bluuebunny/crossref_metadata_2025_split huggingface dataset:
Kesejahteraan Gender dan Inklusi Sosial dengan Menghadirkan Inovasi Cocopeat dan Kecap dalam Memanfaatkan Limbah Kelapa
Authors: Susanti Rina , Fikri Haykal , Syakira Annisa , Adisti Suci , Utomo Afrian Ari 
Published: November 2023

Pohon kelapa merupakan tanaman seribu manfaat karena hampir semua bagiannya dapat digunakan dalam kehidupan sehari hari. Bagian yang paling banyak dimanfaatkan dari pohon kelapa ialah buahnya. Namun sayangnya masyarakat Desa Tanjung Belit Selatan hanya sebatas memanfaatkan daging dari buah kelapa tanpa melihat manfaat dari air dan sabut kelapa. Hal ini menyebabkan penumpukan sabut kelapa sehingga menjadikannya limbah yang dapat mengganggu masyarakat dan mencemari lingkungan. Kecap dan cocopeat merupakan salah satu cara untuk meningkat nilai komersial dari kelapa. Inovasi ini merupakan bagian dari program kerja unggulan dengan tema kesetaraan gender dan inklusi sosial. Dengan diperkenalkannya inovasi ini bertujuan untuk meningkat peluang wirausaha bagi masyarakat desa terutama ibu-ibu rumah tangga yang menjadi target utama kegiatan ini agar menjadi lebih produktif sehingga akan meningkat perekonomian keluarga. Terciptanya ibu rumah tangga yang produktif akan meningkat kesejajaran istri dan suami dalam meningkatkan perekonomian keluarga.
Pengenalan Pajak dan Perbankan Syari’ah serta Kiat Belajar Menuju Sukses di MTS Al-Aqsha, Kelapa Gading, Jakarta Utara
Authors: Hidayat Malik , Handari Henni , Arifin Zainal 
Published: November 2023

Tujuan dari dilaksanakan kegiatan pengabdian pada masyarakat ini adalah untuk memberikan pemahaman tentang Pengenalan Pajak, Perbankan Syari’ah, dan Kiat Belajar Menuju Sukses yang baik atau manfaat kepada para Siswa/i MTS Al-Aqsha, Kelapa Gading, Jakarta Utara. Setelah dilaksanakan kegiatan ini diharapkan dapat meningkatkan pemahaman para Siswa/i secara individu dan organisasi. Kegiatan pengabdian masyarakat ini diselenggarakan dalam waktu 1 (satu) hari. Dalam melaksanakan kegiatan pengabdian ini, permasalahan yang ditemukan adalah bahwa para Siswa/i MTS Al-Aqsha masih belum mendapatkan pemahaman tentang pajak, perbankan syari’ah, dan kiat-kiat belajar menuju sukses sesuai tuntunan Alloh SWT dan Rosul-nya. Semua Ilmu diperoleh dari Alloh SWT, Rosul, dan Pemerintah (Diknas) tingkat pendidikan dasar. Hasil dari kegiatan pengabdian masyarakat menunjukkan bahwa telah terjadi penambahan pemahaman pada Siswa/i tentang perpajakan, perbankan syari’ah serta kiat-kiat belajar menuju sukses. Secara keseluruhan kegiatan pengabdian kepada masyarakat ini mendapatkan respon dan antusiasme yang positif dari para Siswa/i MTS Al-Aqsha, Kelapa Gading, Jakarta Utara.
Forming a Modern Therapeutic Resource for Geriatric Dentistry
Authors: Trezubov V. N. , Rozov R. A. , Mishnev M. L. , Parshin Yu. V. 
Published: November 2023

Background. The special status and position of older and oldest old in the therapeutic, diagnostic, and preventive activities of a dentist lead to a firm conviction of an urgent necessity and expediency of creating a new medical specialization — geriatric dentistry.Aim. Based on many years of clinical experience and scientific research, including extensive use of high-tech oral prosthetics for older adults, to make the first attempt at creating an optimal therapeutic resource for a new medical specialization — geriatric dentistry.Materials and methods. Examination and prosthetics were performed on 645 patients aged 60 to 85 years old, with various types of implantable prostheses in the period o 3 to 7 years after their implantation. In addition, 903 implantable prostheses and 3287 of their artificial supports (implants) were also examined.Results. The mean age of patients who visited the orthopedic dentistry department for dental prosthetics was 64.72 ± 6.8 years old. As the main method of rehabilitation of older patients’ masticatory and speech apparatus, we have used implant-supported prosthesis with its digital transformation. Most of the patients underwent reasonably radical oral cavity preparation for prosthetics. The original state retention of the tissues of the implant bed ranged from 78.04 to 100%. At the same time, fixed structures of implantable prostheses were characterized by higher indicators. The preservation of the implants was from 96.8 to 100%, depending on the observation period.Conclusion. The high values of implant and prosthesis retention rates, good condition of the peri-implant mucous membrane and bone in remote periods after prosthetics, as well as a high level of patient satisfaction and significantly higher achieved level of their quality of life, along with high medical and economic efficiency of the method, allow us to consider it a promising standard of geriatric dentistry. Thus, a modern therapeutic, or rather, rehabilitation, resource for effective pre-prosthetic preparation and implant prosthesis has been developed and justified, which is the optimal approach in geriatric dentistry.
The Nutritional Status and Oral Health: A New Look at the Problem
Authors: Turusheva A. V. , Frolova E. V. , Trezubov V. N. , Rozov R. A. , Kabanov M. Yu. 
Published: November 2023

Introduction. According to research, the condition of the oral cavity in older adults is one of the risk factors for the development of malnutrition; however, even with complete loss of teeth, malnutrition does not develop in all patients.Objective. The aim of our study was to evaluate the prevalence of malnutrition in patients with tooth loss and the factors associated with a reduced risk of developing malnutrition in them.Methods. Epidemiological study of the EVCALIPT random sample of individuals aged 65 years and older (n=396). Main study parameters: oral health assessment questionnaire, non-communicable chronic disease, nutritional assessment using the Mini Nutritional assessment, comprehensive geriatric assessment, blood count test.Results. The prevalence of malnourishment does not depend on the number of remaining teeth and the use of dentures or implants (p>0.05). The main independent factors affecting the risk malnutrition in patients with oral frailty are complaints about difficulty with mastication [OR (95% CI) 2.100 (1.100–4.010)] and pronunciation of words [OR (95%CI) 2.203 (1.007–4.816)]. Maintaining high rates of grip strength [OR (95% CI) 0.314 (0.167–0.590)] and absence of depression [OR (95% CI) 0.408 (0.196–0.846)] are associated with a reduced risk of malnutrition in patients with oral frailty.Conclusion. The fact of the absence of teeth or prostheses / implants does not lead to an increase in the risk of malnutrition in older adults. Complaints about mastication and words pronunciation difficulties are more significant contributors to the risk of malnutrition in this age group. High rates of grip strength and the absence of depression in patients with impaired chewing of food and pronunciation of words are associated with a diminished risk of malnutrition.
Managing Older and Oldest-Old with Frailty in Outpatient and Inpatient Clinics of Moscow (Treatment Algorithm Based on CGA Rresults)
Authors: Trukhanov A. V. , Runikhina N. K. , Reshetova A. A. , Tkacheva O. N. , Kotovskaya Yu. V. , Sharashkina N. V. 
Published: November 2023

The article is aimed at improving the management of older and oldest-older in outpatient and inpatient medical facilities of Moscow. Represented algorithm of therapeutic and preventive measures allows the geriatrician, in accordance with CGA domains and possible clinical situations, to timely and efficiently draw up a patient management plan based on the results of CGA and current clinical guidelines.
The Influence of Chronic Diseases on Motoric Cognitive Risk Syndrome Development
Authors: Turusheva A. V. , Frolova E. V. 
Published: November 2023

Introduction. Motoric cognitive risk (MCR) syndrome is a syndrome characterized by cognitive complaints or mild cognitive impairment (MCI) identified during tests and accompanied by slow gait but without dementia or autonomy decline. The concept of MCR is relatively new, and its natural course has not been sufficiently studied to date.Objective. To estimate the prevalence of MCR, factors contributing to the risk of its development and the impact on mortality.Methods. A prospective cohort Crystal study, random sample of individuals aged 65 and older. The total follow-up period was 9 years. Evaluation covered: gait speed, the Mini-Mental State Examination, chronic disease, blood pressure, lab tests.Results. To diagnose the motor cognitive risk syndrome, the value of the gait speed was used, corresponding to the 2nd and 3rd quartiles — from 0.75 to 0.4 m/s. MCR was diagnosed in 16.7%. Type 2 diabetes was associated with an increased incidence of MCR [OR (95% CI) 7.275 (1.520–34.829)]. With an increase in systolic blood pressure (SBP) for every 30 mm Hg. the probability of detecting motoric cognitive risk syndrome increases by 6 times [OR (95% CI) 5.796 (1.388–24.200)]. After adjusting for sex, age, presence of type 2 diabetes, and blood pressure level, the addition of each component of the motoric cognitive syndrome increases the risk of all-cause death over 9 years of follow-up by 35% [HR (95% CI) 1.348 (1.001–1.814)].Conclusion. The main chronic diseases associated with the development of MCR were type 2 diabetes and arterial hypertension. MCR is associated with a higher risk of mortality in older age, even with a slight decrease in gait speed. Gait speed within the 2nd and 3rd quarter may be a component of motoric cognitive risk syndrome.
Scaling K2. VII. Evidence For a High Occurrence Rate of Hot Sub-Neptunes at Intermediate Ages
Authors: Christiansen Jessie L. , Zink Jon K. , Hardegree-Ullman Kevin K. , Fernandes Rachel B. , Hopkins Philip F. , Rebull Luisa M. , Boley Kiersten M. , Bergsten Galen J. , Bhure Sakhee 
Published: November 2023

Abstract
The NASA K2 mission obtained high-precision time-series photometry for four young clusters, including the near-twin 600–800 Myr old Praesepe and Hyades clusters. Hot sub-Neptunes are highly prone to mass-loss mechanisms, given their proximity to the host star and the weakly bound gaseous envelopes, and analyzing this population at young ages can provide strong constraints on planetary evolution models. Using our automated transit detection pipeline, we recover 15 planet candidates across the two clusters, including 10 previously confirmed planets. We find a hot sub-Neptune occurrence rate of 79%–107% for GKM stars in the Praesepe cluster. This is 2.5–3.5σ higher than the occurrence rate of

16.54

−
0.98

+
1.00

% for the same planets orbiting the ∼3–9 Gyr old GKM field stars observed by K2, even after accounting for the slightly supersolar metallicity ([Fe/H] ∼ 0.2 dex) of the Praesepe cluster. We examine the effect of adding ∼100 targets from the Hyades cluster and extending the planet parameter space under examination, and we find similarly high occurrence rates in both cases. The high occurrence rate of young, hot sub-Neptunes could indicate either that these planets are undergoing atmospheric evolution as they age, or that planetary systems that formed when the Galaxy was much younger are substantially different than from today. Under the assumption of the atmospheric mass-loss scenario, a significantly higher occurrence rate of these planets at the intermediate ages of Praesepe and Hyades appears more consistent with the core-powered mass-loss scenario for the origin of the planet radius valley, compared to the photoevaporation scenario.
The Far Side of the Galactic Bar/Bulge Revealed through Semi-regular Variables
Authors: Hey Daniel R. , Huber Daniel , Shappee Benjamin J. , Bland-Hawthorn Joss , Tepper-García Thor , Sanderson Robyn , Chakrabarti Sukanya , Saunders Nicholas , Hunt Jason A. S. , Bedding Timothy R. , Tonry John 
Published: November 2023

Abstract
The Galactic bulge is critical to our understanding of the Milky Way. However, due to the lack of reliable stellar distances, the structure and kinematics of the bulge/bar beyond the Galactic center have remained largely unexplored. Here, we present a method to measure distances of luminous red giants using a period–amplitude–luminosity relation anchored to the Large Magellanic Cloud, with random uncertainties of 10%–15% and systematic errors below 1%–2%. We apply this method to data from the Optical Gravitational Lensing Experiment to measure distances to 190,302 stars in the Galactic bulge and beyond out to 20 kpc. Using this sample, we measure a distance to the Galactic center of R
0 = 8108 ± 106stat ± 93sys pc, consistent with direct measurements of stars orbiting Sgr A*. We cross-match our distance catalog with Gaia DR3 and use the subset of 39,566 overlapping stars to provide the first constraints on the Milky Way’s velocity field (V

R
, V

ϕ
, V

z
) beyond the Galactic center. We show that the V

R
quadrupole from the bar’s near side is reflected with respect to the Galactic center, indicating that the bar is bisymmetric and aligned with the inner disk. We also find that the vertical height V

Z
map has no major structure in the region of the Galactic bulge, which is inconsistent with a current episode of bar buckling. Finally, we demonstrate with N-body simulations that distance uncertainty plays a factor in the alignment of the major and kinematic axes of the bar, necessitating caution when interpreting results for distant stars.
CD –27°11535: Evidence for a Triple System in the β Pictoris Moving Group
Authors: Thomas Andrew D. , Nielsen Eric L. , De Rosa Robert J. , Peck Anne E. , Macintosh Bruce , Chilcote Jeffrey , Kalas Paul , Wang Jason J. , Blunt Sarah , Greenbaum Alexandra , Konopacky Quinn M. , Ireland Michael J. , Tuthill Peter , Ward-Duong Kimberly , Hirsch Lea A. , Czekala Ian , Marchis Franck , Marois Christian , Millar-Blanchaer Max A. , Roberson William , Smith Adam , Gallamore Hannah , Klusmeyer Jessica 
Published: November 2023

Abstract
We present new spatially resolved astrometry and photometry of the CD –27°11535 system, a member of the β Pictoris moving group consisting of two resolved K-type stars on a ∼20 yr orbit. We fit an orbit to relative astrometry measured from NIRC2, GPI, and archival NaCo images, in addition to literature measurements. However, the total mass inferred from this orbit is significantly discrepant from that inferred from stellar evolutionary models using the luminosity of the two stars. We explore two hypotheses that could explain this discrepant mass sum: a discrepant parallax measurement from Gaia due to variability, and the presence of an additional unresolved companion to one of the two components. We find that the ∼20 yr orbit could not bias the parallax measurement, but that variability of the components could produce a large-amplitude astrometric motion, an effect that cannot be quantified exactly without the individual Gaia measurements. The discrepancy could also be explained by an additional star in the system. We jointly fit the astrometric and photometric measurements of the system to test different binary and triple architectures for the system. Depending on the set of evolutionary models used, we find an improved goodness of fit for a triple system architecture that includes a low-mass (M = 0.177 ± 0.055 M
⊙) companion to the primary star. Further studies of this system will be required in order to resolve this discrepancy, either by refining the parallax measurement with a more complex treatment of variability-induced astrometric motion or by detecting a third companion.
A Solution to Continuous RFI in Narrowband Radio SETI with FAST: The MultiBeam Point-source Scanning Strategy
Authors: Huang Bo-Lun , Tao Zhen-Zhao , Zhang Tong-Jie 
Published: November 2023

Abstract
Narrowband radio search for extraterrestrial intelligence (SETI) in the 21st century suffers severely from radio frequency interference (RFI), resulting in a high number of false positives, and it could be the major reason why we have not yet received any messages from space. We thereby propose a novel observation strategy, called MultiBeam Point-source Scanning (MBPS), to revolutionize the way RFI is identified in narrowband radio SETI and provide a prominent solution to the current situation. The MBPS strategy is a simple yet powerful method that sequentially scans over the target star with different beams of a telescope, creating real-time references in the time domain for cross-verification and thus potentially identifying all continuous RFI with a level of certainty never achieved in any previous attempts. By applying the MBPS strategy during the observation of TRAPPIST-1 with the Five-hundred-meter Aperture Spherical radio Telescope, we successfully identified all 6972 received signals as RFI using the solid criteria introduced by the MBPS strategy. Therefore, we present the MBPS strategy as a promising tool that should bring us much closer to the first discovery of a genuine galactic greeting.
HH 80/81: Structure and Kinematics of the Fastest Protostellar Outflow
Authors: Bally John , Reipurth Bo 
Published: November 2023

Abstract
Hubble Space Telescope (HST) images obtained in 2018 are combined with archival HST data taken in 1995 to detect changes and measure proper motions in the HH 80/81 shock complex, which is powered by the fastest known jet driven by a forming star, the massive object IRAS 18162-2048. Some persistent features close to the radio jet axis have proper motions of >1000 km s−1 away from IRAS 18162-2048. About 3–5 pc downstream from the IRAS source and beyond HH 80/81, Hα emission traces the rim of a parsec-scale bubble blown by the jet. Lower speed motions are seen in [S ii] away from the jet axis; these features have a large component of motion at right angles to the jet. We identify new HH objects and H2 shocks in the counterflow opposite HH 80/81. The northeastern counterflow to HH 80/81 exhibits an extended but faint complex of 2.12 μm H2 shocks. The inner portion of the outflow is traced by dim 1.64 μm [Fe ii] emission. The full extent of this outflow is at least 1500″ (∼10 pc in projection at a distance of 1.4 kpc). We speculate about the conditions responsible for the production of the ultrafast jet and the absence of prominent large-scale molecular outflow lobes.
Predicting the Radiation Field of Molecular Clouds Using Denoising Diffusion Probabilistic Models
Authors: Xu Duo , Offner Stella S. R. , Gutermuth Robert , Grudić Michael Y. , Guszejnov Dávid , Hopkins Philip F. 
Published: November 2023

Abstract
Accurately quantifying the impact of radiation feedback in star formation is challenging. To address this complex problem, we employ deep-learning techniques known as denoising diffusion probabilistic models (DDPMs) to predict the interstellar radiation field (ISRF) strength based on three-band dust emission at 4.5, 24, and 250 μm. We adopt magnetohydrodynamic simulations from the STARFORGE project that model star formation and giant molecular cloud (GMC) evolution. We generate synthetic dust emission maps matching observed spectral energy distributions in the Monoceros R2 (MonR2) GMC. We train DDPMs to estimate the ISRF using synthetic three-band dust emission. The dispersion between the predictions and true values is within a factor of 0.1 for the test set. We extended our assessment of the diffusion model to include new simulations with varying physical parameters. While there is a consistent offset observed in these out-of-distribution simulations, the model effectively constrains the relative intensity to within a factor of 2. Meanwhile, our analysis reveals a weak correlation between the ISRF solely derived from dust temperature and the actual ISRF. We apply our trained model to predict the ISRF in MonR2, revealing a correspondence between intense ISRF, bright sources, and high dust emission, confirming the model’s ability to capture ISRF variations. Our model robustly predicts radiation feedback distribution, even in complex, poorly constrained ISRF environments like those influenced by nearby star clusters. However, precise ISRF predictions require an accurate training data set mirroring the target molecular cloud’s unique physical conditions.
A Chandra Study of the NGC 7618/UGC 12491 Major Group Merger at Apogee: Multiple Cold Fronts, Boxy Wings, Filaments, and Arc-shaped Slingshot Tails
Authors: Machacek M. E. , Jones C. , Kraft R. P. , Forman W. R. , Roediger E. , Sheardown A. , Wan J. T. 
Published: November 2023

Abstract
Analyses of major group mergers are key to understanding the evolution of large-scale structure in the Universe and the microphysical properties of the hot gas in these systems. We present imaging and spectral analyses of deep Chandra observations of hot gas structures formed in the major merger of the NGC 7618 and UGC 12491 galaxy groups and compare the observed hot gas morphology, temperatures, and abundances with recent simulations. The morphology of the observed multiple cold front edges and boxy wings are consistent with those expected to be formed by Kelvin–Helmholtz instabilities and gas sloshing in inviscid gas. The arc-shaped slingshot tail morphologies seen in each galaxy suggest that the dominant galaxies are near their orbital apogee after having experienced at least one core passage at a large impact parameter.
Unraveling the Thermodynamic Enigma between Fast and Slow Coronal Mass Ejections
Authors: Khuntia Soumyaranjan , Mishra Wageesh , Mishra Sudheer K. , Wang Yuming , Zhang Jie , Lyu Shaoyu 
Published: November 2023

Abstract
Coronal mass ejections (CMEs) are the most energetic expulsions of magnetized plasma from the Sun that play a crucial role in space weather dynamics. This study investigates the diverse kinematics and thermodynamic evolution of two CMEs (CME1: 2011 September 24 and CME2: 2018 August 20) at coronal heights where thermodynamic measurements are limited. The peak 3D propagation speed of CME1 is high (1885 km s−1) with two-phase expansion (rapid and nearly constant), while the peak 3D propagation speed of CME2 is slow (420 km s−1) with only a gradual expansion. We estimate the distance-dependent variations in the polytropic index, heating rate, temperature, and internal forces implementing the revised FRIS model, taking inputs of 3D kinematics estimated from the graduated cylindrical shell model. We find CME1 exhibiting heat release during its early-rapid acceleration decrease and jumps to the heat-absorption state during its constant acceleration phase. In contrast to CME1, CME2 shows a gradual transition from the near-adiabatic to the heat-absorption state during its gradually increasing acceleration. Our analysis reveals that although both CMEs show differential heating, they experience heat absorption during their later propagation phases, approaching the isothermal state. The faster CME1 achieves an adiabatic state followed by an isothermal state at smaller distances from the Sun than the slower CME2. We also find that the expansion of CMEs is primarily influenced by centrifugal and thermal pressure forces, with the Lorentz force impeding expansion. Multiwavelength observations of flux-ropes at source regions support the FRIS-model-derived findings at initially observed lower coronal heights.