bluuebunny/crossref_metadata_2025_split huggingface dataset:
UPAYA PENINGKATAN AKTIVITAS DAN HASIL BELAJAR MATERI SENAM LANTAI GERAKAN ROLL DEPAN MELALUI PENGGUNAAN METODE LATIHAN CIRCUIT TRAINING DALAM PEMBELAJARAN PENJAS PADA SISWA SMA
Authors: Kosta Vinsensa Lisa , Bayo Ola Tapo Yohanes , Natal Yanuarius Ricardus 
Published: April 2023

ABSTRAK

Upaya Peningkatan Aktivitas dan Hasil Belajar Materi Senam Lantai Gerakan Roll Depan Melalui Penggunaan Metode Latihan Circuit Training dalam Pembelajaran Penjas pada Siswa Kelas XI SMAN I Soa.
Lisa Vinsensa Kosta ,Yohanes Bayo Ola Tapo, Yanuarius Ricardus Natal.

Penelitian ini bertujuan untuk mengetahui peningkatan aktivitas dan hasil belajar siswa pada materi senam lantai dalam pembelajaran penjas melalui penerapan model latihan sircuit trainingpada siswa kelas XI SMAN I SOA. Jenis penelitian ini adalah PTK (Penelitian Tindakan Kelas) dan subyek penelitian ini adalah siswa kelas XI SMA Negeri 1 Soa Tahun Ajaran 2020/2011 yang berjumlah 27 orang, yang terdiri dari 15 siswa dan 13 siswi. Penelitian tindakan kelas ini dilaksanakan dalam 2 siklus, dengan empat tahapan yaitu : perencanaan, pelaksanaan, observasi, dan refleksi. Data tentang aktivitas belajar siswa dikumpulkan dengan melakukan observasi dan data tentang hasil belajar siswa dikumpulkan dengan teknik tes. Instrumen pengumpulan data aktivitas belajar menggunakan lembar observasi sedangkan hasil belajar menggunakan tes objektif. Data yang diperoleh dalam penelitian dianalisis dengan menggunakan metode analisis data deskriptif kuantitatif. Hasil penelitian meujukkan bahwa:1) Aktivitas belajar senam lantai gerak roll depan meningkat melalui metode latihan circuit training. Hal ini dapat dilihat dari rata-rata aktivitas belajar siswa dari observasi awal hingga pada pelaksanaan siklus I mengalami peningkatan sebesar 0,9 yaitu dari 36,6 (kategori cukup aktif) menjadi 37,5 (kategori cukup aktif).Rata-rata aktivitas belajar siswa dari siklus I kesiklus II mengalami peningkatan sebesar 8,7 yakni dari 37,5 (kategori cukup aktif) menjadi 46,2 (kategori aktif). Rata-rata aktivitas belajar siswa dari observasi awal hingga siklus II mengalami peningkatan sebesar 9,6 yakni dari 36,6 (kategori cukup aktif) menjadi 46,2 (kategoriaktif).2) Hasil belajar senam lantai gerak roll depan meningkat melalui metode latihan circuit training.Hal ini terlihat dari rata-rata hasil belajar siswa dari observasi awal ke siklus I mengalami peningkatan sebesar 3,6 yakni dari 64,9 (kategori cukup) menjadi 68,5 (kategori baik). Rata-rata hasil belajar siswa dari siklus I ke siklus II mengalami peningkatan sebesar 6,5 yakni dari 68,5 (kategoribaik) menjadi 75,0 (kategori sangat baik). Rata-rata hasil belajar siswa dari observasi awal ke siklus II mengalami peningkatan sebesar 10,2 yakni dari 64,9 (kategori cukup) menjadi 75,0 (kategori sangat baik). Dengan demikian dapat disimpulkan bahwa penerapan metode latihan circuit training dapat menignkatkan aktivitas dan hasil belajar materi senam lantai gerakan roll depan pada siswa kelas XI SMA Negeri 1 Soa.
Lomber Disk Hernisi Ameliyatı Geçiren Hastaların Sağlık Okuryazarlık Düzeyinin Taburcu Olmaya Hazır Olma Durumuna Etkisi
Authors: ÖZTÜRK Keziban , DURMAZ Melike , KURŞUN Şerife 
Published: April 2023

Amaç: Bu araştırma, lomber disk hernisi (LDH) ameliyatı geçiren hastaların sağlık okuryazarlık düzeyinin taburcu olmaya hazır olma durumuna etkisinin belirlenmesi amacıyla yapıldı.
Yöntem: Bu araştırma tanımlayıcı-ilişki arayıcı bir araştırmadır. Araştırma evrenini, bir üniversite hastanesinin beyin cerrahi servisinde planlı LDH ameliyatı yapılan hastalar oluşturdu. Örneklem büyüklüğünü 120 hasta oluşturdu. Veriler, tanıtıcı bilgi formu, Sağlık Okuryazarlığı Ölçeği ve Taburcu Olmaya Hazır Olma Ölçeği-Kısa Formu ile toplandı. Verilerin analizinde, sayı, yüzde dağılımı, Mann Whitney U testi, Kruskall Wallis testi ve Spearman korelasyon analizi kullanıldı.
Bulgular: Katılımcıların Sağlık Okuryazarlık Ölçeği toplam puanı 94.60±15.22 olup sağlık okuryazarlık düzeylerinin ortanın üstünde olduğu bulundu. Taburcu Olmaya Hazır Olma Ölçeği puanlarına göre katılımcıların, %57.5 (n=69)’inin taburculuğa hazır olmadıkları belirlendi. Hastaların tanıtıcı özelliklerinden sadece hastanede kalış süresine göre Taburcu Olmaya Hazır Olma Ölçeği puan ortalamalarının farklı olduğu belirlendi (p
Özel Durumlarda Yardımcı Üreme Tekniklerinin Kullanımı
Authors: ASLAN DEMİRTAŞ Fatma , ASLAN Ergül 
Published: April 2023

Amaç: Yardımcı üreme teknikleri (YÜT) infertil bireylerin çocuk sahibi olmalarına yardımcı olan ileri düzey teknik uygulamalardır. Cinsel yolla bulaşıcı enfeksiyonlar (CYBE), İnsan İmmün Yetmezlik Virüsü pozitif (HIV+) olanlar, onkolojik hastalık ve engellilik gibi özel durumu olan infertil bireyler ebeveyn olmak isteyebilmektedir. Buna bağlı olarak bu makalede CYBE olanlar, HIV olanlar, onkolojik tedavi hastaları ve engelli bireyler infertilitede özel gruplar olarak ele alınmıştır.
Yöntem: Derleme türündeki bu makalede anahtar kelime olarak “CYBE”, “HIV+”, “engellilik”, “kanser”, “infertilite ve “yardımcı üreme teknikleri” kullanılarak Google Scholar, Pubmed, Science Direct ve Ulakbim veri tabanları taranmıştır. Ocak 2013-Şubat 2022 tarihleri arasında ulusal ve uluslararası dergilerde yayınlanmış çalışmalar değerlendirilmiştir.
Bulgular: Literatür incelemesi sonucunda, CYBE’nin eşe veya fetüse geçişini önlemek, kanser hastalarının doğurganlığını korumak ve engeli olan bireylerin gebeliğini engel olacak sorunları önlemek amacı ile YÜT’ten yararlandığı belirlenmiştir. Ayrıca bu bireylerin ebeveyn olma isteklerine aile, çevre ve sağlık personelleri tarafından ön yargılı yaklaşıldığı veya göz ardı edildiği saptanmıştır.
Sonuç: Araştırmalar sonucunda bireylerin bulunduğu özel duruma ve sağlık durumuna göre uygun kullanılabilecek YTÜ bulunmaktadır. Buna bağlı olarak sağlık profesyonelleri özel durumları göz önünde bulundurarak YÜT hakkında kapsamlı danışmanlık yapmalı, soru sormaya cesaretlendirmeli ve ruhsal destek sağlamalıdır.
Immigrant Families in the Neonatal Intensive Care Unit: Barriers in Nursing Care
Authors: ÇETİNKAYA Bengü , CEYLAN Sibel Serap 
Published: April 2023

Objective: The number of immigrants in the world is increasing rapidly. The vast majority of female immigrants are of reproductive age. Immigrant infants are added to the population every day. The purpose of this study is to determine challenges for neonatal intensive care unit nurses who care for infants of immigrant families.
Methods: A qualitative phenomenological research design based on a semi-structured in-depth interview with 11 neonatal intensive care nurses. The interviews were recorded and transcribed for content analysis and responses were categorized into themes.
Results: The two major themes identified from the data were: (1) language-related barriers and (2) culture-related barriers.
Conclusion: Neonatal intensive care nurses who care for infants of immigrant families have communication problems as a result of the lack of interpreters and because of challenges cultural differences. This has the potential to affect the well-being. Study results can be used by nurses to improve the quality of care of immigrant infants and their families.
Calibrating X-Ray Binary Luminosity Functions via Optical Reconnaissance. II. The High-mass XLF and Globular Cluster Population of X-Ray Binaries in the Low Star-forming Spiral M81
Authors: Hunt Qiana , Gallo Elena , Chandar Rupali , Mok Angus , Prestwich Andrea 
Published: April 2023

Abstract
We characterize the optical counterparts to the compact X-ray source population within the nearby spiral galaxy M81 using multiband Hubble Space Telescope (HST) imaging data. By comparing the optical luminosities and colors measured for candidate donor stars and host clusters to stellar and cluster evolutionary models, respectively, we estimate the likely masses and upper age limits of the field and cluster X-ray binaries. We identify 15 low-mass X-ray binaries (i.e., donor star mass ≲ 3 M
⊙) within ancient globular clusters, as well as 42 candidate high-mass X-ray binaries (i.e., donor star mass ≳ 8 M
⊙). To estimate the likelihood of misclassifications, we inject 4000 artificial sources into the HST mosaic image and conclude that our classifications of globular clusters and high-mass X-ray binaries are reliable at the >90% level. We find that globular clusters that host X-ray binaries are on average more massive and more compact than globular clusters that do not. However, there is no apparent correlation between the X-ray brightness of the clusters and their masses or densities, nor are X-ray binary hosts more X-ray luminous than the general field population of low-mass X-ray binaries. This work represents one of the first in-depth analyses of the population of X-ray binaries within globular clusters in a spiral galaxy.
The Evolution of Protostellar Outflow Cavities, Kinematics, and Angular Distribution of Momentum and Energy in Orion A: Evidence for Dynamical Cores
Authors: Hsieh 謝 Cheng-Han 承翰 , Arce Héctor G. , Li Zhi-Yun , Dunham Michael , Offner Stella , Stephens Ian W. , Stutz Amelia , Megeath Tom , Kong Shuo , Plunkett Adele , Tobin John J. , Zhang Yichen , Mardones Diego , Pineda Jaime E. , Stanke Thomas , Carpenter John 
Published: April 2023

Abstract
We present Atacama Large Millimeter/submillimeter Array observations of the ∼10,000 au environment surrounding 21 protostars in the Orion A molecular cloud tracing outflows. Our sample is composed of Class 0 to flat-spectrum protostars, spanning the full ∼1 Myr lifetime. We derive the angular distribution of outflow momentum and energy profiles and obtain the first two-dimensional instantaneous mass, momentum, and energy ejection rate maps using our new approach: the pixel flux-tracing technique. Our results indicate that by the end of the protostellar phase, outflows will remove ∼2–4 M
⊙ from the surrounding ∼1 M
⊙ low-mass core. These high values indicate that outflows remove a significant amount of gas from their parent cores and continuous core accretion from larger scales is needed to replenish core material for star formation. This poses serious challenges to the concept of cores as well-defined mass reservoirs, and hence to the simplified core-to-star conversion prescriptions. Furthermore, we show that cavity opening angles, and momentum and energy distributions all increase with protostar evolutionary stage. This is clear evidence that even garden-variety protostellar outflows: (a) effectively inject energy and momentum into their environments on 10,000 au scales, and (b) significantly disrupt their natal cores, ejecting a large fraction of the mass that would have otherwise fed the nascent star. Our results support the conclusion that protostellar outflows have a direct impact on how stars get their mass, and that the natal sites of individual low-mass star formation are far more dynamic than commonly accepted theoretical paradigms.
Search for X-Ray Quasiperiodicity of Six AGNs Using the Gaussian Process Method
Authors: Zhang Haoyang , Yang Shenbang , Dai Benzhong 
Published: April 2023

Abstract
The quasiperiodic oscillations (QPOs) found in active galactic nuclei (AGNs) are a very interesting observational phenomenon implying an unknown physical mechanism around supermassive black holes. Several AGNs have been found to have QPO phenomena in the X-ray energy band. Long-duration X-ray observations were collected and reduced for six AGNs with a suspected QPO. The Gaussian process model celerite was used to fit the light curves and to search for the quasiperiodicity behavior. The power spectral density and parameter posterior distributions of each light curve were calculated with the optimal model. Of the six AGNs, only RE J1034+396 was found to have a QPO of about 3600 s. The other five sources do not show QPO modulation behavior. We propose that a hot spot on the accretion disk is a possible physical mechanism resulting in this quasiperiodic behavior of AGNs.
Detection of a Supervirial Hot Component in the Milky Way Circumgalactic Medium Along Multiple Sight Lines by Using the Stacking Technique
Authors: Lara-DI Armando , Mathur Smita , Krongold Yair , Das Sanskriti , Gupta Anjali 
Published: April 2023

Abstract
The study of the elusive hot component (T ≳ 107 K) of the Milky Way circumgalactic medium (CGM) is a novel topic for understanding Galactic formation and evolution. In this work, we use the stacking technique through 46 lines of sight with Chandra ACIS-S HETG totaling over 10 Ms of exposure time and nine lines of sight with ACIS-S LETG observations totaling over 1 Ms of exposure time, to study in absorption the presence of highly ionized metals arising from the supervirial temperature phase of the CGM. Focusing in the spectral range 4–8 Å, we were able to confirm the presence of this hot phase with high significance. We detected transitions of Si XIV K
α (with a total significance of 6.0σ) and, for the first time, S XVI K
α (total significance of 4.8σ) in the rest frame of our own galaxy. For S XVI K
α we found a column density of

1.50

−
0.38

+
0.44

×

10

16

cm

−
2

. For Si XIV K
α we measured a column density of 0.87 ± 0.16 × 1016 cm−2. The lines of sight used in this work are spread across the sky, probing widely separated regions of the CGM. Therefore, our results indicate that this newly discovered hot medium extends throughout the halo and is not related only to the Galactic bubbles. The hot gas location, distribution, and covering factor, however, remain unknown. This component might contribute significantly to the missing baryons and metals in the Milky Way.
Recovering Cosmic Microwave Background Polarization Signals with Machine Learning
Authors: Yan Ye-Peng , Wang Guo-Jian , Li Si-Yu , Xia Jun-Qing 
Published: April 2023

Abstract
Primordial B-mode detection is one of the main goals of current and future cosmic microwave background (CMB) experiments. However, the weak B-mode signal is overshadowed by several Galactic polarized emissions, such as thermal dust emission and synchrotron radiation. Subtracting foreground components from CMB observations is one of the key challenges in searching for the primordial B-mode signal. Here, we construct a deep convolutional neural network (CNN) model, called CMBFSCNN (Cosmic Microwave Background Foreground Subtraction with CNN), which can cleanly remove various foreground components from simulated CMB observational maps at the sensitivity of the CMB-S4 experiment. Noisy CMB Q (or U) maps are recovered with a mean absolute difference of 0.018 ± 0.023 μK (or 0.021 ± 0.028 μK). To remove the residual instrumental noise from the foreground-cleaned map, inspired by the needlet internal linear combination method, we divide the whole data set into two “half-split maps,” which share the same sky signal, but have uncorrelated noise, and perform a cross-correlation technique to reduce the instrumental noise effects at the power spectrum level. We find that the CMB EE and BB power spectra can be precisely recovered with significantly reduced noise effects. Finally, we apply this pipeline to current Planck observations. As expected, various foregrounds are cleanly removed from the Planck observational maps, with the recovered EE and BB power spectra being in good agreement with the official Planck results.
Global Dynamic Scaling Relations of H i-rich Ultra-diffuse Galaxies
Authors: Hu 胡 Hui-Jie 慧杰 , Guo 郭 Qi 琦 , Zheng 郑 Zheng 征 , Yang 杨 Hang 航 , Tsai 蔡 Chao-Wei 肇伟 , Zhang 张 Hong-Xin 红欣 , Zhang 张 Zhi-Yu 智昱 
Published: April 2023

Abstract
The baryonic Tully–Fisher relation (BTFR), which connects the baryonic mass of galaxies with their circular velocities, has been validated across a wide range of galaxies, from dwarf galaxies to massive galaxies. Recent studies have found that several ultra-diffuse galaxies (UDGs) deviate significantly from the BTFR, indicating a galaxy population with abnormal dynamical properties. However, such studies were still confined within a small sample size. In this study, we used the 100% complete Arecibo Legacy Fast Arecibo L-band Feed Array (ALFALFA) to investigate the BTFR of 88 H i-rich UDGs (HUDGs), which is the largest UDG sample with dynamical information. We found that the HUDGs form a continuous distribution in the BTFR diagram, with high-velocity galaxies consistent with normal dwarf galaxies at a 1σ level, and low-velocity galaxies deviating from the BTFR, in line with that reported in the literature. We point out that the observed deviation may be subject to various selection effects or systemic biases. Nevertheless, we found that the significance of the deviation of HUDGs from the BTFR and TFR are different, i.e., they either deviate from the BTFR or from the TFR. Our result indicates that a high gas fraction may play an important role in explaining the deviation of HUDGs from BTFR.
Résonances sensorielles en thérapie familiale psychanalytique
Authors: Lebon Cristelle 
Published: April 2023

L’auteure propose une écoute des formes sensorielles et climatiques en thérapie familiale psychanalytique. Elle dégage les logiques archaïques d’un processus de symbolisation primaire à l’œuvre en séance, et en présente deux formes particulières : le souvenir hybride et la rupture climatique dans le transfert. Elle développe une approche des organisateurs psychiques inconscients du néo-groupe permettant d’en repérer certains de registre archaïque, comme les signifiants formels. L’article se conclut sur le rôle des résonances sensorielles en tfp et leurs spécificités par rapport aux résonances fantasmatiques.
Attachement, narrativité et psychanalyse familiale. Esquisse d’un maillage conceptuel
Authors: Boudarse Khalid 
Published: April 2023

Considérant l’étude de la narrativité comme un champ commun à la psychanalyse et à la théorie de l’attachement, nous envisageons dans cet article théorique des maillages entre les deux corpus afin de les mettre au service de la consultation familiale psychanalytique. Après avoir traité de l’identité narrative selon Paul Ricœur et des tensions entre vérité historique et récit à la fois en philosophie de l’histoire et dans les travaux sur l’attachement, nous décrirons trois nœuds du maillage conceptuel : l’exploration de la trame psychique familiale, le mirroring groupal et le sentiment de sécurité familial. Nous traiterons enfin la médiation thérapeutique, qui est particulièrement conseillée, comme un lieu privilégié pour l’étude et l’appréhension du rapport de ces trois nœuds à la créativité familiale.
Le renoncement à la parentalité chez un couple : « ils se marièrent et n’eurent pas d’enfant »
Authors: Mazoyer Anne-Valérie , Bourdet-Loubère Sylvie 
Published: April 2023

L’article interroge les situations, de plus en plus fréquemment rencontrées dans la clinique actuelle, des hommes ou des femmes présentant un refus conscient d’enfant. L’exploration de l’élaboration de la position en « contre » vis-à-vis de la reproduction et, au-delà, de la parentalité chez un couple montre les aléas et avatars du désir d’enfant infantile et de l’histoire subjective et conjugale. Ce renoncement dit volontaire à la parentalité questionne les liens d’alliance, le choix d’objet originel et peut être éclairé par des blessures liées à la filiation. Ce travail illustre par ailleurs les effets d’un espace de mise en narration (même dans un contexte de recherche) sur la relance des processus psychiques et les remaniements (positionnements identificatoires) qui peuvent en découler.
How the Unfolded Protein Response Is a Boon for Tumors and a Bane for the Immune System
Authors: Raines Lydia N , Huang Stanley Ching-Cheng 
Published: April 2023

Abstract
The correct folding of proteins is essential for appropriate cell function and is tightly regulated within the endoplasmic reticulum (ER). Environmental challenges and cellular conditions disrupt ER homeostasis and induce ER stress, which adversely affect protein folding and activate the unfolded protein response (UPR). It is now becoming recognized that cancer cells can overcome survival challenges posed within the tumor microenvironment by activating the UPR. Furthermore, the UPR has also been found to impose detrimental effects on immune cells by inducing immunoinhibitory activity in both tumor-infiltrating innate and adaptive immune cells. This suggests that these signaling axes may be important therapeutic targets, resulting in multifaceted approaches to eradicating tumor cells. In this mini-review, we discuss the role of the UPR in driving tumor progression and modulating the immune system’s ability to target cancer cells. Additionally, we highlight some of the key unanswered questions that may steer future UPR research.
Comparative efficacy of high-frequency repetitive transcranial magnetic stimulation to left dorsolateral prefrontal cortex as an augmentation strategy versus pharmacological augmentation in non-psychotic, unipolar, treatment-resistant depression: A randomized controlled trial
Authors: Chail Amit , Bhat Pookala S. , Singh Harpreet , Saini Rajiv Kumar 
Published: April 2023

ABSTRACT

Background:
Depression causes significant morbidity, disability and mortality, along with socioeconomic losses. Patients with depression who don’t remit even with the second trial of anti-depressants need optimization, combination or augmentation strategies. Pharmacological strategies sometimes have unacceptable adverse effects.

Aim:
The aim of this study is to compare the efficacy of high-frequency repetitive transcranial magnetic stimulation (HF-rTMS) to left dorsolateral prefrontal cortex (DLPFC) with that of pharmacological augmentation strategies in unipolar non-psychotic treatment-resistant depression.

Method:
This is a randomized controlled trial.

Subjects:
Cases of unipolar, non-psychotic, treatment-resistant depression between ages 20 and 60 years were taken.

Period of Study:
The study period was from November 2016 to May 2018.

Randomization:
Cases diagnosed as per ICD-10 criteria by a qualified psychiatrist. Cases of treatment-resistant depression (100) were divided into two arms by using a random number generator: rTMS arm and treatment as usual (TAU) arm.

Intervention:
HF-rTMS to left DLPFC (rTMS group) and pharmacological augmentation with lithium, serotonin-dopamine antagonist, buspirone or thyroxine.

Results:
In the rTMS arm, 44 patients and in TAU arm 41 completed the study. After 4 weeks of treatment augmentation, rTMS and TAU groups showed response rates of 52% and 46%, respectively. The difference between the two groups in terms of number of responders at the end of 4 weeks is not statistically significant. Additionally, factors associated with good response to rTMS were absence of a family history of psychiatric illness, no concomitant psychoactive substance use, being first episode of depression and mild–moderate severity of illness.

Conclusion:
The study did not find rTMS augmentation to be significantly better than standard pharmacological augmentation therapies.