bluuebunny/crossref_metadata_2025_split huggingface dataset:
Rancang Bangun Game 2D “Finding Tajwid” Dengan Metode Finite State Mechine Menggunakan Software Unity Hub
Authors: Anggraini Asfilia Nova , Fadila Juniardi Nur , Nugroho Fressy 
Published: January 2022

Abstract - It is undeniable that along with the development of gaming technology that has become a means of entertainment has also developed into a means of education. One of the forms is as a teaching material in tajwid. Tajwid that many kinds make children sometimes feel difficult in the learning process. Based on the above problems, the author uses technology to construct schooling content that can boost children's learning enthusiasm, namely 2D games. 2D games are designed as attractively as possible by using Unity Hub software that utilizes the Finite State Mechine method. The purpose of making this 2D game is to increase children's learning interest in getting to know tajwid and help to remember what hijaiyah letters are contained in each law.Keywords - 2D Games, Unity Hub, Tajwid, Finite State Mechine. Abstrak – Tidak dapat dipungkiri seiring perkembangan teknologi game yang telah menjadi sarana hiburan turut berkembang menjadi sarana pendidikan. Salah satu bentuknya adalah sebagai bahan ajar dalam tajwid. Tajwid yang banyak macamnya membuat anak-anak kadang merasa kesulitan dalam proses belajar. Penelitian ini bertujuan untuk merancang sebuah game yang digunakan untuk membantu dalam proses pembelajaran ilmu tajwid dengan menggunakan metode Finite State Mechine. Finite State Mechine merupakan metode yang mengimplementasikan keadaan, kejadian dan aksi yang akan lebih menarik dalam proses pembelajaran dengan bermain. Sehingga hasilnya adalah anak-anak akan lebih mudah untuk mengenal dan mempelajari hukum tajwid yang ada dalam Al-Quran. Kesimpulan yang dapat diambil dari rancang bangun game ini adalah anak-anak dapat belajar dimana saja dan kapan saja ilmu tajwid dengan metode ang lebih menarik dan mudah untuk dihafalkan. Kata Kunci - Game 2D, Unity Hub, Tajwid, Finite State Mechine.
Kajian Literatur Tentang Reduksi Kromium dalam Air Limbah Penyamakan Kulit dengan Fitoremediasi
Authors: Astuti Dwi , Sukmawati Nurul , Asyfiradayati Rezania , Darnoto Sri 
Published: January 2022

Industri penyamakan kulit merupakan penyumbang polutan krom (Cr) pada limbahnya. Fitoremediasi memanfaatkan tanaman eceng gondok pada penurunan krom dalam limbah industri. Tujuan penelitian ini yaitu untuk mengetahui penerapan fitorremediasi dalam menurunkan kandungan krom pada limbah industri penyamakan kulit. Metode penelitian menggunakan desain penelitian kajian literatur yang menggunakan database Google Scholar, SINTA, Science Direct. Penelusuran literatur dimulai pada tahun terbit 2011 sampai tahun 2021 untuk dilakukan analisis. Kata kunci yang digunakan dalam penelusuran artikel menggunakan bahasa Indonesia dan bahasa Inggris yaitu penurunan Cr, air limbah industri penyamakan kulit, efisiensi eceng gondok, fitoremediasi pada industri penyamakan kulit. Kriteria inklusi tujuan penelitian dalam artikel yaitu penurunan logam berat kromium pada limbah industri penyamakan kulit menggunakan fitoremediasi, dapat diakses secara full text, metode kuantitatif eksperimen, jurnal yang diterbitkan ber-ISSN dan SINTA 1 – 6. Berdasarkan penelusuran diperoleh semua jurnal berhasil menurunkan kromium dalam air limbah dalam durasi lama waktu kontak 7 hari, 14, hari, 21 hari, 10 hari, 20 hari, 25 hari, 15 hari, 42 hari. Hasil penurunan dikatakan efektif jika berhasil menurunkan kandungan Cr hingga sesuai standar baku mutu yaitu pada lama waktu kontak 10 hari, 20 hari dan 28 hari. Metode fitoremediasi memiliki beragam kemudahan karena memanfaatkan tumbuhan air yang mudah diberdayakan. Oleh karena itu, pemanfaatan metode fitoremediasi ini diperlukan pengawasan terhadap pertumbuhan tanaman eceng gondok agar dapat bekerja optimal menurunkan kandungan logam krom dalam air limbah.
The Problem of International Private Law in the Pursuit of Cultural Relics Overseas
Authors: Li Yuxi , Yi Yuan 
Published: January 2022

With the rapid development of the economy, people’s awareness of the protection of cultural relics gradually increased. As a result, the issue of recursive overseas cultural relics is worthy of our attention. The urgency of recapturing overseas cultural relics has been greatly increased in order to avert the onset of a new era of cultural relics crisis. Faced with the difficulties of recourse, a low success rate, complicated recourse processes, and an immature international situation, what type of effort should we make? The overseas loss of cultural relics as the subject of study, a brief analysis of its research value, and the state of our recourse process, in the process of the challenges faced, and put forward the appropriate measures to address the situation are all covered in this paper. Furthermore, the subject of international private law is discussed.
Methods and Paths of Ideological and Political Education for College Students in The Hotan Teachers’ College during the Pandemic Period: Based on the Perspective of “Sanjin Lianglian Yijiaoyou”
Authors: Yan Zhenzhen 
Published: January 2022

How to perform a good job in ideological and political education for students during the pandemic time is a serious concern at colleges and universities, impacted by the pandemic condition of new Coronavirus disease. This paper analyses how to perform the ideological and political education well for college students under the pandemic condition and strengthen the sense of responsibility and mission of college students based on the activities of “Sanjin Lianglian Yijiaoyou” in colleges and universities.
The Effect of Functional Strength Training Using Relative Weights on Some Special Physical Abilities and Achieving 400m running for Men
Authors: Mohamed Ahmed Fadel , Al-Shamaa Haider Faeq 
Published: January 2022

The research aimed at designing functional strength training using relative weights that develop special abilities and 400m running achievement for men. The researchers used the experimental method on (8) elite 400m runners (over 20 years) divided equally into two groups; experimental and control to conclude that there is a significant development in the level of special abilities for 400m running due to functional strength training with weights. The researchers recommended using this training for developing muscular strength in all sport activities in general and in 400m running in particular. They also recommended making similar studies using a relative weight that are adjustable.
Farklı inseminasyon teknikleri ile elde edilmiş insan embriyolarının erken fertilizasyon ve klivaj dinamikleri yönünden morfokinetik analizi: Prospektif kardeş oosit çalışması
Authors: KARLİKAYA Güvenç , FINDIKLI Necati , AKSOY Turan , OLCAY Orçun , TEKE Bilgen , BOYNUKALIN Kübra , KARAKIŞ Lale Susan , BAHCECİ Mustafa 
Published: January 2022

Amaç: Bu çalışmada kendi gamet hücreleri kullanılarak Yardımcı Üreme Teknikleri (YÜT) tedavisi gören çiftlerde, inseminasyon için kullanılan In Vitro Fertilizasyon (IVF) veya Intra- Sitoplazmik Sperm Enjeksiyonu (ICSI) yönteminin embriyo morfokinetik gelişim zamanlarında bir değişiklik yapıp yapmadığının araştırılması amaçlanmıştır.
Gereçler ve Yöntem: Çalışma Nisan 2014 – Ekim 2015 tarihleri arasında Bahçeci Fulya IVF Merkezinde gerçekleştirildi. Çalışmada, YÜT uygulanan 37 siklus dahil edildi. Her bir siklusta alınan oositler IVF ve ICSI adı ile rastgele ve mümkün olduğu ölçüde eşit sayıda iki gruba ayrıldı ve adı geçen yöntemle eş zamanlı olarak insemine edildi. Fertilizasyon kontrolü sonrasında oluşan tüm embriyolar time lapse inkübatör içinde inkübe edilerek, embriyo dondurma veya transfer aşamasına kadar olan süreçte morfokinetik kontrol noktalarına göre skorlandı.
Bulgular: Dinamik embriyo gelişim parametreleri karşılaştırıldığında, takip başlangıç kriteri olarak inseminasyon zamanı alındığında, çalışmanın her iki kolunda olan embriyolar benzer klivaj dinamikleri ve kalite oranları gösterdiler. Pronukleus silinme zamanı takip başlangıç kriteri olarak alındığında ise, çalışma grupları arasında ekspanse blastokist aşamasına ulaşım süresi IVF ile insemine edilen embriyolar lehine anlamlı farklılık gösterdi (p
How specific are CA-125 levels in ruling out extra-uterine extension of endometrial serous papillary cancer?
Authors: KELES Esra , AKIŞ Serkan , ÖZYÜREK Şefik , ÖZTÜRK Uğur Kemal , PURUT Yunus Emre , KABACA Canan , APİ Murat 
Published: January 2022

Abstract
Aim: To investigate the CA-125 levels in uterine serous carcinoma (UPSC) patients to predict the extent of disease.
Materials and Method: Medical records of patients operated for UPSC/mix serous carcinoma, endometrioid carcinoma; their preoperative CA-125 levels, as well as parameters including age, tumor size, lymph node involvement, lymphovascular space invasion (LVSI), depth of myometrial invasion (MI) and stage were documented.
Results: Twenty-six UPSC/mix serous carcinoma cases and forty-five endometrioid carcinoma cases were included. When we analyzed the serous cancer group in terms of CA-125; there was no association between CA-125 and age (≤60 vs >60), tumor size (≤40 vs >40mm), MI, lymph node metastasis or LVSI. The mean CA-125 levels were signiﬁcantly higher among patients with stage III/IV (median=54 U/ml), compared to stage I/II (median=11 U/mL). The mean CA-125 value for tumors spread beyond the uterus were 281.2 U/ml, and 14.3 U/ml for the tumors confined within the uterus (p=0.002). The optimum threshold value to predict extrauterine spread was 28.5 U/mL. CA-125 level was related to extrauterine involvement and advanced stage.
Conclusion: CA-125 level is a useful test for extrauterine involvement and advanced stage. We suggest a less aggressive treatment modality with CA-125
Postmenopozal hastalarda endometrial örnekleme sonuçlarının değerlendirilmesi; yetersiz endometrial örneklemenin önemi
Authors: ATAK Zeliha , RAHIMLI OCAKOGLU Sakine , TURHAN Ezgi Işıl 
Published: January 2022

Amaç
Postmenopozal hasta populasyonunda endometrial örnekleme sonuçlarının değerlendirilmesi ve yetersiz endometrial örnekleme sıklığının belirlenmesi amaçlanmıştır.
Gereç ve Yöntem Bu retrospektif çalışmada Bursa Şehir Hastanesi kadın hastalıkları ve doğum bölümüne Temmuz 2019 ve Mart 2021 tarihleri arasında başvuran postmenopozal dönemdeki 825 hastadan alınan endometrial biyopsi sonuçları değerlendirilmiştir.
Bulgular Postmenopozal dönemde olan 825 hastadan alınan 922 endometrial örnekleme sonucu değerlendirildi. Hastaların yaş ortalaması 56.96±7.21 olup, ortalama menopoz süresi 7.43±7.14 yıldır. Hastalardan alınan 1. endometrial örneklemenin histopatolojik değerlendirmesi yapıldığında 25.45 % yetersiz endometrial örneklemeye rastlanırken postmenopozal kanama şikayeti ile başvuran hasta grubunda ise bu oran %21.61 dir. En sık endometrial patoloji endometrial polip (22.1%) olup çalışma grubumuzda malignite sıklığı %6.18 idi. Alt grup analizlerde malignite görülme sıklığı >60 yaş grubunda daha yüksek (%18.80) iken yaş ile birlikte yetersiz endometrial örneklemenin de arttığı belirlenmiştir. Birinci endometrial örnekleme sonucu yetersiz olan hastaların sadece %20 sinden tekrar biyopsi alınabilmiştir. Bu hastalardan 3 ünde endometrium kanseri ve 1 hastada atipili endometrial hiperplazi varlığı tespit edilmiştir.
Sonuç
Artan yaş ile birlikte endometrium kanseri sıklığı artmasına rağmen yetersiz endometrial örneklemenin de arttığı gözlenmiştir. Özellikle bu hasta populasyonunda endometrium kanseri risk faktörlerini de göz önünde bulundurarak takiplere gelmesi konusunda yeterli bilgilendirmenin yapılması önem taşımaktadır.
TOI-1842b: A Transiting Warm Saturn Undergoing Reinflation around an Evolving Subgiant
Authors: Wittenmyer Robert A. , Clark Jake T. , Trifonov Trifon , Addison Brett C. , Wright Duncan J. , Stassun Keivan G. , Horner Jonathan , Lowson Nataliea , Kielkopf John , Kane Stephen R. , Plavchan Peter , Shporer Avi , Zhang Hui , Bowler Brendan P. , Mengel Matthew W. , Okumura Jack , Rabus Markus , Johnson Marshall C. , Harbeck Daniel , Tronsgaard René , Buchhave Lars A. , Collins Karen A. , Collins Kevin I. , Gan Tianjun , Jensen Eric L. N. , Howell Steve B. , Furlan E. , Gnilka Crystal L. , Lester Kathryn V. , Matson Rachel A. , Scott Nicholas J. , Ricker George R. , Vanderspek Roland , Latham David W. , Seager S. , Winn Joshua N. , Jenkins Jon M. , Rudat Alexander , Quintana Elisa V. , Rodriguez David R. , Caldwell Douglas A. , Quinn Samuel N. , Essack Zahra , Bouma Luke G. 
Published: January 2022

Abstract
The imminent launch of space telescopes designed to probe the atmospheres of exoplanets has prompted new efforts to prioritize the thousands of transiting planet candidates for follow-up characterization. We report the detection and confirmation of TOI-1842b, a warm Saturn identified by TESS and confirmed with ground-based observations from Minerva-Australis, NRES, and the Las Cumbres Observatory Global Telescope. This planet has a radius of

1.04

−
0.05

+
0.06

R
J, a mass of

0.214

−
0.038

+
0.040

M
J, an orbital period of

9.5739

−
0.0001

+
0.0002

days, and an extremely low density (ρ = 0.252 ± 0.091 g cm−3). TOI-1842b has among the best known combinations of large atmospheric scale height (893 km) and host-star brightness (J = 8.747 mag), making it an attractive target for atmospheric characterization. As the host star is beginning to evolve off the main sequence, TOI-1842b presents an excellent opportunity to test models of gas giant reinflation. The primary transit duration of only 4.3 hr also makes TOI-1842b an easily-schedulable target for further ground-based atmospheric characterization.
An Imaging Search for Post-main-sequence Planets of Sirius B
Authors: Lucas Miles , Bottom Michael , Ruane Garreth , Ragland Sam 
Published: January 2022

Abstract
We present deep imaging of Sirius B, the closest and brightest white dwarf, to constrain post-main-sequence planetary evolution in the Sirius system. We use Keck/NIRC2 in L′ band (3.776 μm) across three epochs in 2020 using the technique of angular differential imaging. Our observations are speckle-limited out to 1 au and background-limited beyond. The 5σ detection limits from our best-performing epoch are 17–20.4 L′ absolute magnitude. We consider multiple planetary formation pathways in the context of Sirius B’s evolution to derive mass sensitivity limits, and achieve sub-Jupiter sensitivities at sub-astronomical unit separations, reaching 1.6–2.4 M
J at 0.5 au down to a sensitivity of 0.7–1.2 M
J at >1 au. Consistent with previous results, we do not detect any companions around Sirius B. Our strong detection limits demonstrate the potential of using high-contrast imaging to characterize nearby white dwarfs.
The Scorpion Planet Survey: Wide-orbit Giant Planets Around Young A-type Stars
Authors: Wagner Kevin , Apai Dániel , Kasper Markus , McClure Melissa , Robberto Massimo 
Published: January 2022

Abstract
The first directly imaged exoplanets indicated that wide-orbit giant planets could be more common around A-type stars. However, the relatively small number of nearby A-stars has limited the precision of exoplanet demographics studies to ≳10%. We aim to constrain the frequency of wide-orbit giant planets around A-stars using the VLT/SPHERE extreme adaptive optics system, which enables targeting ≳100 A-stars between 100 and 200 pc. We present the results of a survey of 84 A-stars within the nearby ∼5–17 Myr old Sco OB2 association. The survey detected three companions—one of which is a new discovery (HIP 75056Ab), whereas the other two (HD 95086b and HIP 65426b) are now-known planets that were included without a priori knowledge of their existence. We assessed the image sensitivity and observational biases with injection and recovery tests combined with Monte Carlo simulations to place constraints on the underlying demographics. We measure a decreasing frequency of giant planets with increasing separation, with measured values falling between 10% and 2% for separations of 30–100 au, and 95% confidence-level upper limits of ≲45%–8% for planets on 30–100 au orbits, and ≲5% between 200 and 500 au. These values are in excellent agreement with recent surveys of A-stars in the solar neighborhood−supporting findings that giant planets out to separations of ≲100 au are more frequent around A-stars than around solar-type hosts. Finally, the relatively low occurrence rate of super-Jupiters on wide orbits, the positive correlation with stellar mass, and the inverse correlation with orbital separation are consistent with core accretion being their dominant formation mechanism.
Evolution of the Spin, Spectrum and Superorbital Period of the Ultraluminous X-Ray Pulsar M51 ULX7
Authors: Brightman Murray , Bachetti Matteo , Earnshaw Hannah , Fürst Felix , Heida Marianne , Israel Gian Luca , Pike Sean , Stern Daniel , Walton Dominic J 
Published: January 2022

Abstract
M51 ULX7 is among a small group of known ultraluminous X-ray pulsars (ULXPs). The neutron star powering the source has a spin period of 2.8 s, orbits its companion star with a period of 2 days, and a superorbital period of 38 days is evident in its X-ray lightcurve. Here we present NuSTAR and XMM-Newton data on the source from 2019 obtained when the source was near its peak brightness. We detect the pulsations, having spun up at a rate of 3 ± 0.5 × 10−10 s s−1 since they were previously detected in 2018. The data also provide the first high-quality broadband spectrum of the source. We find it to be very similar to that of other ULXPs, with two disk-like components, and a high-energy tail. When combined with XMM-Newton data obtained in 2018, we explore the evolution of the spectral components with superorbital phase, finding that the luminosity of the hotter component drives the superorbital flux modulation. The inclination the disk components appear to change with phase, which may support the idea that these superorbital periods are caused by disk precession. We also reexamine the superorbital period with 3 yr of Swift/XRT monitoring, finding that the period is variable, increasing from 38.2 ± 0.5 days in 2018–2019 to 44.2 ± 0.9 days in 2020–2021, which rules out alternative explanations for the superorbital period.
Photometric Objects around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. I. Methods
Authors: Xu Kun , Zheng Yun , Jing Yipeng 
Published: January 2022

Abstract
We provide a method for estimating the projected density distribution

n

¯

2

w

p

(

r

p

)

of photometric objects around spectroscopic objects in a spectroscopic survey. This quantity describes the distribution of photometric sources with certain physical properties (e.g., luminosity, mass, and color) around cosmic webs (PAC) traced by the spectroscopic objects. The method can make full use of current and future deep and wide photometric surveys to explore the formation of galaxies up to medium redshift (z

s
< 2)
3

3

Throughout the paper, we use z

s
for redshift, z for the z-band magnitude, z

p
for the photometric redshift.
with the aid of cosmological spectroscopic surveys that sample only a fairly limited species of objects (e.g., emission line galaxies). As an example, we apply the PAC method to the CMASS spectroscopic and HSC-SSP PDR2 photometric samples to explore the distribution of galaxies for a wide range of stellar masses from 109.0 to 1012.0
M
⊙ around massive galaxies at z

s
≈ 0.6. Using the abundance-matching method, we model

n

¯

2

w

p

(

r

p

)

in N-body simulation using Markov chain Monte Carlo sampling, and we accurately measure the stellar–halo mass relation and stellar mass function for the whole mass range. We can also measure the conditional stellar mass function of satellites for central galaxies of different mass. The PAC method has many potential applications for studying the evolution of galaxies.
Modeling a Coronal Mass Ejection as a Magnetized Structure with EUHFORIA
Authors: Sindhuja G. , Singh Jagdev , Asvestari E. , Raghavendra Prasad B. 
Published: January 2022

Abstract
We studied an Earth-directed coronal mass ejection (CME) that erupted on 2015 March 15. Our aim was to model the CME flux rope as a magnetized structure using the European Heliospheric Forecasting Information Asset (EUHFORIA). The flux rope from eruption data (FRED) output was applied to the EUHFORIA spheromak CME model. In addition to the geometrical properties of the CME flux rope, we needed to input the parameters that determine the CME internal magnetic field like the helicity, tilt angle, and toroidal flux of the CME flux rope. According to the FRED technique geometrical properties of the CME flux rope are obtained by applying a graduated cylindrical shell fitting of the CME flux rope on the coronagraph images. The poloidal field magnetic properties can be estimated from the reconnection flux in the source region utilizing the post-eruption arcade method, which uses the Heliospheric Magnetic Imager magnetogram together with the Atmospheric Imaging Assembly (AIA) 193 Å images. We set up two EUHFORIA runs with RUN-1 using the toroidal flux obtained from the FRED technique and RUN-2 using the toroidal flux that was measured from the core dimming regions identified from the AIA 211 Å images. We found that the EUHFORIA simulation outputs from RUN-1 and RUN-2 are comparable to each other. Overall using the EUHFORIA spheromak model, we successfully obtained the magnetic field rotation of the flux rope, while the arrival time near Earth and the strength of the interplanetary CME magnetic field at Earth are not as accurately modeled.
L’impromptu de Bohême : la réception de Molière en pays tchèques
Authors: Boutan Jean 
Published: January 2022

La réception de Molière en pays tchèques tombe au xviii e siècle dans une période de transition où les techniques de jeu évoluent d’un théâtre d’improvisation au théâtre à texte que nous connaissons aujourd’hui, si bien qu’on a pu la croire insignifiante au vu du caractère lacunaire des sources. L’étude du répertoire montre pourtant de nombreux phénomènes de transferts, d’assimilation et d’adaptation libre, qui participent à cette diffusion invisible de l’œuvre de Molière en Europe centrale.
La société de cour sur la scène hongroise : le théâtre de Molière et A filosófus ( Le Philosophe , 1777) de György Bessenyei
Authors: Studer-Kovacs Veronika 
Published: January 2022

L’article propose l’analyse d’un code moral caractéristique de la culture viennoise des années 1770 et, à travers lui, des éléments empruntés au théâtre de Molière dans une comédie de György Bessenyei, auteur canonique de la littérature hongroise du xviii e siècle, formé à Vienne. L’article s’intéresse surtout à la façon dont Bessenyei dessine, en adaptant le modèle du Misanthrope , des portraits de l’aristocratie de cour, des intellectuels cosmopolites et des nobles de campagne hongrois.
Time Limiting Boundaries of Reversible Clinical Death in Rats Subjected to Ultra-Deep Hypothermia
Authors: Gagarinskiy Evgeniy L , Averin Aleksey S , Uteshev Viktor K , Sherbakov Pavel V , Telpuhov Vladimir I , Shvirst Nikolay E , Karpova Yulya A , Gurin Artem E , Varlachev Aleksandr V , Kovtun Anatoliy L , Fesenko Eugeny E 
Published: January 2022

Background:
It is well known that body temperature maintenance between 20 and 35°C prevents hypoxic damage. However, data regarding the ideal duration and permissible temperature boundaries for ultra-deep hypothermia below 20°C are rather fragmentary. The aim of the present study was to determine the time limits of reversible clinical death in rats subjected to ultra-deep hypothermia at 1–8°C.

Results:
Rat survival rates were directly dependent on the duration of clinical death. If clinical death did not exceed 35 min, animal viability could be restored. Extending the duration of clinical death longer than 45 min led to rat death, and cardiac functioning in these animals was not recovered. The rewarming rate and the lowest temperature of hypothermia experienced did not directly influence survival rates.

Conclusions:
In a rat model, reversible ultra-deep hypothermia as low as 1–8°C could be achieved without the application of hypercapnia or pharmacological support. The survival of animals was dependent on the duration of clinical death, which should not exceed 35 min.