in line with expectations, where participants were very enthusiastic about asking questions about the accounting process, the concept of business entities and answering the given accounting exercise questions, where the results of the assessment obtained an average score of 62 to 73.
Minimal reporting guideline for research involving eye tracking (2023 edition)
Authors: Dunn Matt J. , Alexander Robert G. , Amiebenomo Onyekachukwu M. , Arblaster Gemma , Atan Denize , Erichsen Jonathan T. , Ettinger Ulrich , Giardini Mario E. , Gilchrist Iain D. , Hamilton Ruth , Hessels Roy S. , Hodgins Scott , Hooge Ignace T. C. , Jackson Brooke S. , Lee Helena , Macknik Stephen L. , Martinez-Conde Susana , Mcilreavy Lee , Muratori Lisa M. , Niehorster Diederick C. , Nyström Marcus , Otero-Millan Jorge , Schlüssel Michael M. , Self Jay E. , Singh Tarkeshwar , Smyrnis Nikolaos , Sprenger Andreas 
Published: July 2023

AbstractA guideline is proposed that comprises the minimum items to be reported in research studies involving an eye tracker and human or non-human primate participant(s). This guideline was developed over a 3-year period using a consensus-based process via an open invitation to the international eye tracking community. This guideline will be reviewed at maximum intervals of 4 years.
Discovery of a New Local Group Dwarf Galaxy Candidate in UNIONS: Boötes V
Authors: Smith Simon E. T. , Jensen Jaclyn , Roediger Joel , Sestito Federico , Hayes Christian R. , McConnachie Alan W. , Cuillandre Jean-Charles , Gwyn Stephen , Magnier Eugene , Chambers Ken , Hammer Francois , Hudson Mike J. , Martin Nicolas , Navarro Julio , Scott Douglas 
Published: July 2023

Abstract
We present the discovery of Boötes V, a new ultra-faint dwarf galaxy (UFD) candidate. This satellite is detected as a resolved overdensity of stars during an ongoing search for new Local Group dwarf galaxy candidates in the UNIONS photometric data set. It has a physical half-light radius of

26.9

−
5.4

+
7.5

pc, a V-band magnitude of −4.5 ± 0.4 mag, and resides at a heliocentric distance of approximately 100 kpc. We use Gaia DR3 astrometry to identify member stars, characterize the systemic proper motion, and confirm the reality of this faint stellar system. The brightest star in this system was followed up using Gemini GMOS-N long-slit spectroscopy and is measured to have a metallicity of [Fe/H] = −2.85 ± 0.10 dex and a heliocentric radial velocity of v

r
= 5.1 ± 13.4 km s−1. Boötes V is larger (in terms of scale radius), more distant, and more metal-poor than the vast majority of globular clusters. It is likely that Boötes V is an UFD, though future spectroscopic studies will be necessary to definitively classify this object.
Cerium Features in Kilonova Near-infrared Spectra: Implication from a Chemically Peculiar Star
Authors: Tanaka Masaomi , Domoto Nanae , Aoki Wako , Ishigaki Miho N. , Wanajo Shinya , Hotokezaka Kenta , Kawaguchi Kyohei , Kato Daiji , Lee Jae-Joon , Lee Ho-Gyu , Hirano Teruyuki , Kotani Takayuki , Kuzuhara Masayuki , Nishikawa Jun , Omiya Masashi , Tamura Motohide , Ueda Akitoshi 
Published: July 2023

Abstract
Observations of the kilonova from the neutron star merger event GW170817 opened a way to study r-process nucleosynthesis directly using neutron star mergers. It is, however, challenging to identify individual elements in kilonova spectra due to a lack of complete atomic data, in particular at near-infrared (NIR) wavelengths. In this paper, we demonstrate that spectra of chemically peculiar stars with enhanced heavy-element abundances can provide us with an excellent astrophysical laboratory for kilonova spectra. We show that the photosphere of the late B-type, chemically peculiar star HR 465 has similar lanthanide abundances and ionization degrees with those in the line-forming region in a kilonova at ∼2.5 days after the merger. The NIR spectrum of HR 465 taken with Subaru/IRD indicates that Ce iii lines give the strongest absorption feature around 16000 Å and there are no other comparably strong transitions around these lines. The Ce iii lines nicely match with the broad absorption feature at 14500 Å observed in GW170817 with a blueshift of v = 0.1 c, which supports recent identification of this feature as Ce iii by Domoto et al.
Six More Ultra-faint Milky Way Companions Discovered in the DECam Local Volume Exploration Survey
Authors: Cerny W. , Martínez-Vázquez C. E. , Drlica-Wagner A. , Pace A. B. , Mutlu-Pakdil B. , Li T. S. , Riley A. H. , Crnojević D. , Bom C. R. , Carballo-Bello J. A. , Carlin J. L. , Chiti A. , Choi Y. , Collins M. L. M. , Darragh-Ford E , Ferguson P. S. , Geha M. , Martínez-Delgado D. , Massana P. , Mau S. , Medina G. E. , Muñoz R. R. , Nadler E. O. , Noël N. E. D. , Olsen K. A. G. , Pieres A. , Sakowska J. D. , Simon J. D. , Stringfellow G. S. , Tollerud E. J. , Vivas A. K. , Walker A. R. , Wechsler R. H. ,   DELVE Collaboration
Published: July 2023

Abstract
We report the discovery of six ultra-faint Milky Way satellites identified through matched-filter searches conducted using Dark Energy Camera (DECam) data processed as part of the second data release of the DECam Local Volume Exploration (DELVE) survey. Leveraging deep Gemini/GMOS-N imaging (for four candidates) as well as follow-up DECam imaging (for two candidates), we characterize the morphologies and stellar populations of these systems. We find that these candidates all share faint absolute magnitudes (M

V
≥ −3.2 mag) and old, metal-poor stellar populations (τ > 10 Gyr, [Fe/H] < −1.4 dex). Three of these systems are more extended (r
1/2 > 15 pc), while the other three are compact (r
1/2 < 10 pc). From these properties, we infer that the former three systems (Boötes V, Leo Minor I, and Virgo II) are consistent with ultra-faint dwarf galaxy classifications, whereas the latter three (DELVE 3, DELVE 4, and DELVE 5) are likely ultra-faint star clusters. Using data from the Gaia satellite, we confidently measure the proper motion of Boötes V, Leo Minor I, and DELVE 4, and tentatively detect a proper-motion signal from DELVE 3 and DELVE 5; no signal is detected for Virgo II. We use these measurements to explore possible associations between the newly discovered systems and the Sagittarius dwarf spheroidal, the Magellanic Clouds, and the Vast Polar Structure, finding several plausible associations. Our results offer a preview of the numerous ultra-faint stellar systems that will soon be discovered by the Vera C. Rubin Observatory and highlight the challenges of classifying the faintest stellar systems.
Missing Giants: Predictions on Dust-obscured Galaxy Stellar Mass Assembly Throughout Cosmic Time
Authors: Long Arianna S. , Casey Caitlin M. , del P. Lagos Claudia , Lambrides Erini L. , Zavala Jorge A. , Champagne Jaclyn , Cooper Olivia R. , Cooray Asantha R. 
Published: July 2023

Abstract
Due to their extremely dust-obscured nature, much uncertainty still exists surrounding the stellar mass growth and content in dusty, star-forming galaxies (DSFGs) at z > 1. In this work, we present a numerical model built using empirical data on DSFGs to estimate their stellar mass contributions across the first ∼10 Gyr of cosmic time. We generate a dust-obscured stellar mass function that extends beyond the mass limit of star-forming stellar mass functions in the literature, and predict that massive DSFGs constitute as much as 50%–100% of all star-forming galaxies with M ≥1011
M
⊙ at z > 1. We predict the number density of massive DSFGs and find general agreement with observations, although more data is needed to narrow wide observational uncertainties. We forward-model mock massive DSFGs to their quiescent descendants and find remarkable agreement with observations from the literature demonstrating that, to first order, massive DSFGs are a sufficient ancestral population to describe the prevalence of massive quiescent galaxies at z > 1. We predict that massive DSFGs and their descendants contribute as much as 25%–60% to the cosmic stellar mass density during the peak of cosmic star formation, and predict an intense epoch of population growth during the ∼1 Gyr from z = 6 to 3 during which the majority of the most massive galaxies at high-z grow and then quench. Future studies seeking to understand massive galaxy growth and evolution in the early universe should strategize synergies with data from the latest observatories (e.g., JWST and the Atacama Large Millimeter/submillimeter Array) to better include the heavily dust-obscured galaxy population.
Using [Ne v]/[Ne iii] to Understand the Nature of Extreme-ionization Galaxies
Authors: Cleri Nikko J. , Olivier Grace M. , Hutchison Taylor A. , Papovich Casey , Trump Jonathan R. , Amorín Ricardo O. , Backhaus Bren E. , Berg Danielle A. , Fernández Vital , Finkelstein Steven L. , Fujimoto Seiji , Hirschmann Michaela , Kartaltepe Jeyhan S. , Kocevski Dale D. , Simons Raymond C. , Wilkins Stephen M. , Yung L. Y. Aaron 
Published: July 2023

Abstract
Spectroscopic studies of extreme-ionization galaxies (EIGs) are critical to our understanding of exotic systems throughout cosmic time. These EIGs exhibit spectral features requiring >54.42 eV photons: the energy needed to ionize helium into He2+ fully and emit He ii recombination lines. Spectroscopic studies of EIGs can probe exotic stellar populations or accretion onto intermediate-mass black holes (∼102–105
M
⊙), which are the possibly key contributors to the reionization of the Universe. To facilitate the use of EIGs as probes of high-ionization systems, we focus on ratios constructed from several rest-frame UV/optical emission lines: [O iii] λ5008, Hβ, [Ne iii] λ3870, [O ii] λ
λ3727, 3729, and [Ne v] λ3427. These lines probe the relative intensity at energies of 35.12, 13.62, 40.96, 13.62, and 97.12 eV, respectively, covering a wider range of ionization than traced by other common rest-frame UV/optical techniques. We use the ratios of these lines ([Ne v]/[Ne iii] ≡ Ne53, [O iii]/Hβ, and [Ne iii]/[O ii]), which are nearby in wavelength, mitigating the effects of dust attenuation and uncertainties in flux calibration. We make predictions from photoionization models constructed from Cloudy that use a broad range of stellar populations and black hole accretion models to explore the sensitivity of these line ratios to changes in the ionizing spectrum. We compare our models to observations from the Hubble Space Telescope and JWST of galaxies with strong high-ionization emission lines at z ∼ 0, z ∼ 2, and 5 < z < 8.5. We show that the Ne53 ratio can separate galaxies with ionization from “normal” stellar populations from those with active galactic nuclei and even “exotic” Population III models. We introduce new selection methods to identify galaxies with photoionization driven by Population III stars or intermediate-mass black hole accretion disks that could be identified in upcoming high-redshift spectroscopic surveys.
Characterizing the Spectral Structure of Weak Impulsive Narrowband Quiet Sun Emissions
Authors: Mondal Surajit , Oberoi Divya , Biswas Ayan , Kansabanik Devojyoti 
Published: July 2023

Abstract
Weak Impulsive Narrowband Quiet Sun Emissions (WINQSEs) are a newly discovered class of radio emission from the solar corona. These emissions are characterized by their extremely impulsive, narrowband, and ubiquitous nature. We have systematically been working on their detailed characterization, including their strengths, morphologies, temporal characteristics, energies, etc. This work is the next step in this series and focuses on the spectral nature of WINQSEs. Given that their strength is only a few percent of the background solar emission, we have adopted an extremely conservative approach to reliably identify WINQSES. Only a handful of WINQSEs meet all of our stringent criteria. Their flux densities lie in the 20–50 Jy range and they have compact morphologies. For the first time, we estimate their bandwidths and find them to be less than 700 kHz, consistent with expectations based on earlier observations. Interestingly, we also find similarities between the spectral nature of WINQSEs and the solar radio spikes. This is consistent with our hypothesis that the WINQSEs are the weaker cousins of the type III radio bursts and are likely to be the low-frequency radio counterparts of the nanoflares, originally hypothesized as a possible explanation for coronal heating.
Sliding methods for tempered fractional parabolic problem
Authors: Peng Shaolong 
Published: July 2023

AbstractIn this article, we are concerned with the tempered fractional parabolic problem
$$ \begin{align*}\frac{\partial u}{\partial t}(x, t)-\left(\Delta+\lambda\right)^{\frac{\alpha}{2}} u(x, t)=f(u(x, t)), \end{align*} $$
where
$-\left (\Delta +\lambda \right )^{\frac {\alpha }{2}}$
is a tempered fractional operator with
$\alpha \in (0,2)$
and
$\lambda $
is a sufficiently small positive constant. We first establish maximum principle principles for problems involving tempered fractional parabolic operators. And then, we develop the direct sliding methods for the tempered fractional parabolic problem, and discuss how they can be used to establish monotonicity results of solutions to the tempered fractional parabolic problem in various domains. We believe that our theory and methods can be conveniently applied to study parabolic problems involving other nonlocal operators.
The role of plasma atherogenic index in patients with NAFLD
Authors: KIRIK Ali , ŞEN Hacer 
Published: July 2023

Background Plasma atherogenic index (PAI) is a novel index investigated in recent years related to cardiovascular disease and atherosclerosis. The role of PAI is not clear in non-alcoholic fatty liver disease (NAFLD). This study aimed to examine the role of PAI in patients with NAFLD and its relationship with metabolic components.
Material and Methods This study was designed as a retrospective study, and the patients' files admitted to the Internal Medicine unit were retrospectively scanned. Within the scope of the study, demographic and laboratory data of the groups with and without NAFLD were compared.
Results A total of 234 patients were evaluated, 159 of which were NAFLD (age: 39.52 ± 10.38 years) and 75 controls (age: 38.07 ± 12.11 years) (p = 0.374). PAI level was statistically significantly higher in the NAFLD group compared to the control group (p = 0.006). In the whole group correlation analysis, PAI level and body mass index (p < 0.001, r = 0.363), waist circumference (p < 0.001, r = 0.366), systolic blood pressure (p < 0.001, r = 0.333), diastolic blood pressure (p = 0.001, r = 0.210), ALT (p < 0.001, r = 0.312), AST (p = 0.005, r = 0.182), fasting plasma glucose (p = 0.017, r = 0.157) and insulin resistance (p < 0.001, r = 0.302) values were positively correlated.
Conclusions PAI level was higher in patients with NAFLD; this index was associated with other metabolic components, especially insulin resistance. This indicates that the PAI level may be associated with clinical progression in the pathogenesis and course of the disease.
Political, socio-cultural and economic organization of the Twa and Teke (Boma) in the plateaux department in the Republic of Congo: case of the Ngo district from 1960 to 2013
Authors: Oba Dominique 
Published: July 2023

In Africa as everywhere else, African societies have known several forms of organization that can be found in Central Africa in the Kongo, Loango and Teke kingdoms. This form of organization is also found in the plateau department and more precisely in the region of Ngo where the Bantu and Tswa have lived since time immemorial. Benefiting from several privileges, gradually becoming lord of the land, although occupying space after the Tswa, the Bantu exert a far-reaching influence and domination over the tswa to the point of considering and transforming them as sub-men. The relations between these two peoples are generally to the advantage of the Bantu. In the region of Ngo, the twa and Teke knew a political, socio-cultural and economic organization which was at the base of their civilization. This study tries to show the influence of this multidimensional organization of these two groups which continue to coexist to this day, particularly from 1960 to 2013.
Current trends in private financing of public primary education in Congo Brazzaville
Authors: Okoua Béatrice Perpétue 
Published: July 2023

The study carried out on current trends in private financing of primary education in Congo Brazzaville has the main objective of verifying the financing capacity of the State and parents in the education of children in public primary school. To answer questions relating to free education and the difficulties that the Congolese experience in financing the education of children, we have retained as data collection instruments, the documentary study and the interview. We have selected a sample of five ( 05) schools per constituency chosen out of twenty five (25) and questioned two hundred (200) parents distributed by category according to their income. The results obtained confirm our initial hypotheses that the Congolese State is experiencing enormous difficulties in resuming the educational situation hand and free appears as a concept which does not evoke any reality with the parents, (80.5%) deny free, (19.5%) grant him a credit.
The hypotheses formulated and validated allowed us to propose suggestions for solution approaches to the main education partners.
Active Learning to Find Concepts and Algorithms in Decimal Material in Class V Elementary School
Authors: Tampubolon Taruly , Harianja Robert , Sibarani Sariayu 
Published: July 2023

Prior to learning, pre-tests and questionnaires were given to determine students' abilities and interests in learning decimal. Based on the results of the initial test, it was found that students' initial abilities were very low with an average grade of 15.50, and from the results of the questionnaire, all students said they did not like decimal learning. After active learning to find the concept of algorithms in decimal material, the class average value was 86.27, meaning that the level of classical student mastery was 86.27. This indicated that the student mastery level was relatively high. Of the 20 students, there were 19 people or 95.0% who had finished studying, thus that classically learning decimal material had been completed. Judging from the specific learning objectives, all of them achieved above 65%. The results of the student questionnaire after the decimal material learning outcomes test was completed, obtained data that students felt happy with the learning they had just participated in. Students argue, the way is easy to understand and understand. With simple but interesting teaching aids, it can increase students' enthusiasm and interest in learning Mathematics.
The classical learning outcomes have been completed based on the learning completeness criteria specified in the curriculum, specific learning objectives have been achieved based on the learning objectives achievement criteria, the student's response to learning is positive, the student's mastery of the material is high. It can be concluded that learning on decimal material in class V SD. already effective.