bluuebunny/crossref_metadata_2025_split huggingface dataset:
Effectiveness of Sirsak Fruit Juice Therapy to Decreasing Elderly Acid Acid Levels in Tresna Werdha Social Beach Pagar Dewa Bengkulu
Authors: Dwiana Dian , Effendi Santoso Ujang , Vaudyah Vusva 
Published: July 2020

Uric acid is the end product or a waste product resulting from the metabolism/ breakdown of purines .. The purpose of this study was to determine the effectiveness of Soursop fruit juice therapy to decrease uric acid levels in the Elderly Social Institution Tresna Werdha Pagar Dewa Bengkulu year 2018. The design of this Penenlitian pre- experimental. The population in this study who had the Uric Acid in Elderly Social Institution Tresna Pagar Dewa Bengkulu which amount 17 people. The sampling technique used Total sampling technique. Collecting data in this study is the observation uric acid levels before and after therapy soursop juice for 2 minggu..Hasil research showed: (1) there are 17 people (100%) with high levels of uric acid 6 mg / dl; (2) there are 13 people (76.5%) had decreased levels of uric acid, and 4 (23, 5%) who did not experience decreased levels of uric acid; (3) No effect Soursop fruit juice therapy to decrease uric acid levels in the Elderly Social Institution Tresna Werdha Pagar Dewa Bengkulu. Keywords: elderly, uric acid, soursop juice
Knowledge, Attitudes of Mothers, and Mothers’s Participation in Pregnant Mother Class in Working Area of Sidodadi Public Health Center Bengkulu
Authors: Rahmadhaniati Yuni , Wulandari Elza , Wahyuni Rida 
Published: July 2020

Class of pregnant women is a study group of pregnant women with gestational age between 20 weeks to 36 weeks (before delivery) with a maximum number of participants of 10 people. This study aims to study the relationship between knowledge and attitudes of mothers with the participation of classes of pregnant women in the Sidodadi Public Health Center Working Area in Central Bengkulu Regency. This study used a cross sectional design. The population in this study were third trimester pregnant women who lived in the Sidodadi Public Health Center Working Area in June 2018 as many as 58 pregnant women. Taking sample cases using the Total Sampling technique is that all pregnant women in the third trimester who live in the Sidodadi Public Health Center Working Area as many as 58 pregnant women are sampled. The results were obtained: (1) there were 24 with a percentage of 41.4% who did not take classes in pregnant women and 34 people with a percentage of 58.6% who attended classes in pregnant women; (2) there are 19 pregnant women with a percentage of 32.8% who lack knowledge, there are 22 pregnant women with a percentage of 37.9% who have sufficient knowledge and there are 17 pregnant women with a percentage of 29.3% who are well-informed; (3) there are 26 pregnant women with a percentage of 44.8% who do not support, and there are 32 pregnant women with a percentage of 55.2% who support; (4) There was a significant relationship between knowledge with the participation of pregnant women with a moderate relationship category; (5) There was a significant relationship between the attitude of mothers and the participation of classes of pregnant women with the category of moderate relationships. It was recommended to Sidodadi Public Health Center to further improve health services, provide health related information during pregnancy and encourage pregnant women to take part in pregnancy exercises.] Keywords: class of pregnant women, knowledge, mother's attitude
Husband’s Support, Work Environment, and Exclusive Breastfeeding in Health Department of Bengkulu Province
Authors: Sanisahhuri Sanisahhuri , Wahyuni Sri , Wulan Susilo 
Published: July 2020

Every baby has the right to get exclusive mother's water from birth for 6 (six) months, except for medical indications. During the provision of breast milk, the family, the government, the local government and the community must fully support the mother's baby with the provision of special time and facilities. Provision of special facilities is held at work and in public places. The purpose of this study was to determine the factors related to the provision of exclusive breastfeeding by mothers who worked in the Bengkulu Provincial Health Office. The study was conducted using Cross Sectional research design. The population in this study is all mothers who have children under the age of five years using total sampling technique. Data collection techniques using primary data by distributing questionnaires and secondary data are data obtained from the study of documents or files in the Bengkulu Provincial Health Office. Data were analyzed by univariate and bivariate using Chi-Square statistical test. The results of this study indicate that there is a significant relationship between the knowledge of mothers with exclusive breastfeeding by working mothers in the Bengkulu Provincial Health Office, namely 63.6% of mothers who have sufficient knowledge not to provide exclusive breastfeeding, then there is no significant relationship between husband's support and work environment with Exclusive breastfeeding by working mothers at the Bengkulu Provincial Health Office. Keywords: exclusive breastfeeding, husband’s support, mother knowledge, work environment
The Analysis of Sanitation and Hygiene Application of Food Management Place in Restaurant Bengkulu City
Authors: Khairani Nurul , Effendi Santoso Ujang , Lestari Refti Febli , Fauzi Yusran 
Published: July 2020

Restaurant is a commercial venue where the scope of its activities provide food and beverages to the public in the place of business. This restaurant arises and develops in line with the development of society in serving the needs of consumers. This if not supported by hygiene food processing and good sanitation conditions it will cause food poisoning or diseases such as diarrhea. The purpose of this research is to analysis of sanitation and hygiene application of food management place in restaurant Bengkulu City. Type of research used is descriptive with qualitative method, Informant in this research amounted to 4 person that is, owner of restaurant A, owner of restaurant B, restaurant owner C, Head of Environmental Health Counseling Dinkes Kota Bengkulu. The instruments used are observation sheets and interview guides. Data analysis was done by collecting interview result data then described to describe applying sanitation hygiene in restaurant with Triangulation technique. The result of this research is the application of sanitation hygiene at restaurant A (776), B (721) and C (720) have fulfilled the health requirement which refers to Permenkes Number: 1098 / Menkes / SK / VII / 2003 so that the restaurant is sanitary hygiene and safe for public consumption, between input and process restaurants A, B, and C input it has been referring to the foundation and the existing regulations as well as the supervision of sanitarian power has been executed so that at the stage of the process have a good effect on the restaurant supported by the assessment of sanitarian power. It is expected that local health agencies to more often hold activities that are promotive and preventive about the importance of the application of hygiene sanitation food processing in restaurants. Keywords : hygiene, restaurant, sanitation
Metode Penyelesaian Ta’arudh al-Adillah dalam Metodologi Hukum Islam
Authors: Fathoni Khoirul 
Published: July 2020

The efforts of mujtahids in exploring the law are certainly not as easy as we imagine. Often they find difficulties because our legal basis is sometimes miraculous. Not infrequently there is a conflict between the arguments of one with another argument, which in ushul fiqh is called ta'arudh al adillah. Usul experts mutually engaged in trying to solve the problem. In this paper, we will discuss the meaning of ta'arudh al adillah and how the method of completion is done. And also components related to ta'arudh, such as nasakh mansukh, ‘amm khash, muthlaq muqayyad, and lughawiyyah rules. This paper is in the form of descriptive, which describes the meaning of ta'arudh and how to solve it, and also matters relating to the efforts to complete ta'arudh. The author concludes that ta'arudh are two propositions, each of which denies what is pointed out by other propositions. There are two methods that are put forward in this paper, namely the Hanafiyah method and the Mutakallimin method or Jumhur Ulama. According to them there are four ways in completing ta'arudh, namely nasakh, tajih, al jam'u wa al taufiq, and tasaqut al dalilain.
Usaha para mujtahid dalam menggali hukum tentu saja tidak semudah yang kita bayangkan. Sering kali mereka menemukan kesulitan karena dasar hukum kita yang kadang bersifat mujmal. Tidak jarang terjadi pertentangan antara dalil satu dengan dalil lain, yang dalam ushul fiqh disebut ta’arudh al adillah. Para ahli ushul saling berijtihad dalam usaha memecahkan permasalahan tersebut. Dalam tulisan ini akan dibahas tentang pengertian ta’arudh al adillah berikut bagaimana metode penyeleseiannya. Dan juga komponen-komponen yang berhubungan dengan ta’arudh, seperti nasakh mansukh, ‘amm khash, muthlaq muqayyad, dan kaidah lughawiyyah. Tulisan ini berbentuk deskriptif, yaitu mendeskripsikan pengertian ta’arudh serta cara penyeleseiannya, dah juga hal-hal yang berhubungan dalam usaha penyeleseian ta’arudh. Penulis memberi kesimpulan bahwa ta’arudh ini sebagai dua dalil yang masing-masing menafikan apa yang ditunjuk oleh dalil lain. Ada dua metode yang penulisan kemukakan dalam tulisan ini, yaitu metode Hanafiyah dan metode Mutakallimin atau Jumhur Ulama. Menurut mereka ada empat cara dalam menyeleseikan ta’arudh, yaitu nasakh, tajih, al jam’u wa al taufiq, dan tasaqut al dalilain.
Taṭwīru Waḥdah Al-iliktrūni Litanmiyah Al-mahārah Al-qirā’ah; Al-taḥlīl Al-Waqi’ī bi Al-Madrasah Al-Śānawiyyah Baḥr Al-‘Ulūm Tambak Beras Jombang
Authors: Aisa Aufia , Jannah Siti Nur , Rahmawati Rina Dian 
Published: July 2020

أما أهداف هذا البحث هي معرفة تطوير المادة التعليمية الوحدة الإلكترونية (e-modul) لتنمية مهارة القراءة في الفصل العاشر بالمدرس الثانوية بحر العلوم تامباك براس جومبانج ولمعرفة فعالية تطوير المادة التعليمية الوحدة الإلكترونية (e-modul) لتنمية مهارة القراءة في الفصل العاشر بالمدرسة الثانوية بحر العلوم تامباك براس جومبانج.
تستخدم هذه الدراسة نموذج ADDIE. يتم إنشاء جمع البيانات عن طريق الملاحظة والاستبانة والمقابلة والاختبار. أظهرت نتائج التحقق من خبراء المواد 4.5 ٪ والتطبيق العملي من خبراء المواد التي أظهرت 90 ٪ وخبراء الإعلام بنسبة 4.9 ٪ والتطبيق العملي من خبراء الإعلام التي أظهرت 95 ٪. بناءً على ذلك، فإن الوسائط التي تم تطويرها للتأهيل لائق جدًا تشير نتائج تصميم الوسائط التعليمية التي أجراها الباحثة إلى أن التعلم باستخدام المادة التعليمية الوحدة الإلكترونية. وتثبت من خلال قيمة سيج. (2 - الذيل) من اختبار ما بعد أصغر من سيج. 0.05وهو 0.000 استنتاج هذه النتائج هو يوجد الفرق الدال بين كفاءة الطالبات التي لايعلمن بإستخدام المادة التعليمية وحدة الإلكترونية ويعلمن بإستخدامها مقبول.
COVID-19 Pandemic in Nigeria: A review
Authors: Elikwu Charles , Walker Oladapo 
Published: July 2020

Background: An ongoing outbreak of pneumonia associated with a novel coronavirus was reported in Wuhan city, China. This new virus was named severe acute respiratory syndrome coronavirus 2 (SARS-CoV-2) by the Coronavirus Study Group (CSG) of the International Committee on Taxonomy of Viruses. That disease, caused by the SARS-CoV-2, has been named coronavirus disease 2019 (COVID-19) by the WHO. The outbreak has since spread across the globe, including countries in Africa.
Main body: The dominant mode of transmission is from the respiratory tract, via droplets or indirectly via fomites, and to a lesser extent via aerosols.
The rapidity with which the infection spread throughout the world was unexpected. The disease has now affected 212 countries, areas, or territories, with more than 2.1 million total confirmed cases and over 144 thousand fatalities as at the time of writing. It, therefore, behooves countries of the world to take firm public health measures for the pandemic is to be contained.
Conclusion: Nigeria, with a population of at least 170 million people, is of global interest because a rapid rise in the number of infected people will have serious implications not only for the country but for the whole African continent.%MCEPASTEBIN%
Orbits for Eight Binaries
Authors: Cvetković Z. , Pavlović R. 
Published: July 2020

Abstract
The subject of the present paper is the analysis of the orbital solutions for eight binaries: WDS 02402+0436 = HDS 347, WDS 02552+5950 = MLR 520, WDS 03119+6131 = HDS 407, WDS 04570+7350 = YSC 145, WDS 05202+4105 = HDS 701, WDS 06467+0822 = HDS 940AB, WDS 08259–1623 = HDS 1199, and WDS 22550+5132 = HU 785. Seven orbits are determined for the first time, and the remaining orbit is a revision. The five binaries are HDS, discovered during the Hipparcos mission, two binaries were discovered before, 1902 and 1974, and one binary was discovered afterwards, 2009. All measured separations are less than 1 arcsecond, and in most studied pairs they are less than 0.4 arcseconds. The number of measurements is relatively small, from 9 to 16, except for one pair which has only been measured six times so far. The median orbital period is 95.1 yr, the shortest period is 12.5 yr, and the longest period is 362.7 yr. In addition to the orbital elements, we also give absolute magnitudes, spectral types, estimates of the masses, dynamical parallaxes, and

residuals in θ and ρ.
Stellar Variability in a Forming Massive Star Cluster
Authors: Cheng Yu , Andersen Morten , Tan Jonathan 
Published: July 2020

Abstract
We present a near-infrared (NIR) variability analysis for a 6′ × 6′ region, which encompasses the massive protocluster G286.21+0.17. The total sample comprises more than 5000 objects, of which 562 show signs of a circumstellar disk based on their infrared colors. The data includes Hubble Space Telescope observations taken in two epochs separated by 3 yr in the F110W and F160W bands. 363 objects (7% of the sample) exhibit NIR variability at a significant level (Stetson index >1.7), and a higher variability fraction (14%) is found for the young stellar objects with disk excesses. We identified four high amplitude (>0.6 mag) variables seen in both NIR bands. Follow-up and archival observations of the most variable object in this survey (G286.2032+0.1740) reveal a rising light curve over 8 yr from 2011 to 2019, with a K band brightening of 3.5 mag. Overall the temporal behavior of G286.2032+0.1740 resembles that of typical FU Ori objects; however, its pre-burst luminosity indicates it has a very low mass (<0.12 M
⊙), making it an extreme case of an outburst event that is still ongoing.
Properties of Galactic B[e] Supergiants. V. 3 Pup–Constraining the Orbital Parameters and Modeling the Circumstellar Environments
Authors: Miroshnichenko A. S. , Danford S. , Zharikov S. V. , Klochkova V. G. , Chentsov E. L. , Vanbeveren D. , Zakhozhay O. V. , Manset N. , Pogodin M. A. , Omarov C. T. , Kuratova A. K. , Khokhlov S. A. 
Published: July 2020

Abstract
We report the results of long-term spectroscopic monitoring of the A-type supergiant with the B[e] phenomenon 3 Pup = HD 62623. We confirm earlier findings that it is a binary system. The orbital parameters were derived using cross-correlation of the spectra in a range of 4460–4632 Å, which contains over 30 absorption lines. The orbit was found to be circular with a period of 137.4 ± 0.1 days, radial velocity semiamplitude K
1 = 5.0 ± 0.8 km s−1, systemic radial velocity γ = +26.4 ± 2.0 km s−1, and mass function

M
⊙. The object may have evolved from a pair with initial masses of ∼6.0

and ∼3.6 M
⊙ with an initial orbital period of ∼5 days. Based on the fundamental parameters of the A-supergiant (luminosity log L/L
⊙ = 4.1 ± 0.1 and effective temperature T
eff = 8500 ± 500 K) and evolutionary tracks of mass-transferring binaries, we found current masses of the gainer M
2 = 8.8 ± 0.5 M
⊙ and donor M
1 = 0.75 ± 0.25 M
⊙. We also modeled the object’s IR-excess and derived a dust mass of ∼5 × 10−5
M
⊙ in the optically thin dusty disk. The orbital parameters and properties of the Hα line profile suggest that the circumstellar gaseous disk is predominantly circumbinary. The relatively low mass of the gainer led us to a suggestion that 3 Pup should be excluded from the B[e] supergiant group and moved to the FS CMa group. Overall these results further support our original suggestion that FS CMa objects are binary systems, where an earlier mass transfer caused formation of the circumstellar envelope.
Imaging the 511 keV Positron Annihilation Sky with COSI
Authors: Siegert Thomas , Boggs Steven E. , Tomsick John A. , Zoglauer Andreas C. , Kierans Carolyn A. , Sleator Clio C. , Beechert Jacqueline , Brandt Theresa J. , Jean Pierre , Lazar Hadar , Lowell Alex W. , Roberts Jarred M. , Ballmoos Peter von 
Published: July 2020

Abstract
The balloon-borne Compton Spectrometer and Imager (COSI) had a successful 46-day flight in 2016. The instrument is sensitive to photons in the energy range 0.2–5 MeV. Compton telescopes have the advantage of a unique imaging response and provide the possibility of strong background suppression. With its high-purity germanium detectors, COSI can precisely map γ-ray line emission. The strongest persistent and diffuse γ-ray line signal is the 511 keV emission line from the annihilation of electrons with positrons from the direction of the Galactic center. While many sources have been proposed to explain the amount of positrons,

, the true contributions remain unsolved. In this study, we aim at imaging the 511 keV sky with COSI and pursue a full-forward modeling approach, using a simulated and binned imaging response. For the strong instrumental background, we describe an empirical approach to take the balloon environment into account. We perform two alternative methods to describe the signal: Richardson–Lucy deconvolution, an iterative method toward the maximum likelihood solution, and model fitting with predefined emission templates. Consistently with both methods, we find a 511 keV bulge signal with a flux between 0.9 and

, confirming earlier measurements, and also indications of more extended emission. The upper limit we find for the 511 keV disk,

, is consistent with previous detections. For large-scale emission with weak gradients, coded aperture mask instruments suffer from their inability to distinguish isotropic emission from instrumental background, while Compton telescopes provide a clear imaging response, independent of the true emission.
Selection of Massive Evolved Galaxies at 3 ≤ z ≤ 4.5 in the CANDELS Fields
Authors: Shahidi Abtin , Mobasher Bahram , Nayyeri Hooshang , Hemmati Shoubaneh , Wiklind Tommy , Chartab Nima , Dickinson Mark , Finkelstein Steven L , Pacifici Camilla , Papovich Casey , Ferguson Henry C. , Fontana Adriano , Giavalisco Mauro , Koekemoer Anton , Newman Jeffery , Sattari Zahra , Somerville Rachel 
Published: July 2020

Abstract
Using the CANDELS photometric catalogs for the Hubble Space Telescope/ACS and WFC3, we identified massive evolved galaxies at 3 < z < 4.5 employing three different selection methods. We find the comoving number density of these objects to be ∼2 × 10−5 and 8 × 10−6 Mpc−3 after correction for completeness for two redshift bins centered at z = 3.4, 4.7. We quantify a measure of how much confidence we should have for each candidate galaxy from different selections and what the conservative error estimates propagated into our selection are. Then we compare the evolution of the corresponding number densities and their stellar mass density with numerical simulations, semianalytical models, and previous observational estimates, which shows slight tension at higher redshifts as the models tend to underestimate the number and mass densities. By estimating the average halo masses of the candidates (M

h
≈ 4.2, 1.9, and 1.3 × 1012
M
⊙ for redshift bins centered at z = 3.4, 4.1, and 4.7), we find them to be consistent with halos that were efficient in turning baryons to stars, relatively immune to the feedback effects, and on the verge of transition into hot-mode accretion. This can suggest the relative cosmological starvation of the cold gas followed by an overconsumption phase in which the galaxy rapidly consumes the available cold gas as one of the possible drivers for the quenching of the massive evolved population at high redshift.
Long-term Near-infrared Brightening of Nonvariable OH/IR Stars
Authors: Kamizuka Takafumi , Nakada Yoshikazu , Yanagisawa Kenshi , Ohsawa Ryou , Ita Yoshifusa , Izumiura Hideyuki , Mito Hiroyuki , Onozato Hiroki , Asano Kentaro , Ueta Toshiya , Miyata Takashi 
Published: July 2020

Abstract
Nonvariable OH/IR stars are thought to have just left the asymptotic giant branch (AGB) phase. In this conventional picture, they must still show strong circumstellar extinction caused by the dust ejected during the AGB phase, and the extinction is expected to decrease over time because of the dispersal of the circumstellar dust after the cessation of stellar mass loss. The reduction of extinction makes the stars become apparently brighter and bluer with time, especially in the near-infrared (NIR) range. We look for such long-term brightening of nonvariable OH/IR stars by using 2MASS, UKIDSS, and OAOWFC survey data. As such, we obtain multiepoch NIR data taken over a 20 yr period (1997–2017) for 6 of 16 nonvariable OH/IR stars, and all 6 objects are found to be brightening. The K-band brightening rate of five objects ranges from 0.010 to 0.130 mag yr−1, which is reasonably explained with the conventional picture. However, one OH/IR star, OH 31.0−0.2, shows a rapid brightening, which cannot be explained only by the dispersal of the dust shell. Multicolor (J-, H-, and K-band) data are obtained for three objects, OH 25.1−0.3, OH 53.6−0.2, and OH 77.9+0.2. Surprisingly, none of them appears to have become bluer, and OH 53.6−0.2 is found to have reddened at a rate of 0.013 mag yr−1 in (J – K). Our findings suggest other mechanisms such as rapid changes in stellar properties (temperature or luminosity) or a generation of a new batch of dust grains.
Estimating the Energy Dissipation from Kelvin–Helmholtz Instability Induced Turbulence in Oscillating Coronal Loops
Authors: Hillier Andrew , Van Doorsselaere Tom , Karampelas Konstantinos 
Published: July 2020

Abstract
Kelvin–Helmholtz instability induced turbulence is one promising mechanism by which loops in the solar corona can be heated by MHD waves. In this Letter we present an analytical model of the dissipation rate of Kelvin–Helmholtz instability induced turbulence ε
D, finding it scales as the wave amplitude (d) to the third power (ε
D ∝ d
3). Based on the concept of steady-state turbulence, we expect the turbulence heating throughout the volume of the loop to match the total energy injected through its footpoints. In situations where this holds, the wave amplitude has to vary as the cube-root of the injected energy. Comparing the analytic results with those of simulations shows that our analytic formulation captures the key aspects of the turbulent dissipation from the numerical work. Applying this model to the observed characteristics of decayless kink waves we predict that the amplitudes of these observed waves are insufficient to turbulently heat the solar corona.