bluuebunny/crossref_metadata_2025_split huggingface dataset:
Penerapan Nilai-Nilai Serviam di Sekolah Ursulin Jenjang SMP
Authors: Tuba Elisabeth , Mohammad Ali  
Published: March 2023

Pendidikan integratif yang tidak hanya berorientasi pada upaya mencerdaskan anak bangsa secara intelektual, tetapi juga secara spiritual, sosial-emosional dan kinestetik, harus menjadi perhatian semua stakeholder pendidikan. Hal ini juga menjadi perhatian pemangku kepentingan pendidikan pada sekolah-sekolah Ursulin. Sekolah-sekolah Ursulin memiliki nilai-nilai utama atau core values yaitu Serviam yang artinya “Saya Mengabdi”. Nilai-nilai Serviam meliputi cinta dan belas kasih, integritas, keberanian dan kesungguhan, persatuan, totalitas dan pelayanan. Nilai-nilai ini bersumber pada kitab suci, ajaran Gereja dan spiritualitas Santa Angela. Bagaimana penerapan nilai-nilai Serviam dalam pendidikan ursulin? Sejauh ini, belum ada penelitian tentang hal ini. Penelitian ini dilakukan untuk mengisi kesejangan ini dengan tujuan menggali dan mendeskripsikan model penerapan nilai-nilai Serviam dalam pendidikan pada sekolah – sekolah Ursulin. Metode yang digunakan adalah metode kualitatif. Data diperoleh dengan teknik wawancara, observasi dan studi dokumentasi. Validasi data dilakukan dengan cara triangulasi teknik dan sumber. Selanjutnya data dianalisis dengan tahapan reduksi data, penyajian data, dan penarikan kesimpulan. Hasil penelitian menunjukkan bahwa penerapan nilai-nilai Serviam dilakukan melalui (1) kegiatan pembelajaran dalam semua mata pelajaran baik pada perencanaan (96,3% guru menyusun RPP berkarakter Serviam), pelaksanaan (88,9% guru menerapkan RPP berkarakter Serviam dalam pembelajaran) maupun penilaian (100% guru mengisi jurnal penilaian sikap berisi nilai-nilai karakter Serviam); (2) pengembangan budaya sekolah melalui kegiatan rutin, kegiatan spontan, keteladanan dan pengkondisian; (3) kegiatan ekstrakurikuler dan (4) kegiatan harian di rumah dan masyarakat. Penelitian ini berkontribusi memperkaya literatur tentang pendidikan karakter dan memberikan input penting bagi para pemangku kepentingan tentang pengembangan pendidikan karakter yang bersifat integrative dan sistematis sehingga dapat menjadi bahan masukan dalam melakukan prove and improve konstruksi kurikulum dalam tataran dokumen maupun praktik di lapangan sehingga peserta didik memiliki panggilan hidup dan siap mengabdi dalam kehidupannya.
Rethinking Education Reform in Morocco Beyond the Imperatives of Determinism
Authors: Morchid Nabil 
Published: March 2023

The deterministic tradition abides by the principles of intuitionistic logic, in which the current state of all systems is determined by prior versions of what they are. Systemic determinism, where the present simultaneously substantiates pre-existing conditions and predicts imminent realities, has long championed the logic of the natural sciences, providing substance and legitimacy for an infallible cause-effect agency. Advocacy for deterministic agency is well sensed in the organization and administration of education. Many educational reforms are conceived with practices that espouse the logic of linear progression. The intent of this paper is to interrogate the legitimacy of the deterministic approach to educational reform in Morocco against its capacity to predict change. In particular, the outputs from five educational reforms carried out in Morocco over the 1999-2022 period were subjected to content analysis for obtaining data on the statistical distribution of changes in relation to three research dimensions: access to primary education, adult literacy and gender equality . In a later stage, the outputs from the quantitative analysis were optimized to enable inferential modes of analysis. The findings from this study revealed that systemic determinism is incapacitated by the principle of cause-effect agency that hyperbolizes the influences of the past on the imperatives of the present.

Received: 25 October 2022 / Accepted: 24 February 2022 / Published: 6 March 2023
A Study on the Elasticity of Time in a Perceived Polychronic Culture
Authors: Amoah Kenneth , Gyamfi Esther , Mensah Ronald Osei 
Published: March 2023

This study sought to measure polychronicity in the Ghanaian public sector. A qualitative approach was applied to the data collection. An improved polychronic attitude scale was used as the overall measure of monochronic/polychronic tendencies. This scale had been developed, tested and modified for the management setting to be utilized in measuring departmental or organizational polychronicity. A convenience selection of 30 participants from the Takoradi Technical University was done, and those selected were interviewed, using a semi-structured interview guide. Creswell and Poth’s (2018) Analysis Spiral Plan used was to handle the data, and the findings showed a disposition towards monochronic behavior. There was evidence of generally positive results when the impact of the polychronicity of the participants was evaluated, although participants exhibiting monochronic tendencies benefited the most. All the participants, irrespective of their polychronicity inclination, demonstrated that their time use preference helped them get work done. Again, their communication context aided them to achieve their communication objective. Also, the managements of public sector organizations, knowing the monochronic tendencies of their administators should strategize and implement policies such as polychronic superiors being tolerant with their surbordinates who are likely to be monochronic in their approach to work. In addtition, the institution should device and adopt a means of communication which is low context in nature to correspond with the monochronic tendencies of the workers.

Received: 25 November 2022 / Accepted: 30 December 2022 / Published: 6 March 2023
SISTEM INFORMASI KUNJUNGAN PASIEN PADA KLINIK MITRA MEDIKA
Authors: Yoga Titan Parama , Marwondo Marwondo , Nurhasanah Seny 
Published: March 2023

Sistem Informasi Kunjungan Pasien merupakan suatu sistem informasi yang diperuntukan mengolah data-data yang berhubungan dengan kunjungan pasien yang ada di Klinik Mitra Medika. Belum optimalnya sistem informasi kunjungan pasien yang ada saat ini mengakibatkan kesulitan dalam pencarian data dan pembuatan laporan-laporan yang menunjang kemajuan Klinik. Peneliti mengembangkan sistem informasi yang lebih baik sehingga dapat mempermudah pengolahan data serta pelaporan-pelaporannya.
Hasil yang diperoleh adalah sistem baru yang terintegrasi, pencarian data-data kunjungan pasien menjadi cepat dan laporan-laporan yang dihasilkan menjadi akurat. Peneliti menggunakan SHPS (Siklus Hidup Pengembanga Sistem), dengan alat bantu flowchart, ERD, DFD dan Diagram Konteks dalam pengembangan sistemnya. Pengumpulan data dilakukan dengan teknik wawancara, observasi, dan studi pustaka.
Rancang Bangun Aplikasi Monitoring Debit Air Berbasis Android PDAM Giri Nawa Tirta Kab. Pasuruan
Authors: Rosadi Muhammad Imron , Soleh Nur Moh 
Published: March 2023

Dalam hal ini informasi data debit air dapat digunakan sebagai acuan dalam penanggulangan kebocoran pipa. Hal ini menjadi permasalahan yang terjadi pada PDAM Giri Nawa Tirta Kab. Pasuruan. Maka dibutuhkannya alat monitoring otomatis untuk mengetahui debit air yang mengalir setiap harinya. Maka dari itu diperlukan suatu sistem monitoring debit air pada penyaluran air secara realtime untuk mengetahui arus air, jumlah air dan tingkat kehilangan air. Pada aplikasi ini menggunakan metode Sistem yang dibuat ini menggunakan system development life cycle (SDLC) yang memiliki 4 fase datar antara lain, planning, analysis, design dan implementation. Pada penelitian ini menghasilkan sebuah sistem android yang mampu menerima informasi berupa debit air yang diperoleh secara realtime setiap saat yang memiliki tampilan dan fitur berupa debit air, history dan kehilangan air dengan tampilan yang sederhana serta user friendly.
Analysis of Twitter Sentiment Towards Madrasahs Using Classification Methods
Authors: Panggabean Supriadi , Gata Windu , Setiawan Tri Agus 
Published: March 2023

In today's digital era, the influence and use of the internet has become a necessity, especially in Indonesia itself, internet users in early 2021 reached 202.6 million people. The most widely used internet use by Indonesians is social media. Several incidents of sexual violence that occurred in the madrasa environment as reported in the media, the emergence of radical Islamic issues which he said were the fruit of thoughts from the madrasa environment, terrorism which was also said to come from misinterpreting knowledge from madrasahs, intolerance to different religions, changes in the character of madrasah students and so on will cause negative thoughts towards madrasah. To find out how the sentiment of social media users towards madrasahs, a study was conducted on analisis twitter sentiment towards madrasah using the classification method. The methods used are Naïve Bayes (NB), Decision Tree (DT) and K – Nearest Neighbor (K-NN). Toimprove the performance of the classification method is carried out using the Particle Swarm Optimization (PSO) selection feature. On the other hand, tools gataframework, execute Python script dan rapidminer diguna kan jug a dalam penelitian this to membantu preprocessi ng dan cleansing pa da datasethingga membantu menciptaka n corpus dan sentiment ana lysis. Acuration obtained from the Naïve Bayes algorithm accuracy: 76.86% +/- 5.24% (micro average: 76.86%), Decision Tree accuracy: 61.38% +/- 5.46% (micro average: 61.35%), K-NN accuracy: 74.70% +/- 4.83% (micro average: 74.67%), Naïve Bayes PSO accuracy: 80.80% +/- 4.86% (micro average: 80.79%, Decision Tree PSO accuracy: 65.27% +/- 5.26% (micro average: 65.28%), and K-NN PSO accuracy: 67.24% +/- 7.92% (micro average: 67.25%). The results showed that the Naïve Bayes PSO algorithm got the best and accurate results. This study succeeded in obtaining an effective and best algorithm in classifying positive comments and negative comments related to sentiment analysis towards madrasahs by classification method.
Pengetahuan Ibu Nifas Mengenai Baby Blues di Ruangan Rawat Inap Nifas RSUD Kota Bandung
Authors: Indriati Maya , Rahmawati Naili , Astriani Astriani 
Published: March 2023

Baby blues merupakan perasaan hipersensitif yang wajar terjadi pada ibu setelah melahirkan, tetapi yang perlu diwaspadai, hal ini dapat bertambah serius dan bertahan lama yang biasanya disebut dengan postpartum depression. Pengetahuan seseorang dapat diinterpretasikan dengan skala yang bersifat kualitatif, yaitu pengetahuan baik : 76 % - 100 , pengetahuan cukup : 60 % - 75 %, pengetahuan kurang : < 60 %. Tujuan penelitian ini adalah untuk mengetahui gambaran pengetahuan ibu nifas mengenai baby blues meliputi pengetahuan baby blues secara umum, pengertian baby blues, tanda gejala baby blues, penyebab baby blues, dan pencegahan baby blues. Jenis penelitian yang digunakan adalah penelitian deskriptif dengan populasi 30 orang ibu nifas Instrument penelitian yang digunakan berupa kuesioner yang disebarkan kepada responden ibu nifas yang dirawat di ruang rawat inap RSUD Kota Bandung.
Hasil penelitian menunjukan pengetahuan ibu nifas secara umum mengenai baby blues sudah baik 63%, pengetahuan ibu nifas mengenai pengertian baby blues sudah baik 73%, pengetahuan ibu nifas mengenai tanda gejala baby blues sudah baik 63%, pengetahuan ibu nifas mengenai penyebab baby blues sudah baik 83%, pengetahuan ibu nifas mengenai pencegahan baby blues sudah baik 53%.
A Measurement of the Cosmic Optical Background and Diffuse Galactic Light Scaling from the R < 50 au New Horizons-LORRI Data
Authors: Symons Teresa , Zemcov Michael , Cooray Asantha , Lisse Carey , Poppe Andrew R. 
Published: March 2023

Abstract
Direct photometric measurements of the cosmic optical background (COB) provide an important point of comparison to both other measurement methodologies and models of cosmic structure formation, and permit a cosmic consistency test with the potential to reveal additional diffuse sources of emission. The COB has been challenging to measure from Earth due to the difficulty of isolating it from the diffuse light scattered from interplanetary dust in our solar system. We present a measurement of the COB using data taken by the Long-Range Reconnaissance Imager on NASA's New Horizons mission, considering all data acquired to 47 au. We employ a blind methodology where our analysis choices are developed against a subset of the full data set, which is then unblinded. Dark current and other instrumental systematics are accounted for, including a number of sources of scattered light. We fully characterize and remove structured and diffuse astrophysical foregrounds including bright stars, the integrated starlight from faint unresolved sources, and diffuse galactic light. For the full data set, we find the surface brightness of the COB to be

λ

I

λ

COB

=
21.98
±
1.23

(
stat
.
)
±
1.36

(
cal
.
)

nW m−2 sr−1. This result supports recent determinations that find a factor of 2–3× more light than expected from the integrated light from galaxies and motivate new diffuse intensity measurements with more capable instruments that can support spectral measurements over the optical and near-IR.
Dependence of Cosmological Constraints on Gray Photometric Zero-point Uncertainties of Supernova Surveys
Authors: Brownsberger Sasha R. , Brout Dillon , Scolnic Daniel , Stubbs Christopher W. , Riess Adam G. 
Published: March 2023

Abstract
Type Ia supernova (SN) measurements of the Hubble constant, H
0; cosmic mass density, Ω
M
; and dark energy equation-of-state parameter, w, rely on heterogeneous SN surveys across three decades of observation. These distinct surveys may have undiagnosed, relative photometric zero-point errors. We determine the sensitivities of the SH0ES+Pantheon+ cosmological constraints to unknown gray systematics in the photometric zero-point calibration between the 19 surveys that comprise the Pantheon+ SN compendium. Varying the surveys’ gray zero-points simultaneously with cosmological parameters, we determine that the SH0ES+Pantheon+ measurement of H
0 is robust against gray intersurvey photometric miscalibration. Specifically, uncalibrated intersurvey systematics could represent a source of uncertainty no larger than 0.39 km s−1 Mpc−1 for H
0. This modest increase in H
0 uncertainty could not account for the 7 km s−1 Mpc−1 “Hubble tension” between the SH0ES measurement of H
0 and the Planck ΛCDM-based inference of H
0. However, the SH0ES+Pantheon+ best-fit values of Ω
M
and w are not robust against gray zero-point error, slipping by up to 0.16 and −0.63. Because measurements of Ω
M
and w depend on intrasurvey cross-band calibration, the hypothetical gray miscalibration underestimates the sensitivity of these measurements to zero-point miscalibration. Because the Pantheon+ compendium contains many surveys that share low-z Hubble flow (HF) and Cepheid-paired SNe, intersurvey photometric calibration errors do not significantly impede the joint use of SH0ES and Pantheon+ to measure H
0 to 1% accuracy. However, H
0 constraints that rely on one HF survey but numerous galactic distance calibration surveys are susceptible to intersurvey photometric miscalibration.
gyre_tides: Modeling Binary Tides within the GYRE Stellar Oscillation Code
Authors: Sun 孙 Meng 萌 , Townsend R. H. D. , Guo Zhao 
Published: March 2023

Abstract
We describe new functionality in the GYRE stellar oscillation code for modeling tides in binary systems. Using a multipolar expansion in space and a Fourier-series expansion in time, we decompose the tidal potential into a superposition of partial tidal potentials. The equations governing the small-amplitude response of a spherical star to an individual partial potential are the linear, non-radial, nonadiabatic oscillation equations with an extra inhomogeneous forcing term. We introduce a new executable, gyre_tides, that directly solves these equations within the GYRE numerical framework. Applying this to selected problems, we find general agreement with results in the published literature but also uncover some differences between our direct solution methodology and the modal decomposition approach adopted by many authors. In its present form gyre_tides can model equilibrium and dynamical tides of aligned binaries in which radiative diffusion dominates the tidal dissipation (typically, intermediate- and high-mass stars on the main sequence). Milestones for future development include incorporation of other dissipation processes, spin–orbit misalignment, and the Coriolis force arising from rotation.
Does the HCN/CO Ratio Trace the Star-forming Fraction of Gas? I. A Comparison with Analytical Models of Star Formation
Authors: Bemis Ashley R. , Wilson Christine D. 
Published: March 2023

Abstract
We use archival ALMA observations of the HCN and CO J = 1–0 transitions, in addition to the radio continuum at 93 GHz, to assess the relation between dense gas, star formation, and gas dynamics in 10 nearby (ultra)luminous IR galaxies (U)LIRGs and late-type galaxy centers. We frame our results in the context of turbulent and gravoturbulent models of star formation to assess whether the HCN/CO ratio tracks the gravitationally bound star-forming gas in molecular clouds (f
grav) at subkiloparsec scales in nearby galaxies. We confirm that the HCN/CO ratio is a tracer of gas above n
SF ≈ 104.5 cm−3, but the subkiloparsec variations in HCN/CO do not universally track f
grav. We find strong evidence for the use of varying star formation density-threshold models, which are able to reproduce trends observed in t
dep and ϵ
ff that fixed-threshold models do not reproduce. Composite lognormal and power-law models outperform pure lognormal models in reproducing the observed trends, even when a fixed power-law slope is used. The ability of the composite models to better reproduce the star formation properties of the gas provides additional indirect evidence that the star formation efficiency per freefall time is proportional to the fraction of gravitationally bound gas.
New Determination of the 12C(α, γ)16O Reaction Rate and Its Impact on the Black-hole Mass Gap
Authors: Shen Yangping , Guo Bing , deBoer Richard J. , Li Ertao , Li Zhihong , Li Yunju , Tang Xiaodong , Pang Danyang , Adhikari Sucheta , Basu Chinmay , Su Jun , Yan Shengquan , Fan Qiwen , Liu Jiancheng , Chen Chen , Han Zhiyu , Li Xinyue , Lian Gang , Ma Tianli , Nan Wei , Nan Weike , Wang Youbao , Zeng Sheng , Zhang Hao , Liu Weiping 
Published: March 2023

Abstract
We present a precise measurement of the asymptotic normalization coefficient (ANC) for the 16O ground state (GS) through the 12C(11B, 7Li)16O transfer reaction using the Quadrupole‐3‐Dipole (Q3D) magnetic spectrograph. The present work sheds light on the existing discrepancy of more than 2 orders of magnitude between the previously reported GS ANC values. This ANC is believed to have a strong effect on the 12C(α, γ)16O reaction rate by constraining the external capture to the 16O ground state, which can interfere with the high-energy tail of the 2+ subthreshold state. Based on the new ANC, we determine the astrophysical S-factor and the stellar rate of the 12C(α, γ)16O reaction. An increase of up to 21% in the total reaction rate is found within the temperature range of astrophysical relevance compared with the previous recommendation of a recent review. Finally, we evaluate the impact of our new rate on the pair-instability mass gap for black holes (BH) by evolving massive helium core stars using the MESA stellar evolution code. The updated 12C(α, γ)16O reaction rate decreases the lower and upper edges of the BH gap about 12% and 5%, respectively.
VERITAS and Fermi-LAT Constraints on the Gamma-Ray Emission from Superluminous Supernovae SN2015bn and SN2017egm
Authors: Acharyya A. , Adams C. B. , Bangale P. , Benbow W. , Buckley J. H. , Capasso M. , Dwarkadas V. V. , Errando M. , Falcone A. , Feng Q. , Finley J. P. , Foote G. M. , Fortson L. , Furniss A. , Gallagher G. , Gent A. , Hanlon W. F , Hervet O. , Holder J. , Humensky T. B. , Jin W. , Kaaret P. , Kertzman M. , Kherlakian M. , Kieda D. , Kleiner T. K , Kumar S. , Lang M. J. , Lundy M. , Maier G. , McGrath C. E , Millis J. , Moriarty P. , Mukherjee R. , Nievas-Rosillo M. , O’Brien S. , Ong R. A. , Patel S. R. , Pfrang K. , Pohl M. , Pueschel E. , Quinn J. , Ragan K. , Reynolds P. T. , Ribeiro D. , Roache E. , Ryan J. L. , Sadeh I. , Santander M. , Sembroski G. H. , Shang R. , Splettstoesser M. , Tak D. , Tucci J. V. , Weinstein A. , Williams D. A. ,   VERITAS collaboration, Metzger B. D. , Nicholl M. , Vurm I. 
Published: March 2023

Abstract
Superluminous supernovae (SLSNe) are a rare class of stellar explosions with luminosities ∼ 10–100 times greater than ordinary core-collapse supernovae. One popular model to explain the enhanced optical output of hydrogen-poor (Type I) SLSNe invokes energy injection from a rapidly spinning magnetar. A prediction in this case is that high-energy gamma-rays, generated in the wind nebula of the magnetar, could escape through the expanding supernova ejecta at late times (months or more after optical peak). This paper presents a search for gamma-ray emission in the broad energy band from 100 MeV to 30 TeV from two Type I SLSNe, SN2015bn, and SN2017egm, using observations from Fermi-LAT and VERITAS. Although no gamma-ray emission was detected from either source, the derived upper limits approach the putative magnetar’s spin-down luminosity. Prospects are explored for detecting very-high-energy (VHE; 100 GeV–100 TeV) emission from SLSNe-I with existing and planned facilities such as VERITAS and CTA.
Role of Small-scale Impulsive Events in Heating the X-Ray Bright Points of the Quiet Sun
Authors: Mondal Biswajit , Klimchuk James A , Vadawale Santosh V. , Sarkar Aveek , Del Zanna Giulio , Athiray P. S. , Mithun N. P. S. , Mason Helen E. , Bhardwaj Anil 
Published: March 2023

Abstract
Small-scale impulsive events, known as nanoflares, are thought to be one of the prime candidates that can keep the solar corona hot at its multimillion-Kelvin temperature. Individual nanoflares are difficult to detect with the current generation of instruments; however, their presence can be inferred through indirect techniques such as Differential Emission Measure (DEM) analysis. Here, we employ this technique to investigate the possibility of nanoflare heating of the quiet corona during the minimum of solar cycle 24. We estimate the DEM of disk-integrated quiet Sun and X-ray bright points (XBP) using the observations from XSM on board the Chandrayaan-2 orbiter and AIA on board the Solar Dynamic Observatory. XBPs are found to be the dominant contributor to disk-integrated X-rays, with a radiative flux of ∼2 × 105 erg cm−2 s−1. XBPs consist of small-scale loops associated with bipolar magnetic fields. We simulate such XBP loops using the EBTEL hydrodynamic code. The lengths and magnetic field strengths of these loops are obtained through a potential field extrapolation of the photospheric magnetogram. Each loop is assumed to be heated by random nanoflares having an energy that depends on the loop properties. The composite nanoflare energy distribution for all the loops has a power-law slope close to −2.5. The simulation output is then used to obtain the integrated DEM. It agrees remarkably well with the observed DEM at temperatures above 1 MK, suggesting that the nanoflare distribution, as predicted by our model, can explain the XBP heating.