bluuebunny/crossref_metadata_2025_split huggingface dataset:
К ВОПРОСУ ПРЕПОДАВАНИЯ БАЗОВЫХ ДИСЦИПЛИН В СВЕТЕ МОДЕРНИЗАЦИИ МЕДИЦИНСКОГО ОБРАЗОВАНИЯ
Authors: Ж.К. Смаилова , Р.Р. Олжаева , А.Р. Алимбаева , Д.Д. Муртазина , К.Т. Сыдыкова , Б.С. Советов , А.Ш. Омарова , Р.Т. Динжуманова , Н.Н. Сентябрев 
Published: November 2024

В свете модернизации высшего медицинского образования в Казахстане формирование фундаментальных знаний принадлежит к числу актуальных проблем общей подготовки врачей, для которых биохимические методы исследования являются значительным источником диагностической информации. Понимание сути и взаимосвязи биохимических процессов в организме способствует формированию клинического мышления современного специалиста. С учетом актуальности проблемы статья посвящена определению методов и форм усовершенствования процесса преподавания биохимии в медицинском вузе. Рассмотрены активные методы и формы обучения, описаны различные методики проведения интегрированных занятий с использованием клинических ситуационных задач. На основании накопленного опыта преподавания биохимии на кафедре сформулированы рекомендации по улучшению учебного процесса, позволяющие повысить качество обучения.
In light of the modernization of higher medical education in Kazakhstan, the formation of fundamental knowledge is one of the main problems of General training of doctors for whom biochemical research methods are a significant source of diagnostic information. Understanding the nature and relationship of biochemical processes in the organism to the formation of clinical thinking of the modern specialist. Taking into account the urgency of the problem, the article is devoted to the definition of methods and forms of improving the process of teaching biochemistry in medical school. The active methods and forms of training are considered, various methods of integrated training with the use of clinical situational problems are described. Based on the experience of teaching biochemistry at the Department formulated recommendations to improve the educational process, to improve the quality of education.
Қазақстанда жоғары медициналық білім беруді жетілдіру аясында негізгі базалық білімнің қалыптасуы болашақ дәрігерлердің жалпы дайындауындағы өзекті мәселелердің бірі болып табылады, оларға биохимиялық зерттеу әдістері – диагностикалық ақпарат алудың негізгі көзі. Ағзадағы биохимиялық үрдістердің мәні мен өзара байланысын түсіну заманауи маманның клиникалық ой-танымының қалыптасуына ықпал етеді. Мәселенің өзектілігін ескере келе, мақала медициналық жоғары оқу орнында биохимия пәнін оқытудың әдістерін және жетілдірудің түрлерін анықтауға арналған. Білім берудің белсенді әдістері мен түрлері қарастырылған, клиникалық есептерді пайдалана отыра интеграциялық сабақтар өткізудің түрлі әдістемелері сипатталған. Кафедрада биохимияны оқытудың көптеген жылдар бойы жиналған тәжірибесінің негізінде білім сапасын арттыруға, білім беру үрдісін жақсартуға ықпал ететін ұсыныстар берілген.
СОЦИАЛЬНОЕ ПАРТНЁРСТВО В ПСИХИАТРИИ
Authors: С.Н. Молчанов , М.Т. Шакирова 
Published: November 2024

Резюме В Республике Казахстан в следующем 2019 году ожидаются кардинальные перемены в сфере оказания помощи больным с психическими заболеваниями. Основные усилия специалистов будут направлены на реабилитационную составляющую, и здесь ощутимую помощь могут оказать неправительственные организации, работающие в данном направлении.
In the Republic of Kazakhstan in the next year of 2019 cardinal changes are expected in the sphere of rendering assistance to patients with mental illnesses. The main efforts of specialists will be directed to the rehabilitation component, and here the tangible assistance can be provided by non-governmental organizations working in this direction.
Қазақстан Республикасында келесі 2019 жылы психикалық аурулары бар науқастарға көмек көрсету саласында кардиналды өзгерістер күтіліп отыр. Мамандардың негізгі күші оңалтулық құрамға бағытталмақ және осы кезде осы бағытта істейтін басқарушы емес ұйымдар айтарлықтай басым көмек көрсете алады.
DESEMPENHO E SATISFAÇÃO SEXUAL ENTRE MULHERES SUBMETIDAS À RADIOTERAPIA COMBINADA COM QUIMIOTERAPIA
Authors: Ferreira Édria Aparecida , Paula Carmen Lucia de , França Bartolomeu Expedito da Câmara , Velarde Luis Guillermo Coca , Marinheiro Lizanka Paola Figueiredo 
Published: November 2024

O câncer do colo do útero gera dificuldades na dinâmica sexual, cuja origem pode estar relacionada aos sintomas da doença, ao tratamento oncológico, entre outras situações que provoquem angústia, medo e assim comprometam a qualidade de vida. O objetivo desse estudo foi investigar o desempenho e satisfação sexual de mulheres que concluíram o tratamento para câncer do colo do útero. Foi realizado um estudo prospectivo, observacional, transversal e descritivo com a participação de 24 mulheres submetidas à radioterapia e quimioterapia combinada. Os dados sociodemográficos, clínicos e sobre desempenho sexual foram analisados por estatística descritiva através da metodologia de frequência, médias, medianas e desvio padrão. Os resultados demonstraram que houve predominância de mulheres pardas (58,3%), com mais de 9 anos de estudo (62,5%), solteiras (66,7%) e da religião protestante e católica (70,8%). A maioria (87%) apresentava doença avançada, sendo todas submetidas à radioterapia e quimioterapia combinada. Os resultados indicaram disfunção sexual entre quase um terço (29,1%) das mulheres após o tratamento, conforme Quociente Sexual Feminino (QS-F) com desempenho sexual variando do nulo ao regular e alterações em todas as fases da resposta sexual. Mesmo entre aquelas com desempenho regular pode haver carência de orientações para então melhorar a satisfação sexual, principalmente após o tratamento oncológico. Para todas as mulheres acometidas por câncer do colo do útero devem ser apresentados os possíveis efeitos do tratamento sobre função sexual bem como as possibilidades de manejo. Para o caso de disfunção sexual deve-se prover atendimento multiprofissional especializado.
DESENVOLVIMENTO DE UM GUIA INFORMATIVO COM ORIENTAÇÕES ACERCA DA PRESERVAÇÃO DO PATRIMÔNIO PÚBLICO DOS SERVIÇOS DE SAÚDE E SUA RELAÇÃO COM A SAÚDE DA POPULAÇÃO
Authors: Carneiro Helen Regina Marques , Furtado Rebeca Lopes , Guimarães Vitória Gabrielle Teixeira , Leopoldino Pedro Victor Barriga , Gonçalves Giovanna Dias , Nascimento Mauro Rodrigues , Dias George Alberto da Silva , Dias Biatriz Araújo Cardoso , ALVES R. C. 
Published: November 2024

A educação em saúde pode ser realizada de diversas formas e com o auxílio das tecnologias educacionais objetiva-se facilitar esse aprendizado. A Organização Mundial de Saúde (OMS), define a saúde como um estado de bem-estar geral físico, mental e social, sendo influenciado pelo ambiente em que o indivíduo está inserido. Nesse sentido, o conceito de Patrimônio Público está intimamente relacionado com o direito ao meio ambiente, impulsionando a ligação entre ambiente e saúde. Tendo isso em vista, os serviços de saúde podem ser caracterizados como patrimônio público, por esse motivo descuidar desse espaço pode afetar negativamente a qualidade de vida das pessoas que frequentam esses lugares. Esse estudo teve como objetivo construir uma tecnologia educacional sobre a preservação do patrimônio público nos serviços de saúde e sua relação com a saúde da população. Foi realizado em três etapas: diagnóstico situacional, revisão da literatura e construção da tecnologia educacional. Participaram do estudo 1 profissional e 4 acadêmicos da área da saúde.
A STUDY TO COMPARE THE EFFECTIVENESS OF SPINAL MOBILIZATION WITH ARM MOVEMENT VERSUS NEURAL TISSUE MOBILIZATION ALONG WITH MUSLE ENERGY TECHNIQUE AMONG CERVICAL RADICULOPATHY PATIENTS
Authors: S. Santhosh  , N. Priyanka  
Published: November 2024

Background: Cervical Radiculopathy is a disease of the cervical spine and a space occupying lesion that occurs because of pathological problems with cervical nerve roots. It usually causes the pain in the neck ,radiating to one arm with reduced motor function and reflex changes in the affected nerve root and commonly affect the middle aged to elderly person.
Objective: A study to compare the effectiveness of spinal mobilization with arm movement versus neural tissue mobilization along with muscle energy technique among cervical radiculopathy patients.
Method: Comparative study, 30 patients were selected from Sri Venkateshwara group of institution. They were allocated into two groups, group A(n=15) spinal mobilization with arm movement along with MET, group B (n= 15) neural tissue mobilization with MET given for 3 days per week for 6 weeks, the outcome measures NPRS and goniometric measurement were used.
Result: Data analysis was done by paired ‘t’ test for within the group and unpaired ‘t’ test for between the group analysis respectively. The statistical analysis shows that the group A had significant improvement than group B. It has been concluded that group A showed reduction in the pain and improvement in ROM than group B.
Conclusion: This study concludes that spinal mobilization with arm movement along with MET for group A shows more significant in reducing the pain and improve ROM among cervical radiculopathy patients than neural tissue mobilization with MET in group B.
Assessing the Association between the Globular Cluster NGC 4147 and the Sagittarius Dwarf Galaxy
Authors: Zhang Ying-Hua , Nie Jundan , Tian Hao , Liu Chao 
Published: November 2024

Abstract
The potential association of the globular cluster (GC) NGC 4147 with the Sagittarius (Sgr) dwarf spheroidal galaxy has been proposed due to their comparable locations and radial velocities. However, there are still debates about this connection. In this study, we use data from the Dark Energy Spectroscopic Instrument Legacy Imaging Surveys to assess their association. We redetermine the fundamental parameters of NGC 4147 and find that the cluster is 11.0 Gyr old, has a metallicity of Z = 0.0006, and is located 18.5 kpc from the Sun. We utilize the matched filter algorithm to identify extratidal structures in the surrounding sky of NGC 4147. The multiarmed tidal structures we find align more closely with the result of internal two-body relaxation processes within the cluster itself. The orientations of the dispersed tidal structures, the orbital direction of the cluster, and the mean orbital direction of Sgr do not show any apparent connection to each other. It seems to challenge the hypothesis of a common origin between the cluster and Sgr. To further investigate the association, we study the kinematics of NGC 4147 with the newly determined fundamental parameters. We find that the orbit, orbital energy, and angular momentum of NGC 4147 are not compatible with those of Sgr or its streams. This suggests that the cluster is not dynamically associated with Sgr. The morphology and dynamics of NGC 4147 are more consistent with it being a GC that formed with another origin rather than being accreted from the Sgr dwarf galaxy.
Image of the Kerr–Newman Black Hole Surrounded by a Thin Accretion Disk
Authors: Guo Sen , Huang Yu-Xiang , Liang En-Wei , Liang Yu , Jiang Qing-Quan , Lin Kai 
Published: November 2024

Abstract
The image of a Kerr–Newman (KN) black hole (BH) surrounded by a thin accretion disk is derived. By employing elliptic integrals and ray-tracing methods, we analyze photon trajectories around the KN BH. At low observation inclination angles, the secondary image of particles is embedded within the primary image. However, as the inclination increases, the primary and secondary images separate, forming a hat-like structure. The spin and charge of the BH, along with the observer’s inclination angle, affect the image’s asymmetry and the distortion of the inner shadow. To investigate the redshift distribution on the accretion disk, we extended the inner boundary of the accretion disk to the event horizon. The results show that the redshift distribution is significantly influenced by the observation inclination angle. Furthermore, we conducted a detailed analysis of the KN BH image using fisheye camera ray-tracing techniques and found that the optical appearance and intensity distribution of the BH vary at different observation frequencies (specifically at 230 GHz and 86 GHz). We also examined differences in intensity distribution for prograde and retrograde accretion disk scenarios. Comparing observational at the two frequencies, we found that both the total intensity and peak intensity at 86 GHz are higher than those at 230 GHz.
On the Formation Height of Low-corona and Chromospheric Channels of the Atmospheric Imaging Assembly (AIA) onboard the Solar Dynamics Observatory (SDO)
Authors: Sanjay Y. , Prasad S. Krishna , Erdélyi R. , Korsós M. B. , Banerjee D. , Rawat P. S. 
Published: November 2024

Abstract
The multiwavelength data from the Solar Dynamics Observatory is extensively used in studying the physics of the Sun and its atmosphere. In this study, we estimate the formation heights of low-corona and chromospheric channels of the Atmospheric Imaging Assembly (AIA) over the atmospheres of sunspot umbrae during the quiet condition period within 20 different active regions. The upward propagating slow magnetoacoustic waves of a 3 minute period, which are perpetually present in sunspots, are utilized for this purpose. Employing a cross-correlation technique, the most frequent time lag between different channel pairs is measured. By combining this information with the local sound speed obtained from the characteristic formation temperatures of individual channels, we estimate the respective formation heights. The median values of formation heights obtained across all active regions in our sample are 356, 368, 858, 1180, and 1470 km, respectively, for the AIA 1600, 1700, 304, 131, and 171 Å channels. The corresponding ranges in the formation heights are 247–453, 260–468, 575–1155, 709–1937, and 909–2585 km, respectively. These values are measured with respect to the Helioseismic Magnetic Imager continuum. We find the formation height of UV channels is quite stable (between 250 and 500 km) and displays only a marginal difference between the AIA 1600 and 1700 Å channels during quiet conditions. On the other hand, the formation height of coronal channels is quite variable.
Parametric Instability of Alfvén Waves and Wave Packets in Periodic and Open Systems
Authors: Marriott Maile , Tenerani Anna 
Published: November 2024

Abstract
The parametric decay instability of Alfvén waves has been widely studied, but few investigations have examined wave packets of finite size and the effect of different boundary conditions on the growth rate. In this paper, we perform a linear analysis of circular and arc-polarized wave trains and wave packets in periodic and open boundary systems in a low-β plasma. We find that both types of wave are 3–5 times more stable in open boundary conditions compared to periodic. Additionally, once the wave packet width ℓ becomes smaller than the system size L, the growth rate decreases nearly with a power law γ ∝ ℓ/L. This study demonstrates that the stability of a pump wave cannot be separated from the laboratory settings, and that the growth rate of daughter waves depends on the conditions downstream and upstream of the pump wave and on the fraction of volume it fills. Our results can explain simulations and experiments of localized Alfvén waves. They also suggest that Alfvénic fluctuations in the solar wind, including sharp impulses known as switchbacks, can be more stable than traditional theory suggests depending on wind conditions.
A Possible Explanation of W-type Phenomena in V694 Peg
Authors: Xu Hu-Shan , Zhu Li-Ying 
Published: November 2024

Abstract
Three sets of complete multicolor light curves of V694 Peg observed in 2013, 2015, and 2019 were presented and analyzed. Our photometric solutions show that this system was an A-type shallow contact binary in 2013 and 2015 while it converted to a W-type one in 2019. A large cool spot on the component of this binary could explain the conversion, implying the W-type phenomena may be caused by the magnetic activity of the components. We have collected available data on this binary and calculated 505 times of light minimum, which spans 17 yr. The orbital period investigation based on these timings shows there is a long-term period increase at a rate of dP/dt = 4.3(±0.3)×10−9 day yr−1 superposed on a periodic variation with a period of 11.81(±0.06) yr. The cyclic orbital variation may be the result of magnetic activity cycles or the existence of a third body. Until now, only eight transformed systems, including V694 Peg, have been reported. Compared with other converting contact systems between A-type and W-type, V694 Peg is recorded as the shortest-period one. All of these converting systems are late-type (later than F7) contact binaries with the O’Connell effect and show cyclic period variation, which indicates that magnetic activity may be the reason for the conversion between the two types of contact binaries. For investigating the nature of A-type and W-type phenomena, the discovery of more converting contact binaries is essential.
JWST/NIRSpec Observations of Lyman α Emission in Star-forming Galaxies at 6.5 ≲ z ≲ 13
Authors: Tang Mengtao , Stark Daniel P. , Topping Michael W. , Mason Charlotte , Ellis Richard S. 
Published: November 2024

Abstract
We present an analysis of JWST Lyα spectroscopy of z ≳ 6.5 galaxies, using observations in the public archive covering galaxies in four independent fields: Great Observatories Origins Deep Survey (GOODS)-N, GOODS-S, A2744, and the Extended Groth Strip (EGS). We measure the Lyα emission line properties for a sample of 210 z ≃ 6.5–13 galaxies, with redshifts confirmed independently of Lyα in all cases. We present three new detections of Lyα emission in JWST spectra, including a large equivalent width (EW; =143 Å) Lyα emitter (LAE) with strong C iv emission (EW = 21 Å) at z = 7.1 in GOODS-N. We measure the redshift-dependent Lyα EW distribution across our sample. We find that strong Lyα emission (EW > 25 Å) becomes increasingly rare at earlier epochs, suggesting that the transmission of Lyα photons decreases by 4× between z ≃ 5 and z ≃ 9. We describe potential implications for the intergalactic medium neutral fraction. There is significant field-to-field variance in the LAE fraction. In contrast to the three other fields, the EGS shows no evidence for reduced transmission of Lyα photons at z ≃ 7–8, suggesting a significantly ionized sight line may be present in the field. We use available NIRCam grism observations from the First Reionization Epoch Spectroscopically Complete Observations survey to characterize overdensities on large scales around known LAEs in the GOODS fields. The strongest overdensities appear linked with extremely strong Lyα detections (EW > 50 Å) in most cases. Future Lyα spectroscopy with JWST has the potential to constrain the size of ionized regions around early galaxy overdensities, providing a new probe of the reionization process.
An Intermediate-mass Black Hole Hidden behind Thick Obscuration
Authors: Boorman Peter G. , Stern Daniel , Assef Roberto J. , Borkar Abhijeet , Brightman Murray , Buchner Johannes , Chen Chien-Ting , Earnshaw Hannah P. , Harrison Fiona A. , Matzeu Gabriele A. , Pfeifle Ryan W. , Ricci Claudio , Svoboda Jiří , Torres-Albà Núria , Zaw Ingyin 
Published: November 2024

Abstract
Recent models suggest approximately half of all accreting supermassive black holes (SMBHs; M
BH ≳ 105
M
⊙) are expected to undergo intense growth phases behind Compton-thick (N
H > 1.5 × 1024 cm−2) veils of obscuring gas. However, despite being a viable source for the seeding of SMBHs, there are currently no examples known of a Compton-thick accreting intermediate-mass black hole (IMBH; M
BH ∼ 102–105
M
⊙). We present a detailed X-ray spectral analysis of IC 750—the only active galactic nuclei (AGN) to date with a precise megamaser-based intermediate mass <105
M
⊙. We find the equivalent width of neutral 6.4 keV Fe Kα to be

1.9

−
1.0

+
2.2

keV via phenomenological modeling of the coadded 177 ks Chandra spectrum. Such large equivalent widths are seldom produced by processes other than fluorescence from dense obscuration. We fit three physically motivated X-ray spectral models to infer a range of possible intrinsic 2–10 keV luminosity posteriors that encompass the systematic uncertainties associated with a choice of model. Despite a wide range of predicted intrinsic 2–10 keV luminosities between ∼ 1041 and 1043 erg s−1, all three models agree that IC 750 has a Compton-thick line-of-sight column density to >99% confidence. Compton-thick obscuration is well-documented to impinge substantial bias on the pursuit of SMBH AGN. Our results thus provide the first indication that Compton-thick obscuration should also be properly considered to uncover and understand the IMBH population in an unbiased manner.
An Efficient Method for Batch Derivation of Detached Eclipsing Binary Parameters: Analysis of 34,907 OGLE Systems
Authors: Wang JinLiang , Ding Xu , Liu Wei , Yu LiHuan , Xu Chong , Ji KaiFan 
Published: November 2024

Abstract
Detached eclipsing binary (EB) systems are crucial for measuring the physical properties of stars that evolve independently. Large-scale time-domain surveys have released a substantial number of light curves for detached EBs. Utilizing the Physics of Eclipsing Binaries package in conjunction with Markov Chain Monte Carlo (MCMC) methods for batch parameter derivation poses significant computational challenges, primarily due to the high computational cost and time demands. Therefore, this paper develops an efficient method based on the neural network model and the stochastic variational inference method (denoted NNSVI) for the rapid derivation of parameters for detached EBs. For studies involving more than three systems, the NNSVI method significantly outperforms techniques that combine MCMC methods in terms of parameter inference speed, making it highly suitable for the batch derivation of large numbers of light curves. We efficiently derived parameters for 34,907 detached EBs, selected from the Optical Gravitational Lensing Experiment catalog and located in the Galactic bulge, using the NNSVI method. A catalog detailing the parameters of these systems is provided. Additionally, we compared the parameters of two double-lined detached EBs with those from previous studies and found the estimated parameters to be essentially identical.