bluuebunny/crossref_metadata_2025_split huggingface dataset:
Media Pembelajaran dalam Meningkatkan Mutu Pendidikan Agama Islam di SMK Paramarta Jombang Ciputat
Authors: Mudzakir  
Published: April 2024

Dalam Penelitian ini Dalam usaha meningkatkan kualitas pendidikan, guru kerap menghadapi kesulitan dalam menyampaikan materi pembelajaran. Penggunaan media pembelajaran menjadi salah satu langkah untuk meningkatkan proses pembelajaran. Dengan demikian, media pembelajaran di lingkungan sekolah maupun di luar sekolah dapat menjadi solusi atas berbagai masalah yang muncul dalam proses belajar mengajar. Penelitian ini bertujuan untuk mengidentifikasi media pembelajaran yang efektif dalam meningkatkan mutu Pendidikan Agama Islam di SMK Paramarta Jombang Ciputat, (2) Dalam usaha meningkatkan kualitas pendidikan, guru kerap menghadapi kesulitan dalam menyampaikan materi pembelajaran. Penggunaan media pembelajaran menjadi salah satu langkah untuk meningkatkan proses pembelajaran. Dengan demikian, media pembelajaran di lingkungan sekolah maupun di luar sekolah dapat menjadi solusi atas berbagai masalah yang muncul dalam proses belajar mengajar. Penelitian ini bertujuan untuk mengidentifikasi media pembelajaran yang efektif dalam meningkatkan mutu Pendidikan Agama Islam.
Teachers often struggle to provide adequate learning materials to ensure quality education. Utilizing learning media is a key strategy to enhance the teaching and learning process. This study focused on identifying the learning media used to improve the quality of Islamic Religious Education at Paramarta Jombang Ciputat Vocational High School. The research, a qualitative descriptive study, aimed to explore the impact of learning media on the quality of Islamic Religious Education at SMK Paramarta Jombang Ciputat.
ЭФФЕКТИВНОСТЬ ПРИМЕНЕНИЯ АНТИСТРЕССОВОГО ПРЕПАРАТА «ГИДРО РЕКС ВИТАЛ» ПРИ ВЫРАЩИВАНИИ ЦЫПЛЯТ-БРОЙЛЕРОВ В ПЕРЕХОДНЫЙ ПЕРИОД ГОДА
Authors: Аблаева Эльмира , Кавтарашвили Алексей , Махатов Болатхан , Кусаинова Жанар , Саркулова Нурсулу 
Published: April 2024

Изучена эффективность применения антистрессового препарата «Гидро Рекс Витал» при выращивании цыплят-бройлеров в переходный период года. В суточном возрасте методом аналогов были сформированы 4 группы (одна контрольная и три опытные). Птицу всех групп до 42-дневного возраста содержали в одном помещении (идентичных секциях) на глубокой подстилке. В контрольной группе 1 препарат не использовался, а в опытных группах 2, 3 и 4 дозировкая выпаеваемого с питьевой водой препарата составила 200, 300 и 400 мл на 1 тонну воды, соответственно. Результаты исследования показали, что сохранность поголовья в группах 1(к), 2, 3 и 4 составила 90,0; 93,3; 96,7; 96,7 %, живая масса птицы в 42-дневном возрасте – 2,49; 2,60; 2,65 и 2,57 кг, среднесуточный прирост живой массы – 58,3; 60,8; 62,0 и 60,0 г, затраты корма на 1 кг прироста живой массы – 1,85; 1,74; 1,69 и 1,57 кг, убойный выход потрошенной тушки – 72,2; 74,9; 76,3 и 74,0%, рентабельность производства – 17,0; 26,3; 31,3 и 30,8%, соответственно. Рекомендовано цыплятам-бройлерам в целях повышения жизнеспособности и продуктивности, снижения затрат кормов на единицу продукции и себестоимость мяса, повышения рентабельности производства выпаивать с водой антистрессовый препарат «Гидро Рекс Витал» в дозировке 300 мл на 1 тонну воды с суточного до конца периода выращивания. В исследованиях для быстрого определения выигрышной группы, целесообразно места европейского индекса продуктивности, использовать российский индекс эффективности производства мяса.
Pengaruh Perendaman Bertingkat Garam Dan Atung (Parinarium glaberimum, Hassk) Terhadap Kualitas Ikan Cakalang (Katsuwonus pelamis, Linn.) Asin Kering
Authors: Moniharapon Trijunianto , Pattipeilohy Fredy , Moniharapo Erynola 
Published: April 2024

Tujuan penelitian ini adalah untuk mengetahui efektivitas perendaman bertingkat garam dan buah atung (Parinarium glaberimum, Hassk) terhadap kualitas ikan cakalang (Katsuwonus pelamis, Linn.) asin kering. Perlakuan terdiri dari 2 faktor yaitu konsentrasi garam (5, 10 %) dan konsentrasi atung (3,4 dan 5 %). Data dianalisis dengan menggunakan RAL (Rancangan acak Lengkap dilanjutkan dengan uji BNJ. Parameter yang dilihat adalah kadar air, kadar protein, kadar garam dan kandungan TPC Konsentrasi perendaman garam 10% atung 5% efektif menghasilkan kadar air, kadar protein, kadar garam dan kandungan TPC ikan cakalang asin kering terurut yaitu: 28,31%; 67,02%; 4,60% dan 6,2 x 103 koloni; garam 10% atung 4%: 27,68%; 68,63%; 3,65% dan 2,0 x 104 koloni; garam 10% atung 3%: 27,38%; 69,23%; 3,10% dan 5,9 x 103 koloni; garam 5% atung 5%: 27,30%; 66,23%; 5,25% dan 5,9 x 103 koloni; garam 5% atung 4%: 30,54%; 65,94%; 2,95% dan 3,6 x 103 koloni; garam 5% atung 3%: 28,80%; 65,20%; 5,20% dan 1,9 x 104 koloni; dan kontrol 25%: 32,34%; 54,31%; 13,5% dan 2,3 x 103 koloni. Denaturasi protein yang terjadi pada pengolahan cakalang asin kering dengan perlakuan perendaman bertingkat garam dan atung antara sekitar 1,6 - 7,3%, sedangkan kontrol 22,8%.
Probing Dark Energy and Modifications of Gravity with Ground-based millimeter-wavelength Line Intensity Mapping
Authors: Moradinezhad Dizgah Azadeh , Bellini Emilio , Keating Garrett K. 
Published: April 2024

Abstract
Line intensity mapping (LIM) can provide a powerful means to constrain the theory of gravity and the nature of dark energy at low and high redshifts by mapping the large-scale structure over many redshift epochs. In this paper, we investigate the potential of the next generation ground-based millimeter-wavelength LIM surveys in constraining several models beyond ΛCDM, involving either a dynamic dark energy component or modifications of the theory of gravity. Limiting ourselves to two-point clustering statistics, we consider the measurements of auto-spectra of several CO rotational lines (from J = 2−1 to J = 6−5) and the [C ii] fine structure line in the redshift range of 0.25 < z < 12. We consider different models beyond ΛCDM, each one with different signatures and peculiarities. Among them, we focus on Jordan–Brans–Dicke and axion-driven early dark energy models as examples of well-studied scalar-tensor theories acting at late and early times, respectively. Additionally, we consider three phenomenological models based on an effective description of gravity at cosmological scales. We show that LIM surveys deployable within a decade (with ∼108 spectrometer hours) have the potential to improve upon the current bounds on all considered models significantly. The level of improvements range from a factor of a few to an order of magnitude.
Pulsed Iron Line Emission from the First Galactic Ultraluminous X-Ray Pulsar Swift J0243.6+6124
Authors: Xiao Y. X. , Xu Y. J. , Ge M. Y. , Lu F. J. , Zhang S. N. , Zhang S. , Tao L. , Qu J. L. , Wang P. J. , Kong L. D. , Tuo Y. L. , You Y. , Zhao S. J. , Peng J. Q. , Du Y. F. , Zhang Y. H. , Ye W. T. 
Published: April 2024

Abstract
We report the phase-resolved spectral results of the first Galactic pulsating ultraluminous X-ray source (PULX) Swift J0243.6+6124, modeling its 2017–2018 outburst peak using data collected by the Hard X-ray Modulation Telescope (Insight-HXMT). The broad energy coverage of Insight-HXMT allows us to obtain a more accurate spectral continuum to reduce the coupling of broad iron line profiles with other components. We use three different continuum spectrum models but obtain similar iron line results. For the first time, we detect the pulse characteristics of the broad iron line in a PULX. The variation in the width and intensity of this iron line with σ ∼ 1.2–1.5 keV has a phase offset of about 0.25 from the pulse phase. We suggest that the uneven irradiation of the thick inner disk by the accretion column produces the modulated variation of the broad iron line. In addition, the nonpulsed narrow line is suggested to come from the outer disk region.
Insight into the Solar Plage Chromosphere with DKIST
Authors: Kuridze David , Uitenbroek Han , Wöger Friedrich , Mathioudakis Mihalis , Morgan Huw , Campbell Ryan , Fischer Catherine , Cauzzi Gianna , Schad Thomas , Reardon Kevin , da Silva Santos João M. , Beck Christian , Tritschler Alexandra , Rimmele Thomas 
Published: April 2024

Abstract
The strongly coupled hydrodynamic, magnetic, and radiation properties of the plasma in the solar chromosphere make it a region of the Sun's atmosphere that is poorly understood. We use data obtained with the high-resolution Visible Broadband Imager (VBI) equipped with an Hβ filter and the Visible Spectro-Polarimeter (ViSP) on the Daniel K. Inouye Solar Telescope to investigate the fine-scale structure of the plage chromosphere. To aid in the interpretation of the VBI imaging data, we also analyze spectra from the CHROMospheric Imaging Spectrometer on the Swedish Solar Telescope. The analysis of spectral properties, such as enhanced line widths and line depths, explains the high contrast of the fibrils relative to the background atmosphere demonstrating that Hβ is an excellent diagnostic for the enigmatic fine-scale structure of the chromosphere. A correlation between the parameters of the Hβ line indicates that opacity broadening created by overdense fibrils could be the main reason for the spectral line broadening frequently observed in chromospheric fine-scale structures. Spectropolarimetric inversions of the ViSP data in the Ca ii 8542 Å and Fe i 6301/6302 Å lines are used to construct semiempirical models of the plage atmosphere. Inversion outputs indicate the existence of dense fibrils in the Ca ii 8542 Å line. The analyses of the ViSP data show that the morphological characteristics, such as orientation, inclination, and length of fibrils, are defined by the topology of the magnetic field in the photosphere. Chromospheric maps reveal a prominent magnetic canopy in the area where fibrils are directed toward the observer.
Field Line Universal relaXer (FLUX): A Fluxon Approach to Coronal Magnetic Field Modeling
Authors: Lowder Chris , Gilly Chris , DeForest Craig 
Published: April 2024

Abstract
We describe a novel method for modeling the global, steady solar wind using photospheric magnetic fields as a driving boundary condition. Prior wind models in this class include both rapid heuristic methods that use potential field extrapolation and variants thereof, trading rigor for computation speed, and detailed 3D magnetohydrodynamic (MHD) models that attempt to simulate the entire solar corona with a degree of physical rigor, but require large amounts of computation. The Field Line Universal relaXer, an open-source numerical code that implements the “fluxon” semi-Lagrangian approach to MHD modeling, provides an intermediate approach between these two general classes. In particular, the fluxon approach to MHD describes the magnetic field through discrete analogs of magnetic field lines, relaxing these structures to a stationary state of force balance. In this work we introduce a 1D solar wind solution along each field line, providing an ensemble of solutions that are interpolated back onto a uniform grid at an outer boundary surface. This provides advantages in physical rigor over heuristic semianalytic techniques, and in computational efficiency over full 3D MHD techniques. Here we describe the underlying methodology and the FLUXPipe modeling pipeline process.
A Relook at the Black Hole Binary Candidate J1328+2752 with VLBI
Authors: Nandi Sumana , Kharb Preeti , Caproni Anderson , Roy Rupak , Sebastian Biny 
Published: April 2024

Abstract
We present multiband follow-up observations of the supermassive binary black hole (BBH) candidate and misaligned double–double radio galaxy, J1328+2752. To investigate its parsec-scale structure, we have carried out observations with the Very Long Baseline Array (VLBA) and the European Very Long Baseline Interferometry (VLBI) Network. Additionally, we have obtained optical spectroscopic observations with the 3.6 m Devasthal Optical Telescope. Within 3.5 yr of our previous VLBI observations, the central parsec-scale radio structure of J1328+2752 has changed from a double component to a single central component and its flux density has increased by a factor of 3 in the 5 GHz VLBA observations. The new radio component is largely unresolved at 3, 5, and 8 GHz. The multifrequency radio data shows a convex-shaped spectrum for this unresolved component. The turnover frequency is at ∼3 GHz. While the total intensity image does not reveal any details, a super-resolved VLBA 5 and 8 GHz spectral index image does indicate the presence of two components at a separation of ∼4.2 pc with spectral indices −0.5 ± 0.3 and −0.9 ± 0.3. We have not observed a simultaneous change in the optical line profiles or intensities over the past few years. The radio structure, the variation of the flux density, and spectral shape can potentially be consistent both with the signature of a young radio source or a BBH at the center of J1328+2752.
The Role of a Neutron Component in the Photospheric Emission of Long-duration Gamma-Ray Burst Jets
Authors: Walker Nathan , Parsotan Tyler , Lazzati Davide 
Published: April 2024

Abstract
Long-duration gamma-ray bursts (LGRBs), thought to be produced during core-collapse supernovae, may have a prominent neutron component in the outflow material. If present, neutrons can change how photons scatter in the outflow by reducing its opacity, thereby allowing the photons to decouple sooner than if there were no neutrons present. Understanding the details of this process could therefore allow us to probe the central engine of LGRBs, which is otherwise hidden. Here, we present results of the photospheric emission from an LGRB jet, using a combination of relativistic hydrodynamic simulations and radiative transfer postprocessing using Monte Carlo radiation transfer code. We control the size of the neutron component in the jet material by varying the equilibrium electron fraction Y

e
, and we find that the presence of neutrons in the GRB fireball affects the Band parameters α and E
0, while the picture with the β parameter is less clear. In particular, the break energy E
0 is shifted to higher energies. Additionally, we find that increasing the size of the neutron component also increases the total radiated energy of the outflow across multiple viewing angles. Our results not only shed light on LGRBs but are also relevant to short-duration gamma-ray bursts associated with binary neutron star mergers due to the likelihood of a prominent neutron component in such systems.
Tropical Cyclones on Tidally Locked Rocky Planets: Dependence on Rotation Period
Authors: Garcia Valeria , Smith Cole M. , Chavas Daniel R. , Komacek Thaddeus D. 
Published: April 2024

Abstract
Tropical cyclones occur over the Earth’s tropical oceans, with characteristic genesis regions and tracks tied to the warm ocean surface that provide energy to sustain these storms. The study of tropical cyclogenesis and evolution on Earth has led to the development of environmental favorability metrics that predict the strength of potential storms from the local background climate state. Simulations of the gamut of transiting terrestrial exoplanets orbiting late-type stars may offer a test of this Earth-based understanding of tropical cyclogenesis. Previous work has demonstrated that tropical cyclones are likely to form on tidally locked terrestrial exoplanets with intermediate rotation periods of ∼8–10 days. In this study, we test these expectations using ExoCAM simulations with both a sufficient horizontal resolution of 0.°47 × 0.°63 required to permit tropical cyclogenesis along with a thermodynamically active slab ocean. We conduct simulations of tidally locked and ocean-covered Earth-sized planets orbiting late-type M dwarf stars with varying rotation periods from 4–16 days in order to cross the predicted maximum in tropical cyclogenesis. We track tropical cyclones that form in each simulation and assess their location of maximum wind, evolution, and maximum wind speeds. We compare the resulting tropical cyclone locations and strengths to predictions based on environmental favorability metrics, finding good agreement between Earth-based metrics and our simulated storms with a local maximum in both tropical cyclone frequency and intensity at a rotation period of 8 days. Our results suggest that environmental favorability metrics used for tropical cyclones on Earth may also be applicable to temperate tidally locked Earth-sized rocky exoplanets with abundant surface liquid water.
Sensitivity of Cosmological Parameter Estimation to Nonlinear Prescription from Cosmic Shear
Authors: Safi Sarah , Farhang Marzieh 
Published: April 2024

Abstract
Several ongoing and upcoming large-scale structure surveys aim to explore the nonlinear regime of structure formation with high precision. Making reliable cosmological inferences from these observations necessitates precise theoretical modeling of the mildly nonlinear regime. In this work we explore how the choice of nonlinear prescription would impact parameter estimation from cosmic shear measurements for a Euclid-like survey. Specifically, we employ two different nonlinear prescriptions of halofit and the Effective Field Theory of the Large Scale Structure and compare their measurements for the three different cosmological scenarios of ΛCDM, wCDM, and (w
0, w

a
) CDM. We also investigate the impact of different nonlinear cutoff schemes on parameter estimation. We find that the predicted errors on most parameters shrink considerably as smaller scales are included in the analysis, with the amount depending on the nonlinear prescription and the cutoff scheme used. We use predictions from the halofit model to analyze the mock data from DarkSky N-body simulations and quantify the parameter bias introduced in the measurements due to the choice of nonlinear prescription. We observe that σ
8 and n
s have the largest measurement bias induced by inaccuracies of the halofit model.
Low-cost, high-volume imaging for entomological digitization
Authors: Steinke Dirk , McKeown Jaclyn , Zyba Allison , McLeod Joschka , Feng Corey , Hebert Paul 
Published: April 2024

Large-scale digitization of natural history collections requires the automation of image acquisition and processing. Reflecting this fact, various approaches, some highly sophisticated, have been developed to support the imaging of museum specimens. However, most of these systems are complex and expensive, restricting their deployment.
Here we describe a simple, inexpensive technique for imaging arthropods larger than 5 mm. By mounting a digital SLR camera on a CNC (computer numerical control) motor-drive rig, we created a system that captures high-resolution z-axis stacked images (6960 x 4640 pixels) of 95 specimens in 30 minutes.
This system is inexpensive ($1000 USD without camera), easy to set up, and to maintain. By coupling low cost with high production capacity, it represents a solution for the digitization of any natural history collection.
The impact of anticholinergics on cognitive function in patients with neurogenic lower urinary tract dysfunction: A narrative review
Authors: Welk Blayne 
Published: April 2024

ABSTRACT
This narrative review discusses the relationship between anticholinergic medications and cognitive change specifically in patients with neurogenic lower urinary tract dysfunction (NLUTD). NLUTD is prevalent in various conditions, including spinal cord injury (SCI), spina bifida (SB), multiple sclerosis (MS), Parkinson’s, stroke, and dementia and often requires anticholinergic overactive bladder (OAB) medications. In the general population, and among those with OAB, several studies have found a significant association between this class of medications and cognitive side effects, mostly when used for > 90 days. These cognitive side effects may be particularly relevant to people with NLUTD due to their higher baseline risk of cognitive impairment. Two studies (one in people with SCI and another in MS) found evidence of cognitive impairment with the use of OAB anticholinergics (specifically oxybutynin and tolterodine). People with dementia commonly use OAB anticholinergics, and there is evidence that oxybutynin and tolterodine may impair cognition in this population. Two recent studies in children with SB studied 12 months of solifenacin and 6 months of fesoterodine/oxybutynin and found there was no significant change in neuropsychological testing. Clinical studies in people with Parkinson’s disease and prior stroke have not shown that trospium, darifenacin, or fesoterodine have a significant impact on cognitive measures. In summary, oxybutynin and tolterodine may pose a higher risk of cognitive impairment than newer OAB anticholinergics in people with NLUTD; there is no evidence that children with SB experience cognitive impairment with OAB anticholinergics. Further study is necessary to confirm cognitive safety, particularly as the NLUTD population may have a high exposure to OAB anticholinergics. Advocating for potentially safer OAB medications is necessary if there is concern about cognitive risks.
Renal artery pseudoaneurysm post-COVID-19 infection: An unusual delayed complication
Authors: Shubhankar Gautam , Mittal Ankur , Panwar Vikas Kumar , Kumar Siddharth 
Published: April 2024

ABSTRACT
This case report discusses a rare and severe complication of COVID-19 recovery – renal mucormycosis leading to right renal artery pseudoaneurysm. A 59-year-old patient, previously treated for COVID-19, presented with dry cough, flank pain, and hematuria. He was diagnosed with renal artery pseudoaneurysm with renal mucormycosis. Successful management included urgent angioembolization, systemic liposomal amphotericin B, and subsequent radical nephrectomy post-stabilization. The case underscores the importance of vigilant post-COVID-19 follow-up, particularly in patients treated with steroids, and highlights the need for a multidisciplinary approach for timely diagnosis and effective management of mucormycosis related complications.
Survival outcomes of postchemotherapy retroperitoneal lymph node dissection for nonseminomatous germ cell tumors: A retrospective cohort study from a single tertiary center in South India
Authors: Kumar Rakesh , Sadanala Madhuri Evangeline , Nagasubramanian Santosh , Joel Anjana , George Arun Joseph Philip , Gowri S Mahasampath , Mukherjee Partho , Singh Ashish , Mukha Rajiv Paul , Kumar Santosh , Devasia Antony , Nirmal Thampi John 
Published: April 2024

ABSTRACT

Introduction:
Chemotherapy, postchemotherapy retroperitoneal lymph node dissection (pcRPLND), and metastasectomy remain the standard of care for the management of advanced nonseminomatous germ cell tumor (NSGCT).

Methods:
We retrospectively studied 73 patients who had pcRPLND at a single tertiary-care center (2003–2022). Surgical and clinicopathological features and oncological outcomes are presented.

Results:
The mean age was 28.27 years (15–48). Three-fourths had Stage III disease at diagnosis. International Germ Cell Cancer Collaborative Group risk stratification was 54.54% and 21.21% in intermediate risk, and poor risk, respectively. Sixty-two patients had Standard, 7 had Salvage and 4 underwent Desperation pcRPLND. Eleven patients (15.06%) required adjunctive procedures. Thirteen patients (17.8%) had ≥ class 3 Clavien–Dindo complications and postoperative mortality occurred in 5 (6.8%) patients. The histopathologies (HPE) of the pcRPLNDs were necrosis, teratoma, and viable tumor in 39.7%, 45.2%, and 15.1%, respectively. Seven patients underwent metastasectomy. An 85% size reduction in the size of RPLN predicted necrosis. There was 71.4% concordance between pcRPLND and metastasectomy HPEs. The median follow-up was 26.72 months (inter-quartile range – 13.25–47.84). The 2-year recurrence-free survival (RFS) rate was 93% (95% confidence interval [CI]–83%–97%) and the overall survival (OS) rate was 90% (95% CI–80%–95%). This is the largest series of pcRPLND for NSGCT in India to our knowledge.

Conclusion:
Although most of the cohort belonged to stage III, an RFS and OS rate of >90% at 2 years was achieved. We believe that successful management of postchemotherapy residual masses in NSGCT is contingent on the availability of multidisciplinary expertise and is therefore best done at tertiary-care referral centers.