bluuebunny/crossref_metadata_2025_split huggingface dataset:
PENGARUH KOMPETENSI, KOMITMEN ORGANISAS DAN INDEPENDENS TERHADAP KINERJA AUDITOR PADA INSPEKTORAT PROVINS SULAWES BARAT
Authors: Priogandi Andi Mansahid , Manne Firman , Abubakar Herminawati 
Published: June 2021

Penelitian in bertujuan untuk mengetahu dan meng-analisis pengaruh kompetensi, komitmen organisas dan independens terhadap kinerja auditor pada Inspektorat Provins Sulawes Barat. Teknik pengumpulan data melalu kuesioner, observasi, wawancara dan telaah dokumen. Sedangkan teknik analisis data yang diguna-kan adalah uj kualitas data, uj asums klasik, analisis regres linear berganda, pengujian hipotesis, dan koefisien determinasi. Berdasarkan hasil analisis maka diperoleh hasil bahwa kompetens mempunya pengaruh yang positif dan signi-fikan terhadap kinerja auditor pada Kantor Inspektorat Provins Sulawes Barat. Komitmen Organisas mem-punya pengaruh yang positif dan signifikan terhadap kinerja auditor pada Kantor Inspektorat Provins Sulawes Barat. Independens mempunya pengaruh yang positif dan signifikan terhadap kinerja auditor pada Kantor Inspektorat Provins Sulawes Barat. Hasil peng-ujian serempak maka dapat disimpulkan bahwa kompetensi, komitmen organisasi, dan independens mempunya pengaruh secara serempak atau bersama-sama terhadap kinerja auditor pada Kantor Inspektorat Provins Sulawes Barat. Dar hasil pengujian regres maka diketahu bahwa variabel yang dominan berpengaruh terhadap kinerja auditor pada Kantor Inspektorat Provins Sulawes Barat adalah komitmen organisasi.
This study aims to determine and analyze the influence of competence, organizational commitment and independence on auditor performance at the Inspectorate of West Sulawes Province. Data were collected through questionnaires, observation, interviews and document reviews. Meanwhile, the data analysis techniques used are data quality test, classical assumption test, multiple linear regression analysis, hypothesis testing, and the coefficient of determination. Based on the analysis, the results show that competence has a positive and significant effect on the performance of auditors at the Inspectorate Office of West Sulawes Province. Organizational commitment has a positive and significant effect on auditor performance at the Inspectorate Office of West Sulawes Province. Independence has a positive and significant effect on auditor performance at the Inspectorate Office of West Sulawes Province. From the results of simultaneous testing, it can be concluded that competence, organizational commitment, and independence have a simultaneous or joint effect on the performance of auditors at the Inspectorate Office of West Sulawes Province. From the results of regression testing, it is known that the dominant variable affecting the performance of auditors at the Inspectorate Office of West Sulawes Province is organizational commitment.
EFEKTIFITAS PERATURAN DAERAH NOMOR 4 TAHUN 2016 (Studi Tentang Perlindungan Dan Pemberdayaan Petani di Desa Pelem Kecamatan Campurdarat Kabupaten Tulungagung)
Authors: Nunun Nurhajati  , Nur Umi Khasanah  
Published: June 2021

Pertanian merupakan sektor strategis yang sekaligus sektor yang paling banyak menyerap tenaga kerja dan berbasis pedesaan.Era baru pertanian kedepan menghendaki orientasi pada pencapaian nilai tamah,pendapatan, serta kesejahteraan petani sebagai acuan utama dalam pembangunan pertanian.Petani sebagai pelaku utama pembangunan pertanian tentu memiliki berbagai masalah. Masalah ini sering menghambat petani untuk mengembangkan usaha taninya. Masalah yang dihadapi petani ini juga merupakan masalah dasar yang harus diselesaikan untuk melakukan pembangunan pertanian.

Karena banyaknya petani di Tulungagung yang mengalami masalah, pemerintah Kabupaten Tulungagung membuat Peraturan Daerah Kabupaten Tulungagung Nomor 4 Tahun 2016 tentang perlindungan dan pemberdayaan petani. Latar belakang ditetapkanya peraturan daerah tersebut ialah adanya kecenderungan meningkatnya perubahan iklim, gejolak ekonomi global, kerawanan terhadap bencana alam dan resiko gagal usaha, serta adanya sistem pasar yang tidak transparan dan tidak berpihak kepada petani.

Penelitian ini menggunakan jenis penelitian deskriptif kualitatif dengan tujuan untuk bisa memberikan gambaran secara menyeluruh mengenai perlindungan dan pemberdayaan petani melalui Peraturan Daerah Kabupaten Tulungagung Nomor 4 Tahun 2016. Fokus peneitiannya adalah tentang efektifitas Perda nomor 4 Tahun 2016 Kabupaten Tulungagung dan Faktor apa saja yang menjadi pendorong dan penghambatnya.

Kata Kunci : Efektifitas, perlindungan, dan pemberdayaan petani.
Solidaritas Anarkisme Suporter Bola PSIM DAN PSS
Authors: Werdiyanti Tera Puspita , Noor As Martadani , Paharizal Rizal 
Published: June 2021

This research is located in Sleman, Yogyakarta. This research was conducted when researcher saw the solidarity of anarchism of football supporters. Factors related to the solidarity of anarchism of football supporters and the empowerment of football supporters, especially with PSIM and PSS. This research wants to describe more clearly how the solidarity of anarchism is, the factors associated with solidarity of anarchism and the empowerment of suporter in PSIM and PSS football clubs. This research was conducted with a qualitative descriptive research method. Data was collected by Snow Ball sampling until the data was at its saturation point. This method was chosen because the number of actors is large so it could gets more accurate data. The results obtained in the solidarity of football supporters anarchism prove that there are improvements from the supporters. Then the factors related to the solidarity of anarchism are still trying to become supporters who are more loved by the community and the empowerment of PSIM and PSS football supporters has not received training from any party.
Dietary improvement of the iron statute of the rats with experimental anemia
Authors: STURZA Rodica , GUDUMAC Valentin , DESEATNICOVA Olga , GHENDOV-MOSANU Aliona 
Published: June 2021

Introduction. One of the major problems characterizing the nutritional status is the iron deficiency, which leads to decreased immunity, increased incidence of infectious diseases and anemia. Obviously, only well-thought-out corrections can solve these disorders.
Material and methods In order to know the influence of the method of manufacture for iron-fortified products on the iron level, a series of in vivo research was carried out, on a batch of 21 white rats, Wistar line, which were induced experimental drug anemia (EDA). The blood analysis was performed in three stages: initially, after the induction of EDA and after the completion of the experiment.
Results. Investigations showed out that during sufficient iron intake rehabilitation of the body iron reserve depends considerably on the presence of antinutritive factors. In order to decrease the influence of these factors, the production method used for fortified products with mineral origin micronutrients (iron) could be based on the use of the lactic-acid fermentation procedures using wheat bran.
Conclusions. The research carried out on laboratory animals with induced experimental anemia showed that, in the case of the group fed with bread manufactured by the acid-lactic fermentation method, the concentration of serum, iron was completely restored during the experiment, and in the rats fed with fortified bread prepared by the traditional method, the serum iron concentration was only partially restored, 40-45%.
Atypical presentation of a high-grade astrocytoma in a pediatric rheumatology Practice
Authors: REVENCO Ninel , LITOVCENCO Anatol , HADJIU Svetlana , CALCII Cornelia , EREMCIUC Rodica , GAIDARJI Olga 
Published: June 2021

Introduction. Hip pain is common in childhood. The main dilemma is to differentiate between benign conditions and those causing significant morbidity and mortality.
Material and methods. A clinical case report of a toddler presenting with Musculoskeletal (MSK) mask due to a brain tumor.
Results. A 2-year-old boy presented to the ER complaining of hip pain, muscle weakness, and limping. The neurologic exam showed no abnormalities. At the 3rd day of admission, patient condition worsened, and papillary edema was revealed. MRI revealed a tumor in the suprasellar cistern/prepons region.
Conclusions. In case of atypical MSK symptoms, a careful evaluation of children should be carried out to prevent any delay in diagnosis.
COVID-19 Summary Guidelines
Authors: Moses Samuel , Berry Nidhika , Kalhan Atul , Sathe Sonia , Srinivasan Latha , Varadarajan Viju , Shah Hasmukh , Singhal Keshav 
Published: June 2021

Low and Medium Income Countries- May 2021
We note with concern, potential misinformation regarding treatment options is recommended to patients in India. We suggest the following evidence-based practice for the management of SARS CoV2 infection.
Multifilter Observations of the Complex Periodic Variations in the M-dwarf Star RIK 90
Authors: Koen Chris 
Published: June 2021

Abstract
The star RIK 90 is a member of a group of recently discovered young T Tauri stars showing complex periodic modulations of their light output, which have been difficult to explain. As one of the brightest, and having a relatively short period, RIK 90 is of particular interest. Thirty-three hours of contemporaneous BVR

C

I

C
photometry of the star are presented in this paper. An independent secondary periodicity was removed and the remainder of the data phased with the primary 0.25955 day period and smoothed to reveal the detailed structure of the light curves. The ratios of the amplitude in B to those in VR

C

I

C
are 1.2, 1.5, and 1.8. It is found that a collection of five cool starspots with temperatures in the range 2230–2550 K provides an excellent match to almost all observations, small-scale features in the I

C
-band light curve being the notable exception. Starspot modeling of K2 observations of RIK 90 was also attempted. The morphology of the K2 light curve is entirely different from that discussed in this paper but could be accurately modeled by four dark starspots. In order to put these results into context, 15 other distinct K2 light curves belonging to 10 similarly variable T Tauri stars were also studied. Excellent fits were obtained to some of these with models consisting of large cool starspots. The majority of the remaining light curves could be modeled with a combination of hot and cold starspots.
Dynamical Avenues for Mercury’s Origin. II. In Situ Formation in the Inner Terrestrial Disk
Authors: Clement Matthew S. , Chambers John E. 
Published: June 2021

Abstract
Modern terrestrial-planet formation models are highly successful at consistently generating planets with masses and orbits analogous to those of Earth and Venus. In stark contrast to classic theoretical predictions and inferred demographics of multiplanet systems of rocky exoplanets, the mass (≳10) and orbital period (≳2) ratios between Venus and Earth and the neighboring Mercury and Mars are not common outcomes in numerically generated systems. While viable solutions to the small-Mars problem are abundant in the literature, Mercury’s peculiar origin remains rather mysterious. In this paper, we investigate the possibility that Mercury formed in a mass-depleted, inner region of the terrestrial disk (a < 0.5 au). This regime is often ignored in terrestrial-planet formation models because of the high computational cost of resolving hundreds of short-period objects over ∼100 Myr timescales. By testing multiple disk profiles and mass distributions, we identify several promising sets of initial conditions that lead to remarkably successful analog systems. In particular, our most successful simulations consider moderate total masses of Mercury-forming material (0.1–0.25 Earth masses). While larger initial masses tend to yield disproportionate Mercury analogs, smaller values often inhibit the planets’ formation as the entire region of material is easily accreted by Venus. Additionally, we find that shallow surface density profiles and larger inventories of small planetesimals moderately improve the likelihood of adequately reproducing Mercury.
Elementary Process of Galactic Spiral Arm Formation: Phase Synchronization of Epicyclic Motion by Gravitational Scattering
Authors: Yoshida Yuki , Kokubo Eiichiro 
Published: June 2021

Abstract
Swing amplification is a model of spiral arm formation in disk galaxies. Previous N-body simulations show that the epicycle phases of stars in spiral arms are synchronized. However, the elementary process of the phase synchronization is not well understood. In order to investigate phase synchronization, we investigate the orbital evolution of stars due to gravitational scattering by a perturber under the epicycle approximation and its dependence on orbital elements and a disk parameter. We find that gravitational scattering by the perturber can cause phase synchronization of stellar orbits. The epicycle phases are better synchronized for smaller initial epicycle amplitudes of stars and larger shear rates of galactic disks. The vertical motion of stars does not affect the phase synchronization. The phase synchronization forms trailing dense regions, which may correspond to spiral arms.
Cosmological Evolution of Fermi Large Area Telescope Gamma-Ray Blazars Using Novel Nonparametric Methods
Authors: Zeng Houdun , Petrosian Vahé , Yi Tingfeng 
Published: June 2021

Abstract
Multiwavelength analyses of spectra of active galactic nuclei provide useful information on the physical processes in the accretion disk and jets of black holes. This, however, is limited to bright sources and may not represent the population as a whole. Another approach is through the investigation of the cosmological evolution of the luminosity function (LF), which shows varied evolution (luminosity and density) at different wavelengths. These differences and the correlations between luminosities can shed light on the jet-accretion disk connection. Most such studies use forward fitting parametric methods that involve several functions and many parameters. We use nonparametric, nonbinning methods developed by Efron & Petrosian and Lynden-Bell, for obtaining unbiased description of the evolution of the LF, from data truncated by observational selection effects. We present an analysis of the evolution of gamma-ray LF of blazars with a main focus on flat-spectrum radio quasars. This requires analysis of both gamma-ray and optical data, essential for redshift measurements, and a description of the joint LF. We use a new approach that divides the sample into two subsamples, each with its own flux limit. We use the Fermi Large Area Telescope and GAIA observations, and present results on the gamma-ray LF and its evolution, and determine the intrinsic correlation between the gamma-ray and optical luminosities corrected for the well-known false correlation induced by their similar redshift dependence and evolution of the two luminosities. We also present a direct estimation of the contribution of blazars to the spectrum of the extragalactic gamma-ray background.
Impact of Differential Dust Settling on the SED and Polarization: Application to the Inner Region of the HL Tau Disk
Authors: Ueda Takahiro , Kataoka Akimasa , Zhang Shangjia , Zhu Zhaohuan , Carrasco-González Carlos , Sierra Anibal 
Published: June 2021

Abstract
The polarimetric observations of the protoplanetary disk around HL Tau have shown the scattering-induced polarization at ALMA Band 7, which indicates that the maximum dust size is ∼100 μm, while the spectral energy distribution (SED) has suggested that the maximum dust size is approximately a millimeter. To solve the contradiction, we investigate the impact of differential settling of dust grains on the SED and polarization. If the disk is optically thick, a longer observing wavelength traces more interior layers, which would be dominated by larger grains. We find that the SED of the center part of the HL Tau disk can be explained with millimeter-sized grains for a broad range of turbulence strength, while 160 μm–sized grains cannot be explained unless the turbulence strength parameter α
t is lower than 10−5. We also find that the observed polarization fraction can be potentially explained with a maximum dust size of 1 mm if α
t ≲ 10−5, although models with 160 μm–sized grains are also acceptable. However, if the maximum dust size is ∼3 mm, the simulated polarization fraction is too low to explain the observations even if the turbulence strength is extremely small, indicating a maximum dust size of ≲1 mm. The degeneracy between 100 μm– and millimeter-sized grains can be solved by improving the ALMA calibration accuracy or polarimetric observations at (sub)centimeter wavelengths.
SPICY: The Spitzer/IRAC Candidate YSO Catalog for the Inner Galactic Midplane
Authors: Kuhn Michael A. , de Souza Rafael S. , Krone-Martins Alberto , Castro-Ginard Alfred , Ishida Emille E. O. , Povich Matthew S. , Hillenbrand Lynne A. ,   for the COIN Collaboration
Published: June 2021

Abstract
We present ∼120,000 Spitzer/IRAC candidate young stellar objects (YSOs) based on surveys of the Galactic midplane between ℓ ∼ 255° and 110°, including the GLIMPSE I, II, and 3D, Vela-Carina, Cygnus X, and SMOG surveys (613 square degrees), augmented by near-infrared catalogs. We employed a classification scheme that uses the flexibility of a tailored statistical learning method and curated YSO data sets to take full advantage of Spitzer’s spatial resolution and sensitivity in the mid-infrared ∼3–9 μm range. Multiwavelength color/magnitude distributions provide intuition about how the classifier separates YSOs from other red IRAC sources and validate that the sample is consistent with expectations for disk/envelope-bearing pre–main-sequence stars. We also identify areas of IRAC color space associated with objects with strong silicate absorption or polycyclic aromatic hydrocarbon emission. Spatial distributions and variability properties help corroborate the youthful nature of our sample. Most of the candidates are in regions with mid-IR nebulosity, associated with star-forming clouds, but others appear distributed in the field. Using Gaia DR2 distance estimates, we find groups of YSO candidates associated with the Local Arm, the Sagittarius–Carina Arm, and the Scutum–Centaurus Arm. Candidate YSOs visible to the Zwicky Transient Facility tend to exhibit higher variability amplitudes than randomly selected field stars of the same magnitude, with many high-amplitude variables having light-curve morphologies characteristic of YSOs. Given that no current or planned instruments will significantly exceed IRAC’s spatial resolution while possessing its wide-area mapping capabilities, Spitzer-based catalogs such as ours will remain the main resources for mid-infrared YSOs in the Galactic midplane for the near future.
Stellar Metallicities from SkyMapper Photometry. II. Precise Photometric Metallicities of ∼280,000 Giant Stars with [Fe/H] < −0.75 in the Milky Way
Authors: Chiti Anirudh , Frebel Anna , Mardini Mohammad K. , Daniel Tatsuya W. , Ou Xiaowei , Uvarova Anastasiia V. 
Published: June 2021

Abstract
The Milky Way’s metal-poor stars are nearby ancient objects that are used to study early chemical evolution and the assembly and structure of the Milky Way. Here we present reliable metallicities of ∼280,000 stars with −3.75 ≲ [Fe/H] ≲ −0.75 down to g = 17 derived using metallicity-sensitive photometry from the second data release of the SkyMapper Southern Survey. We use the dependency of the flux through the SkyMapper v filter on the strength of the Ca ii K absorption features, in tandem with SkyMapper u, g, i photometry, to derive photometric metallicities for these stars. We find that metallicities derived in this way compare well to metallicities derived in large-scale spectroscopic surveys, and we use such comparisons to calibrate and quantify systematics as a function of location, reddening, and color. We find good agreement with metallicities from the APOGEE, LAMOST, and GALAH surveys, based on a standard deviation of σ ∼ 0.25 dex of the residuals of our photometric metallicities with respect to metallicities from those surveys. We also compare our derived photometric metallicities to metallicities presented in a number of high-resolution spectroscopic studies to validate the low-metallicity end ([Fe/H] < −2.5) of our photometric metallicity determinations. In such comparisons, we find the metallicities of stars with photometric [Fe/H] < −2.5 in our catalog show no significant offset and a scatter of σ ∼ 0.31 dex level relative to those in high-resolution work when considering the cooler stars (g − i > 0.65) in our sample. We also present an expanded catalog containing photometric metallicities of ∼720,000 stars as a data table for further exploration of the metal-poor Milky Way.
Use of a Structured Approach to Develop Best Practices in Interprofessional Education
Authors: Smith Leslie , Keiser Megan , Yorke Amy , Turkelson Carman 
Published: June 2021

Background:
Providing interprofessional education (IPE) is mandated by accrediting agencies for health professions education; however, pedagogical, logistical, and financial challenges exist in implementing and sustaining high-quality IPE. After executing several IPE activities, an IPE team developed a structured approach for organizing, sustaining, and ensuring high-quality IPE. This article introduces the Design-Implement-Assess-Modify (DIAM) Model. A portfolio spreadsheet was developed and includes components from each of the DIAM phases.

Method:
The team documented characteristics from five IPE activities conducted annually for 5 years and tracked progress.

Results:
The DIAM approach has allowed the team to develop a detailed and living portfolio to design, implement, assess, and modify several IPE activities across different professions.

Conclusion:

This approach has led to the intentional planning and development of multiple IPE activities that include the integration of standards of best practice and accreditation, while preparing practitioners for collaborative practice.

[
J Nurs Educ
. 2021;60(6):309–316.]
Assessment of Answer-Changing Behavior of Nursing Students and Faculty Recommendations
Authors: Bultas Margaret W. , Schmuke Ashley D. , Rubbelke Cynthia , Jackson Jennifer , Moran Vicki 
Published: June 2021

Background:
Existing literature identifies a general positive benefit to students' examination scores when students change their answer on examinations. Current shifts toward computerized examinations and in test anxiety warrant a literature update on test-taking behaviors.

Purpose:
This study assessed answer changing on multiple-choice examinations and investigated faculty recommendations related to answer changing.

Method:
This study used a mixed-methods design using retrospective student data from ExamSoft reports and faculty responses from a national survey of nurse educators.

Results:
Findings indicated 55% of students improved their examination score, with an average improvement of 3%, and 24% of students lowered their examination score. However, faculty continue to incorrectly recommend that students should not change answers on examinations.

Conclusion:

The results of this study support prior literature that answer changing benefits students. However, data are lacking on the characteristics of students who improve or lower their examination scores by changing answers.

[
J Nurs Educ
. 2021;60(6):324–328.]

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