bluuebunny/crossref_metadata_2025_split huggingface dataset:
FAKTOR RISIKO USIA DAN PARITAS IBU HAMIL TERHADAP KEJADIAN KETUBAN PECAH DINI
Authors: M Sakriawati , Rahmawati Rahmawati 
Published: April 2022

Ketuban pecah dini atau premature rupture of membran (PROM) adalah salah satu kelainan dalam kehamilan. Risiko yang ditimbulkan jika terjadi masalah tersebut adalah morbiditas dan mortalitas pada ibu maupun bayi terutama pada kejadian prenatal yang cukup tinggi. Tujuan dari penelitian ini adalah untuk melihat faktor risiko usia ibu dan paritas terhadap kejadian ketuban pecah dini di RSUD Salewangang Maros yang dilaksanakan pada bulan Mei-Juni 2019. Penelitian ini merupakan penelitian observasional dengan rancangan Case Control Study (Studi Kasus Kontrol) yaitu penelitian yang mempelajari faktor risiko dengan menggunakan pendekatan retrospektif. Populasi pada penelitian ini yaitu 60 orang dengan metode pengambilan sampel yaitu exhautive sampling (sampel total), ibu hamil yang mengalami kejadian ketuban pecah dini 30 kasus dan ibu hamil yang persalinan pervaginam 30 kontrol. Hasil penelitian ini menunjukkan bahwa usia ibu memiliki nilai p value=0,299 OR=0,365:CI (0,0852-1,576) dan paritas memiliki nilai p value=0,192 OR=2,286:CI (0,804-6,495) yang berarti usia dan paritas tidak menjadi faktor risiko utama pada kejadian KPD di RSUD Salewangang Maros Maros dan kemungkinan ada beberapa faktor lain yang lebih kuat yang menyebabkan kejadian KPD. Bagi ibu hamil hendaknya menjaga kesehatan agar anak yang dilahirkan dapat sehat terlebih dengan ibunya.
PENGARUH DISKUSI KELOMPOK TERHADAP PENGETAHUAN MENGGOSOK GIGI SISWA SD DALAM PENERAPAN PHBS
Authors: Parlaungan Jansen , Situmorang Panel , Suriani Waode 
Published: April 2022

ABSTRAK

Pendahuluan : Kemampuan menggosok gigi secara baik dan benar merupakan faktor yang cukup penting untuk perawatan kesehatan gigi dan mulut.
Tujuan : Mengetahui pengetahuan cara menggosok gigi siswa kelas V SD YPK Klasaman II Kota Sorong Papua Barat setelah dilakukan intervensi metode diskusi kelompok.
Metode : Jenis penelitian ini adalah penelitian eksperimen semi (Quasi Eksperimen) dengan rancangan Non Randomized Control Group Pretest-Posttest Design. Sampel siswa kelas V SD YPK Klasaman II Kota Sorong Papua Barat berjumlah 60 siswa.
Hasil : Penelitian menunjukkan terdapat perbedaan pengetahuan cara menggosok gigi antara sebelum dan sesudah mendapatkan intervensi metode diskusi kelompok pada kelompok eksperimen. Terlihat nilai p (uji t) = 0,000 < 0,05. Terdapat perbedaan post-test pengetahuan cara menggosok gigi kelompok control dan kelompok eksperimen. Terlihat nilai p uji t = 0,004 < 0,05.
Simpulan : Dapat digunakan oleh pihak sekolah agar dapat membuat program sekolah yang berkaitan dengan menambah pengetahuan tentang kesehatan khususnya dalam pengetahuan menggosok gigi, salah satunya dengan mengadakan penyuluhan tentang kesehatan dengan bekerja sama dengan institusi pendidikan kesehatan seperti Poltekkes Kemenkes Sorong.

Kata Kunci : Pengetahuan;Diskusi Kelompok;Menggosok Gigi.
A Theological Perspective of Domestic Violence in Kenya
Authors: Rono Miriam 
Published: April 2022

This paper acknowledges the fact that there is escalation of domestic violence in Kenya despite efforts of the church. Theologically in both Christianity and African religion violence is not accepted and taking away life is not condoned. It recognises how in the traditional African society domestic violence was limited unlike during this era of Christianity. This paper seeks to unveil how the Nandi Addressed domestic violence in the past and how the church can borrow from this in order to incorporate some of the traditional methods of resolving this form of violence. The study adopted a qualitative research design where the perceptions of the respondents were used to gather in-depth information about the field of study. The findings were analysed and presented descriptively. The main sources of domestic violence include drug abuse, poor foundation of children, unclear marital roles and economic problems among others. The major findings of the study are that domestic violence leads to character defamation and even death of persons. Lack of economic resources underpins women’s vulnerability to violence and their inability to disentangle themselves from abusive relationships. This paper recommends that there is need to revisit teachings from traditional institutions of marriage and initiations and incorporate positive forms of teaching with teachings in Christianity for harmony in the society. This paper concludes that the society is no longer knit together due to the brake up of the traditional family and the society in general. Domestic violence in Kenya indicates the laxity and failure of the religious institutions in checking family relationships. It further recommends that there is need to go back to our traditional family settings to reflect on what is expected of the family and to derive the worth of an individual and meaning of life
Forgetting rates of gist and peripheral episodic details in prose recall
Authors: Sacripante Riccardo , Logie Robert H. , Baddeley Alan , Della Sala Sergio 
Published: April 2022

AbstractIn a seminal study, Slamecka and McElree showed that the degree of initial learning of verbal material affected the intercepts but not the slopes of forgetting curves. However, more recent work has reported that memories for central events (gist) and memory for secondary details (peripheral) were forgotten at different rates over periods of days, with gist memory retained more consistently over time than details. The present experiments aimed to investigate whether qualitatively different types of memory scoring (gist vs. peripheral) are forgotten at different rates in prose recall. In three experiments, 232 participants listened to two prose narratives and were subsequently asked to freely recall the stories. In the first two experiments participants were tested repeatedly after days and a month, while in the third experiment they were tested only after a month to control for repeated retrieval. Memory for gist was higher than for peripheral details, which were forgotten at a faster rate over a month, with or without the presence of intermediate recall. Moreover, repeated retrieval had a significant benefit on both memory for gist and peripheral details. We conclude that the different nature of gist and peripheral details leads to a differential forgetting in prose free recall, while repeated retrieval does not have a differential effect on the retention of these different episodic details.
The amplitude of small eye movements can be accurately estimated with video-based eye trackers
Authors: Nyström Marcus , Niehorster Diederick C. , Andersson Richard , Hessels Roy S. , Hooge Ignace T. C. 
Published: April 2022

AbstractEstimating the gaze direction with a digital video-based pupil and corneal reflection (P-CR) eye tracker is challenging partly since a video camera is limited in terms of spatial and temporal resolution, and because the captured eye images contain noise. Through computer simulation, we evaluated the localization accuracy of pupil-, and CR centers in the eye image for small eye rotations (≪ 1 deg). Results highlight how inaccuracies in center localization are related to 1) how many pixels the pupil and CR span in the eye camera image, 2) the method to compute the center of the pupil and CRs, and 3) the level of image noise. Our results provide a possible explanation to why the amplitude of small saccades may not be accurately estimated by many currently used video-based eye trackers. We conclude that eye movements with arbitrarily small amplitudes can be accurately estimated using the P-CR eye-tracking principle given that the level of image noise is low and the pupil and CR span enough pixels in the eye camera, or if localization of the CR is based on the intensity values in the eye image instead of a binary representation.
Emergency Management Practices of Regional and District Officials in Western Russia (1941–1946)
Authors: Кометчиков И.В. 
Published: April 2022

На основе законодательных материалов, делопроизводства партийных, советских органов, органов Народного комиссариата внутренних дел СССР и Народного комиссариата государственной безопасности СССР, военных структур, статистики, источников личного происхождения из федеральных и региональных архивов анализируются причины, проявления и последствия чрезвычайных практик региональной и районной власти на Западе РСФСР в 1941–1946годах. Делается вывод о том, что наряду с факторами военного времени (сокращение количества квалифицированных управленцев из-за мобилизаций на фронт, эвакуация, концентрация власти в чрезвычайных военизированных структурах, милитаризация их работы и др.) важной причиной «чрезвычайщины» был низкий уровень капитализации ключевых отраслей экономики Запада РСФСР, когда распространенность ручного труда обусловливала активное применение чрезвычайных способов его мобилизации. Воспроизводство большинства чрезвычайных практик власти завершилось с переходом к мирному времени. Лишь такие из них, как институт уполномоченных партийных органов, просуществовали в регионе до завершения индустриальной трансформации советского общества в начале 1960-х годов.
Based on legislative materials, the records of the Party, the committees, NKVD (the People’s Commissariat for Internal Affairs), NKGB (the People’s Commissariat for State Security) and military organizations as well as statistical data and private sources from the federal and regional archives, we analyzed the reasons, manifestations and consequences of practices of regional and local authorities in the Western part of the RSFSR (the Russian Soviet Federative Socialist Republic) during the state of emergency in 1941–1946. We came to the conclusion that it was not only the influence of the wartime which entailed a drop in the number of qualified executives due to the mobilization, evacuation, the concentration of power in military organizations and the militarization of their work, that was an important factor in establishing the state of emergency. Besides that, it was caused by a low level of capitalization of key economic sectors in the Western RSFSR under the circumstances of manual labor being extremely widespread and conducive to its urgent mobilization. Most of those practices were abolished after the war was over. Only a few of them, such as “the authority institute”, lived on until the industrial transformation of the Soviet society came to an end in the early 1960s.
Discovery of a Giant Molecular Loop in the Central Region of NGC 253
Authors: Konishi R. , Enokiya R. , Fukui Y. , Muraoka K. , Tokuda K. , Onishi T. 
Published: April 2022

Abstract
NGC 253 is a starburst galaxy of SAB(s)c type with increasing interest because of its high activity at unrivaled closeness. Its energetic event is manifested as the vertical gas features in its central molecular zone, for which stellar feedback was proposed as the driving engine. In order to pursue details of the activity, we have undertaken a kinematic analysis of the ALMA archive data of 12CO(J = 3 − 2) emission at the highest resolution ∼3 pc. We revealed that one of the non-rotating gas components in the central molecular zone shows a loop-like structure of ∼200 pc radius. The loop-like structure is associated with a star cluster, whereas the cluster is not inside the loop-like structure and is not likely as the driver of the loop-like structure formation. Further, we find that the bar potential of NGC 253 seems to be too weak to drive the gas motion by the eccentric orbit. As an alternative, we frame a scenario that magnetic acceleration by the Parker instability is responsible for the creation of the loop-like structure. We show that the observed loop-like structure properties are similar to those in the Milky Way, and argue that recent magneto-hydrodynamics simulations lend support for the picture having the magnetic field strength of ≳100 μG. We suggest that cluster formation was triggered by the falling gas to the footpoint of the loop, which is consistent with a typical dynamical timescale of the loop ∼1 Myr.
Magnetic Braking of Accreting T Tauri Stars II: Torque Formulation Spanning Spin-up and Spin-down Regimes
Authors: Ireland Lewis G. , Matt Sean P. , Zanni Claudio 
Published: April 2022

Abstract
The magnetic interaction between a classical T Tauri star and its surrounding accretion disk is thought to influence its rotational evolution. We use 2.5D magnetohydrodynamic, axisymmetric simulations of star-disk interaction, computed via the PLUTO code, to calculate the net torque acting on these stars. We divide the net torque into three contributions: accretion (spin-up), stellar winds (spin-down), and magnetospheric ejections (MEs) (spin-up or down). In Paper I, we explored interaction regimes in which the stellar magnetosphere truncates the inner disk at a location spinning faster than the star, resulting in a strong net spin-up contribution from accretion and MEs (“steady accretion” regime). In this paper, we investigate interaction regimes in which the truncation radius gets closer to and even exceeds corotation, where it is possible for the disk material to gain angular momentum and be periodically ejected by the centrifugal barrier (“propeller” regime). This reduces the accretion torque, can change the sign of the ME torque, and can result in a net stellar spin-down configuration. These results suggest it is possible to have a net spin-down stellar torque even for truncation radii within the corotation radius (R
t ≳ 0.7R
co). We fit semi-analytic functions for the truncation radius, and the torque associated with star-disk interaction (i.e., the sum of accretion and ME torques) and stellar wind, allowing for the prediction of the net stellar torque for a parameter regime covering both net spin-up and spin-down configurations, as well as the possibility of investigating rotational evolution via 1D stellar evolution codes.
Very High-energy Afterglow Emission of GRB 190829A: Evidence for Its Hadronic Origin?
Authors: Sahu Sarira , Valadez Polanco Isabel Abigail , Rajpoot Subhash 
Published: April 2022

Abstract
The detection of multi-TeV gamma rays from the afterglow phase of GRB 190829A by the High Energy Stereoscopic System telescope is an addition to the already existing list of two GRBs observed in very high-energy (VHE) gamma rays in recent years. Jets of blazars and GRBs have many similarities and the photohadronic model is very successful in explaining the VHE gamma-ray spectra from the high-energy blazars. Recently, the photohadronic model has been successfully applied to study the sub-TeV gamma rays from the afterglow phases of GRB 180720B and GRB 190114C. We employed this model again to explain the VHE spectra observed for the two consecutive nights from GRB 190829A. We show that the spectra of GRB 190829A can be due to the interactions of high-energy protons with the synchrotron self-Compton photons in the forward shock region of the GRB jet, similar to the low emission state of the VHE flaring events of high-energy blazars. We speculate that, if in the future, it is possible to observe the VHE gamma-ray spectra from nearby GRBs in their afterglow phases, then some of them could only be explained by employing two different spectral indices. If confirmed, such VHE spectra could be interpreted as a result of the interactions of the high-energy protons with the photons, both from the synchrotron background and the synchrotron self-Compton background in the forward shock region.
A Single-pulse Study of the Subpulse Drifter PSR J1631+1252 Discovered at FAST
Authors: Wen Z. G. , Yuan J. P. , Wang N. , Li D. , Chen J. L. , Wang P. , Wu Q. D. , Yan W. M. , Yuen R. , Wang Z. , Tedila H. M. , Wang H. G. , Zhu W. W. , Niu J. R. , Miao C. C. , Xue M. Y. , Duan X. F. , Xiang B. B. , He D. L. 
Published: April 2022

Abstract
We report on the pulse-to-pulse energy distribution and longitude-resolved modulation properties of PSR J1631+1252 discovered by the Five-hundred-meter Aperture Spherical radio Telescope. Our analysis made use of the data acquired at 1250 MHz from the follow-up timing observations that lasted over a year. PSR J1631+1252 has a rotational period of ∼0.310 s, and a dispersion measure of ∼32.73 pc cm−3. The energy distribution is well described by a lognormal distribution, the parameters of which do not vary with time. We show that large modulation occurs across the bridge emission of the pulse profile, with sporadic bright bursts at the leading emission region. The fluctuation spectral analysis reveals the existence of subpulse drifting in the leading component with vertical spacing between the drift bands of 3.28 ± 0.08 pulse periods between consecutive drift bands. Possible physical mechanisms for subpulse drifting are discussed.
The Interstellar Medium in the Environment of the Supernova-less Long-duration GRB 111005A
Authors: Leśniewska Aleksandra , Michałowski M. J. , Kamphuis P. , Dziadura K. , Baes M. , Cerón J. M. Castro , Gentile G. , Hjorth J. , Hunt L. K. , Jespersen C. K. , Koprowski M. P. , Floc’h E. Le , Miraghaei H. , Guelbenzu A. Nicuesa , Oszkiewicz D. , Palazzi E. , Polińska M. , Rasmussen J. , Schady P. , Watson D. 
Published: April 2022

Abstract
Long (>2 s) gamma-ray bursts (GRBs) are associated with explosions of massive stars, although in three instances, supernovae (SNe) have not been detected, despite deep observations. With new H i line and archival optical integral-field spectroscopy data, we characterize the interstellar medium (ISM) of the host galaxy of one of these events, GRB 111005A, in order to shed light on the unclear nature of these peculiar objects. We found that the atomic gas, radio continuum, and rotational patterns are in general very smooth throughout the galaxy, which does not indicate a recent gas inflow or outflow. There is also no gas concentration around the GRB position. The ISM in this galaxy differs from that in hosts of other GRBs and SNe, which may suggest that the progenitor of GRB 111005A was not an explosion of a very massive star (e.g., a compact object merger). However, there are subtle irregularities of the GRB 111005A host (most at a 2σ level), which may point to a weak gas inflow or interaction. Because in the SE part of the host there is 15% more atomic gas and half the molecular gas than in the NW part, the molecular gas fraction is low. In the SE part there is also a region with a very high Hα equivalent width. There is more continuum 1.4 GHz emission to the SE and an S-shaped warp in the UV. Finally, there is also a low-metallicity region 3.″5 (1 kpc) from the GRB position. Two galaxies within 300 kpc or a past merger can be responsible for these irregularities.
The Refined Transit Ephemeris of TOI-2180 b
Authors: Dalba Paul A. , Jacobs Thomas Lee , Omohundro Mark , Gagliano Robert , Jursich Jay , Kristiansen Martti H. , LaCourse Daryll M. , Schwengeler Hans M. , Terentev Ivan A. 
Published: April 2022

Abstract
The Transiting Exoplanet Survey Satellite (TESS) observed a single transit of the giant exoplanet TOI-2180 b in Sector 19 of its primary mission. A subsequent effort to characterize this system found that the orbital period of TOI-2180 b is 260.8 ± 0.6 days. This level of precision precludes most efforts to detect future transits and to further understand this exoplanet. We present a new transit of TOI-2180 b observed by TESS in Sector 48 and update the planet’s transit ephemeris with its precisely measured orbital period. The refined ephemeris enables future transit observations to explore this planet’s atmosphere or to search for rings or moons.
Factors Related to Depression among Caregivers Attending Post-Ischemic Stroke Patients
Authors: Khaddafi Muhammad Rio , Loebis Bahagia , Nasution Nazli Mahdinasari , Rambe Aldy Safruddin , Effendy Elmeida , Amin Mustafa M. 
Published: April 2022

BACKGROUND: Stroke is known as chronic disease, leading to disability which makes help from caregivers become necessary. Attending stroke patients possess certain challenges and burdens toward the caregivers.

AIM: We aim to investigate risk factors related to depression among caregivers attending post-ischemic stroke.

METHODS: Eighty-three caregivers and post-ischemic stroke patients were collected consecutively from the Neurology Department of Universitas Sumatera Utara Hospital, Medan, Indonesia. Linear regression was used to analyze the data.

RESULTS: Our multivariate study shows that patient’s age, caregiver’s gender, patient’s gender, and modified Barthel Index are associated with depression with adjusted R2 of 59.3%.

CONCLUSION: Early detection and intervention should be addressed regularly for caregivers attending post-stroke patients.
Ergothérapie en psychiatrie
Authors: Guihard Jean-Philippe 
Published: April 2022

Résumé La folie ou les folies interroge(nt) nos pratiques cliniques quant à leur validité. Mais elle(s) interroge(nt) aussi les concepts qui sous-tendent ces pratiques. Ainsi, pourquoi l’ergothérapie a-t-elle sa place dans le processus thérapeutique relatif au(x) folie(s) et en quoi l’activité, l’acte et l’action sont-ils des données fondamentales dans cette perspective ? La place donnée à la parole est prépondérante alors que le lieu et le lien de rencontre du sujet sont l’activité véritablement porteuse de signification et partageable socialement. Cette thérapie des troubles de l’activité humaine ne serait-elle pas l’ergon-thérapie ?
Ergothérapie en psychiatrie
Authors: Gumy Marc 
Published: April 2022

Résumé Dans un cadre institutionnel, cette communication évoque une partie de l’histoire thérapeutique d’une jeune fille souffrant de graves troubles narcissiques. Son traitement nous a mené à la rencontre des éléments corporels de la composition du narcissisme et des contenants de pensée archaïques. Les moyens mis en œuvre sont exposés chronologiquement : un groupe thérapeutique ; une médiation corporelle : le massage ; un atelier : la sculpture. Ils illustrent une certaine manière d’intégrer un mode de compréhension psychodynamique, le champ cognitif et l’approche corporelle.
Crowdfunding et transition énergétique : analyse empirique des plateformes de financement participatif des projets d’énergies renouvelables en France
Authors: Lesgards Valérie , Stelitano Salvatore 
Published: April 2022

Cet article vise à mieux comprendre la réalité du crowdfunding en France, en termes de contribution à la transition énergétique et en termes d’engagement citoyen dans les projets d’énergies renouvelables. La méthodologie utilisée est une analyse statistique exploratoire quantitative des données en open source recueillies sur 9 plateformes de crowdfunding . Les résultats montrent qu’à l’horizon 2030, les projets de crowdfunding pourraient contribuer à hauteur de 33 % à l’objectif national de 216 TWh de production d’énergies renouvelables fixé par la loi. Cette estimation repose sur la poursuite du modèle actuel dans lequel le citoyen investit en moyenne 2 643 € par projet et finance 14 % en moyenne du coût total du projet. Ces résultats sont comparés avec ceux de la littérature et quelques recommandations sont également formulées pour renforcer le crowdfunding au service de la transition énergétique. Codes JEL : O30, G23