bluuebunny/crossref_metadata_2025_split huggingface dataset:
MODERN TEACHERS’ COGNITIVE STYLES: EXPLORING FROM PHENOMENON DEFINITION TO ITS REALIZATION
Authors: Кац Александра Семеновна 
Published: November 2020

В статье рассматривается проблема совершенствования профессиональной деятельности педагогов в условиях цифровизации образования. Во введении актуализируется вопрос идентификации и исследования когнитивных стилей педагогов как специфической особенности их профессиональной деятельности.Представлены теоретические и эмпирические методы, которые были использованы в ходе проведенного исследования. Результаты исследования раскрывают влияние особенностей цифровизации на педагогическое взаимодействие «педагог - обучающийся - образовательная среда»: массовое внедрение цифровых технологий в процесс обучения, изменение методики преподавания дисциплины в соответствии с потребностями студентов «цифрового поколения». Представлена авторская реализация этапов педагогического взаимодействия педагога и студентов (с акцентом на когнитивный стиль педагога). Выявлены изменения в характере педагогического взаимодействия, обусловленные анализом когнитивных стилей педагогов: индивидуализация процесса обучения студентов при сохранении типовых интеллектуальных (поведенческих) реакций педагога. В выводах приводятся аргументы, свидетельствующие о важности исследования когнитивных стилей педагогов и их практического применения: необходимость постоянного саморазвития и самосовершенствования, выбор индивидуальной траектории саморазвития, совершенствование умения структурировать информацию средствами когниций.
The article deals with the acute problem of enhancing teachers’ professional activity in the conditions of education digitalization. In the introduction the problem of identification and research of teachers’ cognitive styles as a specific feature of their professional activity is actualized. The paper Presents theoretical and empirical methods employed in the research. The research results reveal digitalization specific influence on pedagogical interaction «teacher - learner - educational environment»: mass implementation of digital technologies in the process of teaching, changes in teaching methods in accordance with the needs of «digital generation». The article also provides the author’s realization of the stages of pedagogical interaction between the teacher and students (with an accent on teachers’ cognitive style). It reveals the changes in the character of pedagogical interaction conditioned by the analysis of teachers’ cognitive styles: individualization of students’ learning process while preserving teacher’s typical inteltectual behavior reactions. The results present arguments for the importance of cognitive style research and its practical implementation: need for constant self-development and self-improvement, choice of individual self-development vector, enhanced ability to systemize information via means of cognition.
ATTITUDE OF UNIVERSITY STUDENTS TO DISTANCE LEARNING
Authors: Петрова Татьяна Николаевна , Пьянзина Надежда Николаевна 
Published: November 2020

В последние годы одной из весьма востребованныхформ организации учебного процесса является дистанционное обучение. Быстрому внедрению данной формы обучения в образовательный процесс поспособствовала и пандемия. Предметом исследования является отношение обучающихся к дистанционному формату обучения. Исследование проводилось на основе опроса непосредственных участников данной формы работы - обучающихся. По результатам опроса можно сделать вывод, что дистанционная форма не является для обучающихся совершенно новым форматом организации учебного процесса. Это объясняется тем, что многие преподаватели в своей работе уже используют такую форму обучения студентов на основе информационных технологий. В большинстве своем обучающиеся испытывали трудности в самостоятельной организации своего учебного пространства в условиях «домашнего обучения». При этом основная доля опрошенных считает, что дистанционное обучение - это благоприятная система получения знаний. Проведенное исследование позволило выявить положительные моменты (возможности самообразования и самообучения, индивидуальный темп обучения, экономия времени и т. д.) и имеющиеся проблемы (недостаточный уровень компьютерной грамотности, низкая техническая оснащенность, низкая пропускная способность интернета, недостаточная наполненность дистанционных курсов учебно-методическими материалами) удаленного обучения, что имеет практическое значение для его дальнейшего совершенствования.
In recent years, one of the very popular forms of organization of the educational process is distance learning. The pandemic also contributed to the rapid introduction of this form of education into the educational process. The subject of the study is the attitude of students to the distance learning format. The study was conducted on the basis of a survey of direct participants in this form of work - students. According to the results of the survey, we can conclude that the transition to a distance learning form is not a completely new format for organizing the educational process for students.This is due to the fact that many teachers in their work already use this form of student learning based on information technology. The majority of students experienced difficulties in the independent organization of their educational space in the conditions of «home learning». At the same time, the most respondents consider that distance learning is a favorable system for acquiring knowledge. The study allowed us to identify positive aspects (opportunities for self-education and selftraining, individual learning pace, time saving, etc.) and existing problems (insufficient computer literacy, low technical equipment, low Internet bandwidth, and insufficient content distance courses with teaching materials) distance learning, which is of practical importance for its further improvement.
Mean platelet volume (MPV) and neonatal outcomes of infants born to mothers with preeclampsia
Authors: SELÇUK Sinem Nur , YURDAKÖK Murat , YİĞİT Şule 
Published: November 2020

Aim
Preeclampsia may cause both maternal and neonatal complications. Uteroplacental dysfunction is one of the reasons of fetal and neonatal complications in preeclampsia. Recent findings about the etiology and pathogenesis of the disease shows that inflammation is one of the factors responsible for maternal complications, thus neonatal complications should be associated with the same inflammatory process. We considered evaluating mean platelet volume (MPV) of infants born to mothers with preeclampsia, based on the findings of elevated MPV values in pregnant women with preeclampsia.

Materials and methods
This study was carried out at the Neonatal Intensive Care Unit of Hacettepe University Ihsan Dogramacı Children’s Hospital and consisted of 148 infants born to mothers with preeclampsia and 147 infants as a control group which were selected by stratified sampling system. Hematological parameters (mean platelet volume, hemoglobin values, white blood cell and platelet counts) and common neonatal morbidities (small for gestational age, respiratory distress syndrome, necrotizing enterocolitis, intraventricular hemorrhage and patent ductus arteriosus) were evaluated between groups.

Results
The infants of mothers with preeclampsia had significantly elevated MPV and hemoglobin values (p
Predicting the Kinematic Evidence of Gravitational Instability
Authors: Hall C. , Dong R. , Teague R. , Terry J. , Pinte C. , Paneque-Carreño T. , Veronesi B. , Alexander R. D. , Lodato G. 
Published: November 2020

Abstract
Observations with the Atacama Large Millimeter/Submillimeter Array (ALMA) have dramatically improved our understanding of the site of exoplanet formation: protoplanetary disks. However, many basic properties of these disks are not well understood. The most fundamental of these is the total disk mass, which sets the mass budget for planet formation. Disks with sufficiently high masses can excite gravitational instability and drive spiral arms that are detectable with ALMA. Although spirals have been detected in ALMA observations of the dust, their association with gravitational instability, and high disk masses, is far from clear. Here we report a prediction for kinematic evidence of gravitational instability. Using hydrodynamics simulations coupled with radiative transfer calculations, we show that a disk undergoing such instability has clear kinematic signatures in molecular line observations across the entire disk azimuth and radius, which are independent of viewing angle. If these signatures are detected, it will provide the clearest evidence for the occurrence of gravitational instability in planet-forming disks, and provide a crucial way to measure disk masses.
The First Extensive Spectroscopic Study of Young Stars in the North America and Pelican Nebulae
Authors: Fang Min , Hillenbrand Lynne A. , Kim Jinyoung Serena , Findeisen Krzysztof , Herczeg Gregory J. , Carpenter John M. , Rebull Luisa M. , Wang Hongchi 
Published: November 2020

Abstract
We present a spectroscopic survey of over 3400 potential members in the North America and Pelican Nebulae (NAP) using several low-resolution (R ≈ 1300–2000) spectrographs: Palomar/Norris, WIYN/Hydra, Keck/DEep Imaging Multi-Object Spectrograph (DEIMOS), and the Multiple Mirror Telescope (MMT)/Hectospec. We identify 580 young stars as likely members of the NAP region based on criteria involving infrared excess, Li I 6708 Å absorption, X-ray emission, parallax, and proper motions. The spectral types of individual spectra are derived by fitting them with templates that are either empirical spectra of pre-main-sequence stars or model atmospheres. The templates are artificially veiled, and a best-fit combination of spectral type and veiling parameter is derived for each star. We use the spectral types with archival photometry to derive V-band extinction and stellar luminosity. From the Hertzsprung–Russell diagram, the median age of the young stars is about 1 Myr, with a luminosity dispersion of ∼0.3–0.4 dex. We investigate the photometric variability of the spectroscopic member sample using Zwicky Transient Facility data and conclude that photometric variability, while present, does not significantly contribute to the luminosity dispersion. While larger than the formal errors, the luminosity dispersion is smaller than if veiling were not taken into account in our spectral typing process. The measured ages of the stellar kinematic groups, combined with the inferred ages for embedded stellar populations revealed by Spitzer, suggest a sequential history of star formation in the NAP region.
Texas Spectroscopic Search for Lyα Emission at the End of Reionization. III. The Lyα Equivalent-width Distribution and Ionized Structures at z > 7
Authors: Jung Intae , Finkelstein Steven L. , Dickinson Mark , Hutchison Taylor A. , Larson Rebecca L. , Papovich Casey , Pentericci Laura , Straughn Amber N. , Guo Yicheng , Malhotra Sangeeta , Rhoads James , Song Mimi , Tilvi Vithal , Wold Isak 
Published: November 2020

Abstract
Lyα emission from galaxies can be utilized to characterize the ionization state in the intergalactic medium (IGM). We report our search for Lyα emission at z > 7 using a comprehensive Keck/MOSFIRE near-infrared spectroscopic data set, as part of the Texas Spectroscopic Search for Lyα Emission at the End of Reionization Survey. We analyze data from 10 nights of MOSFIRE observations which together target 72 high-z candidate galaxies in the GOODS-N field, all with deep exposure times of 4.5–19 hr. Utilizing an improved automated emission-line search, we report 10 Lyα emission lines detected (>4σ) at z > 7, significantly increasing the spectroscopically confirmed sample. Our sample includes large equivalent-width (EW) Lyα emitters (>50 Å), and additional tentative Lyα emission lines detected at 3σ–4σ from five additional galaxies. We constrain the Lyα EW distribution at z ∼ 7.6, finding a significant drop from z ≲ 6, suggesting an increasing fraction of neutral hydrogen (H i) in the IGM in this epoch. We estimate the Lyα transmission through the IGM (=EW
z ∼ 7.6/EW

) and infer an IGM H i fraction (X
HI) of

at z ∼ 7.6, which is lower in modest tension (>1σ) with recent measurements at z ∼ 7.6. The spatial distribution of the detected Lyα emitters implies the presence of a potential highly ionized region at z ∼ 7.55, which hosts four Lyα emitters within a ∼40 cMpc spatial separation. The prominence of this ionized region in our data set could explain our lower inferred value of X
HI, though our analysis is also sensitive to the chosen reference Lyα EW distribution values and reionization models.
Remarkable Migration of the Solar System from the Innermost Galactic Disk; a Wander, a Wobble, and a Climate Catastrophe on the Earth
Authors: Tsujimoto Takuji , Baba Junichi 
Published: November 2020

Abstract
Recent knowledge of Galactic dynamics suggests that stars radially move on the disk when they encounter transient spiral arms that are naturally generated during the process of disk formation. We argue that the large movement of the solar system from the innermost disk over its lifetime is inferred from an elemental abundance pattern of the Sun to those of solar twins within the Galactic chemical evolutionary framework. The implied metal-rich environment at the Sun’s birthplace and its formation time are supported by measured silicon isotopic ratios in presolar silicon carbide grains. We perform numerical simulations of the dynamical evolution of disk stars in a Milky Way–like galaxy to identify the lifetime trajectory of the solar system. We find that a solar system born in the proximity of the Galactic bulge could travel to the current locus by the effect of radial migration induced by several major encounters with spiral arms. The frequent feature we identify is the repeated passages of stars inside the same spiral arm owing to the wobble of stars traveling in and out of the spiral arms. We predict that such episodes are evidenced in the Earth’s geological history as snowball Earth and that their occurrence times are within our predictions. In particular, the stellar motion that vertically oscillates during passages through spiral arms occasionally leads to a split into two discrete passage episodes with an interval of several tens of megayears, implying two relevant snowball Earth events that occurred in rapid succession (∼720 and 650 million years ago).
No Evidence for [C ii] Halos or High-velocity Outflows in z ≳ 6 Quasar Host Galaxies
Authors: Novak Mladen , Venemans Bram P. , Walter Fabian , Neeleman Marcel , Kaasinen Melanie , Liang Lichen , Feldmann Robert , Bañados Eduardo , Carilli Chris , Decarli Roberto , Drake Alyssa B. , Fan Xiaohui , Farina Emanuele P. , Mazzucchelli Chiara , Rix Hans-Walter , Wang Ran 
Published: November 2020

Abstract
We study the interstellar medium in a sample of 27 high-redshift quasar host galaxies at z ≳ 6, using the [C ii] 158 μm emission line and the underlying dust continuum observed at ∼1 kpc resolution with Atacama Large Millimeter Array. By performing uv-plane spectral stacking of both the high and low spatial resolution data, we investigate the spatial and velocity extent of gas and the size of the dust-emitting regions. We find that the average surface brightness profile of both the [C ii] and the dust continuum emission can be described by a steep component within a radius of 2 kpc and a shallower component with a scale length of 2 kpc, detected up to ∼10 kpc. The surface brightness of the extended emission drops below ∼1% of the peak at radius of ∼5 kpc, beyond which it constitutes 10%–20% of the total measured flux density. Although the central component of the dust continuum emission is more compact than that of the [C ii] emission, the extended components have equivalent profiles. The observed extended components are consistent with those predicted by hydrodynamical simulations of galaxies with similar infrared luminosities, where the dust emission is powered by star formation. The [C ii] spectrum measured in the mean uv-plane stacked data can be described by a single Gaussian, with no observable [C ii] broad-line emission (velocities in excess of ≳500 km s−1), which would be indicative of outflows. Our findings suggest that we are probing the interstellar medium and associated star formation in the quasar host galaxies up to radii of 10 kpc, whereas we find no evidence for halos or outflows.
Dies Viri, jour de virus et des hommes
Authors: Ostermann Gérard , Lesœurs Guy 
Published: November 2020

Dans cet article, les auteurs explorent, sans concession et avec humour, le corpus sémantique, fantasmatique, archétypal et… floral appliqué à la maladie covid-19 en se référant à une enquête sur les représentations imaginaire et symbolique actuelles. Leur questionnement débouche sur une saine écologie de l’esprit où l’individuation du Soi rejoint une prise de conscience collective et alarmante de la lutte entre Nature et Culture. Les auteurs nous situent le jour d’après le « grand enfermement » et au moment où la pandémie, toujours nocive, par cette épreuve inflationniste et inflammatoire fait vaciller la certitude de notre monde d’avant, porteur, à son insu, de la plaie purulente d’une économie mondiale attisée par notre fièvre d’explosion égotiste.
Prendre en charge les mineurs non accompagnés : spécificités d’un dispositif complémentariste en contexte transculturel
Authors: Guessoum Selim Benjamin , Touhami Fatima , Radjack Rahmeth , Moro Marie Rose , Minassian Sevan 
Published: November 2020

Les mineurs non accompagnés sont des enfants et des adolescents qui ont quitté leurs pays et se trouvent sans adulte référent dans un pays étranger. Ils présentent un taux élevé de symptômes psychiatriques avec des intrications complexes au niveau psycho-traumatique, transculturel, familial, éducatif et judiciaire. Le dispositif clinique NatMIE a été créé à l’Hôpital Cochin à Paris afin de répondre aux besoins spécifiques des mineurs non accompagnés. Il s’agit d’une consultation conjointe psychiatre-psychologue qui associe auprès du jeune le professionnel qui l’accompagne au quotidien, permettant un travail institutionnel. L’approche transculturelle s’avère indispensable, avec le concours systématique d’un médiateur culturel. L’approche narrative apporte une continuité et une cohérence à un récit de vie fragmenté, notamment à travers des objets de médiation. C’est un dispositif qui fait appel à plusieurs approches : psychiatrique et psychologique, transculturelle, narrative et institutionnelle.
L’approche clinique transculturelle en expertise psychologique pénale
Authors: Barbaras Caroline , Titia Rizzi Alice 
Published: November 2020

Cet article établit la nécessité de prendre en considération l’approche transculturelle dans le cadre des expertises psychologiques ordonnées dans une procédure pénale. Elle permet d’éviter trois écueils auxquels le psychologue peut se confronter s’il ne tient pas compte des théories étiologiques du mal ou du désastre que tout sujet produit à partir de sa propre culture : la dissolution de la singularité du sujet dans l’universalité du droit ; le piège de la question de la crédibilité ; le sur-diagnostic de psychose dans le champ pénal. Le sujet du droit est appréhendé ici dans son rapport à la culture en tant que Culture et par le biais du discours qu’il produit de manière singulière sur ce rapport. Trois cas cliniques illustrent cette méthode au service de l’avènement de l’universel concret dans le champ pénal.
À la croisée des chemins. Entre routes de pouvoir et sentiers cliniques
Authors: Zoldan Yann , Rousseau Cécile 
Published: November 2020

Cet article invite le lecteur à croiser les chemins de la psychanalyse et des rapports de pouvoir à l’œuvre dans la société. A travers l’exemple actuel de la théorie de l’intersectionnalité issue des luttes féministes noires américaines, nous interrogeons l’intérêt de cette rencontre pour la prise en charge clinique. Le défi théorique émerge des défis sociétaux auxquels se confronte notre clinique : sociétés multiculturelles, interrogations autour du genre, etc. Ces enjeux de société bousculent les dynamiques de pouvoir et nécessitent de penser la place des privilèges et des discriminations dans nos pratiques cliniques.
Accountability ou Prestação de Contas, CGU ou Tribunais de Contas: o exame de diferentes visões sobre a atuação dos órgãos de controle nos municípios brasileiros.
Authors: Almeida Fernandes Gustavo Andrey , Teixeira Marco Antonio Carvalho 
Published: November 2020

The lack of cognitive models to explain the concept of accountability can be synthesized in the absence of a single term in the Portuguese language since Accountability is usually considered a word whose meaning is incomplete. The impact of cognitive models in the form of audit is taken is very important. Courts of Accounts were established in Brazil since Old Republic while CGU was created in 2003. In this paper, we analyze the conceptual differences between the Courts of Accounts and Federal Comptroller General regarding accountability. Despite many municipal actions receive a dual inspection, data shows a wide divergence between the results obtained by respective TCE and CGU. The performance of the latter is closer to an audit of performance, reporting on average a larger number of irregularities in the cities, whereas in the Courts of Accounts, it is usually done audit of compliance, with relatively minor findings.
Hand Hygiene Perception and Handshaking Practices among Pediatric Inpatient Caregivers
Authors: Temsah Mohamad-Hani , Alsohaime Fahad M. , Al-Eyadhy Ayman , Hasan Gamal , Alarfaj Abdulrahman , Bajri Hazim , Al-Judi Talal , Al-Mazyad Gosay , Al-Shammari Abdulrahman , Jawad Majeed , Sklansky Mark S. , Al-Subaie Sarah , Somily Ali Mohammed 
Published: November 2020

Background:
Direct or indirect hand contact plays a significant role in health-care-associated infections. Family members of pediatric patients may have various hand hygiene practices. We aimed to evaluate the perceptions of hand hygiene and handshaking practices among family caregivers of hospitalized children in a tertiary care hospital.

Methods:
A cross-sectional study was conducted using a pretested two-part questionnaire for a randomly selected caregiver of hospitalized children at King Khalid University Hospital, Riyadh, Saudi Arabia, between January 21 and March 8, 2018. The survey data were analyzed using SPSS version 21.

Results:
One hundred and eighty caregivers voluntarily participated in the study. The mean age was 35.1 years, and female parents comprised 85.6% of the sample. The majority of participants (82.8%) did not receive any previous formal education on hand hygiene. Most of the participants (relative importance index of 84.6%) had correct answers on a modified version of the World Health Organization “Perception Survey for Health-Care Workers.” However, handshaking avoidance was low in general, with caregivers reporting their handshaking practices did not change even when dealing with people who have flu-like symptoms. There was no significant correlation between the participants' characteristics and handshaking avoidance practice, except for those who were working in the medical field, who showed a significantly higher handshaking avoidance.

Conclusion:
Formal education for hospitalized children's caregivers on hand hygiene and handshaking practice is lacking. Information on appropriate hand hygiene and potential risks of infection spread is required, especially for those parents without a previous medical background.